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Tutorial”Œ3https://www.planetmechanic.net/gamit-globk-tutorial”†”Œ!Abdelali Fadil's YouTube Playlist”ŒHhttps://www.youtube.com/playlist?list=PLwvmy9jACWW-2ijMpAFaBW2zEeC_1_SM-”†”ejþ]”jJÿÿÿÿjŒUnaffiliated External Resources”j‰jˆj‰jKj‰j]”(jüjÿejrjujÄjñhj1jÆKFj¶jïubaj·}”(j¹]”j»]”j aj½]”jÀ]”jÂ]”ujÄjìj¶jNjÇjþhj1jÆNubj )”}”(j¦ŒZIndices and tables ================== * :ref:`genindex` * :ref:`modindex` * :ref:`search`”j§]”j±ŒZIndices and tables ================== * :ref:`genindex` * :ref:`modindex` * :ref:`search`”…””}”j¶j sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0ujÄjj¶jNjÇjþhj1jÆKSubej·}”(j¹]”Œ&welcome-to-gamit-globk-s-documentation”aj»]”j½]”Œ'welcome to gamit/globk's documentation!”ajÀ]”jÂ]”ujÄh_j¶jþjÇjþhj1jÆKubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j1j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj1jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j jjjuj_}”(Œrel”j Œdate”jujc}”je}”jg}”jjsji}”j‰sj¹}”jjNsjl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jˆNj‰]”j‹NjÇjþubjùj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jFsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jCjÇjCubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jUjÇjChNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jCjÇjCubj©Œtarget”“”)”}”(j¦Œ.. _intro_eval:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefid”Œ intro-eval”ujÄjdjÆKj¶jCjÇjChŒ>/chandler/home/floyd/public_html/gg/docs/source/intro/eval.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ*Evaluating the Results of Daily Processing”j§]”j±Œ*Evaluating the Results of Daily Processing”…””}”(j¶jvjÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jsjÇjChjrjÆKubj`)”}”(j¦ŒmThere are three primary criteria you should use to determine if your phase processing produced a good result:”j§]”j±ŒmThere are three primary criteria you should use to determine if your phase processing produced a good result:”…””}”(j¶j„jÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆKj¶jsjÇjCubj©Œ bullet_list”“”)”}”(j¦hoj§]”(j©Œ list_item”“”)”}”(j¦Œ'All of the expected data were included.”j§]”j`)”}”(j¦j›j§]”j±Œ'All of the expected data were included.”…””}”(j¶jjÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK j¶j™ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j”jÇjChjrjÆNubj˜)”}”(j¦Œ-The data fit the model at the expected level.”j§]”j`)”}”(j¦j²j§]”j±Œ-The data fit the model at the expected level.”…””}”(j¶j´jÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK j¶j°ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j”jÇjChjrjÆNubj˜)”}”(j¦Œ(The uncertainties are acceptably small. ”j§]”j`)”}”(j¦Œ'The uncertainties are acceptably small.”j§]”j±Œ'The uncertainties are acceptably small.”…””}”(j¶jËjÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK j¶jÇubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j”jÇjChjrjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œbullet”Œ*”ujÄj’hjrjÆK j¶jsjÇjCubj`)”}”(j¦X`In most cases you can assess these three requirements quickly using the GAMIT summary emailed to you by :program:`sh_gamit` (and saved as :file:`sh_gamit_{}.summary` in the day directory) together with the plots of daily repeatabilities created by :program:`sh_glred`. Following is the summary file from day 034 of the Southern California example:”j§]”(j±ŒhIn most cases you can assess these three requirements quickly using the GAMIT summary emailed to you by ”…””}”(j¶jçjÇjChNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jïjÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jçubj±Œ (and saved as ”…””}”(j¶jçjÇjChNjÆNubj˜)”}”(j¦Œ :file:`sh_gamit_{}.summary`”j§]”(j±Œ sh_gamit_”…””}”(j¶jjÇjChNjÆNubj©Œemphasis”“”)”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jubj±Œ.summary”…””}”(j¶jjÇjChNjÆNubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jçubj±ŒS in the day directory) together with the plots of daily repeatabilities created by ”…””}”(j¶jçjÇjChNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j*jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jçubj±ŒP. Following is the summary file from day 034 of the Southern California example:”…””}”(j¶jçjÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK j¶jsjÇjCubj)”}”(j¦X7Input options -expt scal -d 2000 034 -netext a -orbit IGSF -noftp -remakex Y Processing 2000 034 GPS week 1047 4 Raw 0 /chandler/data30/rwk/active/example/034a Disk Usage: 37537 Free 31764.5 Mbyte. Used 55% Number of stations used 5 Total xfiles 5 Postfit RMS rms, total and by satellite RMS IT Site All 01 02 03 04 05 06 07 08 09 10 11 13 14 15 16 17 18 19 21 22 23 24 25 26 27 29 30 31 RMS 26 ALL 4.4 46 35 56 42 38 42 42 38 51 44 61 41 0 42 44 40 40 42 36 52 40 40 38 49 38 37 45 55 Best and Worst two sites: RMS 26 JPLM 3.2 3 3 4 3 3 3 3 3 4 3 3 3 0 3 3 3 3 3 3 4 3 3 3 4 3 3 4 4 RMS 26 MATH 3.5 4 2 5 4 4 3 4 4 4 4 4 3 0 3 3 3 3 3 3 4 3 3 3 4 3 3 3 4 RMS 26 7001 5.2 6 4 7 5 4 5 4 5 6 6 6 5 0 5 6 5 5 5 4 7 4 4 4 6 4 4 5 5 RMS 26 BLYT 5.5 6 4 7 5 5 5 6 5 6 5 7 5 0 6 6 5 5 5 4 6 5 5 4 6 4 5 5 7 Double difference statistics Prefit nrms: 0.25309E+01 Postfit nrms: 0.19379E+00 Prefit nrms: 0.25241E+01 Postfit nrms: 0.20241E+00 Prefit nrms: 0.25309E+01 Postfit nrms: 0.18607E+00 Prefit nrms: 0.25241E+01 Postfit nrms: 0.18889E+00 Number of double differences: 15098 Phase ambiguities (Total WL-fixed NL-fixed: 100 96 88 Phase ambiguities WL fixed 96.0% NL fixed 88.0%”j§]”j±X7Input options -expt scal -d 2000 034 -netext a -orbit IGSF -noftp -remakex Y Processing 2000 034 GPS week 1047 4 Raw 0 /chandler/data30/rwk/active/example/034a Disk Usage: 37537 Free 31764.5 Mbyte. Used 55% Number of stations used 5 Total xfiles 5 Postfit RMS rms, total and by satellite RMS IT Site All 01 02 03 04 05 06 07 08 09 10 11 13 14 15 16 17 18 19 21 22 23 24 25 26 27 29 30 31 RMS 26 ALL 4.4 46 35 56 42 38 42 42 38 51 44 61 41 0 42 44 40 40 42 36 52 40 40 38 49 38 37 45 55 Best and Worst two sites: RMS 26 JPLM 3.2 3 3 4 3 3 3 3 3 4 3 3 3 0 3 3 3 3 3 3 4 3 3 3 4 3 3 4 4 RMS 26 MATH 3.5 4 2 5 4 4 3 4 4 4 4 4 3 0 3 3 3 3 3 3 4 3 3 3 4 3 3 3 4 RMS 26 7001 5.2 6 4 7 5 4 5 4 5 6 6 6 5 0 5 6 5 5 5 4 7 4 4 4 6 4 4 5 5 RMS 26 BLYT 5.5 6 4 7 5 5 5 6 5 6 5 7 5 0 6 6 5 5 5 4 6 5 5 4 6 4 5 5 7 Double difference statistics Prefit nrms: 0.25309E+01 Postfit nrms: 0.19379E+00 Prefit nrms: 0.25241E+01 Postfit nrms: 0.20241E+00 Prefit nrms: 0.25309E+01 Postfit nrms: 0.18607E+00 Prefit nrms: 0.25241E+01 Postfit nrms: 0.18889E+00 Number of double differences: 15098 Phase ambiguities (Total WL-fixed NL-fixed: 100 96 88 Phase ambiguities WL fixed 96.0% NL fixed 88.0%”…””}”j¶jBsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjrjÆKj¶jsjÇjCubj`)”}”(j¦XPCheck first that all of the data you expected got into the processing. The :content:`Total xfiles` should equal the number of raw or RINEX files available. If the :content:`Number of stations used` is less than the total x-files, then some x-files were created but then discarded because they were too small (tracking session too short or data discarded by :program:`makex`) as measured against the :content:`minxf` value you set in :file:`process.defaults`, or because you have excluded them with the :content:`xsite` option in :file:`sites.defaults` or the :program:`sh_gamit` command line.”j§]”(j±ŒKCheck first that all of the data you expected got into the processing. The ”…””}”(j¶jRjÇjChNjÆNubj˜)”}”(j¦Œ:content:`Total xfiles`”j§]”j±Œ Total xfiles”…””}”(j¶jZjÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jRubj±ŒA should equal the number of raw or RINEX files available. If the ”…””}”(j¶jRjÇjChNjÆNubj˜)”}”(j¦Œ":content:`Number of stations used`”j§]”j±ŒNumber of stations used”…””}”(j¶jmjÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jRubj±Œ  is less than the total x-files, then some x-files were created but then discarded because they were too small (tracking session too short or data discarded by ”…””}”(j¶jRjÇjChNjÆNubjj)”}”(j¦Œ:program:`makex`”j§]”j±Œmakex”…””}”(j¶j€jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jRubj±Œ) as measured against the ”…””}”(j¶jRjÇjChNjÆNubj˜)”}”(j¦Œ:content:`minxf`”j§]”j±Œminxf”…””}”(j¶j’jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jRubj±Œ value you set in ”…””}”(j¶jRjÇjChNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶j¥jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jRubj±Œ-, or because you have excluded them with the ”…””}”(j¶jRjÇjChNjÆNubj˜)”}”(j¦Œ:content:`xsite`”j§]”j±Œxsite”…””}”(j¶jºjÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jRubj±Œ option in ”…””}”(j¶jRjÇjChNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jÍjÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jRubj±Œ or the ”…””}”(j¶jRjÇjChNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jâjÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jRubj±Œ command line.”…””}”(j¶jRjÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK,j¶jsjÇjCubj`)”}”(j¦X?There are three indications of data quality and they each measure slightly different things. The block of lines beginning with :content:`RMS` are all extracted from :file:`autcln.post.sum` and show the one-way root-mean-square residuals by satellite and station. In the :content:`RMS` second line, the first value is an overall rms in mm. The remaining values on that line break down the scatter by satellite and report the value in tenths of mm to allow better discernment of differences that might indicate a bad orbital model for one satellite. The last four lines report the values for the two sites with the lowest (JPLM and MATH in the example) and the highest (7001 and BLYT) scatter. In a typical project, the best sites will have values of 3–5 mm, and the worst 7–9 mm. Values between 10 mm and 15 mm indicate high but acceptable levels of noise, but if you reweight the data using :program:`autcln` (default and recommended) the uncertainties in position estimates for these sites will be 2–3 times higher than for the better sites. RMS values greater than 15 mm suggest a poorly tracking receiver, a high multipath environment, severe weather, or a problem with convergence in :program:`autcln`, usually caused by poor coordinates or a short span of data. If the site's coordinates had large adjustments from the preliminary run (e.g., because this was the first day of processing a new site) and the RMS value is high, try simply rerunning the day with the now-updated coordinates. For sites with high scatter, examining the sky plots and phase versus elevation plots in the :file:`figs/` directory may help you understand the source of the noise. If both of the "worst" sites have high rms, you should look at :file:`autcln.post.sum` to check other sites, which might also have high values but did not make the "top two" in the summary.”j§]”(j±ŒThere are three indications of data quality and they each measure slightly different things. The block of lines beginning with ”…””}”(j¶jújÇjChNjÆNubj˜)”}”(j¦Œ:content:`RMS`”j§]”j±ŒRMS”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶júubj±Œ are all extracted from ”…””}”(j¶jújÇjChNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum`”j§]”j±Œautcln.post.sum”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶júubj±ŒR and show the one-way root-mean-square residuals by satellite and station. In the ”…””}”(j¶jújÇjChNjÆNubj˜)”}”(j¦Œ:content:`RMS`”j§]”j±ŒRMS”…””}”(j¶j* jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶júubj±Xc second line, the first value is an overall rms in mm. The remaining values on that line break down the scatter by satellite and report the value in tenths of mm to allow better discernment of differences that might indicate a bad orbital model for one satellite. The last four lines report the values for the two sites with the lowest (JPLM and MATH in the example) and the highest (7001 and BLYT) scatter. In a typical project, the best sites will have values of 3–5 mm, and the worst 7–9 mm. Values between 10 mm and 15 mm indicate high but acceptable levels of noise, but if you reweight the data using ”…””}”(j¶jújÇjChNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j= jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶júubj±X (default and recommended) the uncertainties in position estimates for these sites will be 2–3 times higher than for the better sites. RMS values greater than 15 mm suggest a poorly tracking receiver, a high multipath environment, severe weather, or a problem with convergence in ”…””}”(j¶jújÇjChNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jO jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶júubj±X€, usually caused by poor coordinates or a short span of data. If the site’s coordinates had large adjustments from the preliminary run (e.g., because this was the first day of processing a new site) and the RMS value is high, try simply rerunning the day with the now-updated coordinates. For sites with high scatter, examining the sky plots and phase versus elevation plots in the ”…””}”(j¶jújÇjChNjÆNubj˜)”}”(j¦Œ :file:`figs/`”j§]”j±Œfigs/”…””}”(j¶ja jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶júubj±Œ directory may help you understand the source of the noise. If both of the “worst†sites have high rms, you should look at ”…””}”(j¶jújÇjChNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum`”j§]”j±Œautcln.post.sum”…””}”(j¶jv jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶júubj±Œk to check other sites, which might also have high values but did not make the “top two†in the summary.”…””}”(j¶jújÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK/j¶jsjÇjCubj`)”}”(j¦XüIf either or both of the "best" two sites have 0 RMS, then all of the data from these sites were removed by :program:`autcln`. The most common reason was that :program:`autcln` inserted too many "bias" flags (detection of a possible cycle slip), either because of poor *a priori* coordinates or poor receiver performance. The tables in :file:`autcln.post.sum` allow you to determine the reason. If it is bad *a priori* coordinates, the pseudorange rms at the top of the file will make this immediately clear:”j§]”(j±ŒpIf either or both of the “best†two sites have 0 RMS, then all of the data from these sites were removed by ”…””}”(j¶j‘ jÇjChNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j™ jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j‘ ubj±Œ". The most common reason was that ”…””}”(j¶j‘ jÇjChNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j« jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j‘ ubj±Œa inserted too many “bias†flags (detection of a possible cycle slip), either because of poor ”…””}”(j¶j‘ jÇjChNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j½ jÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j‘ ubj±Œ9 coordinates or poor receiver performance. The tables in ”…””}”(j¶j‘ jÇjChNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum`”j§]”j±Œautcln.post.sum”…””}”(j¶jÏ jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‘ ubj±Œ1 allow you to determine the reason. If it is bad ”…””}”(j¶j‘ jÇjChNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jä jÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j‘ ubj±ŒZ coordinates, the pseudorange rms at the top of the file will make this immediately clear:”…””}”(j¶j‘ jÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK;j¶jsjÇjCubj)”}”(j¦XÁAUTCLN SUMMARY FILE: Version 3.22I Clock and Range noise statistics at iteration 3 Site/PRN Allan SD@100 # Range rms # sec (ppb) (mm) 7001 1.552388 716 772.9 5353 ASH BLYT 0.448878 2876 329.3 21905 ASH JPLM 0.138763 2879 1101.2 19487 TRB LNCO 38.975374 2877 1026.4 19982 TRM MATH 100.000000 2876 482.8 18834 TRM”j§]”j±XÁAUTCLN SUMMARY FILE: Version 3.22I Clock and Range noise statistics at iteration 3 Site/PRN Allan SD@100 # Range rms # sec (ppb) (mm) 7001 1.552388 716 772.9 5353 ASH BLYT 0.448878 2876 329.3 21905 ASH JPLM 0.138763 2879 1101.2 19487 TRB LNCO 38.975374 2877 1026.4 19982 TRM MATH 100.000000 2876 482.8 18834 TRM”…””}”j¶jü sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjrjÆK@j¶jsjÇjCubj`)”}”(j¦ŒóMaximum values of 1–2 m, as in the example, are typical; if the value is greater than 5 m, a bad site coordinate is likely the problem. You can corroborate your assessment using the table reporting what :program:`autcln` did with bias flags:”j§]”(j±ŒÍMaximum values of 1–2 m, as in the example, are typical; if the value is greater than 5 m, a bad site coordinate is likely the problem. You can corroborate your assessment using the table reporting what ”…””}”(j¶j jÇjChNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j ubj±Œ did with bias flags:”…””}”(j¶j jÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆKMj¶jsjÇjCubj)”}”(j¦XÖBIAS FLAG REPORT: Types ORG-Original JMP-Big Jump ION-Ion Jump GAP-Data Gap DDS-DD scan WLS-Wide Lane DDC-DD cleaning SITE # Flagged | # Remaining | # Edited | ORG JMP ION GAP DDS WLS DDC| ORG JMP ION GAP DDS WLS DDC| ORG JMP ION GAP DDS WLS DDC| 7001 0 0 17 21 1 0 0| 0 0 12 9 1 0 0| 0 0 5 12 0 0 0| BLYT 0 0 3 27 3 0 0| 0 0 0 6 1 0 0| 0 0 3 16 2 0 0| JPLM 0 0 32 266 16 0 0| 0 0 22 10 0 0 0| 0 0 10 222 11 0 0| LNCO 0 1 26 61 2 0 0| 0 0 8 9 0 0 0| 0 1 18 28 2 0 0| MATH 0 0 15 87 0 0 0| 0 0 14 10 0 0 0| 0 0 1 12 0 0 0|”j§]”j±XÖBIAS FLAG REPORT: Types ORG-Original JMP-Big Jump ION-Ion Jump GAP-Data Gap DDS-DD scan WLS-Wide Lane DDC-DD cleaning SITE # Flagged | # Remaining | # Edited | ORG JMP ION GAP DDS WLS DDC| ORG JMP ION GAP DDS WLS DDC| ORG JMP ION GAP DDS WLS DDC| 7001 0 0 17 21 1 0 0| 0 0 12 9 1 0 0| 0 0 5 12 0 0 0| BLYT 0 0 3 27 3 0 0| 0 0 0 6 1 0 0| 0 0 3 16 2 0 0| JPLM 0 0 32 266 16 0 0| 0 0 22 10 0 0 0| 0 0 10 222 11 0 0| LNCO 0 1 26 61 2 0 0| 0 0 8 9 0 0 0| 0 1 18 28 2 0 0| MATH 0 0 15 87 0 0 0| 0 0 14 10 0 0 0| 0 0 1 12 0 0 0|”…””}”j¶j, sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjrjÆKQj¶jsjÇjCubj`)”}”(j¦XÚThe block labeled :content:`# Flagged` reports how many bias flags were initially added scan for each station and the reason why—either gap or jump in the data. For example, the :content:`DDS` column indicates the number added during the scanning of the double-difference residuals. If this number is high, :program:`autcln` detected many discontinuities, which can be due to noisy phase data but would also result if there is a large slope in the residuals due to poor coordinates or orbits. The :content:`# Remaining` block reports how many flags remained after :program:`autcln` has finished its editing. You would like all stations to look like BLYT, but this is rarely the case. The :content:`# Edited` block reports the number of bias flags removed by deleting the data affected by the bias flag (as opposed to removing the flag by reliably resolving the integer number of cycles between data segments). Confirmation of :program:`autcln`'s action is given in the editing report:”j§]”(j±ŒThe block labeled ”…””}”(j¶j< jÇjChNjÆNubj˜)”}”(j¦Œ:content:`# Flagged`”j§]”j±Œ # Flagged”…””}”(j¶jD jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j< ubj±ŒŽ reports how many bias flags were initially added scan for each station and the reason why—either gap or jump in the data. For example, the ”…””}”(j¶j< jÇjChNjÆNubj˜)”}”(j¦Œ:content:`DDS`”j§]”j±ŒDDS”…””}”(j¶jW jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j< ubj±Œs column indicates the number added during the scanning of the double-difference residuals. If this number is high, ”…””}”(j¶j< jÇjChNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jj jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j< ubj±Œ­ detected many discontinuities, which can be due to noisy phase data but would also result if there is a large slope in the residuals due to poor coordinates or orbits. The ”…””}”(j¶j< jÇjChNjÆNubj˜)”}”(j¦Œ:content:`# Remaining`”j§]”j±Œ # Remaining”…””}”(j¶j| jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j< ubj±Œ- block reports how many flags remained after ”…””}”(j¶j< jÇjChNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j< ubj±Œk has finished its editing. You would like all stations to look like BLYT, but this is rarely the case. The ”…””}”(j¶j< jÇjChNjÆNubj˜)”}”(j¦Œ:content:`# Edited`”j§]”j±Œ# Edited”…””}”(j¶j¡ jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j< ubj±ŒÛ block reports the number of bias flags removed by deleting the data affected by the bias flag (as opposed to removing the flag by reliably resolving the integer number of cycles between data segments). Confirmation of ”…””}”(j¶j< jÇjChNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j´ jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j< ubj±Œ+’s action is given in the editing report:”…””}”(j¶j< jÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK]j¶jsjÇjCubj)”}”(j¦XŸEDITING REPORT AND SITE PARAMS SITE nCLN MnOUT SNR LSNR GF03 RCLK GF02 BEND BCLS DDSC PFED GFUN BDL2 NODD ELEV EDIT MMRG ELCL Good (deg) (deg) L1 L2 7001 10.0 10.0 0 0 0 0 0 0 74 40 0 17 0 0 12 7 0 0 0 5210 BLYT 10.0 10.0 0 0 0 0 0 104 239 26 0 2 0 0 1091 3512 0 0 0 20547 JPLM 10.0 10.0 0 0 0 0 0 9 59 677 0 26 0 0 677 8 0 0 0 18055 LNCO 10.0 10.0 0 0 0 0 0 0 274 404 0 5 0 0 430 2076 0 0 0 19148 MATH 10.0 10.0 0 0 0 0 0 0 14 44 0 8 0 0 0 0 0 0 0 18768”j§]”j±XŸEDITING REPORT AND SITE PARAMS SITE nCLN MnOUT SNR LSNR GF03 RCLK GF02 BEND BCLS DDSC PFED GFUN BDL2 NODD ELEV EDIT MMRG ELCL Good (deg) (deg) L1 L2 7001 10.0 10.0 0 0 0 0 0 0 74 40 0 17 0 0 12 7 0 0 0 5210 BLYT 10.0 10.0 0 0 0 0 0 104 239 26 0 2 0 0 1091 3512 0 0 0 20547 JPLM 10.0 10.0 0 0 0 0 0 9 59 677 0 26 0 0 677 8 0 0 0 18055 LNCO 10.0 10.0 0 0 0 0 0 0 274 404 0 5 0 0 430 2076 0 0 0 19148 MATH 10.0 10.0 0 0 0 0 0 0 14 44 0 8 0 0 0 0 0 0 0 18768”…””}”j¶jÌ sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjrjÆKej¶jsjÇjCubj`)”}”(j¦XÎNote whether each site has the expected number of "good" data (the original sampling interval for 7001 in this example was 120 s, compared with 30 s for the other receivers, so the number of data is what we would expect). If a site shows many data deleted, the column headers tell you the reason; see the :program:`autcln` help file and Section 4.2 of the `GAMIT Reference Manual `_ for an explanation of each header.”j§]”(j±X5Note whether each site has the expected number of “good†data (the original sampling interval for 7001 in this example was 120 s, compared with 30 s for the other receivers, so the number of data is what we would expect). If a site shows many data deleted, the column headers tell you the reason; see the ”…””}”(j¶jÜ jÇjChNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jä jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÜ ubj±Œ" help file and Section 4.2 of the ”…””}”(j¶jÜ jÇjChNjÆNubj©Œ reference”“”)”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶jø jÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”Œrefuri”Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶jÜ ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit-reference-manual”aj»]”j½]”Œgamit reference manual”ajÀ]”jÂ]”Œrefuri”j ujÄjdŒ referenced”Kj¶jÜ ubj±Œ# for an explanation of each header.”…””}”(j¶jÜ jÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆKpj¶jsjÇjCubj`)”}”(j¦X+The last part of the :program:`sh_gamit` summary file is extracted from the :program:`solve` q-file. The first four lines list, respectively, the normalized rms (square root of :math:`\chi^2` per degree of freedom) for the constrained solution with ambiguities free, constrained solution with ambiguities resolved, loose solution with ambiguities free, and loose solution with ambiguities resolved. With the current weighting of phase observations, all of these should be ~ 0.2. If the constrained nrms values are significantly larger than the loose nrms, the data are good but the constraints you have imposed in the GAMIT solution, either on coordinates (:file:`sittbl.`) or orbits (:file:`sestbl.`), are too tight. If this is the case, try constraining only the most reliable site and look at the adjustments of the others in the q-file. The last line in the summary gives the percentage of wide-lane (WL) and narrow-lane (NL) ambiguities resolved. (Note: This form of the summary is for :content:`LC_AUTCLN`; with :content:`LC_HELP` there are only two numbers, the first being the total number of ambiguities estimated, WL + NL, corresponding to twice the first number in the :content:`LC_AUTCLN` summary, and the second being the number of NL ambiguities resolved.) With :content:`LC_AUTCLN` more than 90% of the WL ambiguities should normally be resolved for any size network unless you have short sessions, noisy pseudoranges, and/or you are not using a :file:`dcb.dat` table that includes estimated values for the epoch of your data. The percentage of NL ambiguities resolved depends on the session length, size and configuration of the network, quality of the orbits and *a priori* coordinates, and atmospheric conditions. If it is less than ~ 80%, there may be deficiencies you can address with a different analysis approach.”•j§]”(j±ŒThe last part of the ”…””}”(j¶j" jÇjChNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j* jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j" ubj±Œ$ summary file is extracted from the ”…””}”(j¶j" jÇjChNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j< jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j" ubj±ŒU q-file. The first four lines list, respectively, the normalized rms (square root of ”…””}”(j¶j" jÇjChNjÆNubj©Œmath”“”)”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶jP jÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶j" ubj±XÒ per degree of freedom) for the constrained solution with ambiguities free, constrained solution with ambiguities resolved, loose solution with ambiguities free, and loose solution with ambiguities resolved. With the current weighting of phase observations, all of these should be ~ 0.2. If the constrained nrms values are significantly larger than the loose nrms, the data are good but the constraints you have imposed in the GAMIT solution, either on coordinates (”…””}”(j¶j" jÇjChNjÆNubj˜)”}”(j¦Œ:file:`sittbl.`”j§]”j±Œsittbl.”…””}”(j¶jb jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j" ubj±Œ ) or orbits (”…””}”(j¶j" jÇjChNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jw jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j" ubj±X#), are too tight. If this is the case, try constraining only the most reliable site and look at the adjustments of the others in the q-file. The last line in the summary gives the percentage of wide-lane (WL) and narrow-lane (NL) ambiguities resolved. (Note: This form of the summary is for ”…””}”(j¶j" jÇjChNjÆNubj˜)”}”(j¦Œ:content:`LC_AUTCLN`”j§]”j±Œ LC_AUTCLN”…””}”(j¶jŒ jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j" ubj±Œ; with ”…””}”(j¶j" jÇjChNjÆNubj˜)”}”(j¦Œ:content:`LC_HELP`”j§]”j±ŒLC_HELP”…””}”(j¶jŸ jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j" ubj±Œ there are only two numbers, the first being the total number of ambiguities estimated, WL + NL, corresponding to twice the first number in the ”…””}”(j¶j" jÇjChNjÆNubj˜)”}”(j¦Œ:content:`LC_AUTCLN`”j§]”j±Œ LC_AUTCLN”…””}”(j¶j² jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j" ubj±ŒL summary, and the second being the number of NL ambiguities resolved.) With ”…””}”(j¶j" jÇjChNjÆNubj˜)”}”(j¦Œ:content:`LC_AUTCLN`”j§]”j±Œ LC_AUTCLN”…””}”(j¶jÅ jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j" ubj±Œ¥ more than 90% of the WL ambiguities should normally be resolved for any size network unless you have short sessions, noisy pseudoranges, and/or you are not using a ”…””}”(j¶j" jÇjChNjÆNubj˜)”}”(j¦Œ:file:`dcb.dat`”j§]”j±Œdcb.dat”…””}”(j¶jØ jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j" ubj±ŒÌ table that includes estimated values for the epoch of your data. The percentage of NL ambiguities resolved depends on the session length, size and configuration of the network, quality of the orbits and ”…””}”(j¶j" jÇjChNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jí jÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j" ubj±Œ‘ coordinates, and atmospheric conditions. If it is less than ~ 80%, there may be deficiencies you can address with a different analysis approach.”…””}”(j¶j" jÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆKtj¶jsjÇjCubj`)”}”(j¦X•The definitive check of your data and processing is provided by the time series generated by :program:`sh_glred` as PostScript files in :file:`gsoln/`. With 24-hr sessions and a robust stabilization, you should obtain uncertainties and repeatabilities at the level of 1–2 mm for horizontal coordinates and 3–5 mm for heights. With 8-hr sessions, the horizontal should be 2–4 mm and height 10–15 mm. If the uncertainties are high for some sites but not others, check the session length (RINEX or x-file), number of data deleted (editing summary of :file:`autcln.post.sum`), and data noise (RMS table and :content:`Elevation angle dependent RMS statistics` of :file:`autcln.post.sum` and/or :content:`A priori receiver measurement error model` in the q-file). If the uncertainties for all sites are high, then check the record of the :program:`glred` and :program:`glorg` run, e.g. :file:`globk_scal_00034.org`:”j§]”(j±Œ]The definitive check of your data and processing is provided by the time series generated by ”…””}”(j¶j jÇjChNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j ubj±Œ as PostScript files in ”…””}”(j¶j jÇjChNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubj±X•. With 24-hr sessions and a robust stabilization, you should obtain uncertainties and repeatabilities at the level of 1–2 mm for horizontal coordinates and 3–5 mm for heights. With 8-hr sessions, the horizontal should be 2–4 mm and height 10–15 mm. If the uncertainties are high for some sites but not others, check the session length (RINEX or x-file), number of data deleted (editing summary of ”…””}”(j¶j jÇjChNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum`”j§]”j±Œautcln.post.sum”…””}”(j¶j4 jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubj±Œ!), and data noise (RMS table and ”…””}”(j¶j jÇjChNjÆNubj˜)”}”(j¦Œ3:content:`Elevation angle dependent RMS statistics`”j§]”j±Œ(Elevation angle dependent RMS statistics”…””}”(j¶jI jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j ubj±Œ of ”…””}”(j¶j jÇjChNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum`”j§]”j±Œautcln.post.sum”…””}”(j¶j\ jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubj±Œ and/or ”…””}”(j¶j jÇjChNjÆNubj˜)”}”(j¦Œ4:content:`A priori receiver measurement error model`”j§]”j±Œ)A priori receiver measurement error model”…””}”(j¶jq jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j ubj±Œ[ in the q-file). If the uncertainties for all sites are high, then check the record of the ”…””}”(j¶j jÇjChNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j„ jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j ubj±Œ and ”…””}”(j¶j jÇjChNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j– jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j ubj±Œ run, e.g. ”…””}”(j¶j jÇjChNjÆNubj˜)”}”(j¦Œ:file:`globk_scal_00034.org`”j§]”j±Œglobk_scal_00034.org”…””}”(j¶j¨ jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubj±Œ:”…””}”(j¶j jÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK€j¶jsjÇjCubj)”}”(j¦Xš +++++++++++++++++++++++++++++++++++++ + GLORG Version 5.11I + +++++++++++++++++++++++++++++++++++++ Stabilization with 20.0% constant, 80.0% site dependent weighting. Delete sites with 4.0-sigma condition. Height variance factor 10.00 Position, 10.00 Velocity For Position: Min dH sigma 0.0050 m; Min RMS 0.0030 m, Min dNE sigma 0.00050 m For Velocity: Min dH sigma 0.0050 m/yr; Min RMS 0.0030 m/yr, Min dNE sigma 0.00010 m/yr Sigma Ratio to allow use: Position 2.00 Velocity 2.00 ======================================================================================== Starting Position stabilization iteration 1 L0002031200_scal.glx For 5 sites in origin, min/max hgt sigma 451.3 452.8 mm; Median 452.2 mm, Tol 10.0 mm Position system stabilization results --------------------------------------- X Translation (m) 0.24048 +- 0.00264 Iter 1 L0002031200_scal.glx Y Translation (m) 0.29123 +- 0.00398 Iter 1 L0002031200_scal.glx Z Translation (m) -0.25412 +- 0.00330 Iter 1 L0002031200_scal.glx Condition Sigmas used 0.0000 0.0000 0.0000 Sites and relative sigmas used in stabilization BLYT_GPS 1.00 7001_GPS 1.00 MATH_GPS 1.00 JPLM_GPS 1.00 LNCO_GPS 1.00 For 15 Position Iter 1 Pre RMS 0.0908 m; Post RMS 0.00362 m L0002031200_scal.glx For 5 sites in origin, min/max NE sigma 1.29 1.96 mm; Median 1.43 mm, Tol 1.00 mm”j§]”j±Xš +++++++++++++++++++++++++++++++++++++ + GLORG Version 5.11I + +++++++++++++++++++++++++++++++++++++ Stabilization with 20.0% constant, 80.0% site dependent weighting. Delete sites with 4.0-sigma condition. Height variance factor 10.00 Position, 10.00 Velocity For Position: Min dH sigma 0.0050 m; Min RMS 0.0030 m, Min dNE sigma 0.00050 m For Velocity: Min dH sigma 0.0050 m/yr; Min RMS 0.0030 m/yr, Min dNE sigma 0.00010 m/yr Sigma Ratio to allow use: Position 2.00 Velocity 2.00 ======================================================================================== Starting Position stabilization iteration 1 L0002031200_scal.glx For 5 sites in origin, min/max hgt sigma 451.3 452.8 mm; Median 452.2 mm, Tol 10.0 mm Position system stabilization results --------------------------------------- X Translation (m) 0.24048 +- 0.00264 Iter 1 L0002031200_scal.glx Y Translation (m) 0.29123 +- 0.00398 Iter 1 L0002031200_scal.glx Z Translation (m) -0.25412 +- 0.00330 Iter 1 L0002031200_scal.glx Condition Sigmas used 0.0000 0.0000 0.0000 Sites and relative sigmas used in stabilization BLYT_GPS 1.00 7001_GPS 1.00 MATH_GPS 1.00 JPLM_GPS 1.00 LNCO_GPS 1.00 For 15 Position Iter 1 Pre RMS 0.0908 m; Post RMS 0.00362 m L0002031200_scal.glx For 5 sites in origin, min/max NE sigma 1.29 1.96 mm; Median 1.43 mm, Tol 1.00 mm”…””}”j¶jà sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjrjÆK†j¶jsjÇjCubj`)”}”(j¦X!The top part of the file records the sites included in the stabilization. As :program:`glorg` iterates the stabilization, it will remove sites that have large height uncertainties or horizontal and/or height residuals compared with the uncertainties. In the final iteration, there should be at least three (and preferable many more) sites left in the stabilization, and the :content:`Post RMS` should be at the level you expect for the uncertainties (1–5 mm). The next part of the file (not shown) echoes the :program:`globk` and :program:`glorg` command files (provided :content:`CMDS` was set in :content:`org_opt`); make sure these match what you intended. The next useful section is the position summary, which shows the adjustments and uncertainties of each of the sites in north, east, and up:”j§]”(j±ŒMThe top part of the file records the sites included in the stabilization. As ”…””}”(j¶jÓ jÇjChNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jÛ jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓ ubj±X iterates the stabilization, it will remove sites that have large height uncertainties or horizontal and/or height residuals compared with the uncertainties. In the final iteration, there should be at least three (and preferable many more) sites left in the stabilization, and the ”…””}”(j¶jÓ jÇjChNjÆNubj˜)”}”(j¦Œ:content:`Post RMS`”j§]”j±ŒPost RMS”…””}”(j¶jí jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÓ ubj±Œv should be at the level you expect for the uncertainties (1–5 mm). The next part of the file (not shown) echoes the ”…””}”(j¶jÓ jÇjChNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓ ubj±Œ and ”…””}”(j¶jÓ jÇjChNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓ ubj±Œ command files (provided ”…””}”(j¶jÓ jÇjChNjÆNubj˜)”}”(j¦Œ:content:`CMDS`”j§]”j±ŒCMDS”…””}”(j¶j$ jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÓ ubj±Œ was set in ”…””}”(j¶jÓ jÇjChNjÆNubj˜)”}”(j¦Œ:content:`org_opt`”j§]”j±Œorg_opt”…””}”(j¶j7 jÇjChNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÓ ubj±Œ·); make sure these match what you intended. The next useful section is the position summary, which shows the adjustments and uncertainties of each of the sites in north, east, and up:”…””}”(j¶jÓ jÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆKŸj¶jsjÇjCubj)”}”(j¦X< SUMMARY POSITION ESTIMATES FROM GLOBK Ver 5.11I Long. Lat. dE adj. dN adj. dE +- dN +- RHO dH adj. dH +- SITE (deg) (deg) (mm) (mm) (mm) (mm) (mm) (mm) 245.285 33.610 -3.78 2.72 1.59 1.37 -0.062 37.86 6.07 BLYT_GPS* 243.531 34.560 0.12 -0.37 1.02 0.98 0.039 -9.53 4.71 7001_GPS* 242.563 33.857 1.33 -0.64 0.86 0.83 0.012 -1.86 4.04 MATH_GPS* 241.827 34.205 0.50 -0.51 0.85 0.80 0.031 -4.66 3.87 JPLM_GPS* 240.942 36.360 -0.27 0.42 1.43 1.37 -0.103 -8.82 5.64 LNCO_GPS* POS STATISTICS: For 5 RefSites WRMS ENU 1.36 1.01 14.27 mm NRMS ENU 1.30 1.02 3.07”j§]”j±X< SUMMARY POSITION ESTIMATES FROM GLOBK Ver 5.11I Long. Lat. dE adj. dN adj. dE +- dN +- RHO dH adj. dH +- SITE (deg) (deg) (mm) (mm) (mm) (mm) (mm) (mm) 245.285 33.610 -3.78 2.72 1.59 1.37 -0.062 37.86 6.07 BLYT_GPS* 243.531 34.560 0.12 -0.37 1.02 0.98 0.039 -9.53 4.71 7001_GPS* 242.563 33.857 1.33 -0.64 0.86 0.83 0.012 -1.86 4.04 MATH_GPS* 241.827 34.205 0.50 -0.51 0.85 0.80 0.031 -4.66 3.87 JPLM_GPS* 240.942 36.360 -0.27 0.42 1.43 1.37 -0.103 -8.82 5.64 LNCO_GPS* POS STATISTICS: For 5 RefSites WRMS ENU 1.36 1.01 14.27 mm NRMS ENU 1.30 1.02 3.07”…””}”j¶jP sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjrjÆK¦j¶jsjÇjCubj`)”}”(j¦X¹The starred sites are those used in the stabilization (all in this case since the :file:`.apr` file is based on a previous solution); if there is sufficient redundancy, the individual adjustments will be useful in determining if the quality (rms) of the stabilization is degraded by the inclusion of particular sites. The stabilization statistics at the end of the position summary are shown for each component (north, east, up) rather than a combination of the three as given in the output at the top of the file. A more detailed discussion of :program:`globk` and :program:`glorg` output can be found in Section 3.5 of the `GLOBK Reference Manual `_.”j§]”(j±ŒRThe starred sites are those used in the stabilization (all in this case since the ”…””}”(j¶j` jÇjChNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jh jÇjChNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j` ubj±Xà file is based on a previous solution); if there is sufficient redundancy, the individual adjustments will be useful in determining if the quality (rms) of the stabilization is degraded by the inclusion of particular sites. The stabilization statistics at the end of the position summary are shown for each component (north, east, up) rather than a combination of the three as given in the output at the top of the file. A more detailed discussion of ”…””}”(j¶j` jÇjChNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j} jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j` ubj±Œ and ”…””}”(j¶j` jÇjChNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j jÇjChNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j` ubj±Œ+ output can be found in Section 3.5 of the ”…””}”(j¶j` jÇjChNjÆNubj÷ )”}”(j¦ŒG`GLOBK Reference Manual `_”j§]”j±ŒGLOBK Reference Manual”…””}”(j¶j¡ jÇjChNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGLOBK Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GLOBK_Ref.pdf”ujÄjö j¶j` ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œglobk-reference-manual”aj»]”j½]”Œglobk reference manual”ajÀ]”jÂ]”Œrefuri”j± ujÄjdj Kj¶j` ubj±Œ.”…””}”(j¶j` jÇjChNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjrjÆK²j¶jsjÇjCubej·}”(j¹]”(Œ*evaluating-the-results-of-daily-processing”jqej»]”j½]”(Œ*evaluating the results of daily processing”Œ intro_eval”ejÀ]”jÂ]”ujÄh_j¶jCjÇjChjrjÆKŒexpect_referenced_by_name”}”jÏ jfsŒexpect_referenced_by_id”}”jqjfsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jrj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjrjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jRjFjajUuj_}”(Œrel”jRŒdate”jaujc}”je}”jq]”jfasjg}”(jÏ jqjÎ jË j j j» j¸ uji}”(jÏ ˆjÎ ‰j ˆj» ˆuj¹}”(jqjsjË jsj j j¸ j² ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”j©Œsystem_message”“”)”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ0Hyperlink target "intro-eval" is not referenced.”…””}”j¶jý sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jú ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”ŒINFO”Œsource”jrŒline”KujÄjø ubajˆNj‰]”j‹NjÇjCubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jjÇjubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j(jÇjhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jjÇjubje)”}”(j¦Œ.. _intro_gnss:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ intro-gnss”ujÄjdjÆKj¶jjÇjhŒD/chandler/home/floyd/public_html/gg/docs/source/intro/gnss/index.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒGNSS Measurements and Analysis”j§]”j±ŒGNSS Measurements and Analysis”…””}”(j¶jFjÇjhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jCjÇjhjBjÆKubjí)”}”(j¦hoj§]”jò)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j¶jjü]”(NŒintro/gnss/obs”†”NŒintro/gnss/model”†”NŒintro/gnss/solve”†”ejþ]”(jajcjeejJÿÿÿÿjNj‰j‰j‰jKj‰j]”ujÄjñhjBjÆKj¶jTubaj·}”(j¹]”j»]”j aj½]”jÀ]”jÂ]”ujÄjìj¶jCjÇjhjBjÆK ubej·}”(j¹]”(Œgnss-measurements-and-analysis”jAej»]”j½]”(Œgnss measurements and analysis”Œ intro_gnss”ejÀ]”jÂ]”ujÄh_j¶jjÇjhjBjÆKjÒ }”juj7sjÔ }”jAj7subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jBj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjBjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j%jj4j(uj_}”(Œrel”j%Œdate”j4ujc}”je}”jA]”j7asjg}”(jujAjtjquji}”(juˆjt‰uj¹}”(jAjCjqjCujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ0Hyperlink target "intro-gnss" is not referenced.”…””}”j¶jŸsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jœubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jBŒline”KujÄjø ubajˆNj‰]”j‹NjÇjubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jºsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j·jÇj·ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jÉjÇj·hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j·jÇj·ubje)”}”(j¦Œ.. _intro_gnss_model:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-gnss-model”ujÄjdjÆKj¶j·jÇj·hŒD/chandler/home/floyd/public_html/gg/docs/source/intro/gnss/model.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ3Modeling the Motions of the Satellites and Stations”j§]”j±Œ3Modeling the Motions of the Satellites and Stations”…””}”(j¶jçjÇj·hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jäjÇj·hjãjÆKubj`)”}”(j¦XîA first requirement of any GNSS geodetic experiment is an accurate model of the satellites' motion. The (3-dimensional) accuracy of the estimated baseline, as a fraction of its length, is roughly equal to the fractional accuracy of the orbital ephemerides used in the analysis. The accuracy of the navigation ("broadcast") orbit computed by the GNSS control centers using pseudorange measurements from < 15 tracking stations is typically 1–5 parts in :math:`10^7` (2–10 m), well within the navigation design specifications for the system but not accurate enough for the study of crustal deformation. By using phase measurements from a global network of over 100 stations, however, the International GNSS Service (IGS) :cite:p:`Beutler_et_al_1994a`, is able to determine the satellites' motion with an accuracy of 1 part in :math:`10^9` (2 cm; 5–20 cm in earlier years; see http://acc.igs.org). For GPS surveys prior to 1994, the global tracking network was much smaller but can still be used to achieve accurate results for regional surveys. If we estimate orbital parameters and include in our analysis observations from widely separated stations whose coordinates are well known, the fractional accuracy of the baselines formed by these stations is transferred through the orbits to the baselines of a regional network. For example, a 10 mm uncertainty in the relative position of sites 2500 km apart introduces an uncertainty of only ~ 1 mm in the components of a 250 km baseline. This scheme can be used successfully even with regional fiducial stations, transferring, for example, the relative accuracy of 250–500 km baselines to a network less than 100 km in extent, a helpful approach with surveys conducted prior to the availability of precise global orbits.”j§]”(j±XËA first requirement of any GNSS geodetic experiment is an accurate model of the satellites’ motion. The (3-dimensional) accuracy of the estimated baseline, as a fraction of its length, is roughly equal to the fractional accuracy of the orbital ephemerides used in the analysis. The accuracy of the navigation (“broadcastâ€) orbit computed by the GNSS control centers using pseudorange measurements from < 15 tracking stations is typically 1–5 parts in ”…””}”(j¶jõjÇj·hNjÆNubjO )”}”(j¦Œ :math:`10^7`”j§]”j±Œ10^7”…””}”(j¶jýjÇj·hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jõubj±X (2–10 m), well within the navigation design specifications for the system but not accurate enough for the study of crustal deformation. By using phase measurements from a global network of over 100 stations, however, the International GNSS Service (IGS) ”…””}”(j¶jõjÇj·hNjÆNubj’)”}”(j¦Œ:cite:p:`Beutler_et_al_1994a`”j§]”j©j*“”)”}”(j¦jj§]”j±ŒBeutler_et_al_1994a”…””}”(j¶jjÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-p”ej½]”jÀ]”jÂ]”ujÄj*j¶jubaj·}”(j¹]”Œid1”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jŒreftype”Œp”Œ refexplicit”‰Œrefwarn”‰j¶ŒBeutler_et_al_1994a”ujÄj‘hjãjÆKj¶jõubj±ŒN, is able to determine the satellites’ motion with an accuracy of 1 part in ”…””}”(j¶jõjÇj·hNjÆNubjO )”}”(j¦Œ :math:`10^9`”j§]”j±Œ10^9”…””}”(j¶j5jÇj·hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jõubj±Œ( (2 cm; 5–20 cm in earlier years; see ”…””}”(j¶jõjÇj·hNjÆNubj÷ )”}”(j¦Œhttp://acc.igs.org”j§]”j±Œhttp://acc.igs.org”…””}”(j¶jGjÇj·hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jIujÄjö j¶jõubj±Xm). For GPS surveys prior to 1994, the global tracking network was much smaller but can still be used to achieve accurate results for regional surveys. If we estimate orbital parameters and include in our analysis observations from widely separated stations whose coordinates are well known, the fractional accuracy of the baselines formed by these stations is transferred through the orbits to the baselines of a regional network. For example, a 10 mm uncertainty in the relative position of sites 2500 km apart introduces an uncertainty of only ~ 1 mm in the components of a 250 km baseline. This scheme can be used successfully even with regional fiducial stations, transferring, for example, the relative accuracy of 250–500 km baselines to a network less than 100 km in extent, a helpful approach with surveys conducted prior to the availability of precise global orbits.”…””}”(j¶jõjÇj·hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjãjÆKj¶jäjÇj·ubj`)”}”(j¦XûThe motion of a satellite can be described, in general, by a set of six initial conditions (Cartesian position and velocity, or osculating Keplerian elements, for example) and a model for the forces acting on the satellite over the span of its trajectory. To model accurately the motion, we require knowledge of the acceleration induced by the gravitational attraction of the Sun, Moon, higher order terms in the Earth's static gravity field, solid-Earth and ocean tides, and some means to account for the action of non-gravitational forces due to direct solar radiation pressure, radiation reflected from the Earth, radiation emitted by the spacecraft's radio transmission, and gas emission by the spacecraft's batteries and attitude-control system. For all GNSS satellites non-gravitational forces are the most difficult to model and have been the source of considerable research over the past 20 years (see :cite:t:`Colombo_1986`, :cite:t:`Beutler_et_al_1994b`, and :cite:t:`Ziebart_et_al_2002` for more discussion).”j§]”(j±X”The motion of a satellite can be described, in general, by a set of six initial conditions (Cartesian position and velocity, or osculating Keplerian elements, for example) and a model for the forces acting on the satellite over the span of its trajectory. To model accurately the motion, we require knowledge of the acceleration induced by the gravitational attraction of the Sun, Moon, higher order terms in the Earth’s static gravity field, solid-Earth and ocean tides, and some means to account for the action of non-gravitational forces due to direct solar radiation pressure, radiation reflected from the Earth, radiation emitted by the spacecraft’s radio transmission, and gas emission by the spacecraft’s batteries and attitude-control system. For all GNSS satellites non-gravitational forces are the most difficult to model and have been the source of considerable research over the past 20 years (see ”…””}”(j¶j`jÇj·hNjÆNubj’)”}”(j¦Œ:cite:t:`Colombo_1986`”j§]”j)”}”(j¦jjj§]”j±Œ Colombo_1986”…””}”(j¶jljÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jhubaj·}”(j¹]”Œid2”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jvŒreftype”Œt”Œ refexplicit”‰Œrefwarn”‰j¶Œ Colombo_1986”ujÄj‘hjãjÆKj¶j`ubj±Œ, ”…””}”(j¶j`jÇj·hNjÆNubj’)”}”(j¦Œ:cite:t:`Beutler_et_al_1994b`”j§]”j)”}”(j¦jj§]”j±ŒBeutler_et_al_1994b”…””}”(j¶j‘jÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jubaj·}”(j¹]”Œid3”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j›Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒBeutler_et_al_1994b”ujÄj‘hjãjÆKj¶j`ubj±Œ, and ”…””}”(j¶j`jÇj·hNjÆNubj’)”}”(j¦Œ:cite:t:`Ziebart_et_al_2002`”j§]”j)”}”(j¦j³j§]”j±ŒZiebart_et_al_2002”…””}”(j¶jµjÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j±ubaj·}”(j¹]”Œid4”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j¿Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒZiebart_et_al_2002”ujÄj‘hjãjÆKj¶j`ubj±Œ for more discussion).”…””}”(j¶j`jÇj·hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjãjÆKj¶jäjÇj·ubj`)”}”(j¦XÅIn principle, a trajectory can be generated either by analytical expressions or by numerical integration of the equations of motion; in practice, numerical integration is almost always used, for both accuracy and convenience. The position of the satellite as a function of time is then read from a table (ephemeris) generated by the numerical integration. In GAMIT the integration is performed by program arc using equations given by :cite:t:`Ash_1972`.”j§]”(j±X²In principle, a trajectory can be generated either by analytical expressions or by numerical integration of the equations of motion; in practice, numerical integration is almost always used, for both accuracy and convenience. The position of the satellite as a function of time is then read from a table (ephemeris) generated by the numerical integration. In GAMIT the integration is performed by program arc using equations given by ”…””}”(j¶jÛjÇj·hNjÆNubj’)”}”(j¦Œ:cite:t:`Ash_1972`”j§]”j)”}”(j¦jåj§]”j±ŒAsh_1972”…””}”(j¶jçjÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jãubaj·}”(j¹]”Œid5”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jñŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒAsh_1972”ujÄj‘hjãjÆKj¶jÛubj±Œ.”…””}”(j¶jÛjÇj·hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjãjÆKj¶jäjÇj·ubj`)”}”(j¦XôBesides the orbital motion of a satellite, we must take into account meter-level offsets between its center of mass and the phase-center of the transmitting antenna, including temporary excursions of several decimeters lasting up to a half-hour during the maneuvers the satellites execute to keep their solar panels facing the Sun when the orbital plane is nearly aligned with the Earth-Sun direction. For the satellites in each orbital plane, this alignment occurs for several weeks twice a year, the so-called "eclipse season". Yoaz Bar-Sever and colleagues at JPL have spent considerable effort developing models of the satellites' orientation, even to point of making the behavior more predictable by getting the US Defense Department to apply a small bias about the yaw axis to GPS satellites—a change that was implemented gradually between June 1994 and November 1995. See :cite:t:`Bar-Sever_1996` and :cite:t:`Kouba_2009` for a discussion of GPS yaw, and :cite:t:`Montenbruck_et_al_2015` for other GNSS.”j§]”(j±XwBesides the orbital motion of a satellite, we must take into account meter-level offsets between its center of mass and the phase-center of the transmitting antenna, including temporary excursions of several decimeters lasting up to a half-hour during the maneuvers the satellites execute to keep their solar panels facing the Sun when the orbital plane is nearly aligned with the Earth-Sun direction. For the satellites in each orbital plane, this alignment occurs for several weeks twice a year, the so-called “eclipse seasonâ€. Yoaz Bar-Sever and colleagues at JPL have spent considerable effort developing models of the satellites’ orientation, even to point of making the behavior more predictable by getting the US Defense Department to apply a small bias about the yaw axis to GPS satellites—a change that was implemented gradually between June 1994 and November 1995. See ”…””}”(j¶j jÇj·hNjÆNubj’)”}”(j¦Œ:cite:t:`Bar-Sever_1996`”j§]”j)”}”(j¦jj§]”j±ŒBar-Sever_1996”…””}”(j¶jjÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jubaj·}”(j¹]”Œid6”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j#Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒBar-Sever_1996”ujÄj‘hjãjÆKj¶j ubj±Œ and ”…””}”(j¶j jÇj·hNjÆNubj’)”}”(j¦Œ:cite:t:`Kouba_2009`”j§]”j)”}”(j¦j;j§]”j±Œ Kouba_2009”…””}”(j¶j=jÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j9ubaj·}”(j¹]”Œid7”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jGŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶Œ Kouba_2009”ujÄj‘hjãjÆKj¶j ubj±Œ" for a discussion of GPS yaw, and ”…””}”(j¶j jÇj·hNjÆNubj’)”}”(j¦Œ :cite:t:`Montenbruck_et_al_2015`”j§]”j)”}”(j¦j_j§]”j±ŒMontenbruck_et_al_2015”…””}”(j¶jajÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j]ubaj·}”(j¹]”Œid8”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jkŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒMontenbruck_et_al_2015”ujÄj‘hjãjÆKj¶j ubj±Œ for other GNSS.”…””}”(j¶j jÇj·hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjãjÆKj¶jäjÇj·ubj`)”}”(j¦X The position of the ground station in the Earth-centered inertial system defined by the satellites' orbits is affected by a number of geophysical phenomena. These include the Earth's rotation, precession and nutation of the spin axis in inertial space, motion of the spin axis with respect to the crust ("wobble"), luni-solar solid-body tides, and loading of the crust by ocean tides and the atmosphere. All of these effects are incorporated into the model of the phase and pseudorange observations computed in program model.”j§]”j±XThe position of the ground station in the Earth-centered inertial system defined by the satellites’ orbits is affected by a number of geophysical phenomena. These include the Earth’s rotation, precession and nutation of the spin axis in inertial space, motion of the spin axis with respect to the crust (“wobbleâ€), luni-solar solid-body tides, and loading of the crust by ocean tides and the atmosphere. All of these effects are incorporated into the model of the phase and pseudorange observations computed in program model.”…””}”(j¶j‡jÇj·hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjãjÆKj¶jäjÇj·ubj`)”}”(j¦XâIn modeling the phase and pseudorange observations, we must also take into account changes in the apparent distance due to variations in the phase centers of the transmitting and receiving antennas. With matched ground antennas in a regional network, these effects nearly cancel, but for longer baselines and/or different antenna types they can amount to several centimeters in estimated heights. Models for the phase center offsets (PCOs) and variations (PCVs) with elevation and azimuth for most commonly used ground antennas have been determined by electro-mechanical measurements [http://gnpcvdb.geopp.de; http://www.ngs.noaa.gov/ANTCAL], and for the satellite antennas by analysis of global tracking data :cite:p:`Schmid_et_al_2007`.”j§]”(j±XIIn modeling the phase and pseudorange observations, we must also take into account changes in the apparent distance due to variations in the phase centers of the transmitting and receiving antennas. With matched ground antennas in a regional network, these effects nearly cancel, but for longer baselines and/or different antenna types they can amount to several centimeters in estimated heights. Models for the phase center offsets (PCOs) and variations (PCVs) with elevation and azimuth for most commonly used ground antennas have been determined by electro-mechanical measurements [”…””}”(j¶j•jÇj·hNjÆNubj÷ )”}”(j¦Œhttp://gnpcvdb.geopp.de”j§]”j±Œhttp://gnpcvdb.geopp.de”…””}”(j¶jjÇj·hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jŸujÄjö j¶j•ubj±Œ; ”…””}”(j¶j•jÇj·hNjÆNubj÷ )”}”(j¦Œhttp://www.ngs.noaa.gov/ANTCAL”j§]”j±Œhttp://www.ngs.noaa.gov/ANTCAL”…””}”(j¶j°jÇj·hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j²ujÄjö j¶j•ubj±ŒF], and for the satellite antennas by analysis of global tracking data ”…””}”(j¶j•jÇj·hNjÆNubj’)”}”(j¦Œ:cite:p:`Schmid_et_al_2007`”j§]”j)”}”(j¦jÅj§]”j±ŒSchmid_et_al_2007”…””}”(j¶jÇjÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-p”ej½]”jÀ]”jÂ]”ujÄj*j¶jÃubaj·}”(j¹]”Œid9”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÑŒreftype”j-Œ refexplicit”‰Œrefwarn”‰j¶ŒSchmid_et_al_2007”ujÄj‘hjãjÆK j¶j•ubj±Œ.”…””}”(j¶j•jÇj·hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjãjÆK j¶jäjÇj·ubj`)”}”(j¦X·Also part of the phase and pseudorange model is the propagation delay caused by the neutral part of the Earth’s atmosphere. This effect is represented by a time-dependent "zenith delay", a "mapping function" that extends the delay to other elevation angles, and a simple function for north-south and east-west gradients. The zenith hydrostatic ("dry") delay (ZHD) can be well represented by surface pressure, available either from an empirical function of latitude, longitude, and season (the GPT2 model of :cite:t:`Lagler_et_al_2013`) or at six-hour intervals from a numerical weather model as computed by TU Vienna (VMF1) :cite:p:`Boehm_et_al_2006a` and distributed in yearly grid files by MIT for GAMIT users. The hydrostatic and "wet" mapping functions are also part of both the GPT2 and VMF1 models. The component of the zenith delay due to water vapor (zenith "wet" delay, ZWD) and the local gradients cannot be accurately determined even from a numerical weather model and must be estimated from the GPS data. The details of these models are described in Chapter 7 of the GAMIT Reference Manual. As noted above the first-order effect of the ionosphere on the signal delay is made nearly negligible by combining L1 and L2 measurements. However, during periods of high ionospheric activity, 2nd and 3rd order effects at the millimeter to centimeter level are possible and can be modeled in GAMIT using the approach described by :cite:t:`Petrie_et_al_2010`.”j§]”(j±X Also part of the phase and pseudorange model is the propagation delay caused by the neutral part of the Earth’s atmosphere. This effect is represented by a time-dependent “zenith delayâ€, a “mapping function†that extends the delay to other elevation angles, and a simple function for north-south and east-west gradients. The zenith hydrostatic (“dryâ€) delay (ZHD) can be well represented by surface pressure, available either from an empirical function of latitude, longitude, and season (the GPT2 model of ”…””}”(j¶jíjÇj·hNjÆNubj’)”}”(j¦Œ:cite:t:`Lagler_et_al_2013`”j§]”j)”}”(j¦j÷j§]”j±ŒLagler_et_al_2013”…””}”(j¶jùjÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jõubaj·}”(j¹]”Œid10”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒLagler_et_al_2013”ujÄj‘hjãjÆK$j¶jíubj±ŒZ) or at six-hour intervals from a numerical weather model as computed by TU Vienna (VMF1) ”…””}”(j¶jíjÇj·hNjÆNubj’)”}”(j¦Œ:cite:p:`Boehm_et_al_2006a`”j§]”j)”}”(j¦jj§]”j±ŒBoehm_et_al_2006a”…””}”(j¶jjÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-p”ej½]”jÀ]”jÂ]”ujÄj*j¶jubaj·}”(j¹]”Œid11”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j'Œreftype”j-Œ refexplicit”‰Œrefwarn”‰j¶ŒBoehm_et_al_2006a”ujÄj‘hjãjÆK$j¶jíubj±X and distributed in yearly grid files by MIT for GAMIT users. The hydrostatic and “wet†mapping functions are also part of both the GPT2 and VMF1 models. The component of the zenith delay due to water vapor (zenith “wet†delay, ZWD) and the local gradients cannot be accurately determined even from a numerical weather model and must be estimated from the GPS data. The details of these models are described in Chapter 7 of the GAMIT Reference Manual. As noted above the first-order effect of the ionosphere on the signal delay is made nearly negligible by combining L1 and L2 measurements. However, during periods of high ionospheric activity, 2nd and 3rd order effects at the millimeter to centimeter level are possible and can be modeled in GAMIT using the approach described by ”…””}”(j¶jíjÇj·hNjÆNubj’)”}”(j¦Œ:cite:t:`Petrie_et_al_2010`”j§]”j)”}”(j¦j?j§]”j±ŒPetrie_et_al_2010”…””}”(j¶jAjÇj·hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j=ubaj·}”(j¹]”Œid12”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jKŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒPetrie_et_al_2010”ujÄj‘hjãjÆK$j¶jíubj±Œ.”…””}”(j¶jíjÇj·hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjãjÆK$j¶jäjÇj·ubej·}”(j¹]”(Œ3modeling-the-motions-of-the-satellites-and-stations”jâej»]”j½]”(Œ3modeling the motions of the satellites and stations”Œintro_gnss_model”ejÀ]”jÂ]”ujÄh_j¶j·jÇj·hjãjÆKjÒ }”jmjØsjÔ }”jâjØsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jãj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjãjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jÆjºjÕjÉuj_}”(Œrel”jÆŒdate”jÕujc}”je}”jâ]”jØasjg}”(jmjâjljiuji}”(jmˆjl‰uj¹}”(jâjäjijäj%jj}jhj¢jjÆj±jøjãj*jjNj9jrj]jØjÃj jõj.jjRj=ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiK s…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ6Hyperlink target "intro-gnss-model" is not referenced.”…””}”j¶j—sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j”ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jãŒline”KujÄjø ubajˆNj‰]”j‹NjÇj·ubjúj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j²sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¯jÇj¯ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jÁjÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¯jÇj¯ubje)”}”(j¦Œ.. _intro_gnss_obs:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-gnss-obs”ujÄjdjÆKj¶j¯jÇj¯hŒB/chandler/home/floyd/public_html/gg/docs/source/intro/gnss/obs.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ"Phase and Pseudorange Observations”j§]”j±Œ"Phase and Pseudorange Observations”…””}”(j¶jßjÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jÜjÇj¯hjÛjÆKubj`)”}”(j¦XÍHigh-precision geodetic measurements with GNSS are performed using the carrier beat phase, the output from a single phase-tracking channel of a GNSS receiver. This observable is the difference between the phase of the carrier wave implicit in the signal received from the satellite, and the phase of a local oscillator within the receiver. The phase can be measured with sufficient precision that the instrumental resolution is a millimeter or less in equivalent path length. The dominant source of error in a phase measurement or series of measurements between a single satellite and ground station is the unpredictable behavior of the time and frequency standards ("clocks") serving as reference for the transmitter and receiver. Even though the satellites carry atomic frequency standards, the instability of these standards would still limit positioning to the several meter level were it not for the possibility of eliminating their effect through signal differencing.”j§]”j±XÑHigh-precision geodetic measurements with GNSS are performed using the carrier beat phase, the output from a single phase-tracking channel of a GNSS receiver. This observable is the difference between the phase of the carrier wave implicit in the signal received from the satellite, and the phase of a local oscillator within the receiver. The phase can be measured with sufficient precision that the instrumental resolution is a millimeter or less in equivalent path length. The dominant source of error in a phase measurement or series of measurements between a single satellite and ground station is the unpredictable behavior of the time and frequency standards (“clocksâ€) serving as reference for the transmitter and receiver. Even though the satellites carry atomic frequency standards, the instability of these standards would still limit positioning to the several meter level were it not for the possibility of eliminating their effect through signal differencing.”…””}”(j¶jíjÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆKj¶jÜjÇj¯ubj`)”}”(j¦X„A second type of GNSS measurement is the pseudo-range, obtained using the codes transmitted by the satellites Pseudo-ranges provide the primary GNSS observation for navigation but are not precise enough to be used directly in geodetic surveys. They are useful, however, for estimating the offsets of receiver clocks, resolving ambiguities, and repairing cycle slips in phase observations.”j§]”j±X„A second type of GNSS measurement is the pseudo-range, obtained using the codes transmitted by the satellites Pseudo-ranges provide the primary GNSS observation for navigation but are not precise enough to be used directly in geodetic surveys. They are useful, however, for estimating the offsets of receiver clocks, resolving ambiguities, and repairing cycle slips in phase observations.”…””}”(j¶jûjÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆK j¶jÜjÇj¯ubj`)”}”(j¦X¬For a single satellite, differencing the phases (or pseudo-ranges) of signals received simultaneously at each of two ground stations eliminates the effect of bias and instabilities in the satellite clock. This measurement is commonly called the between-stations-difference, or *single-difference* observable. Forming a second difference, between satellites, eliminates the effect of bias and instabilities in the station blocks.”j§]”(j±XFor a single satellite, differencing the phases (or pseudo-ranges) of signals received simultaneously at each of two ground stations eliminates the effect of bias and instabilities in the satellite clock. This measurement is commonly called the between-stations-difference, or ”…””}”(j¶j jÇj¯hNjÆNubj )”}”(j¦Œ*single-difference*”j§]”j±Œsingle-difference”…””}”(j¶jjÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j ubj±Œ„ observable. Forming a second difference, between satellites, eliminates the effect of bias and instabilities in the station blocks.”…””}”(j¶j jÇj¯hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆKj¶jÜjÇj¯ubj`)”}”(j¦XSince the phase biases of the satellite and receiver oscillators at the initial epoch are eliminated in doubly differenced observations, the doubly differenced range (in phase units) is the measured phase plus an integer number of cycles. (One cycle has a wavelength of 19 cm at GPS L1 and 24 cm at GPS L2 for code-correlating receivers; half these values for squaring-type receivers used prior to the mid-1990s, and slightly different values for the primary frequencies transmitted by Glonass, Beidou, and Galileo. In the manuals we will use the term "L1" to refer to the higher and "L2" the lower of the two L-band frequencies though these may be, e.g. for Galileo E1(L1) and E5.) If the measurement errors, arising from errors in the models for the orbits and propagation medium as well as receiver noise, are small compared to a cycle, there is the possibility of determining the integer values of the biases, thereby obtaining from the initially ambiguous doubly differenced phase an unambiguous measure of doubly differenced range. Resolution of the phase ambiguities improves the uncertainties in relative position measures by about a factor of 15 for 24-hr sessions, 3 for 8-hr sessions and more than 5 for short sessions (see, e.g., :cite:t:`Blewitt_1989,Dong_and_Bock_1989`).”j§]”(j±XâSince the phase biases of the satellite and receiver oscillators at the initial epoch are eliminated in doubly differenced observations, the doubly differenced range (in phase units) is the measured phase plus an integer number of cycles. (One cycle has a wavelength of 19 cm at GPS L1 and 24 cm at GPS L2 for code-correlating receivers; half these values for squaring-type receivers used prior to the mid-1990s, and slightly different values for the primary frequencies transmitted by Glonass, Beidou, and Galileo. In the manuals we will use the term “L1†to refer to the higher and “L2†the lower of the two L-band frequencies though these may be, e.g. for Galileo E1(L1) and E5.) If the measurement errors, arising from errors in the models for the orbits and propagation medium as well as receiver noise, are small compared to a cycle, there is the possibility of determining the integer values of the biases, thereby obtaining from the initially ambiguous doubly differenced phase an unambiguous measure of doubly differenced range. Resolution of the phase ambiguities improves the uncertainties in relative position measures by about a factor of 15 for 24-hr sessions, 3 for 8-hr sessions and more than 5 for short sessions (see, e.g., ”…””}”(j¶j)jÇj¯hNjÆNubj’)”}”(j¦Œ):cite:t:`Blewitt_1989,Dong_and_Bock_1989`”j§]”j)”}”(j¦j3j§]”j±ŒBlewitt_1989,Dong_and_Bock_1989”…””}”(j¶j5jÇj¯hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j1ubaj·}”(j¹]”Œid1”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”júŒ refdomain”j?Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒBlewitt_1989,Dong_and_Bock_1989”ujÄj‘hjÛjÆKj¶j)ubj±Œ).”…””}”(j¶j)jÇj¯hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆKj¶jÜjÇj¯ubj`)”}”(j¦XKGAMIT incorporates difference-operator algorithms that map the carrier beat phases into singly and doubly differenced phases. These algorithms extract the maximum relative positioning information from the phase data regardless of the number of data outages, and take into account the correlations that are introduced in the differencing process. (See :cite:t:`Bock_et_al_1986,Schaffrin_and_Bock_1988` for a detailed discussion of these algorithms.) An alternative, (nearly) mathematically equivalent approach to processing GNSS phase data is to use formally the (one-way) carrier beat phases but estimate at each epoch the phase offset due to the station and satellite clocks. This approach is used by the autcln program in GAMIT to compute one-way phase residuals for editing, display, and estimating atmospheric and ionospheric slant delays.”j§]”(j±X_GAMIT incorporates difference-operator algorithms that map the carrier beat phases into singly and doubly differenced phases. These algorithms extract the maximum relative positioning information from the phase data regardless of the number of data outages, and take into account the correlations that are introduced in the differencing process. (See ”…””}”(j¶j[jÇj¯hNjÆNubj’)”}”(j¦Œ1:cite:t:`Bock_et_al_1986,Schaffrin_and_Bock_1988`”j§]”j)”}”(j¦jej§]”j±Œ'Bock_et_al_1986,Schaffrin_and_Bock_1988”…””}”(j¶jgjÇj¯hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jcubaj·}”(j¹]”Œid2”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”júŒ refdomain”jqŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶Œ'Bock_et_al_1986,Schaffrin_and_Bock_1988”ujÄj‘hjÛjÆKj¶j[ubj±X» for a detailed discussion of these algorithms.) An alternative, (nearly) mathematically equivalent approach to processing GNSS phase data is to use formally the (one-way) carrier beat phases but estimate at each epoch the phase offset due to the station and satellite clocks. This approach is used by the autcln program in GAMIT to compute one-way phase residuals for editing, display, and estimating atmospheric and ionospheric slant delays.”…””}”(j¶j[jÇj¯hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆKj¶jÜjÇj¯ubj`)”}”(j¦X£In order to provide the maximum sensitivity to geometric parameters, the carrier phase must be tracked continuously throughout an observing session. If there is an interruption of the signal, causing a loss of lock in the receiver, the phase will exhibit a discontinuity of an integer number of cycles ("cycle-slip"). This discontinuity may be only a few cycles due to a low signal-to-noise ratio, or it may be thousands of cycles, as can occur when the satellite is obstructed at the receiver site. Initial processing of phase data is often performed using time differences of doubly differenced phase ("triple differences", or "Doppler" observations) in order to obtain a preliminary estimate of station or orbital parameters in the presence of cycle slips. The GAMIT software uses triple differences in editing but not in parameter estimation. Rather, it allows estimation of extra bias parameters whenever the automatic editor has flagged an epoch as a cycle slip that cannot be repaired. Various algorithms to detect and repair cycle slips are described by :cite:t:`Blewitt_1990`, and also in Chapter 4 of the `GAMIT Reference Manual `_.”j§]”(j±X2In order to provide the maximum sensitivity to geometric parameters, the carrier phase must be tracked continuously throughout an observing session. If there is an interruption of the signal, causing a loss of lock in the receiver, the phase will exhibit a discontinuity of an integer number of cycles (“cycle-slipâ€). This discontinuity may be only a few cycles due to a low signal-to-noise ratio, or it may be thousands of cycles, as can occur when the satellite is obstructed at the receiver site. Initial processing of phase data is often performed using time differences of doubly differenced phase (“triple differencesâ€, or “Doppler†observations) in order to obtain a preliminary estimate of station or orbital parameters in the presence of cycle slips. The GAMIT software uses triple differences in editing but not in parameter estimation. Rather, it allows estimation of extra bias parameters whenever the automatic editor has flagged an epoch as a cycle slip that cannot be repaired. Various algorithms to detect and repair cycle slips are described by ”…””}”(j¶jjÇj¯hNjÆNubj’)”}”(j¦Œ:cite:t:`Blewitt_1990`”j§]”j)”}”(j¦j—j§]”j±Œ Blewitt_1990”…””}”(j¶j™jÇj¯hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j•ubaj·}”(j¹]”Œid3”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”júŒ refdomain”j£Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶Œ Blewitt_1990”ujÄj‘hjÛjÆKj¶jubj±Œ, and also in Chapter 4 of the ”…””}”(j¶jjÇj¯hNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j¹jÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT/Ref.pdf”ujÄjö j¶jubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit-reference-manual”aj»]”j½]”Œgamit reference manual”ajÀ]”jÂ]”Œrefuri”jÉujÄjdj Kj¶jubj±Œ.”…””}”(j¶jjÇj¯hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆKj¶jÜjÇj¯ubj`)”}”(j¦XúAlthough phase variations of the satellite and receiver oscillators effectively cancel in doubly differenced observations, errors in the time of the observations, as recorded by the receiver clocks, do not. However, the pseudo-range measurements, together with reasonable *a priori* knowledge of the station coordinates and satellite position, can be used to determine the offset of the station clock to within a microsecond, adequate to keep errors in the doubly differenced phase observations below 1 mm.”j§]”(j±XAlthough phase variations of the satellite and receiver oscillators effectively cancel in doubly differenced observations, errors in the time of the observations, as recorded by the receiver clocks, do not. However, the pseudo-range measurements, together with reasonable ”…””}”(j¶jájÇj¯hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jéjÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jáubj±Œà knowledge of the station coordinates and satellite position, can be used to determine the offset of the station clock to within a microsecond, adequate to keep errors in the doubly differenced phase observations below 1 mm.”…””}”(j¶jájÇj¯hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆK'j¶jÜjÇj¯ubj`)”}”(j¦X A major source of error in single-frequency GNSS measurements is the variable delay ntroduced by the ionosphere. For day-time observations near solar maximum this effect can exceed several parts per million of the baseline length. Fortunately, the ionospheric delay is dispersive and can usually be reduced to a millimeter or less by forming a particular linear combination (LC) of the L1 and L2 phase measurements:”j§]”j±X A major source of error in single-frequency GNSS measurements is the variable delay ntroduced by the ionosphere. For day-time observations near solar maximum this effect can exceed several parts per million of the baseline length. Fortunately, the ionospheric delay is dispersive and can usually be reduced to a millimeter or less by forming a particular linear combination (LC) of the L1 and L2 phase measurements:”…””}”(j¶jjÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆK*j¶jÜjÇj¯ubje)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒequation-eqn-lc-phase”ujÄjdj¶jÜjÇj¯hjÛjÆNubj©Œ math_block”“”)”}”(j¦Œ+\phi_{LC} = 2.546\phi_{L1} - 1.984\phi_{L2}”j§]”j±Œ+\phi_{LC} = 2.546\phi_{L1} - 1.984\phi_{L2}”…””}”j¶jsbaj·}”(j¹]”jaj»]”j½]”jÀ]”jÂ]”Œdocname”júŒnumber”KŒlabel”Œ eqn:lc_phase”Œnowrap”‰j/j0ujÄjhjÛjÆK.j¶jÜjÇj¯jÒ }”jÔ }”jjsubj`)”}”(j¦X`for GPS (see, e.g., :cite:t:`Bock_et_al_1986` or :cite:t:`Dong_and_Bock_1989`). Forming LC, however, magnifies the effect of other error sources. For baselines less than a few kilometers the ionospheric errors largely cancel, and it is preferable to treat L1 and L2 as two independent observables rather than form the linear combination. The station separation at which the ionospheric errors exceed the phase noise depends on many factors (receiver, antenna, multipath environment, latitude, time of day, sunspot activity) and must be determined empirically by analyzing the data with both observable types.”j§]”(j±Œfor GPS (see, e.g., ”…””}”(j¶j0jÇj¯hNjÆNubj’)”}”(j¦Œ:cite:t:`Bock_et_al_1986`”j§]”j)”}”(j¦j:j§]”j±ŒBock_et_al_1986”…””}”(j¶j<jÇj¯hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j8ubaj·}”(j¹]”Œid4”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”júŒ refdomain”jFŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒBock_et_al_1986”ujÄj‘hjÛjÆK3j¶j0ubj±Œ or ”…””}”(j¶j0jÇj¯hNjÆNubj’)”}”(j¦Œ:cite:t:`Dong_and_Bock_1989`”j§]”j)”}”(j¦j^j§]”j±ŒDong_and_Bock_1989”…””}”(j¶j`jÇj¯hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½•]”jÀ]”jÂ]”ujÄj*j¶j\ubaj·}”(j¹]”Œid5”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”júŒ refdomain”jjŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒDong_and_Bock_1989”ujÄj‘hjÛjÆK3j¶j0ubj±X). Forming LC, however, magnifies the effect of other error sources. For baselines less than a few kilometers the ionospheric errors largely cancel, and it is preferable to treat L1 and L2 as two independent observables rather than form the linear combination. The station separation at which the ionospheric errors exceed the phase noise depends on many factors (receiver, antenna, multipath environment, latitude, time of day, sunspot activity) and must be determined empirically by analyzing the data with both observable types.”…””}”(j¶j0jÇj¯hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆK3j¶jÜjÇj¯ubj`)”}”(j¦X‡In examining phase data for cycle slips, it is often useful to plot several combinations of the L1 and L2 residuals. Single-cycle slips in GPS L1 or L2 will appear as jumps of 2.546 or 1.984 cycles, respectively, in LC. Single-cycle slips in both GPS L1 and L2 (a more common occurrence) appear as jumps of 0.562 cycles in LC, which, though smaller, may be more evident than the jumps in L1 and L2 because the ionosphere has been eliminated. If the L2 phase is tracked using codeless techniques, the carrier signal recorded by the receiver is at twice the L2 frequency, leading to half-cycle jumps when it is combined with full-wavelength data. Hence, a jump of a "single" L2 cycle will appear as 0.992 in LC, and simultaneous jumps in (undoubled) L1 and (doubled) L2 will appear as 1.554 cycles in LC. Another useful combination is the difference between L2 and L1 with both expressed in distance units”j§]”j±X‹In examining phase data for cycle slips, it is often useful to plot several combinations of the L1 and L2 residuals. Single-cycle slips in GPS L1 or L2 will appear as jumps of 2.546 or 1.984 cycles, respectively, in LC. Single-cycle slips in both GPS L1 and L2 (a more common occurrence) appear as jumps of 0.562 cycles in LC, which, though smaller, may be more evident than the jumps in L1 and L2 because the ionosphere has been eliminated. If the L2 phase is tracked using codeless techniques, the carrier signal recorded by the receiver is at twice the L2 frequency, leading to half-cycle jumps when it is combined with full-wavelength data. Hence, a jump of a “single†L2 cycle will appear as 0.992 in LC, and simultaneous jumps in (undoubled) L1 and (doubled) L2 will appear as 1.554 cycles in LC. Another useful combination is the difference between L2 and L1 with both expressed in distance units”…””}”(j¶j†jÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆK8j¶jÜjÇj¯ubje)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒequation-eqn-lg-phase”ujÄjdj¶jÜjÇj¯hjÛjÆNubj)”}”(j¦Œ&\phi_{LG} = \phi_{L2} - 0.779\phi_{L1}”j§]”j±Œ&\phi_{LG} = \phi_{L2} - 0.779\phi_{L1}”…””}”j¶jžsbaj·}”(j¹]”jaj»]”j½]”jÀ]”jÂ]”Œdocname”júŒnumber”KŒlabel”Œ eqn:lg_phase”Œnowrap”‰j/j0ujÄjhjÛjÆK?j¶jÜjÇj¯jÒ }”jÔ }”jj”subj`)”}”(j¦XÅfor GPS, called "LG" because the L2 phase is scaled by the "gear" ratio (:math:`f_2/f_1 = 60/77 = 1227.6/1575.42` for GPS). In the LG phase all geometrical and other non-dispersive delays (e.g., the troposphere) cancel, so that we have a direct measure of the ionospheric variations. One-cycle slips in L1 and L2 are difficult to detect in the LG phase in the presence of much ionospheric noise since they are equivalent for GPS to only 0.221 LG cycles.”j§]”(j±ŒQfor GPS, called “LG†because the L2 phase is scaled by the “gear†ratio (”…””}”(j¶j³jÇj¯hNjÆNubjO )”}”(j¦Œ(:math:`f_2/f_1 = 60/77 = 1227.6/1575.42`”j§]”j±Œ f_2/f_1 = 60/77 = 1227.6/1575.42”…””}”(j¶j»jÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶j³ubj±XT for GPS). In the LG phase all geometrical and other non-dispersive delays (e.g., the troposphere) cancel, so that we have a direct measure of the ionospheric variations. One-cycle slips in L1 and L2 are difficult to detect in the LG phase in the presence of much ionospheric noise since they are equivalent for GPS to only 0.221 LG cycles.”…””}”(j¶j³jÇj¯hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆKDj¶jÜjÇj¯ubj`)”}”(j¦XIf precise (P-code) pseudorange is available for both GNSS frequencies, then a "wide-lane" (WL) combination of L1, L2, P1, and P2 can be formed which is free of both ionospheric and geometric effects and is simply the difference in the integer ambiguities for L1 and L2:”j§]”j±XIf precise (P-code) pseudorange is available for both GNSS frequencies, then a “wide-lane†(WL) combination of L1, L2, P1, and P2 can be formed which is free of both ionospheric and geometric effects and is simply the difference in the integer ambiguities for L1 and L2:”…””}”(j¶jÓjÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆKHj¶jÜjÇj¯ubje)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒequation-eqn-widelane”ujÄjdj¶jÜjÇj¯hjÛjÆNubj)”}”(j¦ŒŽ\begin{align} \text{WL} & = n_2 - n_1 \\ & = \phi_{L2} - \phi_{L1} + \left(P1 + P2\right)\frac{f_1 - f_2}{f_1 + f_2} \end{align}”j§]”j±ŒŽ\begin{align} \text{WL} & = n_2 - n_1 \\ & = \phi_{L2} - \phi_{L1} + \left(P1 + P2\right)\frac{f_1 - f_2}{f_1 + f_2} \end{align}”…””}”j¶jësbaj·}”(j¹]”jêaj»]”j½]”jÀ]”jÂ]”Œdocname”júŒnumber”KŒlabel”Œ eqn:widelane”Œnowrap”‰j/j0ujÄjhjÛjÆKJj¶jÜjÇj¯jÒ }”jÔ }”jêjásubj`)”}”(j¦ŒÍThe WL observable can be used to fix cycle slips in one-way data :cite:p:`Blewitt_1990` but should be combined with LG and doubly differenced LC to rule out slips of an equal number of cycles at L1 and L2.”j§]”(j±ŒAThe WL observable can be used to fix cycle slips in one-way data ”…””}”(j¶jjÇj¯hNjÆNubj’)”}”(j¦Œ:cite:p:`Blewitt_1990`”j§]”j)”}”(j¦j j§]”j±Œ Blewitt_1990”…””}”(j¶j jÇj¯hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-p”ej½]”jÀ]”jÂ]”ujÄj*j¶jubaj·}”(j¹]”Œid6”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”júŒ refdomain”jŒreftype”j-Œ refexplicit”‰Œrefwarn”‰j¶Œ Blewitt_1990”ujÄj‘hjÛjÆKRj¶jubj±Œv but should be combined with LG and doubly differenced LC to rule out slips of an equal number of cycles at L1 and L2.”…””}”(j¶jjÇj¯hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆKRj¶jÜjÇj¯ubj`)”}”(j¦XçThese various combinations of phase and pseudorange observations are used not only in data editing, but also in resolving the phase ambiguities. When the LC observable is used, we determine the L1 and L2 ambiguities by first resolving :math:`n_2 - n_1` ("widelane") and then :math:`n_1` ("narrow lane"). If precise and unbiased pseudoranges are available, the widelane ambiguities can be resolved for baselines up to thousands of kilometers under any ionosphere conditions. For measurements prior to 1995, and possibly prior to 2000, inter-channel receiver biases can corrupt the pseudoranges and it is necessary to use the phase observations alone with a constraint on the ionopshere to resolve the widelane ambiguities (see, e.g., :cite:t:`Blewitt_1989,Dong_and_Bock_1989,Feigl_et_al_1993`). GAMIT gives you the option of selecting the method to be used, either pseudoranges (LC_AUTCLN) or ionospheric constraints (LC_HELP). When using the pseudorange approach with different receiver types, it is important to use the satellite-dependent differential code biases (DCBs) computed from tracking data by the Center for Orbit Determination in Europe (CODE) [http://www.aiub.unibe.ch/ionosphere.html] and updated monthly at MIT in file dcb.dat. Once the wide-lane ambiguity for a given doubly differenced combination has been resolved, resolving the narrow-lane ambiguity for that combination depends on the level of noise from the receiver, multipathing, and the troposphere, and the accuracy of the models employed for the position and motion of the stations and satellites. It is generally more difficult to resolve these ambiguities for the longest baselines, but for data acquired since 2000 we can usually resolve 80–95% of the ambiguities in a global analysis.”j§]”(j±ŒëThese various combinations of phase and pseudorange observations are used not only in data editing, but also in resolving the phase ambiguities. When the LC observable is used, we determine the L1 and L2 ambiguities by first resolving ”…””}”(j¶j2jÇj¯hNjÆNubjO )”}”(j¦Œ:math:`n_2 - n_1`”j§]”j±Œ n_2 - n_1”…””}”(j¶j:jÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶j2ubj±Œ (“widelaneâ€) and then ”…””}”(j¶j2jÇj¯hNjÆNubjO )”}”(j¦Œ :math:`n_1`”j§]”j±Œn_1”…””}”(j¶jLjÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶j2ubj±Xà (“narrow laneâ€). If precise and unbiased pseudoranges are available, the widelane ambiguities can be resolved for baselines up to thousands of kilometers under any ionosphere conditions. For measurements prior to 1995, and possibly prior to 2000, inter-channel receiver biases can corrupt the pseudoranges and it is necessary to use the phase observations alone with a constraint on the ionopshere to resolve the widelane ambiguities (see, e.g., ”…””}”(j¶j2jÇj¯hNjÆNubj’)”}”(j¦Œ::cite:t:`Blewitt_1989,Dong_and_Bock_1989,Feigl_et_al_1993`”j§]”j)”}”(j¦j`j§]”j±Œ0Blewitt_1989,Dong_and_Bock_1989,Feigl_et_al_1993”…””}”(j¶jbjÇj¯hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j^ubaj·}”(j¹]”Œid7”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”júŒ refdomain”jlŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶Œ0Blewitt_1989,Dong_and_Bock_1989,Feigl_et_al_1993”ujÄj‘hjÛjÆKTj¶j2ubj±Xn). GAMIT gives you the option of selecting the method to be used, either pseudoranges (LC_AUTCLN) or ionospheric constraints (LC_HELP). When using the pseudorange approach with different receiver types, it is important to use the satellite-dependent differential code biases (DCBs) computed from tracking data by the Center for Orbit Determination in Europe (CODE) [”…””}”(j¶j2jÇj¯hNjÆNubj÷ )”}”(j¦Œ(http://www.aiub.unibe.ch/ionosphere.html”j§]”j±Œ(http://www.aiub.unibe.ch/ionosphere.html”…””}”(j¶j‚jÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j„ujÄjö j¶j2ubj±X:] and updated monthly at MIT in file dcb.dat. Once the wide-lane ambiguity for a given doubly differenced combination has been resolved, resolving the narrow-lane ambiguity for that combination depends on the level of noise from the receiver, multipathing, and the troposphere, and the accuracy of the models employed for the position and motion of the stations and satellites. It is generally more difficult to resolve these ambiguities for the longest baselines, but for data acquired since 2000 we can usually resolve 80–95% of the ambiguities in a global analysis.”…””}”(j¶j2jÇj¯hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆKTj¶jÜjÇj¯ubj`)”}”(j¦X“Although GAMIT can process data from single-frequency receivers, ionsopheric errors begin to limit relative positioning accuracy for station separations greater than 100–2000 m, depending on time of day, latitude, and the solar sunspot cycle. So for most applications, the use of two frequencies is required to remove first-order ionsospheric effects. Although some GNSS satellites transmit signals on three of more frequencies, GAMIT is currently limited to using only two. GAMIT is also limited to processing data from only one GNSS at a time, though the GAMIT position estimates from several GNSS tracked during a session can easily be combined in GLOBK.”j§]”j±X“Although GAMIT can process data from single-frequency receivers, ionsopheric errors begin to limit relative positioning accuracy for station separations greater than 100–2000 m, depending on time of day, latitude, and the solar sunspot cycle. So for most applications, the use of two frequencies is required to remove first-order ionsospheric effects. Although some GNSS satellites transmit signals on three of more frequencies, GAMIT is currently limited to using only two. GAMIT is also limited to processing data from only one GNSS at a time, though the GAMIT position estimates from several GNSS tracked during a session can easily be combined in GLOBK.”…””}”(j¶j›jÇj¯hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÛjÆK]j¶jÜjÇj¯ubej·}”(j¹]”(Œ"phase-and-pseudorange-observations”jÚej»]”j½]”(Œ"phase and pseudorange observations”Œintro_gnss_obs”ejÀ]”jÂ]”ujÄh_j¶j¯jÇj¯hjÛjÆKjÒ }”j¯jÐsjÔ }”jÚjÐsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jÛj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjÛjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j¾j²jÍjÁuj_}”(Œrel”j¾Œdate”jÍujc}”je}”(jÚ]”jÐaj]”jaj]”j”ajê]”jáaujg}”(j¯jÚj®j«jÓjÐuji}”(j¯ˆj®‰jÓˆuj¹}”(jÚjÜj«jÜjFj1jxjcjªj•jÐjÊjjjMj8jqj\jjžjêjëjjjsj^ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”j†]”(jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ4Hyperlink target "intro-gnss-obs" is not referenced.”…””}”j¶jÜsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÙubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jÛŒline”KujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ;Hyperlink target "equation-eqn-lc-phase" is not referenced.”…””}”j¶jösbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jóubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jÛujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ;Hyperlink target "equation-eqn-lg-phase" is not referenced.”…””}”j¶jsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jÛujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ;Hyperlink target "equation-eqn-widelane" is not referenced.”…””}”j¶j(sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j%ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jÛujÄjø ubejˆNj‰]”j‹NjÇj¯ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jBsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j?jÇj?ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jQjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j?jÇj?ubje)”}”(j¦Œ.. _intro_gnss_solve:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-gnss-solve”ujÄjdjÆKj¶j?jÇj?hŒD/chandler/home/floyd/public_html/gg/docs/source/intro/gnss/solve.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒParameter Estimation”j§]”j±ŒParameter Estimation”…””}”(j¶jojÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jljÇj?hjkjÆKubj`)”}”(j¦XeGAMIT (program :program:`solve`) incorporates a weighted least squares algorithm to estimate the relative positions of a set of stations, orbital and Earth-rotation parameters, zenith delays, and phase ambiguities by fitting to doubly differenced phase observations. Since the functional (mathematical) model relating the observations and parameters is non-linear, GAMIT produces two solutions, the first to obtain coordinates within a few decimeters, and the second to obtain the final estimates. (See the discussion in Section 2.2 of the `GAMIT Reference Manual `_.)”j§]”(j±ŒGAMIT (program ”…””}”(j¶j}jÇj?hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j…jÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j}ubj±Xý) incorporates a weighted least squares algorithm to estimate the relative positions of a set of stations, orbital and Earth-rotation parameters, zenith delays, and phase ambiguities by fitting to doubly differenced phase observations. Since the functional (mathematical) model relating the observations and parameters is non-linear, GAMIT produces two solutions, the first to obtain coordinates within a few decimeters, and the second to obtain the final estimates. (See the discussion in Section 2.2 of the ”…””}”(j¶j}jÇj?hNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j—jÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶j}ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit-reference-manual”aj»]”j½]”Œgamit reference manual”ajÀ]”jÂ]”Œrefuri”j§ujÄjdj Kj¶j}ubj±Œ.)”…””}”(j¶j}jÇj?hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjkjÆKj¶jljÇj?ubj`)”}”(j¦X-In current practice, the GAMIT solution is not usually used directly to obtain the final estimates of station positions from a survey. Rather, we use GAMIT to produce estimates and an associated covariance matrix ("quasi-observations") of station positions and (optionally) orbital and Earth-rotation parameters which are then input to GLOBK or other similar programs to combine the data with those from other networks and times to estimate positions and velocities :cite:p:`Feigl_et_al_1993,Dong_et_al_1998`. GLOBK uses a Kalman filter (equivalent to sequential least squares if there are no stochastic parameters in the solution) which operates on covariance matrices rather than normal equations and hence requires that you specify a non-infinite *a priori* constraint for each parameter estimated (see, e.g., :cite:t:`Herring_et_al_1990`). In order not to bias the combination, GAMIT generates the solution used by GLOBK with loose constraints on the parameters. Since phase ambiguities must be resolved (if possible) in the phase processing, however, GAMIT also generates several intermediate solutions with user-defined constraints before loosening the constraints for its final solution. These steps are described in detail in Section 3.4 of the `GAMIT Reference Manual `_.”j§]”(j±XÖIn current practice, the GAMIT solution is not usually used directly to obtain the final estimates of station positions from a survey. Rather, we use GAMIT to produce estimates and an associated covariance matrix (“quasi-observationsâ€) of station positions and (optionally) orbital and Earth-rotation parameters which are then input to GLOBK or other similar programs to combine the data with those from other networks and times to estimate positions and velocities ”…””}”(j¶j¿jÇj?hNjÆNubj’)”}”(j¦Œ*:cite:p:`Feigl_et_al_1993,Dong_et_al_1998`”j§]”j)”}”(j¦jÉj§]”j±Œ Feigl_et_al_1993,Dong_et_al_1998”…””}”(j¶jËjÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-p”ej½]”jÀ]”jÂ]”ujÄj*j¶jÇubaj·}”(j¹]”Œid1”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÕŒreftype”j-Œ refexplicit”‰Œrefwarn”‰j¶Œ Feigl_et_al_1993,Dong_et_al_1998”ujÄj‘hjkjÆK j¶j¿ubj±Œò. GLOBK uses a Kalman filter (equivalent to sequential least squares if there are no stochastic parameters in the solution) which operates on covariance matrices rather than normal equations and hence requires that you specify a non-infinite ”…””}”(j¶j¿jÇj?hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jëjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j¿ubj±Œ5 constraint for each parameter estimated (see, e.g., ”…””}”(j¶j¿jÇj?hNjÆNubj’)”}”(j¦Œ:cite:t:`Herring_et_al_1990`”j§]”j)”}”(j¦jÿj§]”j±ŒHerring_et_al_1990”…””}”(j¶jjÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jýubaj·}”(j¹]”Œid2”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒHerring_et_al_1990”ujÄj‘hjkjÆK j¶j¿ubj±Xœ). In order not to bias the combination, GAMIT generates the solution used by GLOBK with loose constraints on the parameters. Since phase ambiguities must be resolved (if possible) in the phase processing, however, GAMIT also generates several intermediate solutions with user-defined constraints before loosening the constraints for its final solution. These steps are described in detail in Section 3.4 of the ”…””}”(j¶j¿jÇj?hNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j!jÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶j¿ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œid3”aj»]”j½]”jÀ]”Œgamit reference manual”ajÂ]”Œrefuri”j1ujÄjdj Kj¶j¿ubj±Œ.”…””}”(j¶j¿jÇj?hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjkjÆK j¶jljÇj?ubj`)”}”(j¦XIn parameter estimation based on least-squares, the conventional measure of goodness-of-fit is the :math:`\chi^2` (chi-square) statistic, defined for uncorrelated data as the sum of the squares of each observation residual (post-fit observed minus computed observation, ":math:`\text{o} - \text{c}`") divided by its assigned uncertainty. In a GPS analysis parameter correlations arise (even if not represented in the original data weights) so the computation of :math:`\chi^2` in GAMIT or GLOBK involves a complex matrix operation (see :cite:t:`Dong_et_al_1998`), but the idea is the same. The value of :math:`\chi^2` is usually normalized by dividing by the "degrees of freedom" (:math:`df`), the number of observations minus the number of parameters estimated, so that the ideal value for properly weighted, independent random observations is 1.0. Conversely, with whatever *a priori* weight is assigned to the observations, multiplying the estimated parameter uncertainties by the square root of :math:`\chi^2/df` yields the "formal errors" ("formal standard deviations") of the parameter. With white noise, these formal uncertainties will be realistic and will be inversely proportional to the square root of the number of observations (i.e., will depend strongly on the sampling interval).”j§]”(j±ŒcIn parameter estimation based on least-squares, the conventional measure of goodness-of-fit is the ”…””}”(j¶jIjÇj?hNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶jQjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jIubj±Œ  (chi-square) statistic, defined for uncorrelated data as the sum of the squares of each observation residual (post-fit observed minus computed observation, “”…””}”(j¶jIjÇj?hNjÆNubjO )”}”(j¦Œ:math:`\text{o} - \text{c}`”j§]”j±Œ\text{o} - \text{c}”…””}”(j¶jcjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jIubj±Œ¦â€) divided by its assigned uncertainty. In a GPS analysis parameter correlations arise (even if not represented in the original data weights) so the computation of ”…””}”(j¶jIjÇj?hNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶jujÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jIubj±Œ< in GAMIT or GLOBK involves a complex matrix operation (see ”…””}”(j¶jIjÇj?hNjÆNubj’)”}”(j¦Œ:cite:t:`Dong_et_al_1998`”j§]”j)”}”(j¦j‰j§]”j±ŒDong_et_al_1998”…””}”(j¶j‹jÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j‡ubaj·}”(j¹]”Œid4”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j•Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒDong_et_al_1998”ujÄj‘hjkjÆKj¶jIubj±Œ*), but the idea is the same. The value of ”…””}”(j¶jIjÇj?hNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶j«jÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jIubj±ŒD is usually normalized by dividing by the “degrees of freedom†(”…””}”(j¶jIjÇj?hNjÆNubjO )”}”(j¦Œ :math:`df`”j§]”j±Œdf”…””}”(j¶j½jÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jIubj±Œ¹), the number of observations minus the number of parameters estimated, so that the ideal value for properly weighted, independent random observations is 1.0. Conversely, with whatever ”…””}”(j¶jIjÇj?hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jÏjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jIubj±Œq weight is assigned to the observations, multiplying the estimated parameter uncertainties by the square root of ”…””}”(j¶jIjÇj?hNjÆNubjO )”}”(j¦Œ:math:`\chi^2/df`”j§]”j±Œ \chi^2/df”…””}”(j¶jájÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jIubj±X yields the “formal errors†(“formal standard deviationsâ€) of the parameter. With white noise, these formal uncertainties will be realistic and will be inversely proportional to the square root of the number of observations (i.e., will depend strongly on the sampling interval).”…””}”(j¶jIjÇj?hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjkjÆKj¶jljÇj?ubj`)”}”(j¦XÈThe uncertainties in a GNSS analysis, however, cannot be treated with white noise statistics because errors with temporal correlations dominate both the phase observations and estimates of station coordinates (the quasi-observations input to GLOBK). In the phase residuals (from cview or the sky plots produced by :program:`sh_gamit`), the visible noise—from multipathing and tropospheric fluctuations—is typically correlated over spans of 15–30 minutes. This implies that only samples taken at these intervals are independent, and, to a first approximation, we would get realistic uncertainties by multiplying the formal errors by the square root of the ratio of this interval to the sampling interval used—e.g., for the 2 minute sampling commonly used in :program:`solve`, we would increase the uncertainties by a factor of 3–5. There also errors with longer correlation times that do not show up in the residuals but are absorbed into the parameter adjustments. Assessing the magnitude of these errors requires us to use noise visible in the residuals (phase or coordinates) to infer the character of the noise at lower frequencies. There are a number of excellent studies of the character of the errors discussed in the presentation "Error_Analysis.ppt" from our most recent workshops on the Documentation page of the GAMIT/GLOBK web site (e.g., :cite:t:`Mao_et_al_1999`, :cite:t:`Dixon_et_al_2000`, and :cite:t:`Williams_2003`). Once you have adopted a particular weighting of the data, it is often possible to use external knowledge of the expected behavior of the coordinates or velocities to validate the uncertainties; see :cite:t:`McClusky_et_al_2000`, :cite:t:`Davis_et_al_2003`, and :cite:t:`McCaffrey_et_al_2007`.”j§]”(j±X:The uncertainties in a GNSS analysis, however, cannot be treated with white noise statistics because errors with temporal correlations dominate both the phase observations and estimates of station coordinates (the quasi-observations input to GLOBK). In the phase residuals (from cview or the sky plots produced by ”…””}”(j¶jùjÇj?hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jjÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jùubj±X°), the visible noise—from multipathing and tropospheric fluctuations—is typically correlated over spans of 15–30 minutes. This implies that only samples taken at these intervals are independent, and, to a first approximation, we would get realistic uncertainties by multiplying the formal errors by the square root of the ratio of this interval to the sampling interval used—e.g., for the 2 minute sampling commonly used in ”…””}”(j¶jùjÇj?hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶jjÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jùubj±XG, we would increase the uncertainties by a factor of 3–5. There also errors with longer correlation times that do not show up in the residuals but are absorbed into the parameter adjustments. Assessing the magnitude of these errors requires us to use noise visible in the residuals (phase or coordinates) to infer the character of the noise at lower frequencies. There are a number of excellent studies of the character of the errors discussed in the presentation “Error_Analysis.ppt†from our most recent workshops on the Documentation page of the GAMIT/GLOBK web site (e.g., ”…””}”(j¶jùjÇj?hNjÆNubj’)”}”(j¦Œ:cite:t:`Mao_et_al_1999`”j§]”j)”}”(j¦j'j§]”j±ŒMao_et_al_1999”…””}”(j¶j)jÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j%ubaj·}”(j¹]”Œid5”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j3Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒMao_et_al_1999”ujÄj‘hjkjÆKj¶jùubj±Œ, ”…””}”(j¶jùjÇj?hNjÆNubj’)”}”(j¦Œ:cite:t:`Dixon_et_al_2000`”j§]”j)”}”(j¦jKj§]”j±ŒDixon_et_al_2000”…””}”(j¶jMjÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jIubaj·}”(j¹]”Œid6”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jWŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒDixon_et_al_2000”ujÄj‘hjkjÆKj¶jùubj±Œ, and ”…””}”(j¶jùjÇj?hNjÆNubj’)”}”(j¦Œ:cite:t:`Williams_2003`”j§]”j)”}”(j¦joj§]”j±Œ Williams_2003”…””}”(j¶jqjÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jmubaj·}”(j¹]”Œid7”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j{Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶Œ Williams_2003”ujÄj‘hjkjÆKj¶jùubj±ŒÉ). Once you have adopted a particular weighting of the data, it is often possible to use external knowledge of the expected behavior of the coordinates or velocities to validate the uncertainties; see ”…””}”(j¶jùjÇj?hNjÆNubj’)”}”(j¦Œ:cite:t:`McClusky_et_al_2000`”j§]”j)”}”(j¦j“j§]”j±ŒMcClusky_et_al_2000”…””}”(j¶j•jÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j‘ubaj·}”(j¹]”Œid8”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jŸŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒMcClusky_et_al_2000”ujÄj‘hjkjÆKj¶jùubj±Œ, ”…””}”j¶jùsbj’)”}”(j¦Œ:cite:t:`Davis_et_al_2003`”j§]”j)”}”(j¦j·j§]”j±ŒDavis_et_al_2003”…””}”(j¶j¹jÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jµubaj·}”(j¹]”Œid9”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÃŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒDavis_et_al_2003”ujÄj‘hjkjÆKj¶jùubj±Œ, and ”…””}”j¶jùsbj’)”}”(j¦Œ:cite:t:`McCaffrey_et_al_2007`”j§]”j)”}”(j¦jÛj§]”j±ŒMcCaffrey_et_al_2007”…””}”(j¶jÝjÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jÙubaj·}”(j¹]”Œid10”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jçŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒMcCaffrey_et_al_2007”ujÄj‘hjkjÆKj¶jùubj±Œ.”…””}”(j¶jùjÇj?hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjkjÆKj¶jljÇj?ubj`)”}”(j¦X$In GAMIT/GLOBK there are several ways you can control the uncertainties you obtain for coordinates and velocities, and it is important for you to keep clearly in mind how each of these operates. The uncertainties generated by :program:`solve` and passed to GLOBK in the h-file are determined by the *a priori* error assigned to the phase observations and by the sampling interval—:program:`solve` does *not* rescale by the square root of :math:`\chi^2/df` ("postfit nrms" in the q-file). In the initial ("preliminary") solution, we normally assign an uncertainty of 10 mm to each one-way L1 phase. By Equation :eq:`eqn:lc_phase`, the assigned uncertainty in an LC phase becomes 32 mm. The mean rms of one-way LC residuals is typically ~ 6–9 mm, so the nrms computed by :program:`solve` is 0.2–0.3. In the second ("final") solution, we normally reweight the observations using a constant and elevation-dependent term computed in data editing by program :program:`autcln` from the actual (one-way LC) phase residuals. In order to keep the overall weighting approximately the same as with the 10 mm constant error, the values computed by :program:`autcln` (:content:`ATELV` table in file :file:`autcln.post.sum`) are multiplied by an arbitrary factor of 1.7 (in script :program:`sh_sigelv`) before being input to :program:`solve` (via the N-file). We chose to use inflated values of the *a priori* phase error and not rescale by the nrms in order to generate coordinate uncertainties that (in the presence of correlated noise) are approximately realistic with 2-minute sampling. An equally valid approach would be to rescale by the nrms (i.e. make :math:`\chi^2/df = 1.0`) and compensate later for the unrealistically low coordinate uncertainties. With whatever weighting you use in :program:`solve`, you can increase the coordinate uncertainties used by GLOBK by rescaling all covariances on the h-file or by adding white noise or random-walk noise to the variances of individual stations. We discuss in :numref:`intro_prod_weighting` why the latter approach is usually preferred.”j§]”(j±ŒâIn GAMIT/GLOBK there are several ways you can control the uncertainties you obtain for coordinates and velocities, and it is important for you to keep clearly in mind how each of these operates. The uncertainties generated by ”…””}”(j¶jjÇj?hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j jÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ9 and passed to GLOBK in the h-file are determined by the ”…””}”(j¶jjÇj?hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jubj±ŒI error assigned to the phase observations and by the sampling interval—”…””}”(j¶jjÇj?hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j/jÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ does ”…””}”(j¶jjÇj?hNjÆNubj )”}”(j¦Œ*not*”j§]”j±Œnot”…””}”(j¶jAjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jubj±Œ rescale by the square root of ”…””}”(j¶jjÇj?hNjÆNubjO )”}”(j¦Œ:math:`\chi^2/df`”j§]”j±Œ \chi^2/df”…””}”(j¶jSjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jubj±Œ£ (“postfit nrms†in the q-file). In the initial (“preliminaryâ€) solution, we normally assign an uncertainty of 10 mm to each one-way L1 phase. By Equation ”…””}”(j¶jjÇj?hNjÆNubj’)”}”(j¦Œ:eq:`eqn:lc_phase`”j§]”j˜)”}”(j¦jgj§]”j±Œ eqn:lc_phase”…””}”(j¶jijÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œeq”ej½]”jÀ]”jÂ]”ujÄj—j¶jeubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jN Œreftype”jsŒ refexplicit”‰Œrefwarn”ˆj¶Œ eqn:lc_phase”ujÄj‘hjkjÆKj¶jubj±Œ, the assigned uncertainty in an LC phase becomes 32 mm. The mean rms of one-way LC residuals is typically ~ 6–9 mm, so the nrms computed by ”…””}”(j¶jjÇj?hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j‡jÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ­ is 0.2–0.3. In the second (“finalâ€) solution, we normally reweight the observations using a constant and elevation-dependent term computed in data editing by program ”…””}”(j¶jjÇj?hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j™jÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ¦ from the actual (one-way LC) phase residuals. In order to keep the overall weighting approximately the same as with the 10 mm constant error, the values computed by ”…””}”(j¶jjÇj?hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j«jÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ (”…””}”(j¶jjÇj?hNjÆNubj˜)”}”(j¦Œ:content:`ATELV`”j§]”j±ŒATELV”…””}”(j¶j½jÇj?hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jubj±Œ table in file ”…””}”(j¶jjÇj?hNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum`”j§]”j±Œautcln.post.sum”…””}”(j¶jÐjÇj?hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ:) are multiplied by an arbitrary factor of 1.7 (in script ”…””}”(j¶jjÇj?hNjÆNubjj)”}”(j¦Œ:program:`sh_sigelv`”j§]”j±Œ sh_sigelv”…””}”(j¶jåjÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ) before being input to ”…””}”(j¶jjÇj?hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j÷jÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ: (via the N-file). We chose to use inflated values of the ”…””}”(j¶jjÇj?hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j jÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jubj±Œû phase error and not rescale by the nrms in order to generate coordinate uncertainties that (in the presence of correlated noise) are approximately realistic with 2-minute sampling. An equally valid approach would be to rescale by the nrms (i.e. make ”…””}”(j¶jjÇj?hNjÆNubjO )”}”(j¦Œ:math:`\chi^2/df = 1.0`”j§]”j±Œ\chi^2/df = 1.0”…””}”(j¶jjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jubj±Œp) and compensate later for the unrealistically low coordinate uncertainties. With whatever weighting you use in ”…””}”(j¶jjÇj?hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j-jÇj?hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±ŒÎ, you can increase the coordinate uncertainties used by GLOBK by rescaling all covariances on the h-file or by adding white noise or random-walk noise to the variances of individual stations. We discuss in ”…””}”(j¶jjÇj?hNjÆNubj’)”}”(j¦Œ:numref:`intro_prod_weighting`”j§]”j˜)”}”(j¦jAj§]”j±Œintro_prod_weighting”…””}”(j¶jCjÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶j?ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jMŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_prod_weighting”ujÄj‘hjkjÆKj¶jubj±Œ. why the latter approach is usually preferred.”…””}”(j¶jjÇj?hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjkjÆKj¶jljÇj?ubj`)”}”(j¦XÑTo obtain meaningful estimates of crustal motion, it is necessary to define a reference frame by imposing constraints on the solution. These come in two common flavors: With *finite* constraints, we assign realistic *a priori* uncertainties to the coordinates and velocities of one or more sites. This is the only option available in GAMIT and it is also available in GLOBK. A minimum (non-redundant) constraint with this approach would involve restricting translation by fixing or tightly constraining the three coordinates of one site, and restricting rotation by constraining Earth orientation. Constraining additional sites provides redundancy, but can distort the network and remove your ability to detect errors in those sites except through an increase in :math:`\chi^2`. The second type of constraint, available through the glorg program of GLOBK, is *generalized*. With this approach, we choose as large a set as possible of sites with good *a priori* values and minimize their adjustments while estimating an overall translation, rotation, and scale (Helmert parameters) of the network. Since all of the frame-defining sites are free to move, outliers can be readily detected and removed. Moreover, with generalized constraints there can be no internal distortion of the network: all realizations of the reference frame with a given data set will differ only by a translation and rotation. See :cite:t:`Dong_et_al_1998` for a mathematical description of each of these approaches.”j§]”(j±Œ®To obtain meaningful estimates of crustal motion, it is necessary to define a reference frame by imposing constraints on the solution. These come in two common flavors: With ”…””}”(j¶jijÇj?hNjÆNubj )”}”(j¦Œ*finite*”j§]”j±Œfinite”…””}”(j¶jqjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jiubj±Œ" constraints, we assign realistic ”…””}”(j¶jijÇj?hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jƒjÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jiubj±X uncertainties to the coordinates and velocities of one or more sites. This is the only option available in GAMIT and it is also available in GLOBK. A minimum (non-redundant) constraint with this approach would involve restricting translation by fixing or tightly constraining the three coordinates of one site, and restricting rotation by constraining Earth orientation. Constraining additional sites provides redundancy, but can distort the network and remove your ability to detect errors in those sites except through an increase in ”…””}”(j¶jijÇj?hNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶j•jÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jiubj±ŒR. The second type of constraint, available through the glorg program of GLOBK, is ”…””}”(j¶jijÇj?hNjÆNubj )”}”(j¦Œ *generalized*”j§]”j±Œ generalized”…””}”(j¶j§jÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jiubj±ŒN. With this approach, we choose as large a set as possible of sites with good ”…””}”(j¶jijÇj?hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j¹jÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jiubj±X¼ values and minimize their adjustments while estimating an overall translation, rotation, and scale (Helmert parameters) of the network. Since all of the frame-defining sites are free to move, outliers can be readily detected and removed. Moreover, with generalized constraints there can be no internal distortion of the network: all realizations of the reference frame with a given data set will differ only by a translation and rotation. See ”…””}”(j¶jijÇj?hNjÆNubj’)”}”(j¦Œ:cite:t:`Dong_et_al_1998`”j§]”j)”}”(j¦jÍj§]”j±ŒDong_et_al_1998”…””}”(j¶jÏjÇj?hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jËubaj·}”(j¹]”Œid11”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÙŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒDong_et_al_1998”ujÄj‘hjkjÆK+j¶jiubj±Œ< for a mathematical description of each of these approaches.”…””}”(j¶jijÇj?hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjkjÆK+j¶jljÇj?ubej·}”(j¹]”(Œparameter-estimation”jjej»]”j½]”(Œparameter estimation”Œintro_gnss_solve”ejÀ]”jÂ]”ujÄh_j¶j?jÇj?hjkjÆKjÒ }”jûj`sjÔ }”jjj`subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jkj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjkjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jNjBj]jQuj_}”(Œrel”jNŒdate”j]ujc}”je}”jj]”j`asjg}”(jûjjjúj÷j±j®uji}”(jûˆjú‰j±ˆuj¹}”(jjjlj÷jlj®j¨jÜjÇjjýj8j2jœj‡j:j%j^jIj‚jmj¦j‘jÊjµjîjÙjàjËujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiK s…”R”j„]”jù )”}”(j¦hoj§]”j`)”}”(j¦Œ9Duplicate explicit target name: "gamit reference manual".”j§]”j±Œ=Duplicate explicit target name: “gamit reference manualâ€.”…””}”(j¶j$jÇj?hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j!ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j8aŒlevel”KŒtype”jŒsource”jkŒline”KujÄjø j¶jljÇj?hjkjÆKubaj†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ6Hyperlink target "intro-gnss-solve" is not referenced.”…””}”j¶j@sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j=ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jkŒline”KujÄjø ubajˆNj‰]”j‹NjÇj?ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j[sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jXjÇjXubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jjjÇjXhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jXjÇjXubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒIntroduction to GAMIT/GLOBK”j§]”j±ŒIntroduction to GAMIT/GLOBK”…””}”(j¶j|jÇjXhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jyjÇjXhŒ?/chandler/home/floyd/public_html/gg/docs/source/intro/index.rst”jÆKubjí)”}”(j¦hoj§]”jò)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j¶jjü]”(NŒ intro/preface”†”NŒintro/gnss/index”†”NŒintro/proc/index”†”NŒ intro/eval”†”NŒintro/prod/index”†”NŒ intro/refs”†”ejþ]”(j˜jšjœjžj j¢ejKjNj‰j‰jˆjMçj‰j]”ujÄjñhjŠjÆKj¶j‹ubaj·}”(j¹]”j»]”j aj½]”jÀ]”jÂ]”ujÄjìj¶jyjÇjXhjŠjÆNubej·}”(j¹]”Œintroduction-to-gamit-globk”aj»]”j½]”Œintroduction to gamit/globk”ajÀ]”jÂ]”ujÄh_j¶jXjÇjXhjŠjÆKubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jŠj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjŠjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jgj[jvjjuj_}”(Œrel”jgŒdate”jvujc}”je}”jg}”j±j®sji}”j±‰sj¹}”j®jysjl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jˆNj‰]”j‹NjÇjXubj j£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jÙsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÖjÇjÖubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jèjÇjÖhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÖjÇjÖubje)”}”(j¦Œ.. _intro_preface:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ intro-preface”ujÄjdjÆKj¶jÖjÇjÖhŒA/chandler/home/floyd/public_html/gg/docs/source/intro/preface.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒPreface”j§]”j±ŒPreface”…””}”(j¶jjÇjÖhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jjÇjÖhjjÆKubj`)”}”(j¦XGAMIT/GLOBK is a comprehensive GNSS analysis package developed at MIT, the Harvard-Smithsonian Center for Astrophysics (CfA), Scripps Institution of Oceanography (SIO), and Australian National University (ANU) for estimating station coordinates and velocities, stochastic or functional representations of post-seismic deformation, atmospheric delays, satellite orbits, and Earth orientation parameters. Although the software is currently maintained by the four authors of this document at MIT and ANU, many people have made substantial contributions. The orbital integration and modules used in computing the theoretical phase observable have their origins in the Planetary Ephemeris Program (PEP) written by Michael Ash, Irwin Shapiro, and Bill Smith at Lincoln Laboratory in the 1960s, with later contributions by Bob Reasenberg and John Chandler at MIT. The codes for processing GPS observations were developed at MIT in the 1980s by Chuck Counselman, Sergei Gourevitch, Yehuda Bock, Rick Abbot, and King. GAMIT attained its current form through the efforts of Bock, Danan Dong, Peng Fang (SIO), Kurt Feigl, Herring, King, McClusky (ANU), Mike Moore (ANU), Peter Morgan (Canberra U), Mark Murray (NM Tech), Liz Petrie (U Newcastle), Berkhard Schraffin (Ohio State), Seiichi Shimada (NEID), Paul Tregoning (ANU), and Chris Watson (U Hobart). GLOBK was developed by Herring and Jim Davis at CfA for combination of VLBI data and modified at MIT to incorporate GPS data. Details of these contributions may be found in the references listed at the end of this manual. Funding for the early development of GAMIT was provided by the Air Force Geophysics Laboratory, and for GLOBK by NASA. Current support for development and support of the scientific community comes primarily from the National Science Foundation.”j§]”j±XGAMIT/GLOBK is a comprehensive GNSS analysis package developed at MIT, the Harvard-Smithsonian Center for Astrophysics (CfA), Scripps Institution of Oceanography (SIO), and Australian National University (ANU) for estimating station coordinates and velocities, stochastic or functional representations of post-seismic deformation, atmospheric delays, satellite orbits, and Earth orientation parameters. Although the software is currently maintained by the four authors of this document at MIT and ANU, many people have made substantial contributions. The orbital integration and modules used in computing the theoretical phase observable have their origins in the Planetary Ephemeris Program (PEP) written by Michael Ash, Irwin Shapiro, and Bill Smith at Lincoln Laboratory in the 1960s, with later contributions by Bob Reasenberg and John Chandler at MIT. The codes for processing GPS observations were developed at MIT in the 1980s by Chuck Counselman, Sergei Gourevitch, Yehuda Bock, Rick Abbot, and King. GAMIT attained its current form through the efforts of Bock, Danan Dong, Peng Fang (SIO), Kurt Feigl, Herring, King, McClusky (ANU), Mike Moore (ANU), Peter Morgan (Canberra U), Mark Murray (NM Tech), Liz Petrie (U Newcastle), Berkhard Schraffin (Ohio State), Seiichi Shimada (NEID), Paul Tregoning (ANU), and Chris Watson (U Hobart). GLOBK was developed by Herring and Jim Davis at CfA for combination of VLBI data and modified at MIT to incorporate GPS data. Details of these contributions may be found in the references listed at the end of this manual. Funding for the early development of GAMIT was provided by the Air Force Geophysics Laboratory, and for GLOBK by NASA. Current support for development and support of the scientific community comes primarily from the National Science Foundation.”…””}”(j¶jjÇjÖhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆKj¶jjÇjÖubj`)”}”(j¦X"To control processing the software uses shell scripts (stored in :file:`com/` and mostly named to begin with :program:`sh_`) which invoke the Fortran or C programs compiled in the :file:`libraries/`, :file:`gamit/`, and :file:`kf/` directories. The software is designed to run under any UNIX operating system supporting X-Windows, including LINUX and MacOS. The parameter logic allows a maximum of 99 sites and the standard distribution is dimensioned for 80 sites, but since the run is proportional to the cube of the number of parameters, with networks larger than 50 sites greater efficiency is obtained by parallel processing using connected subnets. IGS processing at MIT includes over 300 sites, and processing at New Mexico Tech for the North American Plate Boundary Observatory over 1000 sites.”j§]”(j±ŒATo control processing the software uses shell scripts (stored in ”…””}”(j¶j"jÇjÖhNjÆNubj˜)”}”(j¦Œ :file:`com/`”j§]”j±Œcom/”…””}”(j¶j*jÇjÖhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j"ubj±Œ and mostly named to begin with ”…””}”(j¶j"jÇjÖhNjÆNubjj)”}”(j¦Œ:program:`sh_`”j§]”j±Œsh_”…””}”(j¶j?jÇjÖhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j"ubj±Œ9) which invoke the Fortran or C programs compiled in the ”…””}”(j¶j"jÇjÖhNjÆNubj˜)”}”(j¦Œ:file:`libraries/`”j§]”j±Œ libraries/”…””}”(j¶jQjÇjÖhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j"ubj±Œ, ”…””}”(j¶j"jÇjÖhNjÆNubj˜)”}”(j¦Œ:file:`gamit/`”j§]”j±Œgamit/”…””}”(j¶jfjÇjÖhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j"ubj±Œ, and ”…””}”(j¶j"jÇjÖhNjÆNubj˜)”}”(j¦Œ :file:`kf/`”j§]”j±Œkf/”…””}”(j¶j{jÇjÖhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j"ubj±X; directories. The software is designed to run under any UNIX operating system supporting X-Windows, including LINUX and MacOS. The parameter logic allows a maximum of 99 sites and the standard distribution is dimensioned for 80 sites, but since the run is proportional to the cube of the number of parameters, with networks larger than 50 sites greater efficiency is obtained by parallel processing using connected subnets. IGS processing at MIT includes over 300 sites, and processing at New Mexico Tech for the North American Plate Boundary Observatory over 1000 sites.”…””}”(j¶j"jÇjÖhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆKj¶jjÇjÖubj`)”}”(j¦XÎThe :doc:`first chapter ` of this manual provides some theoretical background for readers not familiar with high-precision GNSS analysis. :doc:`Chapter 2 ` describes the setup of tables and commands for automatic processing to obtain time series of daily position estimates, and :doc:`Chapter 3 ` provides a guide to evaluating your results. In :doc:`Chapter 4 ` we discuss various approaches to generating time series and estimating station velocities from observations spanning several years. More detailed documentation is available in the longer `GAMIT Reference Manual `_ and `GLOBK Reference Manual `_. There are also tutorials available on-line at http://geoweb.mit.edu/gg/. The most up-to-date information about the commands is available through help files, invoked by typing the name of the shell-script or program without arguments.”j§]”(j±ŒThe ”…””}”(j¶j–jÇjÖhNjÆNubj’)”}”(j¦Œ!:doc:`first chapter `”j§]”j)”}”(j¦j j§]”j±Œ first chapter”…””}”(j¶j¢jÇjÖhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶jžubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”j¬Œreftype”Œdoc”Œ refexplicit”ˆŒrefwarn”ˆj¶Œ gnss/index”ujÄj‘hjjÆKj¶j–ubj±Œq of this manual provides some theoretical background for readers not familiar with high-precision GNSS analysis. ”…””}”(j¶j–jÇjÖhNjÆNubj’)”}”(j¦Œ:doc:`Chapter 2 `”j§]”j)”}”(j¦jÄj§]”j±Œ Chapter 2”…””}”(j¶jÆjÇjÖhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶jÂubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”jÐŒreftype”Œdoc”Œ refexplicit”ˆŒrefwarn”ˆj¶Œ proc/index”ujÄj‘hjjÆKj¶j–ubj±Œ| describes the setup of tables and commands for automatic processing to obtain time series of daily position estimates, and ”…””}”(j¶j–jÇjÖhNjÆNubj’)”}”(j¦Œ:doc:`Chapter 3 `”j§]”j)”}”(j¦jèj§]”j±Œ Chapter 3”…””}”(j¶jêjÇjÖhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶jæubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”jôŒreftype”Œdoc”Œ refexplicit”ˆŒrefwarn”ˆj¶Œeval”ujÄj‘hjjÆKj¶j–ubj±Œ1 provides a guide to evaluating your results. In ”…””}”(j¶j–jÇjÖhNjÆNubj’)”}”(j¦Œ:doc:`Chapter 4 `”j§]”j)”}”(j¦j j§]”j±Œ Chapter 4”…””}”(j¶jjÇjÖhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”jŒreftype”Œdoc”Œ refexplicit”ˆŒrefwarn”ˆj¶Œ prod/index”ujÄj‘hjjÆKj¶j–ubj±Œ¼ we discuss various approaches to generating time series and estimating station velocities from observations spanning several years. More detailed documentation is available in the longer ”…””}”(j¶j–jÇjÖhNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j.jÇjÖhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶j–ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit-reference-manual”aj»]”j½]”Œgamit reference manual”ajÀ]”jÂ]”Œrefuri”j>ujÄjdj Kj¶j–ubj±Œ and ”…””}”(j¶j–jÇjÖhNjÆNubj÷ )”}”(j¦ŒG`GLOBK Reference Manual `_”j§]”j±ŒGLOBK Reference Manual”…””}”(j¶jPjÇjÖhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGLOBK Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GLOBK_Ref.pdf”ujÄjö j¶j–ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œglobk-reference-manual”aj»]”j½]”Œglobk reference manual”ajÀ]”jÂ]”Œrefuri”j`ujÄjdj Kj¶j–ubj±Œ0. There are also tutorials available on-line at ”…””}”(j¶j–jÇjÖhNjÆNubj÷ )”}”(j¦Œhttp://geoweb.mit.edu/gg/”j§]”j±Œhttp://geoweb.mit.edu/gg/”…””}”(j¶jrjÇjÖhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jtujÄjö j¶j–ubj±Œ¢. The most up-to-date information about the commands is available through help files, invoked by typing the name of the shell-script or program without arguments.”…””}”(j¶j–jÇjÖhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆKj¶jjÇjÖubej·}”(j¹]”(Œpreface”jej»]”j½]”(Œpreface”Œ intro_preface”ejÀ]”jÂ]”ujÄh_j¶jÖjÇjÖhjjÆKjÒ }”j‘j÷sjÔ }”jj÷subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jåjÙjôjèuj_}”(Œrel”jåŒdate”jôujc}”je}”j]”j÷asjg}”(j‘jjjjHjEjjjguji}”(j‘ˆj‰jHˆjjˆuj¹}”(jjjjjEj?jgjaujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ3Hyperlink target "intro-preface" is not referenced.”…””}”j¶j»sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j¸ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŒline”KujÄjø ubajˆNj‰]”j‹NjÇjÖubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jÖsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÓjÇjÓubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jåjÇjÓhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÓjÇjÓubje)”}”(j¦Œ.. _intro_proc_autcln.cmd:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-autcln-cmd”u•jÄjdjÆKj¶jÓjÇjÓhŒM/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/autcln.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ:file:`autcln.cmd`”j§]”j˜)”}”(j¦jj§]”j±Œ autcln.cmd”…””}”(j¶jjÇjÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jjÇjÓhjÿjÆKubj`)”}”(j¦XßThe remaining control file for GAMIT is :file:`autcln.cmd`. It is complicated but can almost always be left unchanged. Cases for which you might want alter the default settings include data from codeless receivers, stations for which you cannot get *a priori* coordinates better than 10 m, or short sessions (< ~ 3 hours). For a detailed discussion of the :program:`autcln` settings, see Section 4.2 of the `GAMIT Reference Manual `_.”j§]”(j±Œ(The remaining control file for GAMIT is ”…””}”(j¶jjÇjÓhNjÆNubj˜)”}”(j¦Œ:file:`autcln.cmd`”j§]”j±Œ autcln.cmd”…””}”(j¶j%jÇjÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ¿. It is complicated but can almost always be left unchanged. Cases for which you might want alter the default settings include data from codeless receivers, stations for which you cannot get ”…””}”(j¶jjÇjÓhNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j:jÇjÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jubj±Œa coordinates better than 10 m, or short sessions (< ~ 3 hours). For a detailed discussion of the ”…””}”(j¶jjÇjÓhNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jLjÇjÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ" settings, see Section 4.2 of the ”…””}”(j¶jjÇjÓhNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j^jÇjÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶jubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit-reference-manual”aj»]”j½]”Œgamit reference manual”ajÀ]”jÂ]”Œrefuri”jnujÄjdj Kj¶jubj±Œ.”…””}”(j¶jjÇjÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÿjÆKj¶jjÇjÓubej·}”(j¹]”(Œ autcln-cmd”jþej»]”j½]”(Œ autcln.cmd”Œintro_proc_autcln.cmd”ejÀ]”jÂ]”ujÄh_j¶jÓjÇjÓhjÿjÆKjÒ }”jŒjôsjÔ }”jþjôsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jÿj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjÿjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jâjÖjñjåuj_}”(Œrel”jâŒdate”jñujc}”je}”jþ]”jôasjg}”(jŒjþj‹jˆjxjuuji}”(jŒˆj‹‰jxˆuj¹}”(jþjjˆjjujoujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ;Hyperlink target "intro-proc-autcln-cmd" is not referenced.”…””}”j¶j¶sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j³ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jÿŒline”KujÄjø ubajˆNj‰]”j‹NjÇjÓubjýj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jÑsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÎjÇjÎubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jàjÇjÎhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÎjÇjÎubje)”}”(j¦Œ.. _intro_proc_globk:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-globk”ujÄjdjÆKj¶jÎjÇjÎhŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/globk.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ:file:`globk.cmd`”j§]”j˜)”}”(j¦jj§]”j±Œ globk.cmd”…””}”(j¶jjÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jþubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jûjÇjÎhjújÆKubj`)”}”(j¦XÃThere are two required control files for :program:`sh_glred`. The names :file:`globk.cmd`, and :file:`glorg.cmd` are set by the script but can be overridden with the command line options :option:`-globk_cmd` and :option:`-glorg_cmd`. Unlike the GAMIT :file:`sestbl.` and :file:`sittbl.`, which for which entries must begin in column 1, all GLOBK files, as well as the :program:`sh_gamit` control files :file:`process.defaults` and :file:`sites.defaults`, follow the convention that a non-blank first column denotes a comment (:content:`*` or :content:`#` below in the examples below) except that you can specify (arbitrary) keywords beginning in line 1 that match the :option:`` list at the end of the :program:`globk`/:program:`glred` command line. If the keyword is given as an option, :program:`globk`/:program:`glred` will replace the keyword in the command file by a blank, thus activating the command. For example, with the command file shown below”j§]”(j±Œ)There are two required control files for ”…””}”(j¶jjÇjÎhNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ . The names ”…””}”(j¶jjÇjÎhNjÆNubj˜)”}”(j¦Œ:file:`globk.cmd`”j§]”j±Œ globk.cmd”…””}”(j¶j2jÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ, and ”…””}”(j¶jjÇjÎhNjÆNubj˜)”}”(j¦Œ:file:`glorg.cmd`”j§]”j±Œ glorg.cmd”…””}”(j¶jGjÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±ŒK are set by the script but can be overridden with the command line options ”…””}”(j¶jjÇjÎhNjÆNubj’)”}”(j¦Œ:option:`-globk_cmd`”j§]”j˜)”}”(j¦j^j§]”j±Œ -globk_cmd”…””}”(j¶j`jÇjÎhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j\ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jýŒ refdomain”jjŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -globk_cmd”ujÄj‘hjújÆKj¶jubj±Œ and ”…””}”(j¶jjÇjÎhNjÆNubj’)”}”(j¦Œ:option:`-glorg_cmd`”j§]”j˜)”}”(j¦j‚j§]”j±Œ -glorg_cmd”…””}”(j¶j„jÇjÎhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j€ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jýŒ refdomain”jŽŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -glorg_cmd”ujÄj‘hjújÆKj¶jubj±Œ. Unlike the GAMIT ”…””}”(j¶jjÇjÎhNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶j¤jÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ and ”…””}”j¶jsbj˜)”}”(j¦Œ:file:`sittbl.`”j§]”j±Œsittbl.”…””}”(j¶j¹jÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±ŒR, which for which entries must begin in column 1, all GLOBK files, as well as the ”…””}”(j¶jjÇjÎhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jÎjÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ control files ”…””}”(j¶jjÇjÎhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jàjÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ and ”…””}”j¶jsbj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jõjÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±ŒI, follow the convention that a non-blank first column denotes a comment (”…””}”(j¶jjÇjÎhNjÆNubj˜)”}”(j¦Œ :content:`*`”j§]”j±Œ*”…””}”(j¶j jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jubj±Œ or ”…””}”(j¶jjÇjÎhNjÆNubj˜)”}”(j¦Œ :content:`#`”j§]”j±Œ#”…””}”(j¶jjÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jubj±Œr below in the examples below) except that you can specify (arbitrary) keywords beginning in line 1 that match the ”…””}”(j¶jjÇjÎhNjÆNubj’)”}”(j¦Œ:option:``”j§]”j˜)”}”(j¦j2j§]”j±Œ ”…””}”(j¶j4jÇjÎhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j0ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jýŒ refdomain”j>Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ ”ujÄj‘hjújÆKj¶jubj±Œ list at the end of the ”…””}”(j¶jjÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jTjÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ/”…””}”(j¶jjÇjÎhNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jfjÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ5 command line. If the keyword is given as an option, ”…””}”(j¶jjÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jxjÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ/”…””}”j¶jsbjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jŠjÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ… will replace the keyword in the command file by a blank, thus activating the command. For example, with the command file shown below”…””}”(j¶jjÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆKj¶jûjÇjÎubj)”}”(j¦ŒK$ sh_glred -expt emed -s 2018 34 2018 36 -ncomb 3 -globk_prefix COMB -opt G”j§]”j±ŒK$ sh_glred -expt emed -s 2018 34 2018 36 -ncomb 3 -globk_prefix COMB -opt G”…””}”j¶j¢sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjújÆK j¶jûjÇjÎubj`)”}”(j¦ŒÄwill transform the command file from one appropriate for time series (solution for each day) one that will stack all of the days together and create a combined h-file for the period of the survey.”j§]”j±ŒÄwill transform the command file from one appropriate for time series (solution for each day) one that will stack all of the days together and create a combined h-file for the period of the survey.”…””}”(j¶j²jÇjÎhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆKj¶jûjÇjÎubj)”}”(j¦X‰* globk command file for time series, short-term combinations and velocity solutions * Set COMB as a globk command line option for short-term combinations; since these commands * follow the commands for repeatabilities, they will take precedence when invoked. * Set VEL as a globk command-line option for velocity; since these commands follow * the commands for repeatabilities, they will take precedence when invoked. * Set KEEP to allow glorg to be run separately after run; useful for testing * as a globk command-line option. * Any combination, e.g. COMB+KEEP or VEL+KEEP will use both (or more) options. * Lasted edited 180705 * << column 1 must be blank if not comment >> * Use wild-cards in file names so that parallel runs do not overwrite * each other. The "@" symbol is replaced with the .gdl-file name root. * This group of commands must appear before any others: eq_file ~/gg/tables/igb14_comb.eq ITRF08 eq_file ~/gg/tables/itrf08_comb.eq # Optionally add a second eq_file for analysis-specific renames x eq_file my_eq_file.eq # For time-series glred runs, it's faster not to use the "com_file" command # (com_file need not be created; only needed if glorg or glsave are to be # run by themselves after globk completes). * This group of commands must appear before any others: KEEP com_file @.com ! Allows parallel runs, provide h-file list name is different srt_file @.srt srt_dir +1 # Normally for combined files, make_svs is not needed. Only needed if # orbits are to be estimated. x make_svs @.svs A * End of commands that must appear first * Solution file pointed to by the com file, if used VEL sol_file @.sol ”j§]”j±X‰* globk command file for time series, short-term combinations and velocity solutions * Set COMB as a globk command line option for short-term combinations; since these commands * follow the commands for repeatabilities, they will take precedence when invoked. * Set VEL as a globk command-line option for velocity; since these commands follow * the commands for repeatabilities, they will take precedence when invoked. * Set KEEP to allow glorg to be run separately after run; useful for testing * as a globk command-line option. * Any combination, e.g. COMB+KEEP or VEL+KEEP will use both (or more) options. * Lasted edited 180705 * << column 1 must be blank if not comment >> * Use wild-cards in file names so that parallel runs do not overwrite * each other. The "@" symbol is replaced with the .gdl-file name root. * This group of commands must appear before any others: eq_file ~/gg/tables/igb14_comb.eq ITRF08 eq_file ~/gg/tables/itrf08_comb.eq # Optionally add a second eq_file for analysis-specific renames x eq_file my_eq_file.eq # For time-series glred runs, it's faster not to use the "com_file" command # (com_file need not be created; only needed if glorg or glsave are to be # run by themselves after globk completes). * This group of commands must appear before any others: KEEP com_file @.com ! Allows parallel runs, provide h-file list name is different srt_file @.srt srt_dir +1 # Normally for combined files, make_svs is not needed. Only needed if # orbits are to be estimated. x make_svs @.svs A * End of commands that must appear first * Solution file pointed to by the com file, if used VEL sol_file @.sol ”…””}”j¶jÀsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/globk.cmd”j/j0j&‰hyŒtext”j(}”Œ linenostart”KsujÄjhjújÆKj¶jûjÇjÎubj`)”}”(j¦X¥The first group of commands define files used by :program:`glred`/:program:`globk` and which must be listed first in the command file in order for the program to work properly. For time series computations, all but the :content:`eq_file` can be considered scratch files. The :content:`eq_file`, described below, allows you to exclude sites or to rename them to account for breaks due to earthquakes or instrument changes.”j§]”(j±Œ1The first group of commands define files used by ”…””}”(j¶jÓjÇjÎhNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jÛjÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓubj±Œ/”…””}”(j¶jÓjÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jíjÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓubj±Œ‰ and which must be listed first in the command file in order for the program to work properly. For time series computations, all but the ”…””}”(j¶jÓjÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`eq_file`”j§]”j±Œeq_file”…””}”(j¶jÿjÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÓubj±Œ& can be considered scratch files. The ”…””}”(j¶jÓjÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`eq_file`”j§]”j±Œeq_file”…””}”(j¶j jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÓubj±Œ€, described below, allows you to exclude sites or to rename them to account for breaks due to earthquakes or instrument changes.”…””}”(j¶jÓjÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆKj¶jûjÇjÎubj)”}”(j¦XG* ITRF augmented by now-defunct sites and recent IGS solutions; * matched to igb14_comb.eq (ITRF2014; default) or itrf08_comb.eq ("ITRF08" command-line option) apr_file ~/gg/tables/igb14_comb.apr ITRF08 apr_file ~/gg/tables/itrf08_comb.apr # Optionally add additional apr files for other sites # Do not used an a priori rotation file with multi-day H-files x in_pmu ~/gg/tables/pmu.usno * Correct the pole tide when not compatible with GAMIT. * Use caution here is binary hfiles from SINEX are used since these * file do not contain status of pole tide correction. app_ptid all ”j§]”j±XG* ITRF augmented by now-defunct sites and recent IGS solutions; * matched to igb14_comb.eq (ITRF2014; default) or itrf08_comb.eq ("ITRF08" command-line option) apr_file ~/gg/tables/igb14_comb.apr ITRF08 apr_file ~/gg/tables/itrf08_comb.apr # Optionally add additional apr files for other sites # Do not used an a priori rotation file with multi-day H-files x in_pmu ~/gg/tables/pmu.usno * Correct the pole tide when not compatible with GAMIT. * Use caution here is binary hfiles from SINEX are used since these * file do not contain status of pole tide correction. app_ptid all ”…””}”j¶j+ sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/globk.cmd”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhjújÆKj¶jûjÇjÎubj`)”}”(j¦ŒçThe next two entries specify the *a priori* files to be used for Earth orientation and coordinates. If these are omitted, the values will be taken from the h-file (i.e., the GAMIT solution), which may be fine in many circumstances.”j§]”(j±Œ!The next two entries specify the ”…””}”(j¶j= jÇjÎhNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jE jÇjÎhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j= ubj±Œ¼ files to be used for Earth orientation and coordinates. If these are omitted, the values will be taken from the h-file (i.e., the GAMIT solution), which may be fine in many circumstances.”…””}”(j¶j= jÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆKj¶jûjÇjÎubj)”}”(j¦ŒÌ* Set maximum chi2, prefit coordinate difference (m), and rotation (mas) for an h-file to be used; max_chii 13 3 100 # increase tolerances to include all files for diagnostics x max_chi 100 5.0 20000 ”j§]”j±ŒÌ* Set maximum chi2, prefit coordinate difference (m), and rotation (mas) for an h-file to be used; max_chii 13 3 100 # increase tolerances to include all files for diagnostics x max_chi 100 5.0 20000 ”…””}”j¶j] sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/globk.cmd”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhjújÆK!j¶jûjÇjÎubj`)”}”(j¦X‡The :content:`max_chi` command allows automatic removal of an h-file when the data are bad, detected in :program:`globk` by checking for a high :math:`\chi^2`, a large adjustment of coordinates from their *a priori* values, or a large rotation of the network. For a network less than 10 km in extent, it may be necessary to loosen these values since the rotation will not be well determined.”j§]”(j±ŒThe ”…””}”(j¶jo jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`max_chi`”j§]”j±Œmax_chi”…””}”(j¶jw jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jo ubj±ŒR command allows automatic removal of an h-file when the data are bad, detected in ”…””}”(j¶jo jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jŠ jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jo ubj±Œ by checking for a high ”…””}”(j¶jo jÇjÎhNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶jœ jÇjÎhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jo ubj±Œ/, a large adjustment of coordinates from their ”…””}”(j¶jo jÇjÎhNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j® jÇjÎhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jo ubj±Œ° values, or a large rotation of the network. For a network less than 10 km in extent, it may be necessary to loosen these values since the rotation will not be well determined.”…””}”(j¶jo jÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆK%j¶jûjÇjÎubj)”}”(j¦X* Invoke glorg org_cmd glorg.cmd * Print file options crt_opt NOPR prt_opt NOPR GDLF org_opt PSUM GDLF FIXA RNRP COMB org_opt ERAS PSUM CMDS GDLF FIXA RNRP VEL org_opt ERAS PSUM CMDS GDLF VSUM FIXA RNRP # The output .org-file will be generated from the # .prt-file name from the globk command line # sh_glred will name the glorg print files # To set an explicit name for the glorg print file # globk print file name from the globk command line x org_out glred_------.org xCOMB org_out globk_------.org xVEL org_out globk_------.org ”j§]”j±X* Invoke glorg org_cmd glorg.cmd * Print file options crt_opt NOPR prt_opt NOPR GDLF org_opt PSUM GDLF FIXA RNRP COMB org_opt ERAS PSUM CMDS GDLF FIXA RNRP VEL org_opt ERAS PSUM CMDS GDLF VSUM FIXA RNRP # The output .org-file will be generated from the # .prt-file name from the globk command line # sh_glred will name the glorg print files # To set an explicit name for the glorg print file # globk print file name from the globk command line x org_out glred_------.org xCOMB org_out globk_------.org xVEL org_out globk_------.org ”…””}”j¶jÆ sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/globk.cmd”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhjújÆK(j¶jûjÇjÎubj`)”}”(j¦X˜Including the name of the :program:`glorg` command file (:content:`org_cmd glorg.cmd`) tells globk to call :program:`glorg` for frame definition ("stabilization") after :program:`globk` is run. The :content:`org_opt` command prescribes what is included in the :program:`glorg` print summary (:file:`.org` file). :content:`PSUM` means a summary of position adjustments; :content:`GDLF` means to list the name of the input h-file; and :content:`CMDS` means to echo both the :program:`globk` and :program:`glorg` command files. If you are invoking :program:`glorg`, then the :program:`globk` print will not be very useful and is suppressed by :content:`prt_opt NOPR`.”j§]”(j±ŒIncluding the name of the ”…””}”(j¶jØ jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jà jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jØ ubj±Œ command file (”…””}”(j¶jØ jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`org_cmd glorg.cmd`”j§]”j±Œorg_cmd glorg.cmd”…””}”(j¶jò jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jØ ubj±Œ) tells globk to call ”…””}”(j¶jØ jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j!jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jØ ubj±Œ2 for frame definition (“stabilizationâ€) after ”…””}”(j¶jØ jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j!jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jØ ubj±Œ is run. The ”…””}”(j¶jØ jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`org_opt`”j§]”j±Œorg_opt”…””}”(j¶j)!jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jØ ubj±Œ, command prescribes what is included in the ”…””}”(j¶jØ jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j`_.)”j§]”(j±ŒASites to include in the solution are selected or deselected with ”…””}”(j¶jû"jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`use_site`”j§]”j±Œuse_site”…””}”(j¶j#jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jû"ubj±Œn. The default is to include all sites in the h-file(s), but you can command a subset by started the list with ”…””}”(j¶jû"jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`clear`”j§]”j±Œclear”…””}”(j¶j#jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jû"ubj±X followed by the site names, either four characters (all 8-character versions of the site) or the full eight (to select only certain versions); listing the site preceeded by a minus will remove it from the list. In the example we’ve referred to a separate file (”…””}”(j¶jû"jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`../tables/uselist`”j§]”j±Œ../tables/uselist”…””}”(j¶j)#jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jû"ubj±Œ) rather than include the ”…””}”(j¶jû"jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`use_site`”j§]”j±Œuse_site”…””}”(j¶j<#jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jû"ubj±Œo commands in the main command file. For site selection from an h-file of global processing, you can invoke the ”…””}”(j¶jû"jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`use_pos`”j§]”j±Œuse_pos”…””}”(j¶jO#jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jû"ubj±ŒD to include or exclude sites within a geographical region. (See the ”…””}”(j¶jû"jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jb#jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jû"ubj±Œ! help file or Section 3.1 of the ”…””}”(j¶jû"jÇjÎhNjÆNubj÷ )”}”(j¦ŒG`GLOBK Reference Manual `_”j§]”j±ŒGLOBK Reference Manual”…””}”(j¶jt#jÇjÎhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGLOBK Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GLOBK_Ref.pdf”ujÄjö j¶jû"ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œglobk-reference-manual”aj»]”j½]”Œglobk reference manual”ajÀ]”jÂ]”Œrefuri”j„#ujÄjdj Kj¶jû"ubj±Œ.)”…””}”(j¶jû"jÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆK@j¶jûjÇjÎubj)”}”(j¦Œó* Write out a combined H-file # Can substitute your analysis name for 'COMB' in the file name below COMB out_glb H------_COMB.GLX VEL out_glb @.GLX * Remove scratch files for repeatability and combination runs del_scra yes KEEP del_scra no ”j§]”j±Œó* Write out a combined H-file # Can substitute your analysis name for 'COMB' in the file name below COMB out_glb H------_COMB.GLX VEL out_glb @.GLX * Remove scratch files for repeatability and combination runs del_scra yes KEEP del_scra no ”…””}”j¶jœ#sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/globk.cmd”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhjújÆKGj¶jûjÇjÎubj`)”}”(j¦X(The :content:`out_glb` command, when invoked, tells :program:`globk` to write the solution out in the form of an h-file. This is useful for aggregating data in weekly or monthly averages and/or combining your own processing with global or regional h-files from an external source (see Chapter 4).”j§]”(j±ŒThe ”…””}”(j¶j®#jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`out_glb`”j§]”j±Œout_glb”…””}”(j¶j¶#jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j®#ubj±Œ command, when invoked, tells ”…””}”(j¶j®#jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jÉ#jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®#ubj±Œä to write the solution out in the form of an h-file. This is useful for aggregating data in weekly or monthly averages and/or combining your own processing with global or regional h-files from an external source (see Chapter 4).”…””}”(j¶j®#jÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆKKj¶jûjÇjÎubj)”}”(j¦Œ@* Turn off quake log estimates if in the eq_file free_log -1 ”j§]”j±Œ@* Turn off quake log estimates if in the eq_file free_log -1 ”…””}”j¶já#sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/globk.cmd”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhjújÆKNj¶jûjÇjÎubj`)”}”(j¦XoIf you need to provide for step changes in coordinates (or velocities) and/or to exclude sites during certain periods, you can use an "earthquake-rename" file (:content:`eq_file`) with :program:`globk`. The file has two types of entries. The first renames sites (creates new logical sites for :program:`globk`) automatically based on their proximity to an earthquake:”j§]”(j±Œ¤If you need to provide for step changes in coordinates (or velocities) and/or to exclude sites during certain periods, you can use an “earthquake-rename†file (”…””}”(j¶jó#jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`eq_file`”j§]”j±Œeq_file”…””}”(j¶jû#jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jó#ubj±Œ) with ”…””}”(j¶jó#jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j$jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jó#ubj±Œ\. The file has two types of entries. The first renames sites (creates new logical sites for ”…””}”(j¶jó#jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j $jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jó#ubj±Œ:) automatically based on their proximity to an earthquake:”…””}”(j¶jó#jÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆKRj¶jûjÇjÎubj)”}”(j¦Œï# November 3, 2002, UT=22:12 Lat = 63.52 Lon -147.53 Depth=5 km M 7.9 eq_def DN 63.52 -147.53 700 5. 2002 11 3 22 12 eq_cosei DN 1.0 1.0 1.0 1.8 1.8 0.7 eq_post DN 100 0.1 0.1 0.1 1.8 1.8 0.7 Postseismic: 0.1 mm**2/day eq_rename DN”j§]”j±Œï# November 3, 2002, UT=22:12 Lat = 63.52 Lon -147.53 Depth=5 km M 7.9 eq_def DN 63.52 -147.53 700 5. 2002 11 3 22 12 eq_cosei DN 1.0 1.0 1.0 1.8 1.8 0.7 eq_post DN 100 0.1 0.1 0.1 1.8 1.8 0.7 Postseismic: 0.1 mm**2/day eq_rename DN”…””}”j¶j8$sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjújÆKVj¶jûjÇjÎubj`)”}”(j¦X‰With the lines above included in the :content:`eq_file`, all sites within 700 km of the 2002 Denali (Alaska) earthquake will be renamed (:content:`_gps` to :content:`_gdn`) for h-files with start and stop times later than 22:12 on 3 November 2002. The :content:`eq_cosei` and :content:`eq_post` commands prescribe the constraints applied to the co-seismic and post-seismic changes. (See the :program:`globk` help file and Section 3.1 of the `GLOBK Reference Manual `_.) The second type of command renames sites according to explicit instructions to account for changes in data quality or instrumentation:”j§]”(j±Œ%With the lines above included in the ”…””}”(j¶jH$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`eq_file`”j§]”j±Œeq_file”…””}”(j¶jP$jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jH$ubj±ŒR, all sites within 700 km of the 2002 Denali (Alaska) earthquake will be renamed (”…””}”(j¶jH$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`_gps`”j§]”j±Œ_gps”…””}”(j¶jc$jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jH$ubj±Œ to ”…””}”(j¶jH$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`_gdn`”j§]”j±Œ_gdn”…””}”(j¶jv$jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jH$ubj±ŒQ) for h-files with start and stop times later than 22:12 on 3 November 2002. The ”…””}”(j¶jH$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`eq_cosei`”j§]”j±Œeq_cosei”…””}”(j¶j‰$jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jH$ubj±Œ and ”…””}”(j¶jH$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`eq_post`”j§]”j±Œeq_post”…””}”(j¶jœ$jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jH$ubj±Œa commands prescribe the constraints applied to the co-seismic and post-seismic changes. (See the ”…””}”(j¶jH$jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j¯$jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jH$ubj±Œ" help file and Section 3.1 of the ”…””}”(j¶jH$jÇjÎhNjÆNubj÷ )”}”(j¦ŒG`GLOBK Reference Manual `_”j§]”j±ŒGLOBK Reference Manual”…””}”(j¶jÁ$jÇjÎhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGLOBK Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GLOBK_Ref.pdf”ujÄjö j¶jH$ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œid1”aj»]”j½]”jÀ]”Œglobk reference manual”ajÂ]”Œrefuri”jÑ$ujÄjdj Kj¶jH$ubj±Œ‰.) The second type of command renames sites according to explicit instructions to account for changes in data quality or instrumentation:”…””}”(j¶jH$jÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆK^j¶jûjÇjÎubj)”}”(j¦Œ®rename mate_gps mate_1ps 1999 6 18 0 0 rename kit3_gps kit3_xcl 1997 5 14 0 0 1997 5 18 0 0 rename madr_gps madr_xhi emed 1996 9 26 0 0 1996 10 27 0 0”j§]”j±Œ®rename mate_gps mate_1ps 1999 6 18 0 0 rename kit3_gps kit3_xcl 1997 5 14 0 0 1997 5 18 0 0 rename madr_gps madr_xhi emed 1996 9 26 0 0 1996 10 27 0 0”…””}”j¶jé$sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjújÆKcj¶jûjÇjÎubj`)”}”(j¦X­The first of these lines accounts for a position change with the introduction of a new receiver at Matera; the second removes some bad data at Kitab for a four-day period; the third accounts for the use of an incorrect antenna height in h-files whose names include the substring :content:`emed`. You may use the :content:`equate` feature of :program:`glorg` to force the horizontal adjustments for :content:`madr_gps` and :content:`madr_xhi` to be the same (see Chapter 4). It is also possible to use the :content:`rename` command to shift the position of a site without introducing a new site, useful to apply offsets known from local measurements or assumed from an earthquake model:”j§]”(j±XThe first of these lines accounts for a position change with the introduction of a new receiver at Matera; the second removes some bad data at Kitab for a four-day period; the third accounts for the use of an incorrect antenna height in h-files whose names include the substring ”…””}”(j¶jù$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`emed`”j§]”j±Œemed”…””}”(j¶j%jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jù$ubj±Œ. You may use the ”…””}”(j¶jù$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`equate`”j§]”j±Œequate”…””}”(j¶j%jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jù$ubj±Œ feature of ”…””}”(j¶jù$jÇjÎhNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j'%jÇjÎhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jù$ubj±Œ) to force the horizontal adjustments for ”…””}”(j¶jù$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`madr_gps`”j§]”j±Œmadr_gps”…””}”(j¶j9%jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jù$ubj±Œ and ”…””}”(j¶jù$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`madr_xhi`”j§]”j±Œmadr_xhi”…””}”(j¶jL%jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jù$ubj±Œ@ to be the same (see Chapter 4). It is also possible to use the ”…””}”(j¶jù$jÇjÎhNjÆNubj˜)”}”(j¦Œ:content:`rename`”j§]”j±Œrename”…””}”(j¶j_%jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jù$ubj±Œ£ command to shift the position of a site without introducing a new site, useful to apply offsets known from local measurements or assumed from an earthquake model:”…””}”(j¶jù$jÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆKij¶jûjÇjÎubj)”}”(j¦ŒLrename tigr_gni tigr_gni 2001 2 28 0 0 2100 1 1 0 0 0.0032 0.0033 0.0000 NEU”j§]”j±ŒLrename tigr_gni tigr_gni 2001 2 28 0 0 2100 1 1 0 0 0.0032 0.0033 0.0000 NEU”…””}”j¶jx%sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjújÆKoj¶jûjÇjÎubj`)”}”(j¦XhThe entry applies 3 mm offsets of the north and east coordinates of the site based on an *a priori* model for the Nisqually (:content:`NI`) earthquake near Seattle, Washington. For ITRF sites the :file:`igb14_comb.eq` file provides a set of renames consistent with the :file:`igb14_comb.apr` file (similarly :file:`itrf08_comb.eq` and :file:`itrf08_comb.apr`).”j§]”(j±ŒYThe entry applies 3 mm offsets of the north and east coordinates of the site based on an ”…””}”(j¶jˆ%jÇjÎhNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j%jÇjÎhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jˆ%ubj±Œ model for the Nisqually (”…””}”(j¶jˆ%jÇjÎhNjÆNubj˜)”}”(j¦Œ :content:`NI`”j§]”j±ŒNI”…””}”(j¶j¢%jÇjÎhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jˆ%ubj±Œ:) earthquake near Seattle, Washington. For ITRF sites the ”…””}”(j¶jˆ%jÇjÎhNjÆNubj˜)”}”(j¦Œ:file:`igb14_comb.eq`”j§]”j±Œ igb14_comb.eq”…””}”(j¶jµ%jÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jˆ%ubj±Œ4 file provides a set of renames consistent with the ”…””}”(j¶jˆ%jÇjÎhNjÆNubj˜)”}”(j¦Œ:file:`igb14_comb.apr`”j§]”j±Œigb14_comb.apr”…””}”(j¶jÊ%jÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jˆ%ubj±Œ file (similarly ”…””}”(j¶jˆ%jÇjÎhNjÆNubj˜)”}”(j¦Œ:file:`itrf08_comb.eq`”j§]”j±Œitrf08_comb.eq”…””}”(j¶jß%jÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jˆ%ubj±Œ and ”…””}”(j¶jˆ%jÇjÎhNjÆNubj˜)”}”(j¦Œ:file:`itrf08_comb.apr`”j§]”j±Œitrf08_comb.apr”…””}”(j¶jô%jÇjÎhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jˆ%ubj±Œ).”…””}”(j¶jˆ%jÇjÎhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjújÆKsj¶jûjÇjÎubej·}”(j¹]”(Œ globk-cmd”jùej»]”j½]”(Œ globk.cmd”Œintro_proc_globk”ejÀ]”jÂ]”ujÄh_j¶jÎjÇjÎhjújÆKjÒ }”j&jïsjÔ }”jùjïsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”júj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjújNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jÝjÑjìjàuj_}”(Œrel”jÝŒdate”jìujc}”je}”jù]”jïasjg}”(j&jùj&j&jŽ#j‹#uji}”(j&ˆj&‰jŽ#ˆuj¹}”(jùjûj&jûj‹#j…#jØ$jÒ$ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”jù )”}”(j¦hoj§]”j`)”}”(j¦Œ9Duplicate explicit target name: "globk reference manual".”j§]”j±Œ=Duplicate explicit target name: “globk reference manualâ€.”…””}”(j¶j>&jÇjÎhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j;&ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jØ$aŒlevel”KŒtype”jŒsource”júŒline”KujÄjø j¶jûjÇjÎhjújÆKaubaj†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ6Hyperlink target "intro-proc-globk" is not referenced.”…””}”j¶jZ&sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jW&ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”júŒline”KujÄjø ubajˆNj‰]”j‹NjÇjÎubjéj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶ju&sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jr&jÇjr&ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j„&jÇjr&hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jr&jÇjr&ubje)”}”(j¦Œ.. _intro_proc_glorg:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-glorg”ujÄjdjÆKj¶jr&jÇjr&hŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/glorg.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ:file:`glorg.cmd`”j§]”j˜)”}”(j¦j¤&j§]”j±Œ glorg.cmd”…””}”(j¶j¦&jÇjr&hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¢&ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jŸ&jÇjr&hjž&jÆKubj`)”}”(j¦Œ/The :program:`glorg` command file has the form:”j§]”(j±ŒThe ”…””}”(j¶j¼&jÇjr&hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jÄ&jÇjr&hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¼&ubj±Œ command file has the form:”…””}”(j¶j¼&jÇjr&hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjž&jÆKj¶jŸ&jÇjr&ubj)”}”(j¦XË* glorg command file for time series, short-term combinations and velocity solutions * Set VEL as a globk command-line option for velocity; since these commands follow * the commands for repeatabilities, they will take precedence when invoked. * Add choice of plate for final reference frame (e.g. EURA14 for Eurasia defined by * Altamimi et al.'s (2017) ITRF2014 plate motion model, NOAM08 for North America * defined by Altamimi et al's (2012) ITRF2008 plate motion model, NA1214 for North * America defined by Blewitt et al. (2013) using rotated ITRF2014 velocities, etc. * Last edited by MAF 180519 * << column 1 must be blank if not comment >> * Parameters to be estimated pos_org xtran ytran ztran xrot yrot zrot VEL rate_org xtran ytran ztran xrot yrot zrot # Optionally, if estimated scale in GLOBK: SCALE pos_org xtran ytran ztran xrot yrot zrot scale xSCALE rate_org xtran ytran ztran xrot yrot zrot # or if translation-only x pos_org xtran ytran ztran xVEL rate_org xtran ytran ztran * Downweight of height relative to horizontal (default is 10 10) # Heavy downweight if reference frame robust and heights suspect x cnd_hgt 1000 1000 * Controls for removing sites from the stabilization # Vary these to make the stabilization more robust or more precise stab_it 4 0.8 3.0 x stab_it 4 0.5 4.0 * A priori coordinates to define the analysis reference frame apr_file ~/gg/tables/igb14_comb.apr ITRF08 apr_file ~/gg/tables/itrf08_comb.apr # ITRF2014 plate motion model defined by Altamimi et al. (2017) AMUR14 apr_file ~/gg/tables/igb14_comb_amur08.apr ANTA14 apr_file ~/gg/tables/igb14_comb_anta.apr ARAB14 apr_file ~/gg/tables/igb14_comb_arab.apr AUST14 apr_file ~/gg/tables/igb14_comb_aust.apr CARB14 apr_file ~/gg/tables/igb14_comb_carb08.apr EURA14 apr_file ~/gg/tables/igb14_comb_eura.apr INDI14 apr_file ~/gg/tables/igb14_comb_indi.apr NAZC14 apr_file ~/gg/tables/igb14_comb_nazc.apr NOAM14 apr_file ~/gg/tables/igb14_comb_noam.apr NUBI14 apr_file ~/gg/tables/igb14_comb_nubi.apr PCFC14 apr_file ~/gg/tables/igb14_comb_pcfc.apr SOAM14 apr_file ~/gg/tables/igb14_comb_soam.apr SOMA14 apr_file ~/gg/tables/igb14_comb_soma.apr SUND14 apr_file ~/gg/tables/igb14_comb_sund08.apr # North America defined by Blewitt et al. (2013) NA1214 apr_file ~/gg/tables/igb14_comb_na12.apr # North America defined by Kreemer et al. (2018) NA1714 apr_file ~/gg/tables/igb14_comb_na17.apr # Nubia and Somalia defined by Saria et al. (2013) NU1314 apr_file ~/gg/tables/igb14_comb_nu13.apr SO1314 apr_file ~/gg/tables/igb14_comb_so13.apr # ITRF2008 plate motion model defined by Altamimi et al. (2012) AMUR08 apr_file ~/gg/tables/itrf08_comb_amur.apr ANTA08 apr_file ~/gg/tables/itrf08_comb_anta.apr ARAB08 apr_file ~/gg/tables/itrf08_comb_arab.apr AUST08 apr_file ~/gg/tables/itrf08_comb_aust.apr CARB08 apr_file ~/gg/tables/itrf08_comb_carb.apr EURA08 apr_file ~/gg/tables/itrf08_comb_eura.apr INDI08 apr_file ~/gg/tables/itrf08_comb_indi.apr NAZC08 apr_file ~/gg/tables/itrf08_comb_nazc.apr NOAM08 apr_file ~/gg/tables/itrf08_comb_noam.apr NUBI08 apr_file ~/gg/tables/itrf08_comb_nubi.apr PCFC08 apr_file ~/gg/tables/itrf08_comb_pcfc.apr SOAM08 apr_file ~/gg/tables/itrf08_comb_soam.apr SOMA08 apr_file ~/gg/tables/itrf08_comb_soma.apr SUND08 apr_file ~/gg/tables/itrf08_comb_sund.apr # North America defined by Blewitt et al. (2013) NA1208 apr_file ~/gg/tables/itrf08_comb_na12.apr # North America defined by Kreemer et al. (2018) NA1708 apr_file ~/gg/tables/itrf08_comb_na17.apr # Nubia and Somalia defined by Saria et al. (2013) NU1308 apr_file ~/gg/tables/itrf08_comb_nu13.apr SO1308 apr_file ~/gg/tables/itrf08_comb_so13.apr # Use a regional stablization if available from a prior solution (comment out the itrf08 file) x apr_file ../tables/regional.apr * List of stabilization sites # This should match the well-determined sites in the apr_file stab_site clear x source ~/gg/tables/igb14_hierarchy.stab_site source ~/gg/tables/igb14_comb.stab_site xITRF08 source ~/gg/tables/igb08_hierarchy.stab_site ITRF08 source ~/gg/tables/itrf08.stab_site # Use a regional stabililization if available from a prior solution x source ../tables/regional_stab_site * Estimate rotation (Euler) vectors to be used with sh_org2vel to * to rotate the solution to a block- or region-specific reference frame xVEL plate eurasia kosg_2ps onsa_2ps nyal_4ps graz_2ps tlse_2ps kit3_2ps xVEL plate eurasia vill_3ps mars_3ps cbre xVEL plate weura kosg_2ps tlse_2ps vill_3ps mars_3ps xVEL plate aegean milo kyra xris dioa leon mkn2 bodr roml omal koun seva # Constrain the center-of-mass to the apr-file in plate estimate (comment out for global solutions) xVEL NOPLATETRAN * Equate the velocities of co-located sites VEL eq_dist 1000 ndot VEL eq_dist 1000 edot VEL eq_dist 1000 udot * Equate a few horizontal velocities for sites farther apart VEL equate trab_gps ndot akto_gps ndot VEL equate trab_gps edot akto_gps edot * Unequate velocities that are incompatible VEL unequate mad2_gps ndot VEL unequate mad2_gps edot VEL unequate mad2_gps udot ”•j§]”j±XË* glorg command file for time series, short-term combinations and velocity solutions * Set VEL as a globk command-line option for velocity; since these commands follow * the commands for repeatabilities, they will take precedence when invoked. * Add choice of plate for final reference frame (e.g. EURA14 for Eurasia defined by * Altamimi et al.'s (2017) ITRF2014 plate motion model, NOAM08 for North America * defined by Altamimi et al's (2012) ITRF2008 plate motion model, NA1214 for North * America defined by Blewitt et al. (2013) using rotated ITRF2014 velocities, etc. * Last edited by MAF 180519 * << column 1 must be blank if not comment >> * Parameters to be estimated pos_org xtran ytran ztran xrot yrot zrot VEL rate_org xtran ytran ztran xrot yrot zrot # Optionally, if estimated scale in GLOBK: SCALE pos_org xtran ytran ztran xrot yrot zrot scale xSCALE rate_org xtran ytran ztran xrot yrot zrot # or if translation-only x pos_org xtran ytran ztran xVEL rate_org xtran ytran ztran * Downweight of height relative to horizontal (default is 10 10) # Heavy downweight if reference frame robust and heights suspect x cnd_hgt 1000 1000 * Controls for removing sites from the stabilization # Vary these to make the stabilization more robust or more precise stab_it 4 0.8 3.0 x stab_it 4 0.5 4.0 * A priori coordinates to define the analysis reference frame apr_file ~/gg/tables/igb14_comb.apr ITRF08 apr_file ~/gg/tables/itrf08_comb.apr # ITRF2014 plate motion model defined by Altamimi et al. (2017) AMUR14 apr_file ~/gg/tables/igb14_comb_amur08.apr ANTA14 apr_file ~/gg/tables/igb14_comb_anta.apr ARAB14 apr_file ~/gg/tables/igb14_comb_arab.apr AUST14 apr_file ~/gg/tables/igb14_comb_aust.apr CARB14 apr_file ~/gg/tables/igb14_comb_carb08.apr EURA14 apr_file ~/gg/tables/igb14_comb_eura.apr INDI14 apr_file ~/gg/tables/igb14_comb_indi.apr NAZC14 apr_file ~/gg/tables/igb14_comb_nazc.apr NOAM14 apr_file ~/gg/tables/igb14_comb_noam.apr NUBI14 apr_file ~/gg/tables/igb14_comb_nubi.apr PCFC14 apr_file ~/gg/tables/igb14_comb_pcfc.apr SOAM14 apr_file ~/gg/tables/igb14_comb_soam.apr SOMA14 apr_file ~/gg/tables/igb14_comb_soma.apr SUND14 apr_file ~/gg/tables/igb14_comb_sund08.apr # North America defined by Blewitt et al. (2013) NA1214 apr_file ~/gg/tables/igb14_comb_na12.apr # North America defined by Kreemer et al. (2018) NA1714 apr_file ~/gg/tables/igb14_comb_na17.apr # Nubia and Somalia defined by Saria et al. (2013) NU1314 apr_file ~/gg/tables/igb14_comb_nu13.apr SO1314 apr_file ~/gg/tables/igb14_comb_so13.apr # ITRF2008 plate motion model defined by Altamimi et al. (2012) AMUR08 apr_file ~/gg/tables/itrf08_comb_amur.apr ANTA08 apr_file ~/gg/tables/itrf08_comb_anta.apr ARAB08 apr_file ~/gg/tables/itrf08_comb_arab.apr AUST08 apr_file ~/gg/tables/itrf08_comb_aust.apr CARB08 apr_file ~/gg/tables/itrf08_comb_carb.apr EURA08 apr_file ~/gg/tables/itrf08_comb_eura.apr INDI08 apr_file ~/gg/tables/itrf08_comb_indi.apr NAZC08 apr_file ~/gg/tables/itrf08_comb_nazc.apr NOAM08 apr_file ~/gg/tables/itrf08_comb_noam.apr NUBI08 apr_file ~/gg/tables/itrf08_comb_nubi.apr PCFC08 apr_file ~/gg/tables/itrf08_comb_pcfc.apr SOAM08 apr_file ~/gg/tables/itrf08_comb_soam.apr SOMA08 apr_file ~/gg/tables/itrf08_comb_soma.apr SUND08 apr_file ~/gg/tables/itrf08_comb_sund.apr # North America defined by Blewitt et al. (2013) NA1208 apr_file ~/gg/tables/itrf08_comb_na12.apr # North America defined by Kreemer et al. (2018) NA1708 apr_file ~/gg/tables/itrf08_comb_na17.apr # Nubia and Somalia defined by Saria et al. (2013) NU1308 apr_file ~/gg/tables/itrf08_comb_nu13.apr SO1308 apr_file ~/gg/tables/itrf08_comb_so13.apr # Use a regional stablization if available from a prior solution (comment out the itrf08 file) x apr_file ../tables/regional.apr * List of stabilization sites # This should match the well-determined sites in the apr_file stab_site clear x source ~/gg/tables/igb14_hierarchy.stab_site source ~/gg/tables/igb14_comb.stab_site xITRF08 source ~/gg/tables/igb08_hierarchy.stab_site ITRF08 source ~/gg/tables/itrf08.stab_site # Use a regional stabililization if available from a prior solution x source ../tables/regional_stab_site * Estimate rotation (Euler) vectors to be used with sh_org2vel to * to rotate the solution to a block- or region-specific reference frame xVEL plate eurasia kosg_2ps onsa_2ps nyal_4ps graz_2ps tlse_2ps kit3_2ps xVEL plate eurasia vill_3ps mars_3ps cbre xVEL plate weura kosg_2ps tlse_2ps vill_3ps mars_3ps xVEL plate aegean milo kyra xris dioa leon mkn2 bodr roml omal koun seva # Constrain the center-of-mass to the apr-file in plate estimate (comment out for global solutions) xVEL NOPLATETRAN * Equate the velocities of co-located sites VEL eq_dist 1000 ndot VEL eq_dist 1000 edot VEL eq_dist 1000 udot * Equate a few horizontal velocities for sites farther apart VEL equate trab_gps ndot akto_gps ndot VEL equate trab_gps edot akto_gps edot * Unequate velocities that are incompatible VEL unequate mad2_gps ndot VEL unequate mad2_gps edot VEL unequate mad2_gps udot ”…””}”j¶jÜ&sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/glorg.cmd”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhjž&jÆKj¶jŸ&jÇjr&ubj`)”}”(j¦X/Frame definition (stabilization or spatial filtering) is accomplished in :program:`glorg` by specifying a set of sites for which the *a priori* coordinates are known at the level you expect the frame to be defined (usually 1–2 mm horizontal, 2–5 mm vertical) and the parameters you want to estimate in order to minimize the coordinate adjustments for these sites. If an :content:`apr_file` is included in the :program:`glorg` command file, its coordinates will supersede those used in GAMIT or :program:`globk`, so it is not necessary to use the same *a priori* coordinates for all three programs. For :program:`glorg`, the only coordinates that matter are those for the stabilization sites. The :content:`pos_org` command specifies the parameters to be estimated, either translation only (omit the last three entries) or translation and rotation. The rules for :content:`stab_site` are the same as those for :content:`use_site` in the :program:`globk` command file. See :numref:`intro_prod_refframe` for a more comprehensive discussion of reference frame definition.”j§]”(j±ŒIFrame definition (stabilization or spatial filtering) is accomplished in ”…””}”(j¶jî&jÇjr&hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jö&jÇjr&hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jî&ubj±Œ, by specifying a set of sites for which the ”…””}”(j¶jî&jÇjr&hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j'jÇjr&hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jî&ubj±Œç coordinates are known at the level you expect the frame to be defined (usually 1–2 mm horizontal, 2–5 mm vertical) and the parameters you want to estimate in order to minimize the coordinate adjustments for these sites. If an ”…””}”(j¶jî&jÇjr&hNjÆNubj˜)”}”(j¦Œ:content:`apr_file`”j§]”j±Œapr_file”…””}”(j¶j'jÇjr&hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jî&ubj±Œ is included in the ”…””}”(j¶jî&jÇjr&hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j-'jÇjr&hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jî&ubj±ŒE command file, its coordinates will supersede those used in GAMIT or ”…””}”(j¶jî&jÇjr&hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j?'jÇjr&hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jî&ubj±Œ), so it is not necessary to use the same ”…””}”(j¶jî&jÇjr&hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jQ'jÇjr&hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jî&ubj±Œ) coordinates for all three programs. For ”…””}”(j¶jî&jÇjr&hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jc'jÇjr&hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jî&ubj±ŒN, the only coordinates that matter are those for the stabilization sites. The ”…””}”(j¶jî&jÇjr&hNjÆNubj˜)”}”(j¦Œ:content:`pos_org`”j§]”j±Œpos_org”…””}”(j¶ju'jÇjr&hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jî&ubj±Œ” command specifies the parameters to be estimated, either translation only (omit the last three entries) or translation and rotation. The rules for ”…””}”(j¶jî&jÇjr&hNjÆNubj˜)”}”(j¦Œ:content:`stab_site`”j§]”j±Œ stab_site”…””}”(j¶jˆ'jÇjr&hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jî&ubj±Œ are the same as those for ”…””}”(j¶jî&jÇjr&hNjÆNubj˜)”}”(j¦Œ:content:`use_site`”j§]”j±Œuse_site”…””}”(j¶j›'jÇjr&hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jî&ubj±Œ in the ”…””}”(j¶jî&jÇjr&hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j®'jÇjr&hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jî&ubj±Œ command file. See ”…””}”(j¶jî&jÇjr&hNjÆNubj’)”}”(j¦Œ:numref:`intro_prod_refframe`”j§]”j˜)”}”(j¦jÂ'j§]”j±Œintro_prod_refframe”…””}”(j¶jÄ'jÇjr&hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jÀ'ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jéŒ refdomain”jÎ'Œreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_prod_refframe”ujÄj‘hjž&jÆK j¶jî&ubj±ŒC for a more comprehensive discussion of reference frame definition.”…””}”(j¶jî&jÇjr&hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjž&jÆK j¶jŸ&jÇjr&ubj`)”}”(j¦XThe next two entries in the file control the weighting of the quasi-observations (site coordinates) in the stabilization. For :content:`cnd_hgtv` the first two values specify (for position and velocity, respectively) the down-weighting of heights relative to horizontal coordinates. The default is 10, under the assumption that the uncertainties in heights are about three times higher than for the horizontal coordinates; however, you can increase this ratio if want to define only a horizontal frame or you know that the height estimates are unreliable. The last two values set limits on the uncertainty in height allowed to have a site included and serve to remove from the stabilization poorly determined sites. For :content:`stab_it` the first value is the number of iterations used in the stabilization, the second the amount of reweighting that can take place between iterations, and the third the ratio of residual to uncertainty (sigma) allowed before a site is removed from the stabilization. You can change the last value to fine-tune the inclusion or exclusion of sites from the frame definition. These commands are discussed in more detail in the :program:`glorg` help file and Section 3.2 of the `GLOBK Reference Manual `_.”j§]”(j±Œ~The next two entries in the file control the weighting of the quasi-observations (site coordinates) in the stabilization. For ”…””}”(j¶jê'jÇjr&hNjÆNubj˜)”}”(j¦Œ:content:`cnd_hgtv`”j§]”j±Œcnd_hgtv”…””}”(j¶jò'jÇjr&hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jê'ubj±X? the first two values specify (for position and velocity, respectively) the down-weighting of heights relative to horizontal coordinates. The default is 10, under the assumption that the uncertainties in heights are about three times higher than for the horizontal coordinates; however, you can increase this ratio if want to define only a horizontal frame or you know that the height estimates are unreliable. The last two values set limits on the uncertainty in height allowed to have a site included and serve to remove from the stabilization poorly determined sites. For ”…””}”(j¶jê'jÇjr&hNjÆNubj˜)”}”(j¦Œ:content:`stab_it`”j§]”j±Œstab_it”…””}”(j¶j(jÇjr&hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jê'ubj±X¦ the first value is the number of iterations used in the stabilization, the second the amount of reweighting that can take place between iterations, and the third the ratio of residual to uncertainty (sigma) allowed before a site is removed from the stabilization. You can change the last value to fine-tune the inclusion or exclusion of sites from the frame definition. These commands are discussed in more detail in the ”…””}”(j¶jê'jÇjr&hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j(jÇjr&hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jê'ubj±Œ" help file and Section 3.2 of the ”…””}”(j¶jê'jÇjr&hNjÆNubj÷ )”}”(j¦ŒG`GLOBK Reference Manual `_”j§]”j±ŒGLOBK Reference Manual”…””}”(j¶j*(jÇjr&hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGLOBK Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GLOBK_Ref.pdf”ujÄjö j¶jê'ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œglobk-reference-manual”aj»]”j½]”Œglobk reference manual”ajÀ]”jÂ]”Œrefuri”j:(ujÄjdj Kj¶jê'ubj±Œ.”…””}”(j¶jê'jÇjr&hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjž&jÆKj¶jŸ&jÇjr&ubej·}”(j¹]”(Œ glorg-cmd”j&ej»]”j½]”(Œ glorg.cmd”Œintro_proc_glorg”ejÀ]”jÂ]”ujÄh_j¶jr&jÇjr&hjž&jÆKjÒ }”jX(j“&sjÔ }”j&j“&subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jž&j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjž&jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j&ju&j&j„&uj_}”(Œrel”j&Œdate”j&ujc}”je}”j&]”j“&asjg}”(jX(j&jW(jT(jD(jA(uji}”(jX(ˆjW(‰jD(ˆuj¹}”(j&jŸ&jT(jŸ&jA(j;(ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ6Hyperlink target "intro-proc-glorg" is not referenced.”…””}”j¶j‚(sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j(ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jž&Œline”KujÄjø ubajˆNj‰]”j‹NjÇjr&ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j(sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jš(jÇjš(ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j¬(jÇjš(hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jš(jÇjš(ubje)”}”(j¦Œ.. _intro_proc_control:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-control”ujÄjdjÆKj¶jš(jÇjš(hŒL/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/index.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒEditing the Control Files”j§]”j±ŒEditing the Control Files”…””}”(j¶jÊ(jÇjš(hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jÇ(jÇjš(hjÆ(jÆKubjí)”}”(j¦hoj§]”jò)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j¶jjü]”(NŒ#intro/proc/control/process.defaults”†”NŒ!intro/proc/control/sites.defaults”†”NŒintro/proc/control/sestbl”†”NŒintro/proc/control/sittbl”†”NŒintro/proc/control/autcln”†”NŒintro/proc/control/globk”†”NŒintro/proc/control/glorg”†”ejþ]”(jå(jç(jé(jë(jí(jï(jñ(ejJÿÿÿÿjNj‰j‰j‰jKj‰j]”ujÄjñhjÆ(jÆKj¶jØ(ubaj·}”(j¹]”j»]”j aj½]”jÀ]”jÂ]”ujÄjìj¶jÇ(jÇjš(hjÆ(jÆKubej·}”(j¹]”(Œediting-the-control-files”jÅ(ej»]”j½]”(Œediting the control files”Œintro_proc_control”ejÀ]”jÂ]”ujÄh_j¶jš(jÇjš(hjÆ(jÆKjÒ }”j)j»(sjÔ }”jÅ(j»(subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jÆ(j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjÆ(jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j©(j(j¸(j¬(uj_}”(Œrel”j©(Œdate”j¸(ujc}”je}”jÅ(]”j»(asjg}”(j)jÅ(j)jý(uji}”(j)ˆj)‰uj¹}”(jÅ(jÇ(jý(jÇ(ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ8Hyperlink target "intro-proc-control" is not referenced.”…””}”j¶j+)sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j()ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jÆ(Œline”KujÄjø ubajˆNj‰]”j‹NjÇjš(ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jF)sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jC)jÇjC)ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jU)jÇjC)hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jC)jÇjC)ubje)”}”(j¦Œ .. _intro_proc_process.defaults:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-process-defaults”ujÄjdjÆKj¶jC)jÇjC)hŒW/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/process.defaults.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ:file:`process.defaults`”j§]”j˜)”}”(j¦ju)j§]”j±Œprocess.defaults”…””}”(j¶jw)jÇjC)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶js)ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jp)jÇjC)hjo)jÆKubj`)”}”(j¦ŒŸProgram flow within :program:`sh_gamit` and :program:`sh_glred` is controlled by :file:`process.defaults`, shown below with annotations added for each section:”j§]”(j±ŒProgram flow within ”…””}”(j¶j)jÇjC)hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j•)jÇjC)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j)ubj±Œ and ”…””}”(j¶j)jÇjC)hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j§)jÇjC)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j)ubj±Œ is controlled by ”…””}”(j¶j)jÇjC)hNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶j¹)jÇjC)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j)ubj±Œ6, shown below with annotations added for each section:”…””}”(j¶j)jÇjC)hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjo)jÆKj¶jp)jÇjC)ubj)”}”(j¦Xñ## LOCAL DIRECTORIES # Directory for translation of raw data set rawpth = "$procdir/raw" # Directory path for raw archives (search all levels); e.g. /data18/simon set rawfnd = "" # Input files for RINEX translators set mpth = "$procdir/mkrinex" # RINEX files directory set rpth = "$procdir/rinex" # Directory path for RINEX archives (search all levels); e.g. /data18/simon set rnxfnd = "" # Broadcast orbit directory set bpth = "$procdir/brdc" # IGS files directory set ipth = "$procdir/igs" # G-files directory set gpth = "$procdir/gfiles" # GAMIT and GLOBK tables directory set tpth = "$procdir/tables" # Output directory for skyplots set gifpth = "$procdir/figs" # Globk solution directory set glbpth = "$procdir/gsoln" # Globk binary h-file directory set glfpth = "$procdir/glbf" # Directory path for other h-files (LA, LB, LC options; search all levels) # e.g. "/raid1/tah/SIO_GLL"; ( /raid6/ftp/pub/MIT_GLL/H07 /raid2/simon/gps_analysis/cgps_hfiles ) set hfnd = "" # Template files set templatepth = "$procdir/templates" # Place to store temporary control files set cpth = "$procdir/control" # Archive root directory (cannot be null) set archivepth = "$procdir/archive" ”j§]”j±Xñ## LOCAL DIRECTORIES # Directory for translation of raw data set rawpth = "$procdir/raw" # Directory path for raw archives (search all levels); e.g. /data18/simon set rawfnd = "" # Input files for RINEX translators set mpth = "$procdir/mkrinex" # RINEX files directory set rpth = "$procdir/rinex" # Directory path for RINEX archives (search all levels); e.g. /data18/simon set rnxfnd = "" # Broadcast orbit directory set bpth = "$procdir/brdc" # IGS files directory set ipth = "$procdir/igs" # G-files directory set gpth = "$procdir/gfiles" # GAMIT and GLOBK tables directory set tpth = "$procdir/tables" # Output directory for skyplots set gifpth = "$procdir/figs" # Globk solution directory set glbpth = "$procdir/gsoln" # Globk binary h-file directory set glfpth = "$procdir/glbf" # Directory path for other h-files (LA, LB, LC options; search all levels) # e.g. "/raid1/tah/SIO_GLL"; ( /raid6/ftp/pub/MIT_GLL/H07 /raid2/simon/gps_analysis/cgps_hfiles ) set hfnd = "" # Template files set templatepth = "$procdir/templates" # Place to store temporary control files set cpth = "$procdir/control" # Archive root directory (cannot be null) set archivepth = "$procdir/archive" ”…””}”j¶jÔ)sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒS/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/process.defaults”j/j0j&‰hyŒcsh”j(}”jÒKsujÄjhjo)jÆKj¶jp)jÇjC)ubj`)”}”(j¦XThis first section simply names the directories to be used for the processing. Most of the directories will be created with these names whether or not you include the entry and whether or not you actually use the directory. The only entry you are likely to change is :content:`glbpth`, for which you may want to assign successively different directory names (e.g., :file:`gsoln/`, :file:`hsoln/`, :file:`tsoln/`) if you perform parallel :program:`sh_glred` solutions using, for example, different combinations of data.”j§]”(j±X This first section simply names the directories to be used for the processing. Most of the directories will be created with these names whether or not you include the entry and whether or not you actually use the directory. The only entry you are likely to change is ”…””}”(j¶jæ)jÇjC)hNjÆNubj˜)”}”(j¦Œ:content:`glbpth`”j§]”j±Œglbpth”…””}”(j¶jî)jÇjC)hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jæ)ubj±ŒQ, for which you may want to assign successively different directory names (e.g., ”…””}”(j¶jæ)jÇjC)hNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶j*jÇjC)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæ)ubj±Œ, ”…””}”(j¶jæ)jÇjC)hNjÆNubj˜)”}”(j¦Œ:file:`hsoln/`”j§]”j±Œhsoln/”…””}”(j¶j*jÇjC)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæ)ubj±Œ, ”…””}”j¶jæ)sbj˜)”}”(j¦Œ:file:`tsoln/`”j§]”j±Œtsoln/”…””}”(j¶j+*jÇjC)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæ)ubj±Œ) if you perform parallel ”…””}”(j¶jæ)jÇjC)hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j@*jÇjC)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jæ)ubj±Œ> solutions using, for example, different combinations of data.”…””}”(j¶jæ)jÇjC)hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjo)jÆK j¶jp)jÇjC)ubj)”}”(j¦X¾##GAMIT # Set sampling interval, number of epochs, and start time for processing set sint = '30' set nepc = '2880' set stime = '0 0' # Variables for updating tables set stinf_unique = "-u" set stinf_nosort = "-nosort" set stinf_slthgt = "2.00" # Set "Y" to use RINEX header coordinates not in lfile or apr file set use_rxc = "N" # Broadcast orbits set brdc = 'brdc' # Minimum x-file size to be processed (Def. 300 blocks; most OS use 1 Kb blocks) set minxf = '300' # Set search window for RINEX files which might contain data for day - default check the previous day set rx_doy_plus = 0 set rx_doy_minus = 1 # Default globk .apr file set aprf = igb14_comb.apr # Set compress (copts), delete (dopts) and archive (aopts) options. (Don't forget to set the archivepth.) # Possible d-, c-, and a- opts: D, H, ao, ac, as, b, c, d, e, g, h, i, j, k, l, m, o, p, q, t, x, ps, all" set dopts = ( c ) set copts = ( x k ao ) set aopts = '' ”j§]”j±X¾##GAMIT # Set sampling interval, number of epochs, and start time for processing set sint = '30' set nepc = '2880' set stime = '0 0' # Variables for updating tables set stinf_unique = "-u" set stinf_nosort = "-nosort" set stinf_slthgt = "2.00" # Set "Y" to use RINEX header coordinates not in lfile or apr file set use_rxc = "N" # Broadcast orbits set brdc = 'brdc' # Minimum x-file size to be processed (Def. 300 blocks; most OS use 1 Kb blocks) set minxf = '300' # Set search window for RINEX files which might contain data for day - default check the previous day set rx_doy_plus = 0 set rx_doy_minus = 1 # Default globk .apr file set aprf = igb14_comb.apr # Set compress (copts), delete (dopts) and archive (aopts) options. (Don't forget to set the archivepth.) # Possible d-, c-, and a- opts: D, H, ao, ac, as, b, c, d, e, g, h, i, j, k, l, m, o, p, q, t, x, ps, all" set dopts = ( c ) set copts = ( x k ao ) set aopts = '' ”…””}”j¶jX*sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒS/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/process.defaults”j/j0j&‰hyŒcsh”j(}”jÒKsujÄjhjo)jÆKj¶jp)jÇjC)ubj`)”}”(j¦XÍThe session variables are set here by default but can be overridden with the :option:`-sessinfo` option on the :program:`sh_gamit` command line. They specify, respectively, the sampling interval, number of epochs (2880 is 24 hours at 30 s intervals), and the start time (hr min). The next four entries allow you to control how :file:`station.info` and the L-file are updated. They work with :file:`sites.defaults` entries and are explained in the :doc:`next section `. The :content:`rinex_ftpsites` option specifies what remote archives are to be searched for RINEX files; you may add archives of your choosing by editing :file:`~/gg/tables/ftp_info`. The minimum x-file size option allows you to exclude from GAMIT processing data from sessions too short to be useful for your application. The 300-block (300 Kb on most machines) default sets the limit at about 3 hours of tracking; change this to a small number to process short sessions. The search window options instruct :program:`sh_gamit` to look for RINEX files named with day-of-year different from the one being processed. This assures that you will not miss local data within a file named for a previous day (:content:`rx_doy_minus`), and for midnight-crossing sessions, that you will download and include IGS data from the part of the session on the following day (:content:`rx_doy_plus`). The :content:`rx_doy_minus` option may need to be increased if you have RINEX files covering many days (the GAMIT maximum is 7). Changing these to 0 will save a little time if you know that all of your data are within the expected 0–24h span. Both of these options can be specified in the :program:`sh_gamit` command line if you want to change them on a day-to-day basis.”j§]”(j±ŒMThe session variables are set here by default but can be overridden with the ”…””}”(j¶jj*jÇjC)hNjÆNubj’)”}”(j¦Œ:option:`-sessinfo`”j§]”j˜)”}”(j¦jt*j§]”j±Œ -sessinfo”…””}”(j¶jv*jÇjC)hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jr*ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j€*Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -sessinfo”ujÄj‘hjo)jÆKj¶jj*ubj±Œ option on the ”…””}”(j¶jj*jÇjC)hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j–*jÇjC)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jj*ubj±ŒÅ command line. They specify, respectively, the sampling interval, number of epochs (2880 is 24 hours at 30 s intervals), and the start time (hr min). The next four entries allow you to control how ”…””}”(j¶jj*jÇjC)hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j¨*jÇjC)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jj*ubj±Œ, and the L-file are updated. They work with ”…””}”(j¶jj*jÇjC)hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶j½*jÇjC)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jj*ubj±Œ" entries and are explained in the ”…””}”(j¶jj*jÇjC)hNjÆNubj’)”}”(j¦Œ$:doc:`next section `”j§]”j)”}”(j¦jÔ*j§]”j±Œ next section”…””}”(j¶jÖ*jÇjC)hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶jÒ*ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jà*Œreftype”Œdoc”Œ refexplicit”ˆŒrefwarn”ˆj¶Œsites.defaults”ujÄj‘hjo)jÆKj¶jj*ubj±Œ. The ”…””}”(j¶jj*jÇjC)hNjÆNubj˜)”}”(j¦Œ:content:`rinex_ftpsites`”j§]”j±Œrinex_ftpsites”…””}”(j¶jö*jÇjC)hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jj*ubj±Œ| option specifies what remote archives are to be searched for RINEX files; you may add archives of your choosing by editing ”…””}”(j¶jj*jÇjC)hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/ftp_info`”j§]”j±Œ~/gg/tables/ftp_info”…””}”(j¶j +jÇjC)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jj*ubj±XF. The minimum x-file size option allows you to exclude from GAMIT processing data from sessions too short to be useful for your application. The 300-block (300 Kb on most machines) default sets the limit at about 3 hours of tracking; change this to a small number to process short sessions. The search window options instruct ”…””}”(j¶jj*jÇjC)hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j+jÇjC)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jj*ubj±Œ¯ to look for RINEX files named with day-of-year different from the one being processed. This assures that you will not miss local data within a file named for a previous day (”…””}”(j¶jj*jÇjC)hNjÆNubj˜)”}”(j¦Œ:content:`rx_doy_minus`”j§]”j±Œ rx_doy_minus”…””}”(j¶j0+jÇjC)hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jj*ubj±Œ†), and for midnight-crossing sessions, that you will download and include IGS data from the part of the session on the following day (”…””}”(j¶jj*jÇjC)hNjÆNubj˜)”}”(j¦Œ:content:`rx_doy_plus`”j§]”j±Œ rx_doy_plus”…””}”(j¶jC+jÇjC)hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jj*ubj±Œ). The ”…””}”(j¶jj*jÇjC)hNjÆNubj˜)”}”(j¦Œ:content:`rx_doy_minus`”j§]”j±Œ rx_doy_minus”…””}”(j¶jV+jÇjC)hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jj*ubj±X option may need to be increased if you have RINEX files covering many days (the GAMIT maximum is 7). Changing these to 0 will save a little time if you know that all of your data are within the expected 0–24h span. Both of these options can be specified in the ”…””}”(j¶jj*jÇjC)hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶ji+jÇjC)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jj*ubj±Œ? command line if you want to change them on a day-to-day basis.”…””}”(j¶jj*jÇjC)hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjo)jÆKj¶jp)jÇjC)ubj)”}”(j¦Œü## RESOURCES # Minimum raw disk space in Mbytes set minraw = '100' # Minimum rinex disk space in Mbytes set minrinex = '100' # Minimum archive disk space in Mbytes set minarchive = '100' # Minimum working disk space in Mbytes set minwork = '500' ”j§]”j±Œü## RESOURCES # Minimum raw disk space in Mbytes set minraw = '100' # Minimum rinex disk space in Mbytes set minrinex = '100' # Minimum archive disk space in Mbytes set minarchive = '100' # Minimum working disk space in Mbytes set minwork = '500' ”…””}”j¶j+sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒS/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/process.defaults”j/j0j&‰hyŒcsh”j(}”jÒKsujÄjhjo)jÆK#j¶jp)jÇjC)ubj`)”}”(j¦ŒhThe resource settings prevent processing from starting if there is inadequate disk space to complete it.”j§]”j±ŒhThe resource settings prevent processing from starting if there is inadequate disk space to complete it.”…””}”(j¶j“+jÇjC)hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjo)jÆK'j¶jp)jÇjC)ubj)”}”(j¦XË## SYSTEM-DEPENDENT SETTINGS # UNIX df command must be set to return the correct form # Most machines ( set udf = 'df -mk' # but note that if you have free > 1 Tb, you will need to change this to Mb # set udf = 'df -m' # HP # set udf = 'bdf' # UNIX mail command # Most machines set umail = 'mail -s' # HP # set umail = 'mailx -s' # Mail address for sending the processing report (if '' will default to `whoami` in sh_gamit) set mailto = '' # Host name for email and anonymous ftp password use (if '' will default to `hostname` in sh_gamit) set machine = '' # Ghostscript path set gspath = '/usr/bin' # ImageMagick path fir png conversion # set impath = '/usr/bin/X11' set impath = '/usr/bin' ”j§]”j±XË## SYSTEM-DEPENDENT SETTINGS # UNIX df command must be set to return the correct form # Most machines ( set udf = 'df -mk' # but note that if you have free > 1 Tb, you will need to change this to Mb # set udf = 'df -m' # HP # set udf = 'bdf' # UNIX mail command # Most machines set umail = 'mail -s' # HP # set umail = 'mailx -s' # Mail address for sending the processing report (if '' will default to `whoami` in sh_gamit) set mailto = '' # Host name for email and anonymous ftp password use (if '' will default to `hostname` in sh_gamit) set machine = '' # Ghostscript path set gspath = '/usr/bin' # ImageMagick path fir png conversion # set impath = '/usr/bin/X11' set impath = '/usr/bin' ”…””}”j¶j¡+sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒS/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/process.defaults”j/j0j&‰hyŒcsh”j(}”jÒKsujÄjhjo)jÆK)j¶jp)jÇjC)ubj`)”}”(j¦XjThe only system-dependent setting likely to need changing is the path for the :program:`convert` program, used to convert the sky plots from PostScript to PNG. If your UNIX installation does not have :program:`convert` available, use :option:`-nopngs` in the :program:`sh_gamit` command line so that the sky plots will be left as PostScript in the day directory.”j§]”(j±ŒNThe only system-dependent setting likely to need changing is the path for the ”…””}”(j¶j³+jÇjC)hNjÆNubjj)”}”(j¦Œ:program:`convert`”j§]”j±Œconvert”…””}”(j¶j»+jÇjC)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j³+ubj±Œh program, used to convert the sky plots from PostScript to PNG. If your UNIX installation does not have ”…””}”(j¶j³+jÇjC)hNjÆNubjj)”}”(j¦Œ:program:`convert`”j§]”j±Œconvert”…””}”(j¶jÍ+jÇjC)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j³+ubj±Œ available, use ”…””}”(j¶j³+jÇjC)hNjÆNubj’)”}”(j¦Œ:option:`-nopngs`”j§]”j˜)”}”(j¦já+j§]”j±Œ-nopngs”…””}”(j¶jã+jÇjC)hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jß+ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jí+Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-nopngs”ujÄj‘hjo)jÆK-j¶j³+ubj±Œ in the ”…””}”(j¶j³+jÇjC)hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j,jÇjC)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j³+ubj±ŒT command line so that the sky plots will be left as PostScript in the day directory.”…””}”(j¶j³+jÇjC)hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjo)jÆK-j¶jp)jÇjC)ubej·}”(j¹]”(Œprocess-defaults”jn)ej»]”j½]”(Œprocess.defaults”Œintro_proc_process.defaults”ejÀ]”jÂ]”ujÄh_j¶jC)jÇjC)hjo)jÆKjÒ }”j!,jd)sjÔ }”jn)jd)subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jo)j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjo)jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jR)jF)ja)jU)uj_}”(Œrel”jR)Œdate”ja)ujc}”je}”jn)]”jd)asjg}”(j!,jn)j ,j,uji}”(j!,ˆj ,‰uj¹}”(jn)jp)j,jp)ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±ŒAHyperlink target "intro-proc-process-defaults" is not referenced.”…””}”j¶jK,sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jH,ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jo)Œline”KujÄjø ubajˆNj‰]”j‹NjÇjC)ubjòj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jf,sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jc,jÇjc,ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶ju,jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jc,jÇjc,ubje)”}”(j¦Œ.. _intro_proc_sestbl.:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-sestbl”ujÄjdjÆKj¶jc,jÇjc,hŒM/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sestbl.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ:file:`sestbl.`”j§]”j˜)”}”(j¦j•,j§]”j±Œsestbl.”…””}”(j¶j—,jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j“,ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j,jÇjc,hj,jÆKubj`)”}”(j¦XŠThe processing within GAMIT itself (:program:`arc`, :program:`model`, :program:`autcln`, :program:`solve`) is controlled by :file:`sestbl.`, :file:`sittbl.`, and :file:`autcln.cmd`. The :file:`sestbl.` entries that you are likely to consider in setting up your processing are shown below. The values are generally appropriate for regional or global processing for most data acquired after 1995.”j§]”(j±Œ$The processing within GAMIT itself (”…””}”(j¶j­,jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`arc`”j§]”j±Œarc”…””}”(j¶jµ,jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j­,ubj±Œ, ”…””}”(j¶j­,jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶jÇ,jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j­,ubj±Œ, ”…””}”j¶j­,sbjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jÙ,jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j­,ubj±Œ, ”…””}”j¶j­,sbjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶jë,jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j­,ubj±Œ) is controlled by ”…””}”(j¶j­,jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jý,jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­,ubj±Œ, ”…””}”j¶j­,sbj˜)”}”(j¦Œ:file:`sittbl.`”j§]”j±Œsittbl.”…””}”(j¶j-jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­,ubj±Œ, and ”…””}”(j¶j­,jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`autcln.cmd`”j§]”j±Œ autcln.cmd”…””}”(j¶j'-jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­,ubj±Œ. The ”…””}”(j¶j­,jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶j<-jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­,ubj±ŒÁ entries that you are likely to consider in setting up your processing are shown below. The values are generally appropriate for regional or global processing for most data acquired after 1995.”…””}”(j¶j­,jÇjc,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj,jÆKj¶j,jÇjc,ubj)”}”(j¦XùChoice of Experiment = BASELINE ; BASELINE/RELAX./ORBIT Satellite Constraint = Y ; Y/N (next two lines are read and free-format. only all needed on next line) all a e i n w M D Y B 1UDC 1UDS 1UYC 1UYC 1UBC 1UBS 2UC 2US 4UC 4US SX SY SZ 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.001 0.001 0.001 ”j§]”j±XùChoice of Experiment = BASELINE ; BASELINE/RELAX./ORBIT Satellite Constraint = Y ; Y/N (next two lines are read and free-format. only all needed on next line) all a e i n w M D Y B 1UDC 1UDS 1UYC 1UYC 1UBC 1UBS 2UC 2US 4UC 4US SX SY SZ 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.01 0.001 0.001 0.001 ”…””}”j¶jW-sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒJ/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sestbl.”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhj,jÆK j¶j,jÇjc,ubj`)”}”(j¦XbBy setting :content:`Choice of experiment = BASELINE`, you are fixing the orbits and omitting the orbital parameters from your GAMIT processing and output h-files. If you intend to combine your h-files with those from global processing at, e.g., MIT or SOPAC, or if you are processing a GNSS with poor orbits, then you should set :content:`Choice of experiment = RELAX` and apply constraints to the orbital parameters. The values given for orbital parameters (1 part in :math:`10^9` or about 2 cm) are reasonable for current IGS orbits (see http://acc.igs.org/igsacc_final.html for orbital accuracy over time).”j§]”(j±Œ By setting ”…””}”(j¶ji-jÇjc,hNjÆNubj˜)”}”(j¦Œ*:content:`Choice of experiment = BASELINE`”j§]”j±ŒChoice of experiment = BASELINE”…””}”(j¶jq-jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶ji-ubj±X, you are fixing the orbits and omitting the orbital parameters from your GAMIT processing and output h-files. If you intend to combine your h-files with those from global processing at, e.g., MIT or SOPAC, or if you are processing a GNSS with poor orbits, then you should set ”…””}”(j¶ji-jÇjc,hNjÆNubj˜)”}”(j¦Œ':content:`Choice of experiment = RELAX`”j§]”j±ŒChoice of experiment = RELAX”…””}”(j¶j„-jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶ji-ubj±Œe and apply constraints to the orbital parameters. The values given for orbital parameters (1 part in ”…””}”(j¶ji-jÇjc,hNjÆNubjO )”}”(j¦Œ :math:`10^9`”j§]”j±Œ10^9”…””}”(j¶j—-jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶ji-ubj±Œ; or about 2 cm) are reasonable for current IGS orbits (see ”…””}”(j¶ji-jÇjc,hNjÆNubj÷ )”}”(j¦Œ$http://acc.igs.org/igsacc_final.html”j§]”j±Œ$http://acc.igs.org/igsacc_final.html”…””}”(j¶j©-jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j«-ujÄjö j¶ji-ubj±Œ! for orbital accuracy over time).”…””}”(j¶ji-jÇjc,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj,jÆKj¶j,jÇjc,ubj)”}”(j¦XtChoice of Observable = LC_AUTCLN ; L1_SINGLE/L1&L2/L1_ONLY/L2_ONLY/LC_ONLY/ ; L1,L2_INDEPEND./LC_HELP/LC_AUTCLN Ambiguity resolution WL = 0.15 0.15 1000. 99. 15000. ; used for LC_HELP only Ambiguity resolution NL = 0.15 0.15 1000. 99. 15000. ; Allow long baselines with LC_AUTCLN Ionospheric Constraints = 0.0 mm + 8.00 ppm ”j§]”j±XtChoice of Observable = LC_AUTCLN ; L1_SINGLE/L1&L2/L1_ONLY/L2_ONLY/LC_ONLY/ ; L1,L2_INDEPEND./LC_HELP/LC_AUTCLN Ambiguity resolution WL = 0.15 0.15 1000. 99. 15000. ; used for LC_HELP only Ambiguity resolution NL = 0.15 0.15 1000. 99. 15000. ; Allow long baselines with LC_AUTCLN Ionospheric Constraints = 0.0 mm + 8.00 ppm ”…””}”j¶jÂ-sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒJ/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sestbl.”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhj,jÆKj¶j,jÇjc,ubj`)”}”(j¦X2The next four entries control the observations used and ambiguity resolution. :content:`LC_AUTCLN` and :content:`LC_HELP` are the usual choices with dual-frequency receivers and all but the shortest baselines. With the :content:`LC_AUTCLN` option, the widelane ambiguities are assigned and resolved in :program:`autcln` using the pseudoranges. With :content:`LC_HELP`, the wide-lane ambiguities are resolved by applying an ionospheric constraint (see :cite:t:`Dong_et_al_1998`). For data acquired with codeless receivers (before ~ 1994), :content:`LC_HELP` should be used. The sensitivity parameters for both wide-lane (with :content:`LC_HELP`) and narrow-lane ambiguities are set conservatively but may be varied if you need to squeeze greater accuracy out of short observing sessions. See :cite:t:`Dong_et_al_1998` and Section 3.5 of the `GAMIT Reference Manual `_ for a detailed discussion. For baselines less than a few km, using L1 and L2 independently or only L1 may reduce noise compared to using the ionosphere-free combination. To check for the size of ionospheric errors, it’s wise to try :content:`LC_HELP`, :content:`L1_ONLY`, :content:`L2_ONLY`, and :content:`L1,L2_INDEP` and compare the results. If your data were acquired with a single-frequency receiver, you should set :content:`L1_RECEIVER` in :file:`sestbl.` and also add the :content:`L1only` command to :file:`autcln.cmd` since :program:`autcln` by default will attempt to use both L1 and L2 in cleaning (even if :content:`L1_ONLY` is requested for :program:`solve`).”j§]”(j±ŒNThe next four entries control the observations used and ambiguity resolution. ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`LC_AUTCLN`”j§]”j±Œ LC_AUTCLN”…””}”(j¶jÜ-jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œ and ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`LC_HELP`”j§]”j±ŒLC_HELP”…””}”(j¶jï-jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œb are the usual choices with dual-frequency receivers and all but the shortest baselines. With the ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`LC_AUTCLN`”j§]”j±Œ LC_AUTCLN”…””}”(j¶j.jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œ? option, the widelane ambiguities are assigned and resolved in ”…””}”(j¶jÔ-jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j.jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÔ-ubj±Œ using the pseudoranges. With ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`LC_HELP`”j§]”j±ŒLC_HELP”…””}”(j¶j'.jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±ŒT, the wide-lane ambiguities are resolved by applying an ionospheric constraint (see ”…””}”(j¶jÔ-jÇjc,hNjÆNubj’)”}”(j¦Œ:cite:t:`Dong_et_al_1998`”j§]”j)”}”(j¦j<.j§]”j±ŒDong_et_al_1998”…””}”(j¶j>.jÇjc,hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j:.ubaj·}”(j¹]”Œid1”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jòŒ refdomain”jH.Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒDong_et_al_1998”ujÄj‘hj,jÆKj¶jÔ-ubj±Œ>). For data acquired with codeless receivers (before ~ 1994), ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`LC_HELP`”j§]”j±ŒLC_HELP”…””}”(j¶j^.jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±ŒE should be used. The sensitivity parameters for both wide-lane (with ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`LC_HELP`”j§]”j±ŒLC_HELP”…””}”(j¶jq.jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œ”) and narrow-lane ambiguities are set conservatively but may be varied if you need to squeeze greater accuracy out of short observing sessions. See ”…””}”(j¶jÔ-jÇjc,hNjÆNubj’)”}”(j¦Œ:cite:t:`Dong_et_al_1998`”j§]”j)”}”(j¦j†.j§]”j±ŒDong_et_al_1998”…””}”(j¶jˆ.jÇjc,hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j„.ubaj·}”(j¹]”Œid2”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jòŒ refdomain”j’.Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒDong_et_al_1998”ujÄj‘hj,jÆKj¶jÔ-ubj±Œ and Section 3.5 of the ”…””}”(j¶jÔ-jÇjc,hNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j¨.jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶jÔ-ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit-reference-manual”aj»]”j½]”Œgamit reference manual”ajÀ]”jÂ]”Œrefuri”j¸.ujÄjdj Kj¶jÔ-ubj±Œë for a detailed discussion. For baselines less than a few km, using L1 and L2 independently or only L1 may reduce noise compared to using the ionosphere-free combination. To check for the size of ionospheric errors, it’s wise to try ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`LC_HELP`”j§]”j±ŒLC_HELP”…””}”(j¶jÊ.jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œ, ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`L1_ONLY`”j§]”j±ŒL1_ONLY”…””}”(j¶jÝ.jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œ, ”…””}”j¶jÔ-sbj˜)”}”(j¦Œ:content:`L2_ONLY`”j§]”j±ŒL2_ONLY”…””}”(j¶jð.jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œ, and ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`L1,L2_INDEP`”j§]”j±Œ L1,L2_INDEP”…””}”(j¶j/jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œf and compare the results. If your data were acquired with a single-frequency receiver, you should set ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`L1_RECEIVER`”j§]”j±Œ L1_RECEIVER”…””}”(j¶j/jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œ in ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶j)/jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÔ-ubj±Œ and also add the ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`L1only`”j§]”j±ŒL1only”…””}”(j¶j>/jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œ command to ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`autcln.cmd`”j§]”j±Œ autcln.cmd”…””}”(j¶jQ/jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÔ-ubj±Œ since ”…””}”(j¶jÔ-jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jf/jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÔ-ubj±ŒD by default will attempt to use both L1 and L2 in cleaning (even if ”…””}”(j¶jÔ-jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`L1_ONLY`”j§]”j±ŒL1_ONLY”…””}”(j¶jx/jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÔ-ubj±Œ is requested for ”…””}”(j¶jÔ-jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j‹/jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÔ-ubj±Œ).”…””}”(j¶jÔ-jÇjc,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj,jÆKj¶j,jÇjc,ubj)”}”(j¦XHDMap = GMF ; GMF(default)/NMFH/VMF1 WMap = GMF ; GMF(default)/NMFW/VMF1 Use map.grid = Y ; VMF1 grid file with mapping functions and ZHD Met obs source = UFL GPT 50 ; hierarchical list: RNX ufile GPT/STP [humid value]; default GTP 50 if [humid value] < 0, use RNX or UFL if available Zenith Delay Estimation = Y ; Yes/No (default No) Interval zen = 2 ; 2 hrs = 13 knots/day (default is 1 ZD per day) Zenith Variation = 0.02 100. ; zenith-delay variation, tau in meters/sqrt(hr), hrs (default .02 100.) Elevation Cutoff = 0 ; default 0 to use value in autcln.cmd Atmospheric gradients = Y ; Yes/Np (default No) Number gradients = 2 ; number of gradient parameters per day (NS or ES); default 1 Gradient Constraints = 0.03 ; gradient at 10 deg elevation in meters; default 0.03 m Gradient Variation = .01 100 ; gradient variation Output met = N ; write the a priori met values to a z-file (Y/N) ”j§]”j±XHDMap = GMF ; GMF(default)/NMFH/VMF1 WMap = GMF ; GMF(default)/NMFW/VMF1 Use map.grid = Y ; VMF1 grid file with mapping functions and ZHD Met obs source = UFL GPT 50 ; hierarchical list: RNX ufile GPT/STP [humid value]; default GTP 50 if [humid value] < 0, use RNX or UFL if available Zenith Delay Estimation = Y ; Yes/No (default No) Interval zen = 2 ; 2 hrs = 13 knots/day (default is 1 ZD per day) Zenith Variation = 0.02 100. ; zenith-delay variation, tau in meters/sqrt(hr), hrs (default .02 100.) Elevation Cutoff = 0 ; default 0 to use value in autcln.cmd Atmospheric gradients = Y ; Yes/Np (default No) Number gradients = 2 ; number of gradient parameters per day (NS or ES); default 1 Gradient Constraints = 0.03 ; gradient at 10 deg elevation in meters; default 0.03 m Gradient Variation = .01 100 ; gradient variation Output met = N ; write the a priori met values to a z-file (Y/N) ”…””}”j¶j£/sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒJ/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sestbl.”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhj,jÆK!j¶j,jÇjc,ubj`)”}”(j¦Xu The next block of entries controls the modeling and estimation of the atmospheric delay. The first command specifies the mapping function to be used to project the zenith delay to the elevation angle of the satellites. Different functions must be used for the hydrostatic ("dry") delay and the "wet" delay due to water vapor. The default, sufficient for all but the most accurate studies of heights and for meteorological studies, is the "global mapping function" (GMF) developed by :cite:t:`Boehm_et_al_2006b` from fitting numerical weather model (NWM) data over 20 years. A more accurate reconstruction of the NWM data can be obtained by interpolating hydrostatic and wet mapping function coefficients as a function of time and location from the (large) global grid files compiled by the Vienna group :cite:p:`Boehm_et_al_2006a`. You have access to these values by downloading the VMF1 grid files for each year from ftp://everest.mit.edu/pub/GRIDS/, and setting :content:`Use map.grid = Y`, :content:`DMap = VMF1` and :content:`WMap = VMF1`. The next command controls the source of pressure (most importantly, but also temperature) for the *a priori* zenith hydrostatic delay (ZHD). The most accurate values, if they are available, are from local measurements of surface pressure, which can be written into RINEX met files and stored in a :file:`met/` directory for use by :program:`sh_gamit`. Setting the first option of :content:`Met obs source = RNX` tells GAMIT to use these for any station for which they are available. The next most accurate source would be the ZHD values from the VMF1 grid files. Since GAMIT reads the grid file for all sites used for the day and writes the values into the U-file, you select this option by setting :content:`Met obs source = UFL` and :content:`map.grid = Y`. (If you use a VMF1 station-list file, :file:`map.list`, the second option, :content:`GPT` or :content:`UFL` can be used for stations missing from the list file. Since the only source of NWM ZHD data currently tabulated for GAMIT is the VMF1 mapping-function grids, the :file:`met.grid` and :file:`met.list` files are not yet supported.) Finally, as with the mapping functions, the Vienna group has constructed from the NWM data an analytical model, designated "global pressure and temperature" (GPT2), of :cite:t:`Lagler_et_al_2013`. It reads from table :file:`gpt.grid` in :file:`~/gg/tables/` values of zenith hydrotstatic delay (ZHD), temperature, lapse rate, and dry and wet mapping functions as a function of latitude, longitude, and day-of-year that are averages from a fit to 10-year monthly averages from a global numerical weather model. The option STP implies standard constants (1013.25 hPa, 20°C), used prior to Release 10.3 but now effectively obsolete. To keep errors in height estimates below 2 mm, you need an accuracy of about 10 hPa in *a priori* pressure [Tregoning and Herring, 2006]. The :content:`Interval zen` command controls the number of zenith delay parameters estimated using the session. For geodetic studies, estimating values at 2-hour intervals with the constraints given is more than adequate. For meteorological studies, you may want to estimate more parameters and/or alter the constraints (see Chapter 7 of the `GAMIT Reference Manual `_). For atmospheric gradients, we allow a linear change during the session (two parameters each for N/S and E/W gradients).”j§]”(j±XïThe next block of entries controls the modeling and estimation of the atmospheric delay. The first command specifies the mapping function to be used to project the zenith delay to the elevation angle of the satellites. Different functions must be used for the hydrostatic (“dryâ€) delay and the “wet†delay due to water vapor. The default, sufficient for all but the most accurate studies of heights and for meteorological studies, is the “global mapping function†(GMF) developed by ”…””}”(j¶jµ/jÇjc,hNjÆNubj’)”}”(j¦Œ:cite:t:`Boehm_et_al_2006b`”j§]”j)”}”(j¦j¿/j§]”j±ŒBoehm_et_al_2006b”…””}”(j¶jÁ/jÇjc,hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j½/ubaj·}”(j¹]”Œid3”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jòŒ refdomain”jË/Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒBoehm_et_al_2006b”ujÄj‘hj,jÆK%j¶jµ/ubj±X% from fitting numerical weather model (NWM) data over 20 years. A more accurate reconstruction of the NWM data can be obtained by interpolating hydrostatic and wet mapping function coefficients as a function of time and location from the (large) global grid files compiled by the Vienna group ”…””}”(j¶jµ/jÇjc,hNjÆNubj’)”}”(j¦Œ:cite:p:`Boehm_et_al_2006a`”j§]”j)”}”(j¦jã/j§]”j±ŒBoehm_et_al_2006a”…””}”(j¶jå/jÇjc,hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-p”ej½]”jÀ]”jÂ]”ujÄj*j¶já/ubaj·}”(j¹]”Œid4”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jòŒ refdomain”jï/Œreftype”j-Œ refexplicit”‰Œrefwarn”‰j¶ŒBoehm_et_al_2006a”ujÄj‘hj,jÆK%j¶jµ/ubj±ŒX. You have access to these values by downloading the VMF1 grid files for each year from ”…””}”(j¶jµ/jÇjc,hNjÆNubj÷ )”}”(j¦Œ ftp://everest.mit.edu/pub/GRIDS/”j§]”j±Œ ftp://everest.mit.edu/pub/GRIDS/”…””}”(j¶j0jÇjc,hNjÆNubaj·}”(j¹•2]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j0ujÄjö j¶jµ/ubj±Œ, and setting ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`Use map.grid = Y`”j§]”j±ŒUse map.grid = Y”…””}”(j¶j0jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jµ/ubj±Œ, ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`DMap = VMF1`”j§]”j±Œ DMap = VMF1”…””}”(j¶j+0jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jµ/ubj±Œ and ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`WMap = VMF1`”j§]”j±Œ WMap = VMF1”…””}”(j¶j>0jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jµ/ubj±Œd. The next command controls the source of pressure (most importantly, but also temperature) for the ”…””}”(j¶jµ/jÇjc,hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jQ0jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jµ/ubj±Œ½ zenith hydrostatic delay (ZHD). The most accurate values, if they are available, are from local measurements of surface pressure, which can be written into RINEX met files and stored in a ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ :file:`met/`”j§]”j±Œmet/”…””}”(j¶jc0jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jµ/ubj±Œ directory for use by ”…””}”(j¶jµ/jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jx0jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jµ/ubj±Œ. Setting the first option of ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`Met obs source = RNX`”j§]”j±ŒMet obs source = RNX”…””}”(j¶jŠ0jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jµ/ubj±X  tells GAMIT to use these for any station for which they are available. The next most accurate source would be the ZHD values from the VMF1 grid files. Since GAMIT reads the grid file for all sites used for the day and writes the values into the U-file, you select this option by setting ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`Met obs source = UFL`”j§]”j±ŒMet obs source = UFL”…””}”(j¶j0jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jµ/ubj±Œ and ”…””}”j¶jµ/sbj˜)”}”(j¦Œ:content:`map.grid = Y`”j§]”j±Œ map.grid = Y”…””}”(j¶j°0jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jµ/ubj±Œ(. (If you use a VMF1 station-list file, ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`map.list`”j§]”j±Œmap.list”…””}”(j¶jÃ0jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jµ/ubj±Œ, the second option, ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`GPT`”j§]”j±ŒGPT”…””}”(j¶jØ0jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jµ/ubj±Œ or ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`UFL`”j§]”j±ŒUFL”…””}”(j¶jë0jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jµ/ubj±Œ¢ can be used for stations missing from the list file. Since the only source of NWM ZHD data currently tabulated for GAMIT is the VMF1 mapping-function grids, the ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`met.grid`”j§]”j±Œmet.grid”…””}”(j¶jþ0jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jµ/ubj±Œ and ”…””}”j¶jµ/sbj˜)”}”(j¦Œ:file:`met.list`”j§]”j±Œmet.list”…””}”(j¶j1jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jµ/ubj±ŒË files are not yet supported.) Finally, as with the mapping functions, the Vienna group has constructed from the NWM data an analytical model, designated “global pressure and temperature†(GPT2), of ”…””}”(j¶jµ/jÇjc,hNjÆNubj’)”}”(j¦Œ:cite:t:`Lagler_et_al_2013`”j§]”j)”}”(j¦j*1j§]”j±ŒLagler_et_al_2013”…””}”(j¶j,1jÇjc,hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j(1ubaj·}”(j¹]”Œid5”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jòŒ refdomain”j61Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒLagler_et_al_2013”ujÄj‘hj,jÆK%j¶jµ/ubj±Œ. It reads from table ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`gpt.grid`”j§]”j±Œgpt.grid”…””}”(j¶jL1jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jµ/ubj±Œ in ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶ja1jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jµ/ubj±XÍ values of zenith hydrotstatic delay (ZHD), temperature, lapse rate, and dry and wet mapping functions as a function of latitude, longitude, and day-of-year that are averages from a fit to 10-year monthly averages from a global numerical weather model. The option STP implies standard constants (1013.25 hPa, 20°C), used prior to Release 10.3 but now effectively obsolete. To keep errors in height estimates below 2 mm, you need an accuracy of about 10 hPa in ”…””}”(j¶jµ/jÇjc,hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jv1jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jµ/ubj±Œ- pressure [Tregoning and Herring, 2006]. The ”…””}”(j¶jµ/jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`Interval zen`”j§]”j±Œ Interval zen”…””}”(j¶jˆ1jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jµ/ubj±X; command controls the number of zenith delay parameters estimated using the session. For geodetic studies, estimating values at 2-hour intervals with the constraints given is more than adequate. For meteorological studies, you may want to estimate more parameters and/or alter the constraints (see Chapter 7 of the ”…””}”(j¶jµ/jÇjc,hNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j›1jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶jµ/ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œid6”aj»]”j½]”jÀ]”Œgamit reference manual”ajÂ]”Œrefuri”j«1ujÄjdj Kj¶jµ/ubj±Œz). For atmospheric gradients, we allow a linear change during the session (two parameters each for N/S and E/W gradients).”…””}”(j¶jµ/jÇjc,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj,jÆK%j¶j,jÇjc,ubj)”}”(j¦ŒKUpdate T/L files = L_ONLY ; T_AND_L (default), T_ONLY, L_ONLY, NONE ”j§]”j±ŒKUpdate T/L files = L_ONLY ; T_AND_L (default), T_ONLY, L_ONLY, NONE ”…””}”j¶jÃ1sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒJ/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sestbl.”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhj,jÆK;j¶j,jÇjc,ubj`)”}”(j¦X?The command to update the L-file assures that the second :program:`solve` solution will have adjustments within a linear range and allows :program:`sh_gamit` to apply updated coordinates to the processing of successive days. The criterion for updating is set by default to be adjustments larger than 30 cm (though this can be changed with a :file:`sestbl.` command, not shown). If you know that all of your *a priori* coordinates are accurate to within a few cm and don't want bad data to corrupt the coordinates in the L-file, you can set :content:`Update T/L files = NONE`.”j§]”(j±Œ9The command to update the L-file assures that the second ”…””}”(j¶jÕ1jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶jÝ1jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÕ1ubj±ŒA solution will have adjustments within a linear range and allows ”…””}”(j¶jÕ1jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jï1jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÕ1ubj±Œ¸ to apply updated coordinates to the processing of successive days. The criterion for updating is set by default to be adjustments larger than 30 cm (though this can be changed with a ”…””}”(j¶jÕ1jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶j2jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÕ1ubj±Œ3 command, not shown). If you know that all of your ”…””}”(j¶jÕ1jÇjc,hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j2jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jÕ1ubj±Œ} coordinates are accurate to within a few cm and don’t want bad data to corrupt the coordinates in the L-file, you can set ”…””}”(j¶jÕ1jÇjc,hNjÆNubj˜)”}”(j¦Œ":content:`Update T/L files = NONE`”j§]”j±ŒUpdate T/L files = NONE”…””}”(j¶j(2jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÕ1ubj±Œ.”…””}”(j¶jÕ1jÇjc,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj,jÆK?j¶j,jÇjc,ubj)”}”(j¦ŒµAUTCLN Command File = autcln.cmd ; Filename; default none (use default options) Station Error = ELEVATION 10 5 ; 1-way L1, a**2 + (b**2)(L**2) in mm, ppm, default = 10. 0. ”j§]”j±ŒµAUTCLN Command File = autcln.cmd ; Filename; default none (use default options) Station Error = ELEVATION 10 5 ; 1-way L1, a**2 + (b**2)(L**2) in mm, ppm, default = 10. 0. ”…””}”j¶jA2sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒJ/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sestbl.”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhj,jÆKCj¶j,jÇjc,ubj`)”}”(j¦XYThe next two commands control how the phase data are weighted in the preliminary and final solutions. The :content:`Station Error` entry shown tells :program:`solve` to use elevation-dependent weighting for the phase date. In the preliminary solution, the assigned error is 10 mm with negligible elevation dependence. With :content:`AUTCLN postfit = Y` (default with :content:`Type of analysis = 1-ITER`) the second :program:`solve` run will assign weights to the phase data based on the actual scatter computed by :program:`autcln` in its "postfit" edit, and will contain both a constant and an elevation-dependent term, as recorded in the output print file :file:`autcln.post.sum`. Elevation-dependent weighting is recommended for almost all analyses; an exception might be tests of models (e.g. mapping functions) sensitive to low-elevation observations.”j§]”(j±ŒjThe next two commands control how the phase data are weighted in the preliminary and final solutions. The ”…””}”(j¶jS2jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`Station Error`”j§]”j±Œ Station Error”…””}”(j¶j[2jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jS2ubj±Œ entry shown tells ”…””}”(j¶jS2jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶jn2jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jS2ubj±Œž to use elevation-dependent weighting for the phase date. In the preliminary solution, the assigned error is 10 mm with negligible elevation dependence. With ”…””}”(j¶jS2jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`AUTCLN postfit = Y`”j§]”j±ŒAUTCLN postfit = Y”…””}”(j¶j€2jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jS2ubj±Œ (default with ”…””}”(j¶jS2jÇjc,hNjÆNubj˜)”}”(j¦Œ$:content:`Type of analysis = 1-ITER`”j§]”j±ŒType of analysis = 1-ITER”…””}”(j¶j“2jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jS2ubj±Œ ) the second ”…””}”(j¶jS2jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j¦2jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jS2ubj±ŒS run will assign weights to the phase data based on the actual scatter computed by ”…””}”(j¶jS2jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j¸2jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jS2ubj±Œƒ in its “postfit†edit, and will contain both a constant and an elevation-dependent term, as recorded in the output print file ”…””}”(j¶jS2jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum`”j§]”j±Œautcln.post.sum”…””}”(j¶jÊ2jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jS2ubj±Œ¯. Elevation-dependent weighting is recommended for almost all analyses; an exception might be tests of models (e.g. mapping functions) sensitive to low-elevation observations.”…””}”(j¶jS2jÇjc,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj,jÆKGj¶j,jÇjc,ubj)”}”(j¦ŒöDecimation Factor = 4 ; FOR SOLVE, default = 1 Quick-pre observable = LC_ONLY ; for 1st soln, default same as Choice of observable Quick-pre decimation factor = 10 ; 1st iter or autcln pre, default same as Decimation Factor ”j§]”j±ŒöDecimation Factor = 4 ; FOR SOLVE, default = 1 Quick-pre observable = LC_ONLY ; for 1st soln, default same as Choice of observable Quick-pre decimation factor = 10 ; 1st iter or autcln pre, default same as Decimation Factor ”…””}”j¶jå2sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒJ/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sestbl.”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhj,jÆKNj¶j,jÇjc,ubj`)”}”(j¦XRelated to the error weighting is the sampling of data for the solution. For cleaning purposes (:program:`model`, :program:`autcln`), the full sampling of the x-file (usually 30 s or 15 s) is used. However, since the phase errors are correlated over many minutes, it is not necessary to use sampling this frequent in :program:`solve`. The default decimation factor (:content:`4`, resulting in 2-minute sampling for the usual case) provides formal uncertainties that are usually reasonable within a factor of two while reducing time significantly. (See the discussion of uncertainties in :numref:`intro_gnss_solve`.) For the preliminary solution used to get decimeter-level coordinates for editing and to avoid non-linearity in the final adjustments, 5-minute sampling is sufficient.”j§]”(j±Œ`Related to the error weighting is the sampling of data for the solution. For cleaning purposes (”…””}”(j¶j÷2jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶jÿ2jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j÷2ubj±Œ, ”…””}”(j¶j÷2jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j3jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j÷2ubj±Œº), the full sampling of the x-file (usually 30 s or 15 s) is used. However, since the phase errors are correlated over many minutes, it is not necessary to use sampling this frequent in ”…””}”(j¶j÷2jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j#3jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j÷2ubj±Œ!. The default decimation factor (”…””}”(j¶j÷2jÇjc,hNjÆNubj˜)”}”(j¦Œ :content:`4`”j§]”j±Œ4”…””}”(j¶j53jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j÷2ubj±ŒÑ, resulting in 2-minute sampling for the usual case) provides formal uncertainties that are usually reasonable within a factor of two while reducing time significantly. (See the discussion of uncertainties in ”…””}”(j¶j÷2jÇjc,hNjÆNubj’)”}”(j¦Œ:numref:`intro_gnss_solve`”j§]”j˜)”}”(j¦jJ3j§]”j±Œintro_gnss_solve”…””}”(j¶jL3jÇjc,hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jH3ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jòŒ refdomain”jV3Œreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_gnss_solve”ujÄj‘hj,jÆKRj¶j÷2ubj±Œ©.) For the preliminary solution used to get decimeter-level coordinates for editing and to avoid non-linearity in the final adjustments, 5-minute sampling is sufficient.”…””}”(j¶j÷2jÇjc,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj,jÆKRj¶j,jÇjc,ubj)”}”(j¦X©Antenna Model = AZEL ; NONE/ELEV/AZEL default = ELEV Tides applied = 31 ; Binary coded: 1 earth 2 freq-dep 4 pole tide (zero mean pole) ; 8 ocean 16 pole tide (IERS2010 mean pole) 32 atmosphere S1/S2 ; 64 pole tide (IERS20 secular pole) (31 default ITRF2014, 79 default ITRF2020). Use otl.list = N Use otl.grid = Y ”j§]”j±X©Antenna Model = AZEL ; NONE/ELEV/AZEL default = ELEV Tides applied = 31 ; Binary coded: 1 earth 2 freq-dep 4 pole tide (zero mean pole) ; 8 ocean 16 pole tide (IERS2010 mean pole) 32 atmosphere S1/S2 ; 64 pole tide (IERS20 secular pole) (31 default ITRF2014, 79 default ITRF2020). Use otl.list = N Use otl.grid = Y ”…””}”j¶jr3sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒJ/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sestbl.”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhj,jÆKYj¶j,jÇjc,ubj`)”}”(j¦XNThere are over a dozen :file:`sestbl.` entries controlling the models used in processing the data. These are all given at the bottom of the template file in :file:`~/gg/tables/` and discussed in Section 3.2 of the `GAMIT Reference Manual `_. The three shown here are those most likely to need editing for current applications. Changing :content:`Antenna Model` to :content:`NONE` allows bypassing of the phase-center-variation (PCV) file :file:`antmod.dat`, an option advisable only if you are using identical antennas within a small regional network. The :content:`Tides applied` option is binary coded, allowing any combination of the various tidal models to be applied in :program:`model`. For most applications you may keep the default, which is to apply all of the tidal effects currently available in GAMIT (though the 2-bit for K1 is not necessary with the current IERS 2003 model for the solid-body tides, and the pole tide can be applied later in GLOBK). If your data are not strongly affected by ocean tidal loading ("OTL") or you do not wish to copy over the large ocean loading grid files, you might omit this model, setting :content:`Tides applied = 23` instead of :content:`31`. The OTL components are read from a station list file or a global grid, with station-list values taking precedent if :content:`Use otl.list = Y` and the station is within 10 km of a station in the file. If you have local stations close to an IGS station, it is advisable to use the grid exclusively so that you don't introduce artifacts in the relative motions of two stations.”j§]”(j±ŒThere are over a dozen ”…””}”(j¶j„3jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jŒ3jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j„3ubj±Œw entries controlling the models used in processing the data. These are all given at the bottom of the template file in ”…””}”(j¶j„3jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶j¡3jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j„3ubj±Œ% and discussed in Section 3.2 of the ”…””}”(j¶j„3jÇjc,hNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j¶3jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶j„3ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œid7”aj»]”j½]”jÀ]”Œgamit reference manual”ajÂ]”Œrefuri”jÆ3ujÄjdj Kj¶j„3ubj±Œ`. The three shown here are those most likely to need editing for current applications. Changing ”…””}”(j¶j„3jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`Antenna Model`”j§]”j±Œ Antenna Model”…””}”(j¶jØ3jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j„3ubj±Œ to ”…””}”(j¶j„3jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`NONE`”j§]”j±ŒNONE”…””}”(j¶jë3jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j„3ubj±Œ; allows bypassing of the phase-center-variation (PCV) file ”…””}”(j¶j„3jÇjc,hNjÆNubj˜)”}”(j¦Œ:file:`antmod.dat`”j§]”j±Œ antmod.dat”…””}”(j¶jþ3jÇjc,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j„3ubj±Œd, an option advisable only if you are using identical antennas within a small regional network. The ”…””}”(j¶j„3jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`Tides applied`”j§]”j±Œ Tides applied”…””}”(j¶j4jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j„3ubj±Œ_ option is binary coded, allowing any combination of the various tidal models to be applied in ”…””}”(j¶j„3jÇjc,hNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶j&4jÇjc,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j„3ubj±XÂ. For most applications you may keep the default, which is to apply all of the tidal effects currently available in GAMIT (though the 2-bit for K1 is not necessary with the current IERS 2003 model for the solid-body tides, and the pole tide can be applied later in GLOBK). If your data are not strongly affected by ocean tidal loading (“OTLâ€) or you do not wish to copy over the large ocean loading grid files, you might omit this model, setting ”…””}”(j¶j„3jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`Tides applied = 23`”j§]”j±ŒTides applied = 23”…””}”(j¶j84jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j„3ubj±Œ instead of ”…””}”(j¶j„3jÇjc,hNjÆNubj˜)”}”(j¦Œ :content:`31`”j§]”j±Œ31”…””}”(j¶jK4jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j„3ubj±Œv. The OTL components are read from a station list file or a global grid, with station-list values taking precedent if ”…””}”(j¶j„3jÇjc,hNjÆNubj˜)”}”(j¦Œ:content:`Use otl.list = Y`”j§]”j±ŒUse otl.list = Y”…””}”(j¶j^4jÇjc,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j„3ubj±Œë and the station is within 10 km of a station in the file. If you have local stations close to an IGS station, it is advisable to use the grid exclusively so that you don’t introduce artifacts in the relative motions of two stations.”…””}”(j¶j„3jÇjc,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj,jÆK]j¶j,jÇjc,ubej·}”(j¹]”(Œsestbl”jŽ,ej»]”j½]”(Œsestbl.”Œintro_proc_sestbl.”ejÀ]”jÂ]”ujÄh_j¶jc,jÇjc,hj,jÆKjÒ }”j}4j„,sjÔ }”jŽ,j„,subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j,j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj,jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jr,jf,j,ju,uj_}”(Œrel”jr,Œdate”j,ujc}”je}”jŽ,]”j„,asjg}”(j}4jŽ,j|4jy4jÂ.j¿.uji}”(j}4ˆj|4‰jÂ.ˆuj¹}”(jŽ,j,jy4j,jO.j:.j™.j„.j¿.j¹.jÒ/j½/jö/já/j=1j(1j²1j¬1jÍ3jÇ3ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”(jù )”}”(j¦hoj§]”j`)”}”(j¦Œ9Duplicate explicit target name: "gamit reference manual".”j§]”j±Œ=Duplicate explicit target name: “gamit reference manualâ€.”…””}”(j¶j¦4jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j£4ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j²1aŒlevel”KŒtype”jŒsource”j,Œline”KujÄjø j¶j,jÇjc,hj,jÆK9ubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ9Duplicate explicit target name: "gamit reference manual".”j§]”j±Œ=Duplicate explicit target name: “gamit reference manualâ€.”…””}”(j¶jÁ4jÇjc,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j¾4ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jÍ3aŒlevel”KŒtype”jŒsource”j,Œline”KujÄjø j¶j,jÇjc,hj,jÆKeubej†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ7Hyperlink target "intro-proc-sestbl" is not referenced.”…””}”j¶jÝ4sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÚ4ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j,Œline”KujÄjø ubajˆNj‰]”j‹NjÇjc,ubjîj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jø4sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jõ4jÇjõ4ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jõ4jÇjõ4ubje)”}”(j¦Œ.. _intro_proc_sites.defaults:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-sites-defaults”ujÄjdjÆKj¶jõ4jÇjõ4hŒU/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sites.defaults.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ:file:`sites.defaults`”j§]”j˜)”}”(j¦j'5j§]”j±Œsites.defaults”…””}”(j¶j)5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j%5ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j"5jÇjõ4hj!5jÆKubj`)”}”(j¦XÈThe :file:`sites.defaults` file determines how each station will be used in the processing. Since all sites in your :file:`rinex/` directory will be automatically included in your processing, in most cases you need to list here only those sites for which you want to automatically download data from a remote archive (:content:`ftprnx` token). This assumes that you do not want to include or exclude individual sites from automatic updating in :file:`station.info` (:content:`xstinfo` token) or to exclude from processing sites for which you have RINEX files in the :file:`rinex/` directory (:content:`xsite` token). Note that you must include after each site name the 4-character "experiment" name you use in your processing (shown in the :doc:`example <../example>` as :content:`scal`). This requirement derives from the feature to allow :file:`sites.defaults` to select sites to be used in each of several sub-networks when you are processing multiple sub-networks.”j§]”(j±ŒThe ”…””}”(j¶j?5jÇjõ4hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jG5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?5ubj±ŒZ file determines how each station will be used in the processing. Since all sites in your ”…””}”(j¶j?5jÇjõ4hNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶j\5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?5ubj±Œ¼ directory will be automatically included in your processing, in most cases you need to list here only those sites for which you want to automatically download data from a remote archive (”…””}”(j¶j?5jÇjõ4hNjÆNubj˜)”}”(j¦Œ:content:`ftprnx`”j§]”j±Œftprnx”…””}”(j¶jq5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j?5ubj±Œm token). This assumes that you do not want to include or exclude individual sites from automatic updating in ”…””}”(j¶j?5jÇjõ4hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j„5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?5ubj±Œ (”…””}”(j¶j?5jÇjõ4hNjÆNubj˜)”}”(j¦Œ:content:`xstinfo`”j§]”j±Œxstinfo”…””}”(j¶j™5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j?5ubj±ŒR token) or to exclude from processing sites for which you have RINEX files in the ”…””}”(j¶j?5jÇjõ4hNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶j¬5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?5ubj±Œ directory (”…””}”(j¶j?5jÇjõ4hNjÆNubj˜)”}”(j¦Œ:content:`xsite`”j§]”j±Œxsite”…””}”(j¶jÁ5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j?5ubj±Œˆ token). Note that you must include after each site name the 4-character “experiment†name you use in your processing (shown in the ”…””}”(j¶j?5jÇjõ4hNjÆNubj’)”}”(j¦Œ:doc:`example <../example>`”j§]”j)”}”(j¦jÖ5j§]”j±Œexample”…””}”(j¶jØ5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶jÔ5ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jîŒ refdomain”jâ5Œreftype”Œdoc”Œ refexplicit”ˆŒrefwarn”ˆj¶Œ ../example”ujÄj‘hj!5jÆKj¶j?5ubj±Œ as ”…””}”(j¶j?5jÇjõ4hNjÆNubj˜)”}”(j¦Œ:content:`scal`”j§]”j±Œscal”…””}”(j¶jø5jÇjõ4hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j?5ubj±Œ6). This requirement derives from the feature to allow ”…””}”(j¶j?5jÇjõ4hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶j 6jÇjõ4hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?5ubj±Œj to select sites to be used in each of several sub-networks when you are processing multiple sub-networks.”…””}”(j¶j?5jÇjõ4hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj!5jÆKj¶j"5jÇjõ4ubj)”}”(j¦Xý# File to control the use of stations in the processing # # Format: site expt keyword1 keyword2 .... # # where the first token is the 4- or 8-character site name (GAMIT uses only # 4 characters, GLOBK allows only 4 unless there are earthquakes or renames), # the second token is the 4-character experiment name, and the remaining # tokens, read free-format, indicate how the site is to be used in the processing. # All sites for which there are RINEX files in the local directory will be used # automatically and do not need to be listed. # # ftprnx = sites to ftp from rinex data archives. # ftpraw = sites to ftp from raw data archives. # localrx = site names used to search for rinex files on your local system. # (required in conjunction with rnxfnd path variable set in process.defaults). # xstinfo = sites to exclude from automatic station.info updating. # xsite = sites to exclude from processing, all days or specified days # # Replace 'expt' with your experiment name and edit the following to list sites needed from external archive all_sites expt xstinfo brus_gps expt ftprnx graz_gps expt ftprnx sofi_gps expt ftprnx # templates for removing sites ttth_gps expt xsite:1999_256-1999_278 xsite:1999_300-1999_365 ”j§]”j±Xý# File to control the use of stations in the processing # # Format: site expt keyword1 keyword2 .... # # where the first token is the 4- or 8-character site name (GAMIT uses only # 4 characters, GLOBK allows only 4 unless there are earthquakes or renames), # the second token is the 4-character experiment name, and the remaining # tokens, read free-format, indicate how the site is to be used in the processing. # All sites for which there are RINEX files in the local directory will be used # automatically and do not need to be listed. # # ftprnx = sites to ftp from rinex data archives. # ftpraw = sites to ftp from raw data archives. # localrx = site names used to search for rinex files on your local system. # (required in conjunction with rnxfnd path variable set in process.defaults). # xstinfo = sites to exclude from automatic station.info updating. # xsite = sites to exclude from processing, all days or specified days # # Replace 'expt' with your experiment name and edit the following to list sites needed from external archive all_sites expt xstinfo brus_gps expt ftprnx graz_gps expt ftprnx sofi_gps expt ftprnx # templates for removing sites ttth_gps expt xsite:1999_256-1999_278 xsite:1999_300-1999_365 ”…””}”j¶j&6sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”ŒQ/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sites.defaults”j/j0j&‰hyŒtext”j(}”jÒKsujÄjhj!5jÆK j¶j"5jÇjõ4ubj`)”}”(j¦ŒUThe :option:`-xsite` option can also be used on the :program:`sh_gamit` command line.”j§]”(j±ŒThe ”…””}”(j¶j86jÇjõ4hNjÆNubj’)”}”(j¦Œ:option:`-xsite`”j§]”j˜)”}”(j¦jB6j§]”j±Œ-xsite”…””}”(j¶jD6jÇjõ4hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j@6ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jîŒ refdomain”jN6Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-xsite”ujÄj‘hj!5jÆKj¶j86ubj±Œ option can also be used on the ”…””}”(j¶j86jÇjõ4hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jd6jÇjõ4hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j86ubj±Œ command line.”…””}”(j¶j86jÇjõ4hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj!5jÆKj¶j"5jÇjõ4ubej·}”(j¹]”(Œsites-defaults”j 5ej»]”j½]”(Œsites.defaults”Œintro_proc_sites.defaults”ejÀ]”jÂ]”ujÄh_j¶jõ4jÇjõ4hj!5jÆKjÒ }”j‚6j5sjÔ }”j 5j5subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j!5j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj!5jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j5jø4j5j5uj_}”(Œrel”j5Œdate”j5ujc}”je}”j 5]”j5asjg}”(j‚6j 5j6j~6uji}”(j‚6ˆj6‰uj¹}”(j 5j"5j~6j"5ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ?Hyperlink target "intro-proc-sites-defaults" is not referenced.”…””}”j¶j¬6sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j©6ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j!5Œline”KujÄjø ubajˆNj‰]”j‹NjÇjõ4ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jÇ6sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÄ6jÇjÄ6ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jÖ6jÇjÄ6hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÄ6jÇjÄ6ubje)”}”(j¦Œ.. _intro_proc_sittbl.:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-sittbl”ujÄjdjÆKj¶jÄ6jÇjÄ6hŒM/chandler/home/floyd/public_html/gg/docs/source/intro/proc/control/sittbl.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ:file:`sittbl.`”j§]”j˜)”}”(j¦jö6j§]”j±Œsittbl.”…””}”(j¶jø6jÇjÄ6hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jô6ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jñ6jÇjÄ6hjð6jÆKubj`)”}”(j¦XThe :file:`sittbl.` contains options that can be set on a station-by-station basis. The width of the table is variable, with the entries determined by the column headers present. A complete version is available as :file:`~/gg/tables/sittbl.long`, but the short version shown below contains the only entries you are likely to change—the *a priori* station constraints to be applied in GAMIT to enhance ambiguity resolution and to obtain a solution that you can inspect visually (this assumes that your final solution will come from GLOBK).:”j§]”(j±ŒThe ”…””}”(j¶j7jÇjÄ6hNjÆNubj˜)”}”(j¦Œ:file:`sittbl.`”j§]”j±Œsittbl.”…””}”(j¶j7jÇjÄ6hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j7ubj±ŒÃ contains options that can be set on a station-by-station basis. The width of the table is variable, with the entries determined by the column headers present. A complete version is available as ”…””}”(j¶j7jÇjÄ6hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/sittbl.long`”j§]”j±Œ~/gg/tables/sittbl.long”…””}”(j¶j+7jÇjÄ6hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j7ubj±Œ], but the short version shown below contains the only entries you are likely to change—the ”…””}”(j¶j7jÇjÄ6hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j@7jÇjÄ6hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j7ubj±ŒÁ station constraints to be applied in GAMIT to enhance ambiguity resolution and to obtain a solution that you can inspect visually (this assumes that your final solution will come from GLOBK).:”…””}”(j¶j7jÇjÄ6hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjð6jÆKj¶jñ6jÇjÄ6ubj)”}”(j¦XSITE --COORD.CONSTR.-- << default for regional stations >> ALL 100. 100. 100. << Stations to constrain >> BLYT Blythe_ 0.010 0.010 0.02 JPLM JPL Mesa 0.010 0.010 0.02 MATH Lake Matthews 0.010 0.010 0.02”j§]”j±XSITE --COORD.CONSTR.-- << default for regional stations >> ALL 100. 100. 100. << Stations to constrain >> BLYT Blythe_ 0.010 0.010 0.02 JPLM JPL Mesa 0.010 0.010 0.02 MATH Lake Matthews 0.010 0.010 0.02”…””}”j¶jX7sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjð6jÆK j¶jñ6jÇjÄ6ubj`)”}”(j¦X<The 4-character site name must appear in the first four columns, the 12-character name is of arbitrary length beneath a blank header, and the coordinate constraints are free-format but must fall within the columns denoted by the header :content:`--COORD.CONSTR.--`. The constraints are north, east, and up in meters.”j§]”(j±ŒìThe 4-character site name must appear in the first four columns, the 12-character name is of arbitrary length beneath a blank header, and the coordinate constraints are free-format but must fall within the columns denoted by the header ”…””}”(j¶jh7jÇjÄ6hNjÆNubj˜)”}”(j¦Œ:content:`--COORD.CONSTR.--`”j§]”j±Œ--COORD.CONSTR.--”…””}”(j¶jp7jÇjÄ6hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jh7ubj±Œ4. The constraints are north, east, and up in meters.”…””}”(j¶jh7jÇjÄ6hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjð6jÆKj¶jñ6jÇjÄ6ubej·}”(j¹]”(Œsittbl”jï6ej»]”j½]”(Œsittbl.”Œintro_proc_sittbl.”ejÀ]”jÂ]”ujÄh_j¶jÄ6jÇjÄ6hjð6jÆKjÒ }”j7jå6sjÔ }”jï6jå6subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jð6j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjð6jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jÓ6jÇ6jâ6jÖ6uj_}”(Œrel”jÓ6Œdate”jâ6ujc}”je}”jï6]”jå6asjg}”(j7jï6jŽ7j‹7uji}”(j7ˆjŽ7‰uj¹}”(jï6jñ6j‹7jñ6ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ7Hyperlink target "intro-proc-sittbl" is not referenced.”…””}”j¶j¹7sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j¶7ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jð6Œline”KujÄjø ubajˆNj‰]”j‹NjÇjÄ6ubjÿj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jÔ7sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÑ7jÇjÑ7ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jã7jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÑ7jÇjÑ7ubje)”}”(j¦Œ.. _intro_proc_example:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-example”ujÄjdjÆKj¶jÑ7jÇjÑ7hŒF/chandler/home/floyd/public_html/gg/docs/source/intro/proc/example.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ1Using :program:`sh_gamit` and :program:`sh_glred`”j§]”(j±ŒUsing ”…””}”(j¶j8jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j 8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j8ubj±Œ and ”…””}”(j¶j8jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j8ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jþ7jÇjÑ7hjý7jÆKubj`)”}”(j¦XaNow that we've described the program flow and control files, we'll take you through a simple application of :program:`sh_gamit` and :program:`sh_glred` using the small network in Southern California previously provided (prior to 10.7) in :file:`~/gg/example/`. The command for :program:`sh_gamit` issued at the project-directory level (:file:`2000/`) is”j§]”(j±ŒpNow that we’ve described the program flow and control files, we’ll take you through a simple application of ”…””}”(j¶j/8jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j78jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j/8ubj±Œ and ”…””}”(j¶j/8jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jI8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j/8ubj±ŒW using the small network in Southern California previously provided (prior to 10.7) in ”…””}”(j¶j/8jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/example/`”j§]”j±Œ ~/gg/example/”…””}”(j¶j[8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j/8ubj±Œ. The command for ”…””}”(j¶j/8jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jp8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j/8ubj±Œ( issued at the project-directory level (”…””}”(j¶j/8jÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`2000/`”j§]”j±Œ2000/”…””}”(j¶j‚8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j/8ubj±Œ) is”…””}”(j¶j/8jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶jþ7jÇjÑ7ubj)”}”(j¦Œb$ sh_gamit -expt scal -d 2000 034 035 036 -noftp -pres ELEV -copt x k p -dopt c ao >& sh_gamit.log”j§]”j±Œb$ sh_gamit -expt scal -d 2000 034 035 036 -noftp -pres ELEV -copt x k p -dopt c ao >& sh_gamit.log”…””}”j¶j8sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjý7jÆK j¶jþ7jÇjÑ7ubj`)”}”(j¦XDIn this example, we start with all of the data to be processed already present in the :file:`rinex/` directory. If you wanted to add additional data available from a global or regional archive, you would specify the site names in :file:`sites.defaults`, enter the URL information (if not already present) into :file:`~/gg/tables/ftp_info`, and remove the :option:`-noftp` option from the call to :program:`sh_gamit`. As a result of the command shown, :program:`sh_gamit` will execute for each day the following steps, noted in the screen output redirected to :file:`sh_gamit.log`:”j§]”(j±ŒVIn this example, we start with all of the data to be processed already present in the ”…””}”(j¶j­8jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶jµ8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­8ubj±Œ‚ directory. If you wanted to add additional data available from a global or regional archive, you would specify the site names in ”…””}”(j¶j­8jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jÊ8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­8ubj±Œ:, enter the URL information (if not already present) into ”…””}”(j¶j­8jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/ftp_info`”j§]”j±Œ~/gg/tables/ftp_info”…””}”(j¶jß8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­8ubj±Œ, and remove the ”…””}”(j¶j­8jÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-noftp`”j§]”j˜)”}”(j¦jö8j§]”j±Œ-noftp”…””}”(j¶jø8jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jô8ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j9Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-noftp”ujÄj‘hjý7jÆK j¶j­8ubj±Œ option from the call to ”…””}”(j¶j­8jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j9jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j­8ubj±Œ$. As a result of the command shown, ”…””}”(j¶j­8jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j*9jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j­8ubj±ŒY will execute for each day the following steps, noted in the screen output redirected to ”…””}”(j¶j­8jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sh_gamit.log`”j§]”j±Œ sh_gamit.log”…””}”(j¶j<9jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­8ubj±Œ:”…””}”(j¶j­8jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK j¶jþ7jÇjÑ7ubj©Œenumerated_list”“”)”}”(j¦hoj§]”(j˜)”}”(j¦XAssign parameters for program flow, giving precedence first to the command-line arguments, then to the parameters set in :file:`process.defaults` and :file:`sites.defaults`, and then to default assignments within :program:`sh_gamit` itself. In this case, the command-line entry :option:`-noftp` overrides the default to search archives for requested or updated observation, navigation, and EOP files; and the command-line entries for which files to compress or delete at the end of the run override those set in :file:`process.defaults`.”j§]”j`)”}”(j¦XAssign parameters for program flow, giving precedence first to the command-line arguments, then to the parameters set in :file:`process.defaults` and :file:`sites.defaults`, and then to default assignments within :program:`sh_gamit` itself. In this case, the command-line entry :option:`-noftp` overrides the default to search archives for requested or updated observation, navigation, and EOP files; and the command-line entries for which files to compress or delete at the end of the run override those set in :file:`process.defaults`.”j§]”(j±ŒyAssign parameters for program flow, giving precedence first to the command-line arguments, then to the parameters set in ”…””}”(j¶j`9jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jh9jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j`9ubj±Œ and ”…””}”(j¶j`9jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶j}9jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j`9ubj±Œ), and then to default assignments within ”…””}”(j¶j`9jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j’9jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j`9ubj±Œ. itself. In this case, the command-line entry ”…””}”(j¶j`9jÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-noftp`”j§]”j˜)”}”(j¦j¦9j§]”j±Œ-noftp”…””}”(j¶j¨9jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j¤9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j²9Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-noftp”ujÄj‘hjý7jÆKj¶j`9ubj±ŒÚ overrides the default to search archives for requested or updated observation, navigation, and EOP files; and the command-line entries for which files to compress or delete at the end of the run override those set in ”…””}”(j¶j`9jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jÈ9jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j`9ubj±Œ.”…””}”(j¶j`9jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶j\9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦Œ–Create the day-directory and/or standard directories which do not yet exist (all of these are already present in the :file:`~/gg/example/` directory).”j§]”j`)”}”(j¦jë9j§]”(j±ŒuCreate the day-directory and/or standard directories which do not yet exist (all of these are already present in the ”…””}”(j¶jí9jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/example/`”j§]”j±Œ ~/gg/example/”…””}”(j¶jô9jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jí9ubj±Œ directory).”…””}”(j¶jí9jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶jé9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦ŒÕLink into the day directory (:file:`034/`) the standard tables (see script :program:`links.day`) and the RINEX files that contain data for the specified interval (00:00–24:00 as set in :file:`process.defaults`).”j§]”j`)”}”(j¦j:j§]”(j±ŒLink into the day directory (”…””}”(j¶j:jÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`034/`”j§]”j±Œ034/”…””}”(j¶j :jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j:ubj±Œ") the standard tables (see script ”…””}”(j¶j:jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`links.day`”j§]”j±Œ links.day”…””}”(j¶j5:jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j:ubj±Œ\) and the RINEX files that contain data for the specified interval (00:00–24:00 as set in ”…””}”(j¶j:jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jG:jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j:ubj±Œ).”…””}”(j¶j:jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶j:ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦ŒtDownload orbital SP3 files from a global data center and create GAMIT g-files using script :program:`sh_get_orbits`.”j§]”j`)”}”(j¦jj:j§]”(j±Œ[Download orbital SP3 files from a global data center and create GAMIT g-files using script ”…””}”(j¶jl:jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_get_orbits`”j§]”j±Œ sh_get_orbits”…””}”(j¶js:jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jl:ubj±Œ.”…””}”(j¶jl:jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶jh:ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦ŒïRun :program:`sh_upd_stnfo`, which invokes program :program:`mstinf` to update :file:`station.info` from the RINEX headers. (It is recommended that this step be skipped by setting :content:`xstinfo {} all` in :file:`sites.defaults`.)”j§]”j`)”}”(j¦ŒïRun :program:`sh_upd_stnfo`, which invokes program :program:`mstinf` to update :file:`station.info` from the RINEX headers. (It is recommended that this step be skipped by setting :content:`xstinfo {} all` in :file:`sites.defaults`.)”j§]”(j±ŒRun ”…””}”(j¶j•:jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_upd_stnfo`”j§]”j±Œ sh_upd_stnfo”…””}”(j¶j:jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j•:ubj±Œ, which invokes program ”…””}”(j¶j•:jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`mstinf`”j§]”j±Œmstinf”…””}”(j¶j¯:jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j•:ubj±Œ to update ”…””}”(j¶j•:jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jÁ:jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j•:ubj±ŒQ from the RINEX headers. (It is recommended that this step be skipped by setting ”…””}”(j¶j•:jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`xstinfo {} all`”j§]”j±Œxstinfo {} all”…””}”(j¶jÖ:jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j•:ubj±Œ in ”…””}”(j¶j•:jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jé:jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j•:ubj±Œ.)”…””}”(j¶j•:jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶j‘:ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦Œ‹Run :program:`makexp` to create the input files for :program:`makex` (:file:`scal.makex.batch`) and :program:`fixdrv` (:file:`dscal0.034`).”j§]”j`)”}”(j¦j ;j§]”(j±ŒRun ”…””}”(j¶j;jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`makexp`”j§]”j±Œmakexp”…””}”(j¶j;jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j;ubj±Œ to create the input files for ”…””}”(j¶j;jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`makex`”j§]”j±Œmakex”…””}”(j¶j';jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j;ubj±Œ (”…””}”(j¶j;jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`scal.makex.batch`”j§]”j±Œscal.makex.batch”…””}”(j¶j9;jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j;ubj±Œ) and ”…””}”(j¶j;jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`fixdrv`”j§]”j±Œfixdrv”…””}”(j¶jN;jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j;ubj±Œ (”…””}”j¶j;sbj˜)”}”(j¦Œ:file:`dscal0.034`”j§]”j±Œ dscal0.034”…””}”(j¶j`;jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j;ubj±Œ).”…””}”(j¶j;jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶j ;ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦X!Run :program:`sh_check_sess` to make sure that all of the satellites included in the RINEX observation files are present in the navigation file (:file:`brdc/brdc0340.00n`, previously downloaded at MIT from an IGS archive) and in the g-file (created previously at MIT from an IGS SP3 file).”j§]”j`)”}”(j¦jƒ;j§]”(j±ŒRun ”…””}”(j¶j…;jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_check_sess`”j§]”j±Œ sh_check_sess”…””}”(j¶jŒ;jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j…;ubj±Œu to make sure that all of the satellites included in the RINEX observation files are present in the navigation file (”…””}”(j¶j…;jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`brdc/brdc0340.00n`”j§]”j±Œbrdc/brdc0340.00n”…””}”(j¶jž;jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j…;ubj±Œw, previously downloaded at MIT from an IGS archive) and in the g-file (created previously at MIT from an IGS SP3 file).”…””}”(j¶j…;jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶j;ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦ŒwRun :program:`sh_makej` to create a j-file of satellite clock estimates from the SP3 file (default) or navigation file.”j§]”j`)”}”(j¦jÁ;j§]”(j±ŒRun ”…””}”(j¶jÃ;jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_makej`”j§]”j±Œsh_makej”…””}”(j¶jÊ;jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÃ;ubj±Œ` to create a j-file of satellite clock estimates from the SP3 file (default) or navigation file.”…””}”(j¶jÃ;jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶j¿;ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦XuRun :program:`makex` to create x-files (observations) and k-files (receiver clock estimates) using phase and pseudorange data from the RINEX observation files, broadcast ephemeris from the navigation file, and satellite clocks from the j-file. A record of :program:`makex`, showing the data found and any problematic data encountered is written to :file:`scal.makex.infor`.”j§]”j`)”}”(j¦XuRun :program:`makex` to create x-files (observations) and k-files (receiver clock estimates) using phase and pseudorange data from the RINEX observation files, broadcast ephemeris from the navigation file, and satellite clocks from the j-file. A record of :program:`makex`, showing the data found and any problematic data encountered is written to :file:`scal.makex.infor`.”j§]”(j±ŒRun ”…””}”(j¶jì;jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`makex`”j§]”j±Œmakex”…””}”(j¶jô;jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jì;ubj±Œì to create x-files (observations) and k-files (receiver clock estimates) using phase and pseudorange data from the RINEX observation files, broadcast ephemeris from the navigation file, and satellite clocks from the j-file. A record of ”…””}”(j¶jì;jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`makex`”j§]”j±Œmakex”…””}”(j¶j<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jì;ubj±ŒL, showing the data found and any problematic data encountered is written to ”…””}”(j¶jì;jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`scal.makex.infor`”j§]”j±Œscal.makex.infor”…””}”(j¶j<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jì;ubj±Œ.”…””}”(j¶jì;jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶jè;ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦X!Run :program:`fixdrv` to create the batch file for GAMIT processing. Though not used directly, :program:`fixdrv` also reads the k-file of episodic clock values and fits a first-order polynomial to them as a crude check for jumps and rapid drifts in the receiver clock (:file:`fixdrv.out`).”j§]”j`)”}”(j¦X!Run :program:`fixdrv` to create the batch file for GAMIT processing. Though not used directly, :program:`fixdrv` also reads the k-file of episodic clock values and fits a first-order polynomial to them as a crude check for jumps and rapid drifts in the receiver clock (:file:`fixdrv.out`).”j§]”(j±ŒRun ”…””}”(j¶j=<jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`fixdrv`”j§]”j±Œfixdrv”…””}”(j¶jE<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j=<ubj±ŒJ to create the batch file for GAMIT processing. Though not used directly, ”…””•}”(j¶j=<jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`fixdrv`”j§]”j±Œfixdrv”…””}”(j¶jW<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j=<ubj±Œ also reads the k-file of episodic clock values and fits a first-order polynomial to them as a crude check for jumps and rapid drifts in the receiver clock (”…””}”(j¶j=<jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`fixdrv.out`”j§]”j±Œ fixdrv.out”…””}”(j¶ji<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j=<ubj±Œ).”…””}”(j¶j=<jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶j9<ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦X5Execute the batch run to generate a tabular orbital ephemeris (:program:`arc`), model the phase observations (:program:`model`), edit the data (:program:`autcln`), and estimate parameters (:program:`solve`), a sequence completed twice in order that :program:`autcln` may operate on flat residuals and that the final adjustments in :program:`solve` are well within a linear range. A record of this run is not written to :file:`sh_gamit.log` (to save space) but is recorded in :file:`GAMIT.status`, :file:`GAMIT.warning`, and :file:`GAMIT.fatal` in the day directory.”j§]”j`)”}”(j¦X5Execute the batch run to generate a tabular orbital ephemeris (:program:`arc`), model the phase observations (:program:`model`), edit the data (:program:`autcln`), and estimate parameters (:program:`solve`), a sequence completed twice in order that :program:`autcln` may operate on flat residuals and that the final adjustments in :program:`solve` are well within a linear range. A record of this run is not written to :file:`sh_gamit.log` (to save space) but is recorded in :file:`GAMIT.status`, :file:`GAMIT.warning`, and :file:`GAMIT.fatal` in the day directory.”j§]”(j±Œ?Execute the batch run to generate a tabular orbital ephemeris (”…””}”(j¶jŽ<jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`arc`”j§]”j±Œarc”…””}”(j¶j–<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jŽ<ubj±Œ!), model the phase observations (”…””}”(j¶jŽ<jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶j¨<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jŽ<ubj±Œ), edit the data (”…””}”(j¶jŽ<jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jº<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jŽ<ubj±Œ), and estimate parameters (”…””}”(j¶jŽ<jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶jÌ<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jŽ<ubj±Œ,), a sequence completed twice in order that ”…””}”(j¶jŽ<jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jÞ<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jŽ<ubj±ŒA may operate on flat residuals and that the final adjustments in ”…””}”(j¶jŽ<jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶jð<jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jŽ<ubj±ŒH are well within a linear range. A record of this run is not written to ”…””}”(j¶jŽ<jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sh_gamit.log`”j§]”j±Œ sh_gamit.log”…””}”(j¶j=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŽ<ubj±Œ$ (to save space) but is recorded in ”…””}”(j¶jŽ<jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`GAMIT.status`”j§]”j±Œ GAMIT.status”…””}”(j¶j=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŽ<ubj±Œ, ”…””}”(j¶jŽ<jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`GAMIT.warning`”j§]”j±Œ GAMIT.warning”…””}”(j¶j,=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŽ<ubj±Œ, and ”…””}”(j¶jŽ<jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`GAMIT.fatal`”j§]”j±Œ GAMIT.fatal”…””}”(j¶jA=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŽ<ubj±Œ in the day directory.”…””}”(j¶jŽ<jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK j¶jŠ<ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦XSave the cleaning summary (:file:`autcln.post.sum`) to :file:`autcln.post.sum.scal` (potentially for archiving, though that's not done for this example) and write key information from :program:`model` and :program:`solve` to the :file:`HISTORY` file, which, unlike all other files in the day directory, is appended rather than overwritten in reruns so that a record of previous runs is maintained.”j§]”j`)”}”(j¦jd=j§]”(j±ŒSave the cleaning summary (”…””}”(j¶jf=jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum`”j§]”j±Œautcln.post.sum”…””}”(j¶jm=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jf=ubj±Œ) to ”…””}”(j¶jf=jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum.scal`”j§]”j±Œautcln.post.sum.scal”…””}”(j¶j‚=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jf=ubj±Œg (potentially for archiving, though that’s not done for this example) and write key information from ”…””}”(j¶jf=jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶j—=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jf=ubj±Œ and ”…””}”(j¶jf=jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j©=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jf=ubj±Œ to the ”…””}”(j¶jf=jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`HISTORY`”j§]”j±ŒHISTORY”…””}”(j¶j»=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jf=ubj±Œ™ file, which, unlike all other files in the day directory, is appended rather than overwritten in reruns so that a record of previous runs is maintained.”…””}”(j¶jf=jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK"j¶jb=ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦ŒñCreate sky plots of phase residuals and plots of phase vs elevation angle using the DPH files written by :program:`autcln`; if the Ghostscript program is available, translate the plots from PostScript to PNG and move them into :file:`figs/`.”j§]”j`)”}”(j¦ŒñCreate sky plots of phase residuals and plots of phase vs elevation angle using the DPH files written by :program:`autcln`; if the Ghostscript program is available, translate the plots from PostScript to PNG and move them into :file:`figs/`.”j§]”(j±ŒiCreate sky plots of phase residuals and plots of phase vs elevation angle using the DPH files written by ”…””}”(j¶jà=jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jè=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jà=ubj±Œi; if the Ghostscript program is available, translate the plots from PostScript to PNG and move them into ”…””}”(j¶jà=jÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`figs/`”j§]”j±Œfigs/”…””}”(j¶jú=jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jà=ubj±Œ.”…””}”(j¶jà=jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK#j¶jÜ=ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubj˜)”}”(j¦ŒnInvoke :program:`sh_cleanup` to delete or compress files as specified by :option:`-dopt` and :option:`-copt`. ”j§]”j`)”}”(j¦ŒmInvoke :program:`sh_cleanup` to delete or compress files as specified by :option:`-dopt` and :option:`-copt`.”j§]”(j±ŒInvoke ”…””}”(j¶j>jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_cleanup`”j§]”j±Œ sh_cleanup”…””}”(j¶j'>jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j>ubj±Œ- to delete or compress files as specified by ”…””}”(j¶j>jÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-dopt`”j§]”j˜)”}”(j¦j;>j§]”j±Œ-dopt”…””}”(j¶j=>jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j9>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jG>Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-dopt”ujÄj‘hjý7jÆK%j¶j>ubj±Œ and ”…””}”(j¶j>jÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-copt`”j§]”j˜)”}”(j¦j_>j§]”j±Œ-copt”…””}”(j¶ja>jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j]>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jk>Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-copt”ujÄj‘hjý7jÆK%j¶j>ubj±Œ.”…””}”(j¶j>jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK%j¶j>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jY9jÇjÑ7hjý7jÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œenumtype”Œarabic”Œprefix”hoŒsuffix”Œ.”ujÄjW9j¶jþ7jÇjÑ7hjý7jÆKubj`)”}”(j¦ŒÙ**The most common problems with** :program:`sh_gamit` **are missing or incorrect receiver and antenna information ("metadata") in** :file:`station.info` **and the loss of data due to bad tracking or bad coordinates.**”j§]”(j©Œstrong”“”)”}”(j¦Œ!**The most common problems with**”j§]”j±ŒThe most common problems with”…””}”(j¶jž>jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjœ>j¶j˜>ubj±Œ ”…””}”(j¶j˜>jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j°>jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j˜>ubj±Œ ”…””}”j¶j˜>sbj>)”}”(j¦ŒM**are missing or incorrect receiver and antenna information ("metadata") in**”j§]”j±ŒMare missing or incorrect receiver and antenna information (“metadataâ€) in”…””}”(j¶jÂ>jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjœ>j¶j˜>ubj±Œ ”…””}”j¶j˜>sbj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jÔ>jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j˜>ubj±Œ ”…””}”j¶j˜>sbj>)”}”(j¦Œ@**and the loss of data due to bad tracking or bad coordinates.**”j§]”j±ŒjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjœ>j¶j˜>ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK'j¶jþ7jÇjÑ7ubj`)”}”(j¦XzThere are two approaches you can take to providing metadata to GAMIT. If you have RINEX files for which you know all the headers are correct, you can have :program:`sh_gamit` invoke :program:`sh_upd_stnfo` to update :file:`station.info` for each day using the header entries (no update will be made if the :file:`station.info` entry is present and matches the RINEX header). If the antenna height information is correct but the receiver and antenna names not IGS standard, you can still use this feature if you put into :file:`~/gg/tables/guess_rcvant.dat` a substring that will uniquely match what appears in the header. If you know that all of your receivers and/or antennas are of the same type, you can force their use by specifying them as :content:`ant default` and :content:`rcv default` in :file:`guess_rcvant.dat`. If you expect :program:`sh_gamit` to generate :file:`station.info` entries from the RINEX header information, you should review the antenna and receiver names used in all of the headers before you start (e.g., by :command:`grep`'ing on the RINEX files for :content:`REC #` and :content:`ANT #`). Antenna heights can also be problematic. In the RINEX standard, the header value is supposed to be a vertical height to antenna reference point (ARP), but often a slant height is actually given in the file. If the latter is the case, then :content:`stinf_slthgt` in :file:`process.defaults` can be set to a height above which the value will be assumed to a slant height to the outside edge of the ground plane. (Setting :content:`stinf_slthgt` to 0 or a large number will cause all values to be interpreted as direct height measurements.)”j§]”(j±Œ›There are two approaches you can take to providing metadata to GAMIT. If you have RINEX files for which you know all the headers are correct, you can have ”…””}”(j¶jý>jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jý>ubj±Œ invoke ”…””}”(j¶jý>jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_upd_stnfo`”j§]”j±Œ sh_upd_stnfo”…””}”(j¶j?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jý>ubj±Œ to update ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j)?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jý>ubj±ŒF for each day using the header entries (no update will be made if the ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j>?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jý>ubj±ŒÂ entry is present and matches the RINEX header). If the antenna height information is correct but the receiver and antenna names not IGS standard, you can still use this feature if you put into ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ$:file:`~/gg/tables/guess_rcvant.dat`”j§]”j±Œ~/gg/tables/guess_rcvant.dat”…””}”(j¶jS?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jý>ubj±Œ½ a substring that will uniquely match what appears in the header. If you know that all of your receivers and/or antennas are of the same type, you can force their use by specifying them as ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`ant default`”j§]”j±Œ ant default”…””}”(j¶jh?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jý>ubj±Œ and ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`rcv default`”j§]”j±Œ rcv default”…””}”(j¶j{?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jý>ubj±Œ in ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`guess_rcvant.dat`”j§]”j±Œguess_rcvant.dat”…””}”(j¶jŽ?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jý>ubj±Œ. If you expect ”…””}”(j¶jý>jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j£?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jý>ubj±Œ to generate ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jµ?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jý>ubj±Œ“ entries from the RINEX header information, you should review the antenna and receiver names used in all of the headers before you start (e.g., by ”…””}”(j¶jý>jÇjÑ7hNjÆNubjj)”}”(j¦Œ:command:`grep`”j§]”j±Œgrep”…””}”(j¶jÊ?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jý>ubj±Œ’ing on the RINEX files for ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`REC #`”j§]”j±ŒREC #”…””}”(j¶jÜ?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jý>ubj±Œ and ”…””}”j¶jý>sbj˜)”}”(j¦Œ:content:`ANT #`”j§]”j±ŒANT #”…””}”(j¶jï?jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jý>ubj±Œò). Antenna heights can also be problematic. In the RINEX standard, the header value is supposed to be a vertical height to antenna reference point (ARP), but often a slant height is actually given in the file. If the latter is the case, then ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`stinf_slthgt`”j§]”j±Œ stinf_slthgt”…””}”(j¶j@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jý>ubj±Œ in ”…””}”j¶jý>sbj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶j@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jý>ubj±Œ‚ can be set to a height above which the value will be assumed to a slant height to the outside edge of the ground plane. (Setting ”…””}”(j¶jý>jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`stinf_slthgt`”j§]”j±Œ stinf_slthgt”…””}”(j¶j*@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jý>ubj±Œ_ to 0 or a large number will cause all values to be interpreted as direct height measurements.)”…””}”(j¶jý>jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK)j¶jþ7jÇjÑ7ubj`)”}”(j¦X^If you have *any* doubts about the validity of the RINEX headers, it is better to create (and check!) :file:`station.info` before you start the GAMIT processing. You can create a file with all of the entries for your survey by running :program:`sh_upd_stnfo` manually with your RINEX files, then edit the file as appropriate. In creating this file, it is best to start with a template from the current MIT or SOPAC global :file:`station.info` file (available in :file:`incremental_updates/tables/`) so that you can conveniently add entries for continuous stations from the global file. This template can be header-only, but the preferred approach is to start with the full global :file:`station.info` file and use the :option:`-l {}` option of :program:`sh_upd_stnfo` to extract only the stations you need, either from an existing list or one created automatically by :program:`sh_upd_stnfo` from the sites with :content:`ftprnx` in :file:`sites.defaults` and/or the file names in your experiment :file:`rinex/` directory. Hence, if you have a current copy of the MIT or SOPAC station.info in :file:`~/gg/tables/`, have run run :program:`sh_setup` to copy it into your experiment :file:`tables/` directory, and have edited :file:`sites.defaults` to specify the RINEX files you want from a remote archive (using :content:`ftprnx`), you can run (in :file:`tables/`):”j§]”(j±Œ If you have ”…””}”(j¶jC@jÇjÑ7hNjÆNubj )”}”(j¦Œ*any*”j§]”j±Œany”…””}”(j¶jK@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jC@ubj±ŒU doubts about the validity of the RINEX headers, it is better to create (and check!) ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j]@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±Œq before you start the GAMIT processing. You can create a file with all of the entries for your survey by running ”…””}”(j¶jC@jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_upd_stnfo`”j§]”j±Œ sh_upd_stnfo”…””}”(j¶jr@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jC@ubj±Œ¤ manually with your RINEX files, then edit the file as appropriate. In creating this file, it is best to start with a template from the current MIT or SOPAC global ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j„@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±Œ file (available in ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ#:file:`incremental_updates/tables/`”j§]”j±Œincremental_updates/tables/”…””}”(j¶j™@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±Œ·) so that you can conveniently add entries for continuous stations from the global file. This template can be header-only, but the preferred approach is to start with the full global ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j®@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±Œ file and use the ”…””}”(j¶jC@jÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-l {}`”j§]”j˜)”}”(j¦jÅ@j§]”j±Œ-l {}”…””}”(j¶jÇ@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jÃ@ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jÑ@Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-l {}”ujÄj‘hjý7jÆK3j¶jC@ubj±Œ option of ”…””}”(j¶jC@jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_upd_stnfo`”j§]”j±Œ sh_upd_stnfo”…””}”(j¶jç@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jC@ubj±Œe to extract only the stations you need, either from an existing list or one created automatically by ”…””}”(j¶jC@jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_upd_stnfo`”j§]”j±Œ sh_upd_stnfo”…””}”(j¶jù@jÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jC@ubj±Œ from the sites with ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`ftprnx`”j§]”j±Œftprnx”…””}”(j¶j AjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jC@ubj±Œ in ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jAjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±Œ* and/or the file names in your experiment ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶j3AjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±ŒR directory. Hence, if you have a current copy of the MIT or SOPAC station.info in ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jHAjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±Œ, have run run ”…””}”(j¶jC@jÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_setup`”j§]”j±Œsh_setup”…””}”(j¶j]AjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jC@ubj±Œ! to copy it into your experiment ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶joAjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±Œ directory, and have edited ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶j„AjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±ŒB to specify the RINEX files you want from a remote archive (using ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`ftprnx`”j§]”j±Œftprnx”…””}”(j¶j™AjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jC@ubj±Œ), you can run (in ”…””}”(j¶jC@jÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶j¬AjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jC@ubj±Œ):”…””}”(j¶jC@jÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK3j¶jþ7jÇjÑ7ubj)”}”(j¦Œ&$ sh_upd_stnfo -ref station.info -l sd”j§]”j±Œ&$ sh_upd_stnfo -ref station.info -l sd”…””}”j¶jÇAsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjý7jÆK9j¶jþ7jÇjÑ7ubj`)”}”(j¦X%which will produce :file:`station.info.new` with the global entries for only the :content:`ftprnx` sites. (If the sites you need from the global :file:`station.info` file are not in :file:`sites.defaults` with :content:`ftprnx`, but are present in the :file:`rinex/` directory, you can use :option:`-l sdrnx` or :option:`-l rnx` in the :program:`sh_upd_stnfo` command.) Then make sure the RINEX files in the experiment :file:`rinex/` directory are not compressed, rename :file:`station.info.new` to :file:`station.info` and run (in :file:`tables/`):”j§]”(j±Œwhich will produce ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info.new`”j§]”j±Œstation.info.new”…””}”(j¶jßAjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Aubj±Œ& with the global entries for only the ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`ftprnx`”j§]”j±Œftprnx”…””}”(j¶jôAjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j×Aubj±Œ/ sites. (If the sites you need from the global ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jBjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Aubj±Œ file are not in ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jBjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Aubj±Œ with ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`ftprnx`”j§]”j±Œftprnx”…””}”(j¶j1BjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j×Aubj±Œ, but are present in the ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶jDBjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Aubj±Œ directory, you can use ”…””}”(j¶j×AjÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-l sdrnx`”j§]”j˜)”}”(j¦j[Bj§]”j±Œ-l sdrnx”…””}”(j¶j]BjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jYBubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jgBŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-l sdrnx”ujÄj‘hjý7jÆK=j¶j×Aubj±Œ or ”…””}”(j¶j×AjÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-l rnx`”j§]”j˜)”}”(j¦jBj§]”j±Œ-l rnx”…””}”(j¶jBjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j}Bubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j‹BŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-l rnx”ujÄj‘hjý7jÆK=j¶j×Aubj±Œ in the ”…””}”(j¶j×AjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_upd_stnfo`”j§]”j±Œ sh_upd_stnfo”…””}”(j¶j¡BjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j×Aubj±Œ< command.) Then make sure the RINEX files in the experiment ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶j³BjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Aubj±Œ& directory are not compressed, rename ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info.new`”j§]”j±Œstation.info.new”…””}”(j¶jÈBjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Aubj±Œ to ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jÝBjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Aubj±Œ and run (in ”…””}”(j¶j×AjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jòBjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Aubj±Œ):”…””}”(j¶j×AjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK=j¶jþ7jÇjÑ7ubj)”}”(j¦Œ!$ sh_upd_stnfo -files ../rinex/*o”j§]”j±Œ!$ sh_upd_stnfo -files ../rinex/*o”…””}”j¶j Csbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjý7jÆKAj¶jþ7jÇjÑ7ubj`)”}”(j¦XK:program:`sh_upd_stnfo` also allows entries for :file:`station.info` to be created from IGS log files or SINEX files. If you construct :file:`station.info` in advance of your processing, set :content:`xstinfo {} all` in :file:`sites.defaults` to block any attempt by :program:`sh_gamit` to update the file from RINEX headers.”j§]”(jj)”}”(j¦Œ:program:`sh_upd_stnfo`”j§]”j±Œ sh_upd_stnfo”…””}”(j¶j!CjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œ also allows entries for ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j3CjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±ŒC to be created from IGS log files or SINEX files. If you construct ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jHCjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œ$ in advance of your processing, set ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`xstinfo {} all`”j§]”j±Œxstinfo {} all”…””}”(j¶j]CjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jCubj±Œ in ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jpCjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œ to block any attempt by ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j…CjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œ' to update the file from RINEX headers.”…””}”(j¶jCjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKEj¶jþ7jÇjÑ7ubj`)”}”(j¦Xî Bad *a priori* coordinates will result in :program:`autcln` detecting too many cycle slips and deleting all of the data. A clear indication that this has happened is :content:`Range rms` values greater than about 20 m at the top of the :file:`autcln.prefit.sum` file together with 0 for :content:`DATA AMOUNTS` in the same file. When this happens, you should check the experiment :file:`tables/lfile.` for the source of the coordinates used. If *a priori* coordinates for a station are not available in the L-file (or :file:`.apr` file) from previous processing, :program:`sh_gamit` will by default invoke the :program:`sh_rx2apr` script to perform a pseudorange solution. Coordinates good to 10–20 m can usually be obtained from the data at the station of interest (better if selective availability is off), but the preferred approach is to perform the solution differentially, using also a RINEX file from an IGS station with known coordinates. To make sure this happens, you should specify :content:`ftprnx` in :file:`sites.defaults` and have present in the :file:`rinex/` directory or available via download from an IGS data archive the RINEX files for each day from one or more IGS stations. (You can use this setting to get a differential pseudorange solution even if you have :option:`-noftp` specified for :program:`sh_gamit` provided you copy the IGS data into the :file:`rinex/` directory in advance of the run.) If a differential pseudorange solution was used and you still have bad coordinates, try executing :program:`sh_rx2apr` manually with data from each of several days and compare the coordinates to see if the day you used originally was an anomaly because it was short or had bad pseudorange data. To by-pass :program:`sh_rx2apr` and use the coordinates from the RINEX header, set :content:`use_rxc = Y` in :file:`process.defaults`. This option should be used only if you know that the header values are always present and accurate or if you have RINEX 3 files, which the programs :program:`svpos` and :program:`svdiff` invoked by :program:`sh_rx2apr` will not yet support. Note that a large adjustment of coordinates, due to bad data or a short session, on one day can cause problems with the next day since :file:`lfile.` in the experiment :file:`tables/` directory will be updated. You can avoid this update by copying into the :content:`aprf` file specified in :file:`process.defaults` any site coordinates that you know to be good; the L-file will be initialized with these values as processing begins for each day.”j§]”(j±ŒBad ”…””}”(j¶jCjÇjÑ7hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j¥CjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jCubj±Œ coordinates will result in ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j·CjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œk detecting too many cycle slips and deleting all of the data. A clear indication that this has happened is ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`Range rms`”j§]”j±Œ Range rms”…””}”(j¶jÉCjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jCubj±Œ2 values greater than about 20 m at the top of the ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`autcln.prefit.sum`”j§]”j±Œautcln.prefit.sum”…””}”(j¶jÜCjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œ file together with 0 for ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`DATA AMOUNTS`”j§]”j±Œ DATA AMOUNTS”…””}”(j¶jñCjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jCubj±ŒF in the same file. When this happens, you should check the experiment ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`tables/lfile.`”j§]”j±Œ tables/lfile.”…””}”(j¶jDjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œ, for the source of the coordinates used. If ”…””}”(j¶jCjÇjÑ7hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jDjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jCubj±Œ? coordinates for a station are not available in the L-file (or ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶j+DjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œ! file) from previous processing, ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j@DjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œ will by default invoke the ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_rx2apr`”j§]”j±Œ sh_rx2apr”…””}”(j¶jRDjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Xm script to perform a pseudorange solution. Coordinates good to 10–20 m can usually be obtained from the data at the station of interest (better if selective availability is off), but the preferred approach is to perform the solution differentially, using also a RINEX file from an IGS station with known coordinates. To make sure this happens, you should specify ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`ftprnx`”j§]”j±Œftprnx”…””}”(j¶jdDjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jCubj±Œ in ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jwDjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œ and have present in the ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶jŒDjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±ŒÐ directory or available via download from an IGS data archive the RINEX files for each day from one or more IGS stations. (You can use this setting to get a differential pseudorange solution even if you have ”…””}”(j¶jCjÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-noftp`”j§]”j˜)”}”(j¦j£Dj§]”j±Œ-noftp”…””}”(j¶j¥DjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j¡Dubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j¯DŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-noftp”ujÄj‘hjý7jÆKHj¶jCubj±Œ specified for ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jÅDjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œ) provided you copy the IGS data into the ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶j×DjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œ… directory in advance of the run.) If a differential pseudorange solution was used and you still have bad coordinates, try executing ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_rx2apr`”j§]”j±Œ sh_rx2apr”…””}”(j¶jìDjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œ¼ manually with data from each of several days and compare the coordinates to see if the day you used originally was an anomaly because it was short or had bad pseudorange data. To by-pass ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_rx2apr`”j§]”j±Œ sh_rx2apr”…””}”(j¶jþDjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œ4 and use the coordinates from the RINEX header, set ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`use_rxc = Y`”j§]”j±Œ use_rxc = Y”…””}”(j¶jEjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jCubj±Œ in ”…””}”j¶jCsbj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶j#EjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œ–. This option should be used only if you know that the header values are always present and accurate or if you have RINEX 3 files, which the programs ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`svpos`”j§]”j±Œsvpos”…””}”(j¶j8EjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œ and ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`svdiff`”j§]”j±Œsvdiff”…””}”(j¶jJEjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œ invoked by ”…””}”(j¶jCjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_rx2apr`”j§]”j±Œ sh_rx2apr”…””}”(j¶j\EjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jCubj±Œž will not yet support. Note that a large adjustment of coordinates, due to bad data or a short session, on one day can cause problems with the next day since ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`lfile.`”j§]”j±Œlfile.”…””}”(j¶jnEjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œ in the experiment ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jƒEjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±ŒJ directory will be updated. You can avoid this update by copying into the ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`aprf`”j§]”j±Œaprf”…””}”(j¶j˜EjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jCubj±Œ file specified in ”…””}”(j¶jCjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶j«EjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jCubj±Œƒ any site coordinates that you know to be good; the L-file will be initialized with these values as processing begins for each day.”…””}”(j¶jCjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKHj¶jþ7jÇjÑ7ubj`)”}”(j¦XV:program:`sh_gamit` can also fail if it is unable to download required global RINEX files or orbital information from an IGS archive (CDDIS or SOPAC if not otherwise specified). The :file:`GAMIT.fatal` message will usually make clear what file is missing. In this case, check the connection to the archive manually and restart the processing.”j§]”(jj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jÊEjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÆEubj±Œ£ can also fail if it is unable to download required global RINEX files or orbital information from an IGS archive (CDDIS or SOPAC if not otherwise specified). The ”…””}”(j¶jÆEjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`GAMIT.fatal`”j§]”j±Œ GAMIT.fatal”…””}”(j¶jÜEjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÆEubj±Œ message will usually make clear what file is missing. In this case, check the connection to the archive manually and restart the processing.”…””}”(j¶jÆEjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKVj¶jþ7jÇjÑ7ubj`)”}”(j¦XËFor the most part, you can rerun a day after a failure with simply a remedy of the detected problem (e.g., a bad :file:`station.info` entry). However, in some circumstances old corrupted files will be used: (a) Unless you specify :option:`-remakex Y` in the command line, any existing x-file in a directory will be used again and the script assumes that there is a valid :file:`station.info` entry for this file (if not, the process will fail). (b) Any existing RINEX file linked in the day directory will be assumed to exist. If the link is now empty because you have renamed or removed the file in the remote directory, this may not be detected correctly on all systems. (c) A previously added :file:`station.info` entry will be used (and not replaced) if it applies to the day being processed. (d) Coordinates in the L-file will be used if they exist (so if the entry has been corrupted it should be removed and/or correct coordinates put in to the :file:`.apr` file).”j§]”(j±ŒqFor the most part, you can rerun a day after a failure with simply a remedy of the detected problem (e.g., a bad ”…””}”(j¶j÷EjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jÿEjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j÷Eubj±Œa entry). However, in some circumstances old corrupted files will be used: (a) Unless you specify ”…””}”(j¶j÷EjÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-remakex Y`”j§]”j˜)”}”(j¦jFj§]”j±Œ -remakex Y”…””}”(j¶jFjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jFubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j"FŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -remakex Y”ujÄj‘hjý7jÆKZj¶j÷Eubj±Œy in the command line, any existing x-file in a directory will be used again and the script assumes that there is a valid ”…””}”(j¶j÷EjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j8FjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j÷Eubj±X1 entry for this file (if not, the process will fail). (b) Any existing RINEX file linked in the day directory will be assumed to exist. If the link is now empty because you have renamed or removed the file in the remote directory, this may not be detected correctly on all systems. (c) A previously added ”…””}”(j¶j÷EjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jMFjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j÷Eubj±Œì entry will be used (and not replaced) if it applies to the day being processed. (d) Coordinates in the L-file will be used if they exist (so if the entry has been corrupted it should be removed and/or correct coordinates put in to the ”…””}”(j¶j÷EjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jbFjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j÷Eubj±Œ file).”…””}”(j¶j÷EjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKZj¶jþ7jÇjÑ7ubj`)”}”(j¦ŒÀDescriptions of how to run :program:`sh_gamit` with sessions crossing day boundaries can be found in Section 6.3 of the `GAMIT Reference Manual `_.”j§]”(j±ŒDescriptions of how to run ”…””}”(j¶j}FjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j…FjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j}Fubj±ŒJ with sessions crossing day boundaries can be found in Section 6.3 of the ”…””}”(j¶j}FjÇjÑ7hNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j—FjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶j}Fubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit-reference-manual”aj»]”j½]”Œgamit reference manual”ajÀ]”jÂ]”Œrefuri”j§FujÄjdj Kj¶j}Fubj±Œ.”…””}”(j¶j}FjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKbj¶jþ7jÇjÑ7ubj`)”}”(j¦Œ‚To generate time series from the GAMIT runs for the three days in the example, type at the project-directory level (:file:`2000/`)”j§]”(j±ŒtTo generate time series from the GAMIT runs for the three days in the example, type at the project-directory level (”…””}”(j¶j¿FjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`2000/`”j§]”j±Œ2000/”…””}”(j¶jÇFjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¿Fubj±Œ)”…””}”(j¶j¿FjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKdj¶jþ7jÇjÑ7ubj)”}”(j¦ŒF$ sh_glred -expt scal -s 2000 034 2000 036 -opt H G T >&! sh_glred.log”j§]”j±ŒF$ sh_glred -expt scal -s 2000 034 2000 036 -opt H G T >&! sh_glred.log”…””}”j¶jâFsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjý7jÆKfj¶jþ7jÇjÑ7ubj`)”}”(j¦ŒkThe script will execute the following steps, noted in the screen output redirected to :file:`sh_glred.log`:”j§]”(j±ŒVThe script will execute the following steps, noted in the screen output redirected to ”…””}”(j¶jòFjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`sh_glred.log`”j§]”j±Œ sh_glred.log”…””}”(j¶júFjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jòFubj±Œ:”…””}”(j¶jòFjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKjj¶jþ7jÇjÑ7ubjX9)”}”(j¦hoj§]”(j˜)”}”(j¦X‹Search all day directories between :file:`034/` and :file:`036/` for GAMIT h-files containing the substring :content:`scal` and run :program:`htoglb` to convert these to binary h-files for :program:`glred`. Since each GAMIT h-file contains two solutions, one with ambiguities estimated as real numbers ("biases free") and one with ambiguities resolved ("biases fixed"), :program:`htoglb` will create two binary h-files, with extents :file:`.glr` (GAMIT loose free) and :file:`.glx` (GAMIT loose fixed), respectively. They are stored in the :file:`glbf/` directory and named with the year/month/day/hr/min, e.g :file:`h0002031200_scal.glx` for day 034.”j§]”j`)”}”(j¦X‹Search all day directories between :file:`034/` and :file:`036/` for GAMIT h-files containing the substring :content:`scal` and run :program:`htoglb` to convert these to binary h-files for :program:`glred`. Since each GAMIT h-file contains two solutions, one with ambiguities estimated as real numbers ("biases free") and one with ambiguities resolved ("biases fixed"), :program:`htoglb` will create two binary h-files, with extents :file:`.glr` (GAMIT loose free) and :file:`.glx` (GAMIT loose fixed), respectively. They are stored in the :file:`glbf/` directory and named with the year/month/day/hr/min, e.g :file:`h0002031200_scal.glx` for day 034.”j§]”(j±Œ#Search all day directories between ”…””}”(j¶jGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`034/`”j§]”j±Œ034/”…””}”(j¶j$GjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jGubj±Œ and ”…””}”(j¶jGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`036/`”j§]”j±Œ036/”…””}”(j¶j9GjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jGubj±Œ, for GAMIT h-files containing the substring ”…””}”(j¶jGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`scal`”j§]”j±Œscal”…””}”(j¶jNGjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jGubj±Œ and run ”…””}”(j¶jGjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`htoglb`”j§]”j±Œhtoglb”…””}”(j¶jaGjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jGubj±Œ( to convert these to binary h-files for ”…””}”(j¶jGjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jsGjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jGubj±Œ­. Since each GAMIT h-file contains two solutions, one with ambiguities estimated as real numbers (“biases freeâ€) and one with ambiguities resolved (“biases fixedâ€), ”…””}”(j¶jGjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`htoglb`”j§]”j±Œhtoglb”…””}”(j¶j…GjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jGubj±Œ. will create two binary h-files, with extents ”…””}”(j¶jGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.glr`”j§]”j±Œ.glr”…””}”(j¶j—GjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jGubj±Œ (GAMIT loose free) and ”…””}”(j¶jGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.glx`”j§]”j±Œ.glx”…””}”(j¶j¬GjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jGubj±Œ; (GAMIT loose fixed), respectively. They are stored in the ”…””}”(j¶jGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`glbf/`”j§]”j±Œglbf/”…””}”(j¶jÁGjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jGubj±Œ9 directory and named with the year/month/day/hr/min, e.g ”…””}”(j¶jGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`h0002031200_scal.glx`”j§]”j±Œh0002031200_scal.glx”…””}”(j¶jÖGjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jGubj±Œ for day 034.”…””}”(j¶jGjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKlj¶jGubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jGjÇjÑ7hjý7jÆNubj˜)”}”(j¦ŒrGenerate in the :file:`gsoln/` directory a :file:`.gdl` file (h-file list) for each day (:file:`.glx` is default).”j§]”j`)”}”(j¦jùGj§]”(j±ŒGenerate in the ”…””}”(j¶jûGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶jHjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jûGubj±Œ directory a ”…””}”(j¶jûGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶jHjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jûGubj±Œ" file (h-file list) for each day (”…””}”(j¶jûGjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.glx`”j§]”j±Œ.glx”…””}”(j¶j,HjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jûGubj±Œ is default).”…””}”(j¶jûGjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKoj¶j÷Gubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jGjÇjÑ7hjý7jÆNubj˜)”}”(j¦ŒðRun :program:`glred` for each day, using commands of the form .. code:: console $ glred 6 globk_scat_00034.prt globk_scal_00034.log globk_scal_00034.gdl globk.cmd The :file:`.log` and :file:`.org` files provide a record of the output.”j§]”(j`)”}”(j¦Œ=Run :program:`glred` for each day, using commands of the form”j§]”(j±ŒRun ”…””}”(j¶jQHjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jYHjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jQHubj±Œ) for each day, using commands of the form”…””}”(j¶jQHjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKpj¶jMHubj)”}”(j¦ŒR$ glred 6 globk_scat_00034.prt globk_scal_00034.log globk_scal_00034.gdl globk.cmd”j§]”j±ŒR$ glred 6 globk_scat_00034.prt globk_scal_00034.log globk_scal_00034.gdl globk.cmd”…””}”j¶jqHsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œforce”‰Œhighlight_args”}”j/j0hyŒconsole”ujÄjhjý7jÆKrj¶jMHubj`)”}”(j¦ŒGThe :file:`.log` and :file:`.org` files provide a record of the output.”j§]”(j±ŒThe ”…””}”(j¶jƒHjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.log`”j§]”j±Œ.log”…””}”(j¶j‹HjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jƒHubj±Œ and ”…””}”(j¶jƒHjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶j HjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jƒHubj±Œ& files provide a record of the output.”…””}”(j¶jƒHjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKvj¶jMHubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jGjÇjÑ7hjý7jÆNubj˜)”}”(j¦XRun :program:`sh_plot_pos` to invoke program :program:`tssum` to create PBO-format :file:`.pos` files from the coordinates of each site on each day in the :file:`.org` files and invoke GMT to plot the time series. (Specifying :option:`E` instead of :option:`T` on the command line will use the older program :program:`ensum` to generate :file:`mb_` files for plotting with :program:`sh_plotcrd`.) ”j§]”j`)”}”(j¦XŒRun :program:`sh_plot_pos` to invoke program :program:`tssum` to create PBO-format :file:`.pos` files from the coordinates of each site on each day in the :file:`.org` files and invoke GMT to plot the time series. (Specifying :option:`E` instead of :option:`T` on the command line will use the older program :program:`ensum` to generate :file:`mb_` files for plotting with :program:`sh_plotcrd`.)”j§]”(j±ŒRun ”…””}”(j¶jÅHjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶jÍHjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÅHubj±Œ to invoke program ”…””}”(j¶jÅHjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`tssum`”j§]”j±Œtssum”…””}”(j¶jßHjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÅHubj±Œ to create PBO-format ”…””}”(j¶jÅHjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.pos`”j§]”j±Œ.pos”…””}”(j¶jñHjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÅHubj±Œ< files from the coordinates of each site on each day in the ”…””}”(j¶jÅHjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶jIjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÅHubj±Œ; files and invoke GMT to plot the time series. (Specifying ”…””}”(j¶jÅHjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`E`”j§]”j˜)”}”(j¦jIj§]”j±ŒE”…””}”(j¶jIjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jIubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j)IŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒE”ujÄj‘hjý7jÆKwj¶jÅHubj±Œ instead of ”…””}”(j¶jÅHjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`T`”j§]”j˜)”}”(j¦jAIj§]”j±ŒT”…””}”(j¶jCIjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j?Iubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jMIŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒT”ujÄj‘hjý7jÆKwj¶jÅHubj±Œ0 on the command line will use the older program ”…””}”(j¶jÅHjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`ensum`”j§]”j±Œensum”…””}”(j¶jcIjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÅHubj±Œ to generate ”…””}”(j¶jÅHjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`mb_`”j§]”j±Œmb_”…””}”(j¶juIjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÅHubj±Œ files for plotting with ”…””}”(j¶jÅHjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_plotcrd`”j§]”j±Œ sh_plotcrd”…””}”(j¶jŠIjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÅHubj±Œ.)”…””}”(j¶jÅHjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKwj¶jÁHubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jGjÇjÑ7hjý7jÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j“>j”>j•>hoj–>j—>ujÄjW9j¶jþ7jÇjÑ7hjý7jÆKlubj`)”}”(j¦X»This task could be accomplished in individual steps by running :program:`htoglb` directly with wild cards specifying the day directories, creating a :file:`.gdl` file in :file:`gsoln/` using :console:`ls ../glbf/h*glx`, running the program :program:`glred` (rather than the script :program:`sh_glred`) with this :file:`.gdl` file, and running :program:`sh_plot_pos`. In fact, for velocity solutions and time series using combined files, you will need to use this approach (see Chapter 4). The advantages of the script are threefold: 1) fewer commands, 2) it allows easy daily combination of local h-files with those from an external processing center (e.g. MIT or SOPAC), using the :option:`LA`, :option:`LB` and :option:`LC` options (see :numref:`intro_prod_combine`); and 3) it allows easy aggregation of days into weekly or monthly combined h-files, using the :option:`-ncomb` option (see the :program:`sh_glred` help by typing the command without arguments). You can mix using :program:`sh_glred` with running :program:`glred` directly as long as you keep in mind two differences: 1) :program:`sh_glred`, like :program:`sh_gamit`, is launched from the project directory but executes :program:`glred` within the :file:`gsoln/` directory whereas :program:`glred` is launched directly from within the :file:`gsoln/` directory itself; and 2) :program:`sh_glred` creates a :file:`.gdl` file for each day whereas running :program:`glred` itself efficiently requires creating a single :file:`.gdl` file containing the h-files for all of the days. In a :file:`.gdl` file, the :content:`+` symbol is used to indicate to :program:`glred` that h-files are to be combined before performing the solution. For example, using the file”j§]”(j±Œ?This task could be accomplished in individual steps by running ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`htoglb`”j§]”j±Œhtoglb”…””}”(j¶j¶IjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±ŒE directly with wild cards specifying the day directories, creating a ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶jÈIjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®Iubj±Œ file in ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶jÝIjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®Iubj±Œ using ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:console:`ls ../glbf/h*glx`”j§]”j±Œls ../glbf/h*glx”…””}”(j¶jòIjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j®Iubj±Œ, running the program ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(•j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jJjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ (rather than the script ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jJjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ ) with this ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶j)JjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®Iubj±Œ file, and running ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶j>JjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±X=. In fact, for velocity solutions and time series using combined files, you will need to use this approach (see Chapter 4). The advantages of the script are threefold: 1) fewer commands, 2) it allows easy daily combination of local h-files with those from an external processing center (e.g. MIT or SOPAC), using the ”…””}”(j¶j®IjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`LA`”j§]”j˜)”}”(j¦jRJj§]”j±ŒLA”…””}”(j¶jTJjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jPJubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j^JŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLA”ujÄj‘hjý7jÆKzj¶j®Iubj±Œ, ”…””}”(j¶j®IjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`LB`”j§]”j˜)”}”(j¦jvJj§]”j±ŒLB”…””}”(j¶jxJjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jtJubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j‚JŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLB”ujÄj‘hjý7jÆKzj¶j®Iubj±Œ and ”…””}”(j¶j®IjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`LC`”j§]”j˜)”}”(j¦jšJj§]”j±ŒLC”…””}”(j¶jœJjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j˜Jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j¦JŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLC”ujÄj‘hjý7jÆKzj¶j®Iubj±Œ options (see ”…””}”(j¶j®IjÇjÑ7hNjÆNubj’)”}”(j¦Œ:numref:`intro_prod_combine`”j§]”j˜)”}”(j¦j¾Jj§]”j±Œintro_prod_combine”…””}”(j¶jÀJjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶j¼Jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jÊJŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_prod_combine”ujÄj‘hjý7jÆKzj¶j®Iubj±Œ`); and 3) it allows easy aggregation of days into weekly or monthly combined h-files, using the ”…””}”(j¶j®IjÇjÑ7hNjÆNubj’)”}”(j¦Œ:option:`-ncomb`”j§]”j˜)”}”(j¦jâJj§]”j±Œ-ncomb”…””}”(j¶jäJjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jàJubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jîJŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-ncomb”ujÄj‘hjý7jÆKzj¶j®Iubj±Œ option (see the ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jKjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±ŒB help by typing the command without arguments). You can mix using ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jKjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ with running ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j(KjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ: directly as long as you keep in mind two differences: 1) ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j:KjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ, like ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jLKjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ6, is launched from the project directory but executes ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j^KjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ within the ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶jpKjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®Iubj±Œ directory whereas ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j…KjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ& is launched directly from within the ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶j—KjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®Iubj±Œ directory itself; and 2) ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j¬KjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ creates a ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶j¾KjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®Iubj±Œ# file for each day whereas running ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jÓKjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ/ itself efficiently requires creating a single ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶jåKjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®Iubj±Œ7 file containing the h-files for all of the days. In a ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶júKjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®Iubj±Œ file, the ”…””}”(j¶j®IjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :content:`+`”j§]”j±Œ+”…””}”(j¶jLjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j®Iubj±Œ symbol is used to indicate to ”…””}”(j¶j®IjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j"LjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®Iubj±Œ\ that h-files are to be combined before performing the solution. For example, using the file”…””}”(j¶j®IjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKzj¶jþ7jÇjÑ7ubj)”}”(j¦X../glbf/h1211021200_pan1.glx 1.0 + ../glf/h1211021200_pan2.glx 1.0 + ../glbf/h1211021200_pcnw.glx 1.0 + ../glbf/nmt17125.e.glb 1.0 ../glbf/h1211031200_pan1.glx 1.0 + ../glbf/h1211031200_pan2.glx 1.0 + ../glbf/h1211031200_pcnw.glx 1.0 + ../glbf/nmt17126.e.glb 1.0”j§]”j±X../glbf/h1211021200_pan1.glx 1.0 + ../glf/h1211021200_pan2.glx 1.0 + ../glbf/h1211021200_pcnw.glx 1.0 + ../glbf/nmt17125.e.glb 1.0 ../glbf/h1211031200_pan1.glx 1.0 + ../glbf/h1211031200_pan2.glx 1.0 + ../glbf/h1211031200_pcnw.glx 1.0 + ../glbf/nmt17126.e.glb 1.0”…””}”j¶j:Lsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjý7jÆK†j¶jþ7jÇjÑ7ubj`)”}”(j¦XF:program:`glred` would combine all four h-files for day 2012-11-02 before performing a solution, and then do the same thing for the four files for day 2012-11-03. (Running :program:`globk`, rather than :program:`glred`, would combine all of the files listed into a single solution whether or not the :content:`+` are present).”j§]”(jj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jNLjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jJLubj±Œœ would combine all four h-files for day 2012-11-02 before performing a solution, and then do the same thing for the four files for day 2012-11-03. (Running ”…””}”(j¶jJLjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j`LjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jJLubj±Œ, rather than ”…””}”(j¶jJLjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jrLjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jJLubj±ŒR, would combine all of the files listed into a single solution whether or not the ”…””}”(j¶jJLjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :content:`+`”j§]”j±Œ+”…””}”(j¶j„LjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jJLubj±Œ are present).”…””}”(j¶jJLjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK‘j¶jþ7jÇjÑ7ubj`)”}”(j¦X4Other options of :program:`sh_glred` specify the downloading of data from a remote archive (:option:`F`), removal of old h-files from the :content:`glfpth` directory (:option:`R`), and compressing the h-files at the end of the run (:option:`C`). Type :program:`sh_glred` without arguments to see all options.”j§]”(j±ŒOther options of ”…””}”(j¶jLjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j¥LjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jLubj±Œ8 specify the downloading of data from a remote archive (”…””}”(j¶jLjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`F`”j§]”j˜)”}”(j¦j¹Lj§]”j±ŒF”…””}”(j¶j»LjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j·Lubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jÅLŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒF”ujÄj‘hjý7jÆK”j¶jLubj±Œ#), removal of old h-files from the ”…””}”(j¶jLjÇjÑ7hNjÆNubj˜)”}”(j¦Œ:content:`glfpth`”j§]”j±Œglfpth”…””}”(j¶jÛLjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jLubj±Œ directory (”…””}”(j¶jLjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`R`”j§]”j˜)”}”(j¦jðLj§]”j±ŒR”…””}”(j¶jòLjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jîLubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jüLŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒR”ujÄj‘hjý7jÆK”j¶jLubj±Œ6), and compressing the h-files at the end of the run (”…””}”(j¶jLjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`C`”j§]”j˜)”}”(j¦jMj§]”j±ŒC”…””}”(j¶jMjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jMubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j MŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒC”ujÄj‘hjý7jÆK”j¶jLubj±Œ). Type ”…””}”(j¶jLjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j6MjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jLubj±Œ& without arguments to see all options.”…””}”(j¶jLjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK”j¶jþ7jÇjÑ7ubj`)”}”(j¦X°To avoid overwriting useful h-files or using obsolete ones, it is important to keep in mind the precedence rules of the script. For local data (:program:`sh_gamit` day directories), specifying the :option:`H` option will force :program:`htoglb` to be rerun for all directories within the time span indicated, whether or not a binary file or link exists in the :file:`glbf/` directory. Omitting :option:`H` will cause no new binary files to be created, so it is not possible to retranslate only a selected group of ascii H-files. This is not an important limitation, however, because :program:`htoglb` runs quickly. For global ascii h-files downloaded from SOPAC, setting :option:`H` will also force :program:`htoglb` to be rerun on any ascii H-files present or linked (by :option:`LA`) in the H-file (:file:`glbf/`) directory, but you can safely set :option:`F` since the script will not re-download any remote (ascii) H-files that are present.”j§]”(j±ŒTo avoid overwriting useful h-files or using obsolete ones, it is important to keep in mind the precedence rules of the script. For local data (”…””}”(j¶jNMjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jVMjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNMubj±Œ" day directories), specifying the ”…””}”(j¶jNMjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`H`”j§]”j˜)”}”(j¦jjMj§]”j±ŒH”…””}”(j¶jlMjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jhMubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jvMŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒH”ujÄj‘hjý7jÆK—j¶jNMubj±Œ option will force ”…””}”(j¶jNMjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`htoglb`”j§]”j±Œhtoglb”…””}”(j¶jŒMjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNMubj±Œt to be rerun for all directories within the time span indicated, whether or not a binary file or link exists in the ”…””}”(j¶jNMjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`glbf/`”j§]”j±Œglbf/”…””}”(j¶jžMjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jNMubj±Œ directory. Omitting ”…””}”(j¶jNMjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`H`”j§]”j˜)”}”(j¦jµMj§]”j±ŒH”…””}”(j¶j·MjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j³Mubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jÁMŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶j‡MujÄj‘hjý7jÆK—j¶jNMubj±Œ² will cause no new binary files to be created, so it is not possible to retranslate only a selected group of ascii H-files. This is not an important limitation, however, because ”…””}”(j¶jNMjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`htoglb`”j§]”j±Œhtoglb”…””}”(j¶jÖMjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNMubj±ŒG runs quickly. For global ascii h-files downloaded from SOPAC, setting ”…””}”(j¶jNMjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`H`”j§]”j˜)”}”(j¦jêMj§]”j±ŒH”…””}”(j¶jìMjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jèMubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jöMŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶j‡MujÄj‘hjý7jÆK—j¶jNMubj±Œ will also force ”…””}”(j¶jNMjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`htoglb`”j§]”j±Œhtoglb”…””}”(j¶j NjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNMubj±Œ8 to be rerun on any ascii H-files present or linked (by ”…””}”(j¶jNMjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`LA`”j§]”j˜)”}”(j¦jNj§]”j±ŒLA”…””}”(j¶j!NjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”j+NŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLA”ujÄj‘hjý7jÆK—j¶jNMubj±Œ) in the H-file (”…””}”(j¶jNMjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`glbf/`”j§]”j±Œglbf/”…””}”(j¶jANjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jNMubj±Œ$) directory, but you can safely set ”…””}”(j¶jNMjÇjÑ7hNjÆNubj’)”}”(j¦Œ :option:`F`”j§]”j˜)”}”(j¦jXNj§]”j±ŒF”…””}”(j¶jZNjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jVNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jÿŒ refdomain”jdNŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶jÖLujÄj‘hjý7jÆK—j¶jNMubj±ŒS since the script will not re-download any remote (ascii) H-files that are present.”…””}”(j¶jNMjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆK—j¶jþ7jÇjÑ7ubj`)”}”(j¦XDNote that most of the shell scripts called by :program:`sh_gamit` and :program:`sh_glred` can be run stand-alone for specific processing tasks. The most useful of these are :program:`sh_make_rinex` (templates for running :program:`teqc` to translate raw data files), :program:`sh_get_nav`, :program:`sh_get_rinex`, :program:`sh_get_orbits`, :program:`sh_sp3fit`, :program:`sh_update_eop`, :program:`sh_link_rinex`, :program:`sh_oneway` (to get sky plots from :file:`DPH` files), and :program:`sh_get_hfiles`. Type the name of the script without arguments to see the documentation.”j§]”(j±Œ.Note that most of the shell scripts called by ”…””}”(j¶jNjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j‡NjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ and ”…””}”(j¶jNjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j™NjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±ŒT can be run stand-alone for specific processing tasks. The most useful of these are ”…””}”(j¶jNjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_make_rinex`”j§]”j±Œ sh_make_rinex”…””}”(j¶j«NjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ (templates for running ”…””}”(j¶jNjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`teqc`”j§]”j±Œteqc”…””}”(j¶j½NjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ to translate raw data files), ”…””}”(j¶jNjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_get_nav`”j§]”j±Œ sh_get_nav”…””}”(j¶jÏNjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ, ”…””}”(j¶jNjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_get_rinex`”j§]”j±Œ sh_get_rinex”…””}”(j¶jáNjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ, ”…””}”j¶jNsbjj)”}”(j¦Œ:program:`sh_get_orbits`”j§]”j±Œ sh_get_orbits”…””}”(j¶jóNjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ, ”…””}”j¶jNsbjj)”}”(j¦Œ:program:`sh_sp3fit`”j§]”j±Œ sh_sp3fit”…””}”(j¶jOjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ, ”…””}”j¶jNsbjj)”}”(j¦Œ:program:`sh_update_eop`”j§]”j±Œ sh_update_eop”…””}”(j¶jOjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ, ”…””}”j¶jNsbjj)”}”(j¦Œ:program:`sh_link_rinex`”j§]”j±Œ sh_link_rinex”…””}”(j¶j)OjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ, ”…””}”j¶jNsbjj)”}”(j¦Œ:program:`sh_oneway`”j§]”j±Œ sh_oneway”…””}”(j¶j;OjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±Œ (to get sky plots from ”…””}”(j¶jNjÇjÑ7hNjÆNubj˜)”}”(j¦Œ :file:`DPH`”j§]”j±ŒDPH”…””}”(j¶jMOjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jNubj±Œ files), and ”…””}”(j¶jNjÇjÑ7hNjÆNubjj)”}”(j¦Œ:program:`sh_get_hfiles`”j§]”j±Œ sh_get_hfiles”…””}”(j¶jbOjÇjÑ7hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jNubj±ŒI. Type the name of the script without arguments to see the documentation.”…””}”(j¶jNjÇjÑ7hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjý7jÆKj¶jþ7jÇjÑ7ubej·}”(j¹]”(Œusing-sh-gamit-and-sh-glred”jü7ej»]”j½]”(Œusing sh_gamit and sh_glred”Œintro_proc_example”ejÀ]”jÂ]”ujÄh_j¶jÑ7jÇjÑ7hjý7jÆKjÒ }”j€Ojò7sjÔ }”jü7jò7subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jý7j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjý7jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jà7jÔ7jï7jã7uj_}”(Œrel”jà7Œdate”jï7ujc}”je}”jü7]”jò7asjg}”(j€Ojü7jOj|Oj±Fj®Fuji}”(j€OˆjO‰j±Fˆuj¹}”(jü7jþ7j|Ojþ7j®Fj¨Fujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ8Hyperlink target "intro-proc-example" is not referenced.”…””}”j¶jªOsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j§Oubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jý7Œline”KujÄjø ubajˆNj‰]”j‹NjÇjÑ7ubj j£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jÅOsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÂOjÇjÂOubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jÔOjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÂOjÇjÂOubje)”}”(j¦Œ.. _intro_proc_flow:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-flow”ujÄjdjÆKj¶jÂOjÇjÂOhŒC/chandler/home/floyd/public_html/gg/docs/source/intro/proc/flow.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒSummary of Program Flow”j§]”j±ŒSummary of Program Flow”…””}”(j¶jòOjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jïOjÇjÂOhjîOjÆKubj`)”}”(j¦X<To understand how to set up input controls and evaluate your solution, you need to have in mind the data and solution files produced at each step. The examples below are from the 5-station 2000 February 3rd (day-of-year 034) GPS-only Southern California survey used in previous releases for testing the installation.”j§]”j±X<To understand how to set up input controls and evaluate your solution, you need to have in mind the data and solution files produced at each step. The examples below are from the 5-station 2000 February 3rd (day-of-year 034) GPS-only Southern California survey used in previous releases for testing the installation.”…””}”(j¶jPjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKj¶jïOjÇjÂOubj©hc“”)”}”(j¦hoj§]”j©Œtgroup”“”)”}”(j¦hoj§]”(j©Œcolspec”“”)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œcolwidth”K!ujÄjPj¶jPubjP)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j"PK!ujÄjPj¶jPubjP)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j"PK!ujÄjPj¶jPubj©Œtbody”“”)”}”(j¦hoj§]”(j©Œrow”“”)”}”(j¦hoj§]”(j©j0“”)”}”(j¦hoj§]”j`)”}”(j¦Œ**File**”j§]”j>)”}”(j¦jEPj§]”j±ŒFile”…””}”(j¶jGPjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjœ>j¶jCPubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK j¶j@Pubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j)”}”(j¦jePj§]”j±Œ Name example”…””}”(j¶jgPjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjœ>j¶jcPubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK j¶j`Pubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j)”}”(j¦j…Pj§]”j±Œ Description”…””}”(j¶j‡PjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjœ>j¶jƒPubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKj¶j€Pubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j`_; naming of c-files and a description of the q- and o-files produced by :program:`solve` is in Chapter 3. Of the GAMIT-produced files, only the h-file has more than a one-digit year in its name since it is the only file that is carried beyond the processing for a single survey. The :file:`.org` file is described in Chapter 3 below.”j§]”(j±XNote that GAMIT files are named with single- or two-digit years and day-of-year and have a required format, whereas GLOBK h-filenames are arbitrary but conventionally named with two-digit year, month, day, hour, and minute. A full description of the preprocessing steps undertaken by ”…””}”(j¶jXTjÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`makexp`”j§]”j±Œmakexp”…””}”(j¶j`TjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jXTubj±Œ and ”…””}”(j¶jXTjÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`makex`”j§]”j±Œmakex”…””}”(j¶jrTjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jXTubj±ŒG to produce x-files and the coordinate, clock, and orbit files used by ”…””}”(j¶jXTjÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶j„TjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jXTubj±Œ" can be found in Chapter 2 of the ”…””}”(j¶jXTjÇjÂOhNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j–TjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶jXTubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit-reference-manual”aj»]”j½]”Œgamit reference manual”ajÀ]”jÂ]”Œrefuri”j¦TujÄjdj Kj¶jXTubj±ŒH; naming of c-files and a description of the q- and o-files produced by ”…””}”(j¶jXTjÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶j¸TjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jXTubj±ŒÃ is in Chapter 3. Of the GAMIT-produced files, only the h-file has more than a one-digit year in its name since it is the only file that is carried beyond the processing for a single survey. The ”…””}”(j¶jXTjÇjÂOhNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶jÊTjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jXTubj±Œ& file is described in Chapter 3 below.”…””}”(j¶jXTjÇjÂOhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK%j¶jïOjÇjÂOubj`)”}”(j¦XñIt is also useful to have in mind the way the files containing external data, survey metadata, and command files get from their natural homes to the day directory for processing. "Global" files, which contain information useful for many surveys reside in :file:`~/gg/tables` but are linked by :program:`sh_gamit` into the project :file:`tables/` directory (script :program:`sh_link_tables`) and then into the day directory (script :program:`links.day`), usually under the same name. These include:”j§]”(j±XIt is also useful to have in mind the way the files containing external data, survey metadata, and command files get from their natural homes to the day directory for processing. “Global†files, which contain information useful for many surveys reside in ”…””}”(j¶jåTjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables`”j§]”j±Œ ~/gg/tables”…””}”(j¶jíTjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jåTubj±Œ but are linked by ”…””}”(j¶jåTjÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jUjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jåTubj±Œ into the project ”…””}”(j¶jåTjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jUjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jåTubj±Œ directory (script ”…””}”(j¶jåTjÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`sh_link_tables`”j§]”j±Œsh_link_tables”…””}”(j¶j)UjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jåTubj±Œ*) and then into the day directory (script ”…””}”(j¶jåTjÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`links.day`”j§]”j±Œ links.day”…””}”(j¶j;UjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jåTubj±Œ.), usually under the same name. These include:”…””}”(j¶jåTjÇjÂOhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK+j¶jïOjÇjÂOubjP)”}”(j¦hoj§]”jP)”}”(j¦hoj§]”(jP)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j"PK2ujÄjPj¶jVUubjP)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j"PK2ujÄjPj¶jVUubj6P)”}”(j¦hoj§]”(j;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦ŒEOP tables from the IERS”j§]”j±ŒEOP tables from the IERS”…””}”(j¶jtUjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK1j¶jqUubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jnUubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ:file:`ut1.` :file:`pole.`”j§]”(j˜)”}”(j¦Œ :file:`ut1.`”j§]”j±Œut1.”…””}”(j¶jUjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹Uubj±Œ ”…””}”(j¶j‹UjÇjÂOhNjÆNubj˜)”}”(j¦Œ :file:`pole.`”j§]”j±Œpole.”…””}”(j¶j¤UjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹Uubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK2j¶jˆUubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jnUubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦ŒLunar-solar ephemerides”j§]”j±ŒLunar-solar ephemerides”…””}”(j¶jÍUjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK3j¶jÊUubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jÇUubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ :file:`nbody`”j§]”j˜)”}”(j¦jæUj§]”j±Œnbody”…””}”(j¶jèUjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jäUubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK4j¶jáUubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jÇUubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦Œ :math:`\text{GPST} - \text{UTC}`”j§]”jO )”}”(j¦Œ :math:`\text{GPST} - \text{UTC}`”j§]”j±Œ\text{GPST} - \text{UTC}”…””}”(j¶jVjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jVubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK5j¶j Vubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j Vubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ:file:`leap.sec`”j§]”j˜)”}”(j¦j3Vj§]”j±Œleap.sec”…””}”(j¶j5VjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j1Vubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK6j¶j.Vubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j Vubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦ŒIGS receiver/antenna codes”j§]”j±ŒIGS receiver/antenna codes”…””}”(j¶j]VjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK7j¶jZVubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jWVubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ:file:`rcvant.dat`”j§]”j˜)”}”(j¦jvVj§]”j±Œ rcvant.dat”…””}”(j¶jxVjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jtVubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK8j¶jqVubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jWVubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦Œ$User-defined receiver/antenna codes1”j§]”j±Œ$User-defined receiver/antenna codes1”…””}”(j¶j VjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK9j¶jVubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jšVubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ:file:`guess_rcvant.dat`”j§]”j˜)”}”(j¦j¹Vj§]”j±Œguess_rcvant.dat”…””}”(j¶j»VjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j·Vubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK:j¶j´Vubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jšVubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦Œ$Ground antenna mechanical dimensions”j§]”j±Œ$Ground antenna mechanical dimensions”…””}”(j¶jãVjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK;j¶jàVubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jÝVubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ:file:`hi.dat`”j§]”j˜)”}”(j¦jüVj§]”j±Œhi.dat”…””}”(j¶jþVjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶júVubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKj¶j:Wubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j Wubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦Œ%Ground/SV antenna phase center models”j§]”j±Œ%Ground/SV antenna phase center models”…””}”(j¶jiWjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK?j¶jfWubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jcWubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ:file:`antmod.dat`”j§]”j˜)”}”(j¦j‚Wj§]”j±Œ antmod.dat”…””}”(j¶j„WjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j€Wubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK@j¶j}Wubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jcWubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦ŒP1-C1, P1-P2 code biases”j§]”j±ŒP1-C1, P1-P2 code biases”…””}”(j¶j¬WjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKAj¶j©Wubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j¦Wubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ:file:`dcb.dat`”j§]”j˜)”}”(j¦jÅWj§]”j±Œdcb.dat”…””}”(j¶jÇWjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÃWubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKBj¶jÀWubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j¦Wubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦Œ%Empirical ZHD &mapping functions (MF)”j§]”j±Œ%Empirical ZHD &mapping functions (MF)”…””}”(j¶jïWjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKCj¶jìWubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jéWubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ:file:`gpt.grid`”j§]”j˜)”}”(j¦jXj§]”j±Œgpt.grid”…””}”(j¶j XjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jXubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKDj¶jXubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jéWubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦Œ$Time- and space-dependent ZHD and MF”j§]”j±Œ$Time- and space-dependent ZHD and MF”…””}”(j¶j2XjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKEj¶j/Xubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j,Xubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ!:file:`map.grid` :file:`map.list`”j§]”(j˜)”}”(j¦Œ:file:`map.grid`”j§]”j±Œmap.grid”…””}”(j¶jMXjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jIXubj±Œ ”…””}”(j¶jIXjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`map.list`”j§]”j±Œmap.list”…””}”(j¶jbXjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jIXubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKFj¶jFXubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j,Xubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦Œ Ocean loading”j§]”j±Œ Ocean loading”…””}”(j¶j‹XjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKGj¶jˆXubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j…Xubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ!:file:`otl.grid` :file:`otl.list`”j§]”(j˜)”}”(j¦Œ:file:`otl.grid`”j§]”j±Œotl.grid”…””}”(j¶j¦XjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¢Xubj±Œ ”…””}”(j¶j¢XjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`otl.list`”j§]”j±Œotl.list”…””}”(j¶j»XjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¢Xubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKHj¶jŸXubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j…Xubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦ŒAtmospheric tidal loading”j§]”j±ŒAtmospheric tidal loading”…””}”(j¶jäXjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKIj¶jáXubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jÞXubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ!:file:`atl.grid` :file:`atl.list`”j§]”(j˜)”}”(j¦Œ:file:`atl.grid`”j§]”j±Œatl.grid”…””}”(j¶jÿXjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jûXubj±Œ ”…””}”(j¶jûXjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`atl.list`”j§]”j±Œatl.list”…””}”(j¶jYjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jûXubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKJj¶jøXubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶jÞXubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubj;P)”}”(j¦hoj§]”(j?P)”}”(j¦hoj§]”j`)”}”(j¦ŒNon-tidal atmospheric loading”j§]”j±ŒNon-tidal atmospheric loading”…””}”(j¶j=YjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKKj¶j:Yubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j7Yubj?P)”}”(j¦hoj§]”j`)”}”(j¦Œ#:file:`atml.grid` :file:`atml.list`”j§]”(j˜)”}”(j¦Œ:file:`atml.grid`”j§]”j±Œ atml.grid”…””}”(j¶jXYjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jTYubj±Œ ”…””}”(j¶jTYjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`atml.list`”j§]”j±Œ atml.list”…””}”(j¶jmYjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jTYubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKLj¶jQYubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj0j¶j7Yubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj:Pj¶jkUubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj5Pj¶jVUubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œcols”KujÄjPj¶jSUubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄhcj¶jïOjÇjÂOhNjÆNubj`)”}”(j¦X“The particular version of each of these files is specified by the link in :file:`~/gg/tables/` or the project :file:`tables/` directory. For example, the FES2004 ocean loading model is selected by linking :file:`otl.grid` to :file:`otl_FES2004.grid` in :file:`~/gg/tables/`. For EOP tables, the source (e.g., IERS Bulletin A, coded as :content:`usno` or :content:`usnd`) is specified in :file:`process.defaults` or the :program:`sh_gamit` command line and implemented via the link in the project :file:`tables/` directory. For the non-tidal atmospheric loading (:file:`otl.grid`) and the atmospheric delay (:file:`map.grid`) files the link in the project :file:`tables/` directory is made to a :file:`~/gg/tables/` version for the appropriate year. The grid files for VMF1, atmospheric tidal loading, and non-tidal atmospheric loading may not be needed for most analyses, so their links can remain empty (see below for :file:`sestbl.` entries). **All of these global tables need to be updated from time to time**—the EOP and the VMF1 and ATML grid files daily or weekly if you are processing in near real-time; :file:`dcb.dat` monthly; :file:`leap.sec` yearly; :file:`svnav.dat` whenever a new satellite is launched; and the receiver/antenna tables whenever new instrumentation appears. Note that with the 10.7 release the Earth and Sun positions are obtained from a 20-year tabulation, file named :file:`nbody` which may be linked in :file:`~/gg/tables/` either to the MIT/CfA file :file:`nbody740.2020.asc` used in the past to produce :file:`soltab.` and :file:`luntab.` for each year or to the JPL file :file:`JPL.DE200`, which is the IGS standard. We've found no significant difference in GPS orbital accuracy between the two ephemerides and hence have created the link in :file:`~/gg/tables/` to the MIT/CfA file for continuity. Nutation, which were tabulated in :file:`nutabl.` for each year from an IERS-produced subroutine, are now computed internally from the subroutine. If the :file:`nbody` link is empty, GAMIT will revert to using :file:`soltab.{}`, :file:`luntab.{}`, and :file:`nutabl.{}` which are available through 2018 but will not be created in the future.”j§]”(j±ŒJThe particular version of each of these files is specified by the link in ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶j«YjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ or the project ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jÀYjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±ŒP directory. For example, the FES2004 ocean loading model is selected by linking ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`otl.grid`”j§]”j±Œotl.grid”…””}”(j¶jÕYjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ to ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`otl_FES2004.grid`”j§]”j±Œotl_FES2004.grid”…””}”(j¶jêYjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ in ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jÿYjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ>. For EOP tables, the source (e.g., IERS Bulletin A, coded as ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:content:`usno`”j§]”j±Œusno”…””}”(j¶jZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j£Yubj±Œ or ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:content:`usnd`”j§]”j±Œusnd”…””}”(j¶j'ZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j£Yubj±Œ) is specified in ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶j:ZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ or the ”…””}”(j¶j£YjÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jOZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j£Yubj±Œ: command line and implemented via the link in the project ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jaZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ3 directory. For the non-tidal atmospheric loading (”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`otl.grid`”j§]”j±Œotl.grid”…””}”(j¶jvZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ) and the atmospheric delay (”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`map.grid`”j§]”j±Œmap.grid”…””}”(j¶j‹ZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ ) files the link in the project ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶j ZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ directory is made to a ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jµZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±ŒÍ version for the appropriate year. The grid files for VMF1, atmospheric tidal loading, and non-tidal atmospheric loading may not be needed for most analyses, so their links can remain empty (see below for ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jÊZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ entries). ”…””}”(j¶j£YjÇjÂOhNjÆNubj>)”}”(j¦ŒC**All of these global tables need to be updated from time to time**”j§]”j±Œ?All of these global tables need to be updated from time to time”…””}”(j¶jßZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjœ>j¶j£Yubj±Œe—the EOP and the VMF1 and ATML grid files daily or weekly if you are processing in near real-time; ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`dcb.dat`”j§]”j±Œdcb.dat”…””}”(j¶jñZjÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ monthly; ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`leap.sec`”j§]”j±Œleap.sec”…””}”(j¶j[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ yearly; ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`svnav.dat`”j§]”j±Œ svnav.dat”…””}”(j¶jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±ŒÜ whenever a new satellite is launched; and the receiver/antenna tables whenever new instrumentation appears. Note that with the 10.7 release the Earth and Sun positions are obtained from a 20-year tabulation, file named ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ :file:`nbody`”j§]”j±Œnbody”…””}”(j¶j0[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ which may be linked in ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jE[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ either to the MIT/CfA file ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`nbody740.2020.asc`”j§]”j±Œnbody740.2020.asc”…””}”(j¶jZ[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±• Œ used in the past to produce ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`soltab.`”j§]”j±Œsoltab.”…””}”(j¶jo[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ and ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`luntab.`”j§]”j±Œluntab.”…””}”(j¶j„[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ" for each year or to the JPL file ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`JPL.DE200`”j§]”j±Œ JPL.DE200”…””}”(j¶j™[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œœ, which is the IGS standard. We’ve found no significant difference in GPS orbital accuracy between the two ephemerides and hence have created the link in ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶j®[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±ŒG to the MIT/CfA file for continuity. Nutation, which were tabulated in ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`nutabl.`”j§]”j±Œnutabl.”…””}”(j¶jÃ[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œi for each year from an IERS-produced subroutine, are now computed internally from the subroutine. If the ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ :file:`nbody`”j§]”j±Œnbody”…””}”(j¶jØ[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ+ link is empty, GAMIT will revert to using ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`soltab.{}`”j§]”(j±Œsoltab.”…””}”(j¶jí[jÇjÂOhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jõ[jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jí[ubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ, ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`luntab.{}`”j§]”(j±Œluntab.”…””}”(j¶j\jÇjÂOhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j\ubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±Œ, and ”…””}”(j¶j£YjÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`nutabl.{}`”j§]”(j±Œnutabl.”…””}”(j¶j3\jÇjÂOhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j;\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j3\ubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£Yubj±ŒH which are available through 2018 but will not be created in the future.”…””}”(j¶j£YjÇjÂOhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKNj¶jïOjÇjÂOubj`)”}”(j¦XThe command files (:file:`process.defaults`, :file:`sites.defaults`, :file:`sestbl.`, :file:`sittbl.`, :file:`autcln.cmd`, and the GLOBK files) are usually specific to a particular survey or processing effort, so the main version of these is usually kept in the project :file:`tables/` directory or a higher-level directory common to multiple projects, each of which may pertain only to a single year's data. (It is possible to include multiple years within a single project by pre-pending the year to the day directories, but this introduces complications in linking single-year, meteorological, and loading files into the project :file:`tables/` directory.) When :program:`sh_gamit` runs it will link these files into each day directory. However, if a file by the same name already exists in the day directory, it will not be removed, so if you need to have a different setting for one day (e.g. a day-specific :file:`autcln.cmd` file), you can create it within the day directory and it will be maintained through repeated processing of that day.”j§]”(j±ŒThe command files (”…””}”(j¶j\\jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jd\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j\\ubj±Œ, ”…””}”(j¶j\\jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jy\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j\\ubj±Œ, ”…””}”j¶j\\sbj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jŽ\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j\\ubj±Œ, ”…””}”j¶j\\sbj˜)”}”(j¦Œ:file:`sittbl.`”j§]”j±Œsittbl.”…””}”(j¶j£\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j\\ubj±Œ, ”…””}”j¶j\\sbj˜)”}”(j¦Œ:file:`autcln.cmd`”j§]”j±Œ autcln.cmd”…””}”(j¶j¸\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j\\ubj±Œ•, and the GLOBK files) are usually specific to a particular survey or processing effort, so the main version of these is usually kept in the project ”…””}”(j¶j\\jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jÍ\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j\\ubj±X] directory or a higher-level directory common to multiple projects, each of which may pertain only to a single year’s data. (It is possible to include multiple years within a single project by pre-pending the year to the day directories, but this introduces complications in linking single-year, meteorological, and loading files into the project ”…””}”(j¶j\\jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jâ\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j\\ubj±Œ directory.) When ”…””}”(j¶j\\jÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j÷\jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j\\ubj±Œå runs it will link these files into each day directory. However, if a file by the same name already exists in the day directory, it will not be removed, so if you need to have a different setting for one day (e.g. a day-specific ”…””}”(j¶j\\jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`autcln.cmd`”j§]”j±Œ autcln.cmd”…””}”(j¶j ]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j\\ubj±Œu file), you can create it within the day directory and it will be maintained through repeated processing of that day.”…””}”(j¶j\\jÇjÂOhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆK]j¶jïOjÇjÂOubj`)”}”(j¦X1 The third set of files comprises those that are day-specific. These include the data files shown at the beginning of this section, but also the orbit, clock, and coordinate files created during the processing. The primary orbital information for GAMIT is the (short, ascii) g-file (e.g., :file:`gigg0.034` where the :file:`f` for final in the :option:`-orbt` option has been replaced by :file:`g` to indicate GPS), which contains for each satellite the values of position and velocity at a particular epoch (usually 12:00 on the day being processed) and coefficients of the 9-component solar radiation-pressure model. These 16 parameters are sufficient for :program:`arc` to generate a tabular ephemeris (binary t-file, e.g., :file:`tigsg0.034`) for model to use in computing the theoretical value of the observations. In normal processing, the g-file is created by :program:`sh_gamit` (invoking :program:`sh_sp3fit`) in the :file:`igs/` directory by fitting :program:`arc`'s model to an ascii tabular ephemeris (in the IGS SP3 format) from an external source. :program:`sh_gamit` then copies the g-file to the :file:`gfiles/` directory and creates a link from the day directory to the file in :file:`gfiles/`. This complicated procedure is useful for two reasons: 1) GAMIT requires partial derivatives of the orbital position with respect to the initial parameters in order to estimate these parameters, and these are not available on the SP3 file; 2) the :file:`igs/` and/or :file:`gfiles/` directories can be used to create multiday orbits for processing pre-IGS data. The satellite clock file (e.g., :file:`jcodr0.034` or :file:`jbrdc0.034`) and receiver clock files (e.g., :file:`kblyt0.034`, :file:`iscal0.034`) all exist solely within the day directory. A description of each of these files may be found in Chapters 1 and 2 of the `GAMIT Reference Manual `_. The main coordinate file for the survey is named :file:`lfile.` and kept in the project :file:`tables/` directory. When :program:`sh_gamit` runs it makes a day-specific link, e.g. :file:`lscal0.034` within each day directory, where updates are made by after each of the two solutions and given the names, e.g., :file:`lscala.034` and :file:`lscalb.034`. We discuss in :numref:`intro_proc_flow` the rules for updating :file:`../tables/lfile.`.”j§]”(j±X The third set of files comprises those that are day-specific. These include the data files shown at the beginning of this section, but also the orbit, clock, and coordinate files created during the processing. The primary orbital information for GAMIT is the (short, ascii) g-file (e.g., ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`gigg0.034`”j§]”j±Œ gigg0.034”…””}”(j¶j,]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ where the ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ :file:`f`”j§]”j±Œf”…””}”(j¶jA]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ for final in the ”…””}”(j¶j$]jÇjÂOhNjÆNubj’)”}”(j¦Œ:option:`-orbt`”j§]”j˜)”}”(j¦jX]j§]”j±Œ-orbt”…””}”(j¶jZ]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jV]ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”jd]Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-orbt”ujÄj‘hjîOjÆKbj¶j$]ubj±Œ option has been replaced by ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ :file:`g`”j§]”j±Œg”…””}”(j¶jz]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±X to indicate GPS), which contains for each satellite the values of position and velocity at a particular epoch (usually 12:00 on the day being processed) and coefficients of the 9-component solar radiation-pressure model. These 16 parameters are sufficient for ”…””}”(j¶j$]jÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`arc`”j§]”j±Œarc”…””}”(j¶j]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j$]ubj±Œ7 to generate a tabular ephemeris (binary t-file, e.g., ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`tigsg0.034`”j§]”j±Œ tigsg0.034”…””}”(j¶j¡]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œz) for model to use in computing the theoretical value of the observations. In normal processing, the g-file is created by ”…””}”(j¶j$]jÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j¶]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j$]ubj±Œ (invoking ”…””}”(j¶j$]jÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`sh_sp3fit`”j§]”j±Œ sh_sp3fit”…””}”(j¶jÈ]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j$]ubj±Œ ) in the ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ :file:`igs/`”j§]”j±Œigs/”…””}”(j¶jÚ]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ directory by fitting ”…””}”(j¶j$]jÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`arc`”j§]”j±Œarc”…””}”(j¶jï]jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j$]ubj±ŒZ’s model to an ascii tabular ephemeris (in the IGS SP3 format) from an external source. ”…””}”(j¶j$]jÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j$]ubj±Œ then copies the g-file to the ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`gfiles/`”j§]”j±Œgfiles/”…””}”(j¶j^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±ŒD directory and creates a link from the day directory to the file in ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`gfiles/`”j§]”j±Œgfiles/”…””}”(j¶j(^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œø. This complicated procedure is useful for two reasons: 1) GAMIT requires partial derivatives of the orbital position with respect to the initial parameters in order to estimate these parameters, and these are not available on the SP3 file; 2) the ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ :file:`igs/`”j§]”j±Œigs/”…””}”(j¶j=^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ and/or ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`gfiles/`”j§]”j±Œgfiles/”…””}”(j¶jR^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œp directories can be used to create multiday orbits for processing pre-IGS data. The satellite clock file (e.g., ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`jcodr0.034`”j§]”j±Œ jcodr0.034”…””}”(j¶jg^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ or ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`jbrdc0.034`”j§]”j±Œ jbrdc0.034”…””}”(j¶j|^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ") and receiver clock files (e.g., ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`kblyt0.034`”j§]”j±Œ kblyt0.034”…””}”(j¶j‘^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ, ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`iscal0.034`”j§]”j±Œ iscal0.034”…””}”(j¶j¦^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œz) all exist solely within the day directory. A description of each of these files may be found in Chapters 1 and 2 of the ”…””}”(j¶j$]jÇjÂOhNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶j»^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶j$]ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œid1”aj»]”j½]”jÀ]”Œgamit reference manual”ajÂ]”Œrefuri”jË^ujÄjdj Kj¶j$]ubj±Œ3. The main coordinate file for the survey is named ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`lfile.`”j§]”j±Œlfile.”…””}”(j¶jÝ^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ and kept in the project ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jò^jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ directory. When ”…””}”(j¶j$]jÇjÂOhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j_jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j$]ubj±Œ) runs it makes a day-specific link, e.g. ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`lscal0.034`”j§]”j±Œ lscal0.034”…””}”(j¶j_jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œq within each day directory, where updates are made by after each of the two solutions and given the names, e.g., ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`lscala.034`”j§]”j±Œ lscala.034”…””}”(j¶j._jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ and ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`lscalb.034`”j§]”j±Œ lscalb.034”…””}”(j¶jC_jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ. We discuss in ”…””}”(j¶j$]jÇjÂOhNjÆNubj’)”}”(j¦Œ:numref:`intro_proc_flow`”j§]”j˜)”}”(j¦jZ_j§]”j±Œintro_proc_flow”…””}”(j¶j\_jÇjÂOhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jX_ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”jf_Œreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_proc_flow”ujÄj‘hjîOjÆKbj¶j$]ubj±Œ the rules for updating ”…””}”(j¶j$]jÇjÂOhNjÆNubj˜)”}”(j¦Œ:file:`../tables/lfile.`”j§]”j±Œ../tables/lfile.”…””}”(j¶j|_jÇjÂOhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j$]ubj±Œ.”…””}”(j¶j$]jÇjÂOhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjîOjÆKbj¶jïOjÇjÂOubej·}”(j¹]”(Œsummary-of-program-flow”jíOej»]”j½]”(Œsummary of program flow”Œintro_proc_flow”ejÀ]”jÂ]”ujÄh_j¶jÂOjÇjÂOhjîOjÆKjÒ }”j_jãOsjÔ }”jíOjãOsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jîOj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjîOjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jÑOjÅOjàOjÔOuj_}”(Œrel”jÑOŒdate”jàOujc}”je}”jíO]”jãOasjg}”(j_jíOjœ_j™_j°Tj­Tuji}”(j_ˆjœ_‰j°Tˆuj¹}”(jíOjïOj™_jïOj­Tj§TjÒ^jÌ^ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”jù )”}”(j¦hoj§]”j`)”}”(j¦Œ9Duplicate explicit target name: "gamit reference manual".”j§]”j±Œ=Duplicate explicit target name: “gamit reference manualâ€.”…””}”(j¶jÆ_jÇjÂOhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÃ_ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jÒ^aŒlevel”KŒtype”jŒsource”jîOŒline”KujÄjø j¶jïOjÇjÂOhjîOjÆKoubaj†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ5Hyperlink target "intro-proc-flow" is not referenced.”…””}”j¶jâ_sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jß_ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jîOŒline”KujÄjø ubajˆNj‰]”j‹NjÇjÂOubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jý_sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jú_jÇjú_ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j `jÇjú_hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jú_jÇjú_ubje)”}”(j¦Œ.. _intro_proc:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ intro-proc”ujÄjdjÆKj¶jú_jÇjú_hŒD/chandler/home/floyd/public_html/gg/docs/source/intro/proc/index.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ)Automatic Processing with GAMIT and GLOBK”j§]”j±Œ)Automatic Processing with GAMIT and GLOBK”…””}”(j¶j*`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j'`jÇjú_hj&`jÆKubjí)”}”(j¦hoj§]”jò)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j¶jjü]”(NŒintro/proc/setup/index”†”NŒintro/proc/flow”†”NŒintro/proc/control/index”†”NŒintro/proc/example”†”ejþ]”(jE`jG`jI`jK`ejJÿÿÿÿjNj‰jˆj‰jKj‰j]”ujÄjñhj&`jÆKj¶j8`ubaj·}”(j¹]”j»]”j aj½]”jÀ]”jÂ]”ujÄjìj¶j'`jÇjú_hj&`jÆNubj`)”}”(j¦XNGAMIT is composed of distinct programs which perform the functions of preparing the data for processing (:program:`makexp` and :program:`makex`), generating reference orbit and rotation values for the satellites (:program:`arc`, :program:`yawtab`), interpolating time- and location-specific values of atmospheric and loading models (:program:`grdtab`), computing residual observations (\ ":math:`\text{o} - \text{c}`"s) and partial derivatives from a geometrical model (:program:`model`), detecting outliers or breaks in the data (:program:`autcln`), and performing a least squares analysis (:program:`solve`). Although the modules can be run individually, they are tied together through the data flow, particularly file-naming conventions, in such a way that most processing is best done with shell scripts and a sequence of batch files set up by a driver module (:program:`fixdrv`) for modeling, editing, and estimation. Though the data editing is almost always performed automatically, the solution residuals can be displayed or plotted so that problematic data can be identified (:program:`cview`).”j§]”(j±ŒiGAMIT is composed of distinct programs which perform the functions of preparing the data for processing (”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`makexp`”j§]”j±Œmakexp”…””}”(j¶j]`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±Œ and ”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`makex`”j§]”j±Œmakex”…””}”(j¶jo`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±ŒF), generating reference orbit and rotation values for the satellites (”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`arc`”j§]”j±Œarc”…””}”(j¶j`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±Œ, ”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`yawtab`”j§]”j±Œyawtab”…””}”(j¶j“`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±ŒW), interpolating time- and location-specific values of atmospheric and loading models (”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`grdtab`”j§]”j±Œgrdtab”…””}”(j¶j¥`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±Œ)), computing residual observations ( “”…””}”(j¶jU`jÇjú_hNjÆNubjO )”}”(j¦Œ:math:`\text{o} - \text{c}`”j§]”j±Œ\text{o} - \text{c}”…””}”(j¶j·`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jU`ubj±Œ8â€s) and partial derivatives from a geometrical model (”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶jÉ`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±Œ-), detecting outliers or breaks in the data (”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jÛ`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±Œ,), and performing a least squares analysis (”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶jí`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±X). Although the modules can be run individually, they are tied together through the data flow, particularly file-naming conventions, in such a way that most processing is best done with shell scripts and a sequence of batch files set up by a driver module (”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`fixdrv`”j§]”j±Œfixdrv”…””}”(j¶jÿ`jÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±ŒÊ) for modeling, editing, and estimation. Though the data editing is almost always performed automatically, the solution residuals can be displayed or plotted so that problematic data can be identified (”…””}”(j¶jU`jÇjú_hNjÆNubjj)”}”(j¦Œ:program:`cview`”j§]”j±Œcview”…””}”(j¶jajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jU`ubj±Œ).”…””}”(j¶jU`jÇjú_hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj&`jÆKj¶j'`jÇjú_ubj`)”}”(j¦XÁLikewise, GLOBK operates through distinct programs, which can be invoked with a single command or run separately. The primary functions are to combine quasi-observations—either GAMIT/GLOBK "h-files" or the internationally accepted SINEX format—from multiple networks and/or epochs (:program:`glred` or :program:`globk`), and to impose on this solution a reference frame appropriate to the scientific objective (:program:`glorg`). Note that :program:`globk` and :program:`glred` are the same program, just called in different modes: :program:`glred` to read data from one day at a time for generating time series; :program:`globk` for stacking multiple epochs to obtain a mean position and/or velocity.”j§]”(j±X"Likewise, GLOBK operates through distinct programs, which can be invoked with a single command or run separately. The primary functions are to combine quasi-observations—either GAMIT/GLOBK “h-files†or the internationally accepted SINEX format—from multiple networks and/or epochs (”…””}”(j¶j)ajÇjú_hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j1ajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j)aubj±Œ or ”…””}”(j¶j)ajÇjú_hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jCajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j)aubj±Œ]), and to impose on this solution a reference frame appropriate to the scientific objective (”…””}”(j¶j)ajÇjú_hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jUajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j)aubj±Œ ). Note that ”…””}”(j¶j)ajÇjú_hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jgajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j)aubj±Œ and ”…””}”(j¶j)ajÇjú_hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jyajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j)aubj±Œ7 are the same program, just called in different modes: ”…””}”(j¶j)ajÇjú_hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j‹ajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j)aubj±ŒA to read data from one day at a time for generating time series; ”…””}”(j¶j)ajÇjú_hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j)aubj±ŒH for stacking multiple epochs to obtain a mean position and/or velocity.”…””}”(j¶j)ajÇjú_hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj&`jÆKj¶j'`jÇjú_ubj`)”}”(j¦ŒmThe full sequence of steps to take you from phase data to time series is accomplished with two shell scripts:”j§]”j±ŒmThe full sequence of steps to take you from phase data to time series is accomplished with two shell scripts:”…””}”(j¶jµajÇjú_hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj&`jÆKj¶j'`jÇjú_ubj`)”}”(j¦ŒÛ:program:`sh_gamit` looks for RINEX data over a range of days and invokes the GAMIT programs to produce constrained and loose estimates of coordinates together with sky plots of phase data as a record of the processing;”j§]”(jj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jÇajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÃaubj±ŒÈ looks for RINEX data over a range of days and invokes the GAMIT programs to produce constrained and loose estimates of coordinates together with sky plots of phase data as a record of the processing;”…””}”(j¶jÃajÇjú_hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj&`jÆKj¶j'`jÇjú_ubj`)”}”(j¦ŒÌ:program:`sh_glred` uses the GAMIT results to produce time series of day-to-day repeatability or a combined h-file that may be further combined with those from other epochs to estimate station velocities.”j§]”(jj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jãajÇjú_hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jßaubj±Œ¹ uses the GAMIT results to produce time series of day-to-day repeatability or a combined h-file that may be further combined with those from other epochs to estimate station velocities.”…””}”(j¶jßajÇjú_hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj&`jÆKj¶j'`jÇjú_ubj`)”}”(j¦XThe only preparation required is assembling the meta-data from station logs; setting up the control files, most of which are common to all analyses of a particular era; and assembling RINEX files not available from public archive in one or more directories on your system.”j§]”j±XThe only preparation required is assembling the meta-data from station logs; setting up the control files, most of which are common to all analyses of a particular era; and assembling RINEX files not available from public archive in one or more directories on your system.”…””}”(j¶jûajÇjú_hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj&`jÆKj¶j'`jÇjú_ubj`)”}”(j¦Œ°Note that all of the scripts and programs that use command-line control are self-documenting: to see the input commands, just type the script or program name with no arguments.”j§]”j±Œ°Note that all of the scripts and programs that use command-line control are self-documenting: to see the input commands, just type the script or program name with no arguments.”…””}”(j¶j bjÇjú_hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj&`jÆK#j¶j'`jÇjú_ubej·}”(j¹]”(Œ)automatic-processing-with-gamit-and-globk”j%`ej»]”j½]”(Œ)automatic processing with gamit and globk”Œ intro_proc”ejÀ]”jÂ]”ujÄh_j¶jú_jÇjú_hj&`jÆKjÒ }”jbj`sjÔ }”j%`j`subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j&`j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj&`jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j `jý_j`j `uj_}”(Œrel”j `Œdate”j`ujc}”je}”j%`]”j`asjg}”(jbj%`jbjbuji}”(jbˆjb‰uj¹}”(j%`j'`jbj'`ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ0Hyperlink target "intro-proc" is not referenced.”…””}”j¶jGbsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jDbubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j&`Œline”KujÄjø ubajˆNj‰]”j‹NjÇjú_ubjõj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jbbsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j_bjÇj_bubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jqbjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j_bjÇj_bubje)”}”(j¦Œ.. _intro_proc_setup:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-setup”ujÄjdjÆKj¶j_bjÇj_bhŒJ/chandler/home/floyd/public_html/gg/docs/source/intro/proc/setup/index.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒSetup”j§]”j±ŒSetup”…””}”(j¶jbjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jŒbjÇj_bhj‹bjÆKubjí)”}”(j¦hoj§]”jò)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j¶jõjü]”(NŒintro/proc/setup/sh_gamit”†”NŒintro/proc/setup/sh_glred”†”ejþ]”(jªbj¬bejJÿÿÿÿjNj‰jˆj‰jKj‰j]”ujÄjñhj‹bjÆKj¶jbubaj·}”(j¹]”j»]”j aj½]”jÀ]”jÂ]”ujÄjìj¶jŒbjÇj_bhj‹bjÆNubj`)”}”(j¦ŒáThe first step in running the scripts is to create a project directory (e.g. :file:`emed18/` or :file:`emed/2018/` for data from 2018 for the eastern Mediterranean) with two subdirectories: :file:`rinex/` and :file:`tables/`.”j§]”(j±ŒMThe first step in running the scripts is to create a project directory (e.g. ”…””}”(j¶j¶bjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`emed18/`”j§]”j±Œemed18/”…””}”(j¶j¾bjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¶bubj±Œ or ”…””}”(j¶j¶bjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`emed/2018/`”j§]”j±Œ emed/2018/”…””}”(j¶jÓbjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¶bubj±ŒL for data from 2018 for the eastern Mediterranean) with two subdirectories: ”…””}”(j¶j¶bjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶jèbjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¶bubj±Œ and ”…””}”(j¶j¶bjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jýbjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¶bubj±Œ.”…””}”(j¶j¶bjÇj_bhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‹bjÆK j¶jŒbjÇj_bubj`)”}”(j¦X•Copy into the :file:`rinex/` directory all of the local RINEX files you plan to use in your processing. GAMIT will handle either RINEX 2 or RINEX 3 formats, but the RINEX 3 files must be renamed to the 10-character RINEX 2 naming scheme (lowercase :file:`{}{}{}.{}o` and :file:`brdc{}{}.{}n`; this happens automatically in :program:`sh_gamit`). RINEX files for IGS directories to be downloaded automatically during the processing are specified using entries in a control file (:file:`sites.defaults`) (see :numref:`intro_proc_control` and Section 6.3 of the `GAMIT Reference Manual `_).”j§]”(j±ŒCopy into the ”…””}”(j¶jcjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶j cjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jcubj±ŒÜ directory all of the local RINEX files you plan to use in your processing. GAMIT will handle either RINEX 2 or RINEX 3 formats, but the RINEX 3 files must be renamed to the 10-character RINEX 2 naming scheme (lowercase ”…””}”(j¶jcjÇj_bhNjÆNubj˜)”}”(j¦Œ$:file:`{}{}{}.{}o`”j§]”(j )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j9cjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j5cubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jGcjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j5cubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jUcjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j5cubj±Œ.”…””}”(j¶j5cjÇj_bhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jgcjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j5cubj±Œo”…””}”(j¶j5cjÇj_bhNjÆNubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jcubj±Œ and ”…””}”(j¶jcjÇj_bhNjÆNubj˜)”}”(j¦Œ :file:`brdc{}{}.{}n`”j§]”(j±Œbrdc”…””}”(j¶j†cjÇj_bhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jŽcjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j†cubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jœcjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j†cubj±Œ.”…””}”(j¶j†cjÇj_bhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j®cjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j†cubj±Œn”…””}”(j¶j†cjÇj_bhNjÆNubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jcubj±Œ ; this happens automatically in ”…””}”(j¶jcjÇj_bhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jÍcjÇj_bhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jcubj±Œ‡). RINEX files for IGS directories to be downloaded automatically during the processing are specified using entries in a control file (”…””}”(j¶jcjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jßcjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jcubj±Œ) (see ”…””}”(j¶jcjÇj_bhNjÆNubj’)”}”(j¦Œ:numref:`intro_proc_control`”j§]”j˜)”}”(j¦jöcj§]”j±Œintro_proc_control”…””}”(j¶jøcjÇj_bhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jôcubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jõŒ refdomain”jdŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_proc_control”ujÄj‘hj‹bjÆKj¶jcubj±Œ and Section 6.3 of the ”…””}”(j¶jcjÇj_bhNjÆNubj÷ )”}”(j¦ŒG`GAMIT Reference Manual `_”j§]”j±ŒGAMIT Reference Manual”…””}”(j¶jdjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶jcubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit-reference-manual”aj»]”j½]”Œgamit reference manual”ajÀ]”jÂ]”Œrefuri”j(dujÄjdj Kj¶jcubj±Œ).”…””}”(j¶jcjÇj_bhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‹bjÆKj¶jŒbjÇj_bubj`)”}”(j¦XþThen run :program:`sh_setup` to link or copy into the project :file:`tables/` directory the appropriate control and data files. All of the required templates and tables reside in :file:`~/gg/tables/`, where :file:`~/gg/` is a required alias pointing to the highest level of the GAMIT/GLOBK installation. Executing :program:`sh_setup` will invoke :program:`sh_links.tables` to *link* the standard data tables described in :numref:`intro_proc_flow`) and will *copy* the eight control and data files listed below:”j§]”(j±Œ Then run ”…””}”(j¶j@djÇj_bhNjÆNubjj)”}”(j¦Œ:program:`sh_setup`”j§]”j±Œsh_setup”…””}”(j¶jHdjÇj_bhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j@dubj±Œ" to link or copy into the project ”…””}”(j¶j@djÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jZdjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j@dubj±Œf directory the appropriate control and data files. All of the required templates and tables reside in ”…””}”(j¶j@djÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jodjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j@dubj±Œ, where ”…””}”(j¶j@djÇj_bhNjÆNubj˜)”}”(j¦Œ :file:`~/gg/`”j§]”j±Œ~/gg/”…””}”(j¶j„djÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j@dubj±Œ^ is a required alias pointing to the highest level of the GAMIT/GLOBK installation. Executing ”…””}”(j¶j@djÇj_bhNjÆNubjj)”}”(j¦Œ:program:`sh_setup`”j§]”j±Œsh_setup”…””}”(j¶j™djÇj_bhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j@dubj±Œ will invoke ”…””}”(j¶j@djÇj_bhNjÆNubjj)”}”(j¦Œ:program:`sh_links.tables`”j§]”j±Œsh_links.tables”…””}”(j¶j«djÇj_bhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j@dubj±Œ to ”…””}”(j¶j@djÇj_bhNjÆNubj )”}”(j¦Œ*link*”j§]”j±Œlink”…””}”(j¶j½djÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j@dubj±Œ' the standard data tables described in ”…””}”(j¶j@djÇj_bhNjÆNubj’)”}”(j¦Œ:numref:`intro_proc_flow`”j§]”j˜)”}”(j¦jÑdj§]”j±Œintro_proc_flow”…””}”(j¶jÓdjÇj_bhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jÏdubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jõŒ refdomain”jÝdŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_proc_flow”ujÄj‘hj‹bjÆKj¶j@dubj±Œ ) and will ”…””}”(j¶j@djÇj_bhNjÆNubj )”}”(j¦Œ*copy*”j§]”j±Œcopy”…””}”(j¶jódjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j@dubj±Œ/ the eight control and data files listed below:”…””}”(j¶j@djÇj_bhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‹bjÆKj¶jŒbjÇj_bubj©Œdefinition_list”“”)”}”(j¦hoj§]”(j©Œdefinition_list_item”“”)”}”(j¦X :file:`process.defaults` Edit this file to specify your computation environment, sources for internal and external data and orbit files, start time and sampling interval, instructions for archiving the results, and an email address to receive a summary of the run. ”j§]”(j©Œterm”“”)”}”(j¦Œ:file:`process.defaults`”j§]”j˜)”}”(j¦jej§]”j±Œprocess.defaults”…””}”(j¶jejÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jeubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆKj¶jeubj©Œ definition”“”)”}”(j¦hoj§]”j`)”}”(j¦ŒïEdit this file to specify your computation environment, sources for internal and external data and orbit files, start time and sampling interval, instructions for archiving the results, and an email address to receive a summary of the run.”j§]”j±ŒïEdit this file to specify your computation environment, sources for internal and external data and orbit files, start time and sampling interval, instructions for archiving the results, and an email address to receive a summary of the run.”…””}”(j¶j7ejÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‹bjÆKj¶j4eubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jeubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆKj¶j eubje)”}”(j¦ŒŠ:file:`sites.defaults` Edit this file to specify which local and IGS stations are to be used and how station meta-data are to be handled. ”j§]”(je)”}”(j¦Œ:file:`sites.defaults`”j§]”j˜)”}”(j¦jWej§]”j±Œsites.defaults”…””}”(j¶jYejÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jUeubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆKj¶jQeubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒrEdit this file to specify which local and IGS stations are to be used and how station meta-data are to be handled.”j§]”j±ŒrEdit this file to specify which local and IGS stations are to be used and how station meta-data are to be handled.”…””}”(j¶jrejÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‹bjÆKj¶joeubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jQeubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆKj¶j ejÇj_bubje)”}”(j¦X|:file:`station.info` This file contains the receiver and antenna type and height of instrument (HI) values as a function of time for all occupations of the stations you will use. Although it can be generated during processing by :program:`sh_gamit`, the best approach is usually to construct the file prior to processing using the tools described in :numref:`intro_proc_example`. ”j§]”(je)”}”(j¦Œ:file:`station.info`”j§]”j˜)”}”(j¦j’ej§]”j±Œ station.info”…””}”(j¶j”ejÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jeubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆK j¶jŒeubj3e)”}”(j¦hoj§]”j`)”}”(j¦XfThis file contains the receiver and antenna type and height of instrument (HI) values as a function of time for all occupations of the stations you will use. Although it can be generated during processing by :program:`sh_gamit`, the best approach is usually to construct the file prior to processing using the tools described in :numref:`intro_proc_example`.”j§]”(j±ŒÐThis file contains the receiver and antenna type and height of instrument (HI) values as a function of time for all occupations of the stations you will use. Although it can be generated during processing by ”…””}”(j¶j­ejÇj_bhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jµejÇj_bhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j­eubj±Œf, the best approach is usually to construct the file prior to processing using the tools described in ”…””}”(j¶j­ejÇj_bhNjÆNubj’)”}”(j¦Œ:numref:`intro_proc_example`”j§]”j˜)”}”(j¦jÉej§]”j±Œintro_proc_example”…””}”(j¶jËejÇj_bhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jÇeubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jõŒ refdomain”jÕeŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_proc_example”ujÄj‘hj‹bjÆKj¶j­eubj±Œ.”…””}”(j¶j­ejÇj_bhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‹bjÆKj¶jªeubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jŒeubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆK j¶j ejÇj_bubje)”}”(j¦X?Coordinate files :program:`sh_gamit` maintains in the experiment :file:`tables/` directory two files of *a priori* coordinates. The file ending in :file:`.apr` (set as :content:`aprf = igb14_comb.apr` in the current :file:`~/gg/tables/process.defaults` template) contains the Cartesian coordinates (position and velocity) of stations you wish to have unchanged throughout the processing. The L-file (:file:`lfile.`), which can contain either Cartesian position and velocity (default, same as :file:`.apr` file) or spherical position (GAMIT old-style, use the :option:`-oldfmt_lfile` option in :program:`sh_setup`), is updated after each day is processed if the adjustments exceed a specified value (0.3 m by default). If you have good coordinates for stations not in the :file:`.apr` file, you should append these to the :file:`.apr` file if you want them to be unchanged. For any station that does not have coordinates in :file:`lfile.`, :program:`sh_gamit` will attempt to calculate coordinates via a pseudorange solution, or (if :content:`use_rxc = Y` in :file:`process.defaults`) use the coordinates in the RINEX header. When GAMIT runs, these coordinates will be updated in the project :file:`tables/lfile.` from the phase solution so that for successive days on which the same station is observed, the accurate coordinates will be used. ”j§]”(je)”}”(j¦ŒCoordinate files”j§]”j±ŒCoordinate files”…””}”(j¶jfjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆK(j¶jýeubj3e)”}”(j¦hoj§]”j`)”}”(j¦X-:program:`sh_gamit` maintains in the experiment :file:`tables/` directory two files of *a priori* coordinates. The file ending in :file:`.apr` (set as :content:`aprf = igb14_comb.apr` in the current :file:`~/gg/tables/process.defaults` template) contains the Cartesian coordinates (position and velocity) of stations you wish to have unchanged throughout the processing. The L-file (:file:`lfile.`), which can contain either Cartesian position and velocity (default, same as :file:`.apr` file) or spherical position (GAMIT old-style, use the :option:`-oldfmt_lfile` option in :program:`sh_setup`), is updated after each day is processed if the adjustments exceed a specified value (0.3 m by default). If you have good coordinates for stations not in the :file:`.apr` file, you should append these to the :file:`.apr` file if you want them to be unchanged. For any station that does not have coordinates in :file:`lfile.`, :program:`sh_gamit` will attempt to calculate coordinates via a pseudorange solution, or (if :content:`use_rxc = Y` in :file:`process.defaults`) use the coordinates in the RINEX header. When GAMIT runs, these coordinates will be updated in the project :file:`tables/lfile.` from the phase solution so that for successive days on which the same station is observed, the accurate coordinates will be used.”j§]”(jj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jfjÇj_bhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jfubj±Œ maintains in the experiment ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶j(fjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±Œ directory two files of ”…””}”(j¶jfjÇj_bhNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j=fjÇj_bhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jfubj±Œ! coordinates. The file ending in ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jOfjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±Œ (set as ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ :content:`aprf = igb14_comb.apr`”j§]”j±Œaprf = igb14_comb.apr”…””}”(j¶jdfjÇj_bhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jfubj±Œ in the current ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ$:file:`~/gg/tables/process.defaults`”j§]”j±Œ~/gg/tables/process.defaults”…””}”(j¶jwfjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±Œ” template) contains the Cartesian coordinates (position and velocity) of stations you wish to have unchanged throughout the processing. The L-file (”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`lfile.`”j§]”j±Œlfile.”…””}”(j¶jŒfjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±ŒN), which can contain either Cartesian position and velocity (default, same as ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶j¡fjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±Œ7 file) or spherical position (GAMIT old-style, use the ”…””}”(j¶jfjÇj_bhNjÆNubj’)”}”(j¦Œ:option:`-oldfmt_lfile`”j§]”j˜)”}”(j¦j¸fj§]”j±Œ -oldfmt_lfile”…””}”(j¶jºfjÇj_bhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j¶fubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jõŒ refdomain”jÄfŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -oldfmt_lfile”ujÄj‘hj‹bjÆK#j¶jfubj±Œ option in ”…””}”(j¶jfjÇj_bhNjÆNubjj)”}”(j¦Œ:program:`sh_setup`”j§]”j±Œsh_setup”…””}”(j¶jÚfjÇj_bhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jfubj±ŒŸ), is updated after each day is processed if the adjustments exceed a specified value (0.3 m by default). If you have good coordinates for stations not in the ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jìfjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±Œ& file, you should append these to the ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jgjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±ŒZ file if you want them to be unchanged. For any station that does not have coordinates in ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`lfile.`”j§]”j±Œlfile.”…””}”(j¶jgjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±Œ, ”…””}”(j¶jfjÇj_bhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j+gjÇj_bhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jfubj±ŒJ will attempt to calculate coordinates via a pseudorange solution, or (if ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ:content:`use_rxc = Y`”j§]”j±Œ use_rxc = Y”…””}”(j¶j=gjÇj_bhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jfubj±Œ in ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jPgjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±Œm) use the coordinates in the RINEX header. When GAMIT runs, these coordinates will be updated in the project ”…””}”(j¶jfjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`tables/lfile.`”j§]”j±Œ tables/lfile.”…””}”(j¶jegjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jfubj±Œ‚ from the phase solution so that for successive days on which the same station is observed, the accurate coordinates will be used.”…””}”(j¶jfjÇj_bhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‹bjÆK#j¶jfubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jýeubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆK(j¶j ejÇj_bubje)”}”(j¦Œð:file:`sestbl.` and :file:`sittbl.` Edit these files to set the appropriate options for your analysis. Make sure that any station for which you specify tight constraints in :file:`sittbl.` has accurate coordinates in the :file:`.apr` file. ”j§]”(je)”}”(j¦Œ#:file:`sestbl.` and :file:`sittbl.`”j§]”(j˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶j”gjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jgubj±Œ and ”…””}”(j¶jgjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`sittbl.`”j§]”j±Œsittbl.”…””}”(j¶j©gjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jgubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆK,j¶jŒgubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒËEdit these files to set the appropriate options for your analysis. Make sure that any station for which you specify tight constraints in :file:`sittbl.` has accurate coordinates in the :file:`.apr` file.”j§]”(j±Œ‰Edit these files to set the appropriate options for your analysis. Make sure that any station for which you specify tight constraints in ”…””}”(j¶jÃgjÇj_bhNjÆNubj˜)”}”(j¦Œ:file:`sittbl.`”j§]”j±Œsittbl.”…””}”(j¶jËgjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÃgubj±Œ! has accurate coordinates in the ”…””}”(j¶jÃgjÇj_bhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jàgjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÃgubj±Œ file.”…””}”(j¶jÃgjÇj_bhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‹bjÆK+j¶jÀgubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jŒgubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆK,j¶j ejÇj_bubje)”}”(j¦Œ´:file:`autcln.cmd` Controls for cleaning the data in program :program:`autcln`. This file will usually not require editing unless you encounter unusual data during the processing. ”j§]”(je)”}”(j¦Œ:file:`autcln.cmd`”j§]”j˜)”}”(j¦j hj§]”j±Œ autcln.cmd”…””}”(j¶jhjÇj_bhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j hubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆK0j¶jhubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ Controls for cleaning the data in program :program:`autcln`. This file will usually not require editing unless you encounter unusual data during the processing.”j§]”(j±Œ*Controls for cleaning the data in program ”…””}”(j¶j(hjÇj_bhNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶j0hjÇj_bhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j(hubj±Œe. This file will usually not require editing unless you encounter unusual data during the processing.”…””}”(j¶j(hjÇj_bhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‹bjÆK/j¶j%hubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jhubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj‹bjÆK0j¶j ejÇj_bubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶jŒbjÇj_bhj‹bjÆNubej·}”(j¹]”(Œsetup”jŠbej»]”j½]”(Œsetup”Œintro_proc_setup”ejÀ]”jÂ]”ujÄh_j¶j_bjÇj_bhj‹bjÆKjÒ }”j`hj€bsjÔ }”jŠbj€bsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j‹bj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj‹bjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jnbjbbj}bjqbuj_}”(Œrel”jnbŒdate”j}bujc}”je}”jŠb]”j€basjg}”(j`hjŠbj_hj\hj2dj/duji}”(j`hˆj_h‰j2dˆuj¹}”(jŠbjŒbj\hjŒbj/dj)dujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ6Hyperlink target "intro-proc-setup" is not referenced.”…””}”j¶jŠhsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j‡hubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j‹bŒline”KujÄjø ubajˆNj‰]”j‹NjÇj_bubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j¥hsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¢hjÇj¢hubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j´hjÇj¢hhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¢hjÇj¢hubje)”}”(j¦Œ.. _intro_proc_sh_gamit:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-sh-gamit”ujÄjdjÆKj¶j¢hjÇj¢hhŒM/chandler/home/floyd/public_html/gg/docs/source/intro/proc/setup/sh_gamit.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ:program:`sh_gamit`”j§]”jj)”}”(j¦jÔhj§]”j±Œsh_gamit”…””}”(j¶jÖhjÇj¢hhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÒhubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jÏhjÇj¢hhjÎhjÆKubj`)”}”(j¦XOnce you have edited appropriately the template files, you can start the processing from within the experiment directory by giving :program:`sh_gamit` simply the 4-character code for the project or subnet (termed "experiment") and a range of days to process:”j§]”(j±ŒƒOnce you have edited appropriately the template files, you can start the processing from within the experiment directory by giving ”…””}”(j¶jéhjÇj¢hhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jñhjÇj¢hhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jéhubj±Œp simply the 4-character code for the project or subnet (termed “experimentâ€) and a range of days to process:”…””}”(j¶jéhjÇj¢hhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆKj¶jÏhjÇj¢hubj)”}”(j¦Œ9$ sh_gamit -expt emed -d 2018 034 035 036 >& sh_gamit.log”j§]”j±Œ9$ sh_gamit -expt emed -d 2018 034 035 036 >& sh_gamit.log”…””}”j¶j isbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÎhjÆKj¶jÏhjÇj¢hubj`)”}”(j¦X9The :program:`sh_gamit` command is executed at the project-directory level. The time span can also be specified using :option:`-s {} {}` to indicate a range of consecutive days, or :option:`-r {}` to indicate that you want to process a single day :option:`{}` before the current date. If you plan to process data from more than GPS, use :option:`-gnss {}`, where sys is G for GPS, R for Glonass, C for Beidou, E for Galileo, and I for IRNSS. You may also override some of the parameters specified in :file:`process.defaults`, e.g.:”j§]”(j±ŒThe ”…””}”(j¶jijÇj¢hhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”•j§]”j±Œsh_gamit”…””}”(j¶j!ijÇj¢hhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jiubj±Œ_ command is executed at the project-directory level. The time span can also be specified using ”…””}”(j¶jijÇj¢hhNjÆNubj’)”}”(j¦Œ':option:`-s {} {}`”j§]”j˜)”}”(j¦j5ij§]”j±Œ-s {} {}”…””}”(j¶j7ijÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j3iubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jAiŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-s {} {}”ujÄj‘hjÎhjÆK j¶jiubj±Œ- to indicate a range of consecutive days, or ”…””}”(j¶jijÇj¢hhNjÆNubj’)”}”(j¦Œ:option:`-r {}`”j§]”j˜)”}”(j¦jYij§]”j±Œ -r {}”…””}”(j¶j[ijÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jWiubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jeiŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -r {}”ujÄj‘hjÎhjÆK j¶jiubj±Œ3 to indicate that you want to process a single day ”…””}”(j¶jijÇj¢hhNjÆNubj’)”}”(j¦Œ:option:`{}`”j§]”j˜)”}”(j¦j}ij§]”j±Œ{}”…””}”(j¶jijÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j{iubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j‰iŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ{}”ujÄj‘hjÎhjÆK j¶jiubj±ŒN before the current date. If you plan to process data from more than GPS, use ”…””}”(j¶jijÇj¢hhNjÆNubj’)”}”(j¦Œ:option:`-gnss {}`”j§]”j˜)”}”(j¦j¡ij§]”j±Œ -gnss {}”…””}”(j¶j£ijÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jŸiubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j­iŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -gnss {}”ujÄj‘hjÎhjÆK j¶jiubj±Œ‘, where sys is G for GPS, R for Glonass, C for Beidou, E for Galileo, and I for IRNSS. You may also override some of the parameters specified in ”…””}”(j¶jijÇj¢hhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jÃijÇj¢hhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jiubj±Œ, e.g.:”…””}”(j¶jijÇj¢hhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆK j¶jÏhjÇj¢hubj e)”}”(j¦hoj§]”(je)”}”(j¦Œx:option:`-orbit {}` Type of orbit (e.g. igsf igsr igsu codm gfzm siof; see :program:`sh_get_orbits`; default igsf)”j§]”(je)”}”(j¦Œ:option:`-orbit {}`”j§]”j’)”}”(j¦jçij§]”j˜)”}”(j¦jçij§]”j±Œ-orbit {}”…””}”(j¶jìijÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jéiubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jöiŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-orbit {}”ujÄj‘hjÎhjÆKj¶jåiubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jáiubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ^Type of orbit (e.g. igsf igsr igsu codm gfzm siof; see :program:`sh_get_orbits`; default igsf)”j§]”(j±Œ7Type of orbit (e.g. igsf igsr igsu codm gfzm siof; see 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(default x, k, autcln.out, d)”j§]”(je)”}”(j¦Œ:option:`-copt`”j§]”j’)”}”(j¦j×jj§]”j˜)”}”(j¦j×jj§]”j±Œ-copt”…””}”(j¶jÜjjÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jÙjubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jæjŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-copt”ujÄj‘hjÎhjÆKj¶jÕjubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jÑjubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒLList of files to compress in the day directory (default x, k, autcln.out, d)”j§]”j±ŒLList of files to compress in the day directory (default x, k, autcln.out, d)”…””}”(j¶jkjÇj¢hhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆKj¶jþjubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jÑjubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jÞijÇj¢hubje)”}”(j¦ŒU:option:`-dopt` List of files to delete from the day directory (default C-files only)”j§]”(je)”}”(j¦Œ:option:`-dopt`”j§]”j’)”}”(j¦j!kj§]”j˜)”}”(j¦j!kj§]”j±Œ-dopt”…””}”(j¶j&kjÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j#kubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j0kŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-dopt”ujÄj‘hjÎhjÆKj¶jkubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jkubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒEList of files to delete from the day directory (default C-files only)”j§]”j±ŒEList of files to delete from the day directory (default C-files only)”…””}”(j¶jKkjÇj¢hhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆKj¶jHkubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jkubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jÞijÇj¢hubje)”}”(j¦ŒI:option:`-pres ELEV` Plot phase vs elevation and as skyplots (default no)”j§]”(je)”}”(j¦Œ:option:`-pres ELEV`”j§]”j’)”}”(j¦jkkj§]”j˜)”}”(j¦jkkj§]”j±Œ -pres ELEV”…””}”(j¶jpkjÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jmkubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jzkŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -pres ELEV”ujÄj‘hjÎhjÆKj¶jikubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jekubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ4Plot phase vs elevation and as skyplots (default no)”j§]”j±Œ4Plot phase vs elevation and as skyplots (default no)”…””}”(j¶j•kjÇj¢hhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆKj¶j’kubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jekubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jÞijÇj¢hubje)”}”(j¦Œ]:option:`-nopngs` Do not create PNG files of sky plots (default is to create from PostScript)”j§]”(je)”}”(j¦Œ:option:`-nopngs`”j§]”j’)”}”(j¦jµkj§]”j˜)”}”(j¦jµkj§]”j±Œ-nopngs”…””}”(j¶jºkjÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j·kubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÄkŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-nopngs”ujÄj‘hjÎhjÆKj¶j³kubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶j¯kubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒKDo not create PNG files of sky plots (default is to create from PostScript)”j§]”j±ŒKDo not create PNG files of sky plots (default is to create from PostScript)”…””}”(j¶jßkjÇj¢hhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆKj¶jÜkubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j¯kubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jÞijÇj¢hubje)”}”(j¦Œ<:option:`-yrext` Add year prefix to names of day directories”j§]”(je)”}”(j¦Œ:option:`-yrext`”j§]”j’)”}”(j¦jÿkj§]”j˜)”}”(j¦jÿkj§]”j±Œ-yrext”…””}”(j¶jljÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jlubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jlŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-yrext”ujÄj‘hjÎhjÆKj¶jýkubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jùkubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ+Add year prefix to names of day directories”j§]”j±Œ+Add year prefix to names of day directories”…””}”(j¶j)ljÇj¢hhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆK j¶j&lubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jùkubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆKj¶jÞijÇj¢hubje)”}”(j¦ŒM:option:`-netext {}` Add suffix (character) to names of day directories”j§]”(je)”}”(j¦Œ:option:`-netext {}`”j§]”j’)”}”(j¦jIlj§]”j˜)”}”(j¦jIlj§]”j±Œ-netext {}”…””}”(j¶jNljÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jKlubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jXlŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-netext {}”ujÄj‘hjÎhjÆK!j¶jGlubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆK!j¶jClubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ2Add suffix (character) to names of day directories”j§]”j±Œ2Add suffix (character) to names of day directories”…””}”(j¶jsljÇj¢hhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆK"j¶jplubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jClubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆK!j¶jÞijÇj¢hubje)”}”(j¦ŒZ:option:`-noftp` Don’t try to ftp any data from outside your system (default is to ftp) ”j§]”(je)”}”(j¦Œ:option:`-noftp`”j§]”j’)”}”(j¦j“lj§]”j˜)”}”(j¦j“lj§]”j±Œ-noftp”…””}”(j¶j˜ljÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j•lubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j¢lŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-noftp”ujÄj‘hjÎhjÆK$j¶j‘lubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆK$j¶jlubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒHDon’t try to ftp any data from outside your system (default is to ftp)”j§]”j±ŒHDon’t try to ftp any data from outside your system (default is to ftp)”…””}”(j¶j½ljÇj¢hhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆK$j¶jºlubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jlubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjÎhjÆK$j¶jÞijÇj¢hubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶jÏhjÇj¢hhjÎhjÆNubj`)”}”(j¦XŠMost of the time the parameters may be omitted in favor of the values you have specified in :file:`process.defaults` for the whole experiment. The overrides are useful, however, if you wish to test the effect of processing a day with a different orbit, EOP table, or session length, or for different GNSS, in which case you can create a second directory for the same day by appending a character to its name (e.g., :option:`-netext t` to create :file:`034t/`). When :option:`-gnss` is specified, the day directories will automatically be named with the GNSS code as the extent (e.g. :file:`034E/` for Galileo). Finally, you may launch sh_gamit from anywhere on the system by specifying the full path name of the processing directory with :option:`-dir {}`. When the script runs, it will write to the screen a record of each step, which you may choose to redirect to a file (e.g., :console:`>& sh_gamit.log`). Examining the screen log together with the comments and source code in :file:`~/gg/com/sh_gamit` and the :file:`GAMIT.fatal` file, will allow you to identify the point and reason for failure should that occur. When processing of each day is completed, :program:`sh_gamit` will send a mail message to you (:content:`mailto` in :file:`process.defaults`) giving the number of stations used, the rms of the one-way phase residuals for the two best and two worst stations from the :program:`autcln` postfit summary file, the nrms values from the Q-file, the number of ambiguities resolved, and a list of any large adjustments to station coordinates. These statistics will let you know whether you need to examine the GAMIT output further for possible reprocessing.”j§]”(j±Œ\Most of the time the parameters may be omitted in favor of the values you have specified in ”…””}”(j¶jÝljÇj¢hhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jåljÇj¢hhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÝlubj±X+ for the whole experiment. The overrides are useful, however, if you wish to test the effect of processing a day with a different orbit, EOP table, or session length, or for different GNSS, in which case you can create a second directory for the same day by appending a character to its name (e.g., ”…””}”(j¶jÝljÇj¢hhNjÆNubj’)”}”(j¦Œ:option:`-netext t`”j§]”j˜)”}”(j¦jülj§]”j±Œ -netext t”…””}”(j¶jþljÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶júlubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jmŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -netext t”ujÄj‘hjÎhjÆK&j¶jÝlubj±Œ to create ”…””}”(j¶jÝljÇj¢hhNjÆNubj˜)”}”(j¦Œ :file:`034t/`”j§]”j±Œ034t/”…””}”(j¶jmjÇj¢hhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÝlubj±Œ). When ”…””}”(j¶jÝljÇj¢hhNjÆNubj’)”}”(j¦Œ:option:`-gnss`”j§]”j˜)”}”(j¦j5mj§]”j±Œ-gnss”…””}”(j¶j7mjÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j3mubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jAmŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-gnss”ujÄj‘hjÎhjÆK&j¶jÝlubj±Œf is specified, the day directories will automatically be named with the GNSS code as the extent (e.g. ”…””}”(j¶jÝljÇj¢hhNjÆNubj˜)”}”(j¦Œ :file:`034E/`”j§]”j±Œ034E/”…””}”(j¶jWmjÇj¢hhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÝlubj±ŒŽ for Galileo). Finally, you may launch sh_gamit from anywhere on the system by specifying the full path name of the processing directory with ”…””}”(j¶jÝljÇj¢hhNjÆNubj’)”}”(j¦Œ:option:`-dir {}`”j§]”j˜)”}”(j¦jnmj§]”j±Œ -dir {}”…””}”(j¶jpmjÇj¢hhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jlmubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jzmŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -dir {}”ujÄj‘hjÎhjÆK&j¶jÝlubj±Œ}. When the script runs, it will write to the screen a record of each step, which you may choose to redirect to a file (e.g., ”…””}”(j¶jÝljÇj¢hhNjÆNubj˜)”}”(j¦Œ:console:`>& sh_gamit.log`”j§]”j±Œ>& sh_gamit.log”…””}”(j¶jmjÇj¢hhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶jÝlubj±ŒJ). Examining the screen log together with the comments and source code in ”…””}”(j¶jÝljÇj¢hhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/com/sh_gamit`”j§]”j±Œ~/gg/com/sh_gamit”…””}”(j¶j£mjÇj¢hhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÝlubj±Œ and the ”…””}”(j¶jÝljÇj¢hhNjÆNubj˜)”}”(j¦Œ:file:`GAMIT.fatal`”j§]”j±Œ GAMIT.fatal”…””}”(j¶j¸mjÇj¢hhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÝlubj±Œ€ file, will allow you to identify the point and reason for failure should that occur. When processing of each day is completed, ”…””}”(j¶jÝljÇj¢hhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jÍmjÇj¢hhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÝlubj±Œ" will send a mail message to you (”…””}”(j¶jÝljÇj¢hhNjÆNubj˜)”}”(j¦Œ:content:`mailto`”j§]”j±Œmailto”…””}”(j¶jßmjÇj¢hhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÝlubj±Œ in ”…””}”(j¶jÝljÇj¢hhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jòmjÇj¢hhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÝlubj±Œ~) giving the number of stations used, the rms of the one-way phase residuals for the two best and two worst stations from the ”…””}”(j¶jÝljÇj¢hhNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jnjÇj¢hhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÝlubj±X  postfit summary file, the nrms values from the Q-file, the number of ambiguities resolved, and a list of any large adjustments to station coordinates. These statistics will let you know whether you need to examine the GAMIT output further for possible reprocessing.”…””}”(j¶jÝljÇj¢hhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÎhjÆK&j¶jÏhjÇj¢hubej·}”(j¹]”(Œsh-gamit”jÍhej»]”j½]”(Œsh_gamit”Œintro_proc_sh_gamit”ejÀ]”jÂ]”ujÄh_j¶j¢hjÇj¢hhjÎhjÆKjÒ }”j%njÃhsjÔ }”jÍhjÃhsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jÎhj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjÎhjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j±hj¥hjÀhj´huj_}”(Œrel”j±hŒdate”jÀhujc}”je}”jÍh]”jÃhasjg}”(j%njÍhj$nj!nuji}”(j%nˆj$n‰uj¹}”(jÍhjÏhj!njÏhujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ9Hyperlink target "intro-proc-sh-gamit" is not referenced.”…””}”j¶jOnsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jLnubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jÎhŒline”KujÄjø ubajˆNj‰]”j‹NjÇj¢hubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jjnsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jgnjÇjgnubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jynjÇjgnhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jgnjÇjgnubje)”}”(j¦Œ.. _intro_proc_sh_glred:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-proc-sh-glred”ujÄjdjÆKj¶jgnjÇjgnhŒM/chandler/home/floyd/public_html/gg/docs/source/intro/proc/setup/sh_glred.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ:program:`sh_glred`”j§]”jj)”}”(j¦j™nj§]”j±Œsh_glred”…””}”(j¶j›njÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j—nubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j”njÇjgnhj“njÆKubj`)”}”(j¦XóTo use :program:`sh_glred` to obtain a time series of position estimates, you need to edit one and possibly more control files in the :file:`gsoln/` directory established by :program:`sh_setup`. In the simplest case, in which you want to use all of the sites in your GAMIT solutions and are not combining these solutions with h-files from an external source, you need only edit :file:`glorg.cmd` to specify which sites will be used to define your reference frame. If you want to omit some sites or indicate where steps should be applied in the time series to account for earthquakes or changes in instrumentation, you may need to edit also :file:`globk.cmd` and an earthquake/rename file. These are described in :numref:`intro_proc_globk`. Then run, e.g.,”j§]”(j±ŒTo use ”…””}”(j¶j®njÇjgnhNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j¶njÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®nubj±Œl to obtain a time series of position estimates, you need to edit one and possibly more control files in the ”…””}”(j¶j®njÇjgnhNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶jÈnjÇjgnhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®nubj±Œ directory established by ”…””}”(j¶j®njÇjgnhNjÆNubjj)”}”(j¦Œ:program:`sh_setup`”j§]”j±Œsh_setup”…””}”(j¶jÝnjÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®nubj±Œ¹. In the simplest case, in which you want to use all of the sites in your GAMIT solutions and are not combining these solutions with h-files from an external source, you need only edit ”…””}”(j¶j®njÇjgnhNjÆNubj˜)”}”(j¦Œ:file:`glorg.cmd`”j§]”j±Œ glorg.cmd”…””}”(j¶jïnjÇjgnhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®nubj±Œõ to specify which sites will be used to define your reference frame. If you want to omit some sites or indicate where steps should be applied in the time series to account for earthquakes or changes in instrumentation, you may need to edit also ”…””}”(j¶j®njÇjgnhNjÆNubj˜)”}”(j¦Œ:file:`globk.cmd`”j§]”j±Œ globk.cmd”…””}”(j¶jojÇjgnhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j®nubj±Œ7 and an earthquake/rename file. These are described in ”…””}”(j¶j®njÇjgnhNjÆNubj’)”}”(j¦Œ:numref:`intro_proc_globk`”j§]”j˜)”}”(j¦joj§]”j±Œintro_proc_globk”…””}”(j¶jojÇjgnhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶joubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j'oŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_proc_globk”ujÄj‘hj“njÆKj¶j®nubj±Œ. Then run, e.g.,”…””}”(j¶j®njÇjgnhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“njÆKj¶j”njÇjgnubj)”}”(j¦ŒD$ sh_glred -expt emed -s 2018 34 2018 36 -opt H G T >&! sh_glred.log”j§]”j±ŒD$ sh_glred -expt emed -s 2018 34 2018 36 -opt H G T >&! sh_glred.log”…””}”j¶jCosbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj“njÆK j¶j”njÇjgnubj`)”}”(j¦X|The :option:`H` option tells :program:`sh_glred` to translate GAMIT h-files in the day directory to GLOBK binary h-files and put them into :file:`glbf/`; :option:`G` indicates that :program:`glred` is to be run (you can use :program:`sh_glred` just to do the h-file translation if you wish); and :option:`T` indicates that time series plots are to be generated using :program:`sh_plot_pos` (invoking first :program:`tssum`, the program that extracts coordinates from the :program:`glred` output :file:`.org` file to produce :file:`.pos` files). Prior to Release 10.6, the coordinates could be extracted only with programs :program:`ensum` and :program:`multibase` to produce :file:`mb` files and plotted with :program:`sh_plotcrd`. This option is still available in 10.7 with key letter :option:`E` but will be deprecated in future releases. Finally, it is possible to combine the h-files you have created in the day directories with global or regional h-files generated by an external processing center (e.g. MIT or SOPAC), using the :content:`hfnd` token in the project :file:`tables/process.defaults` (see :numref:`intro_proc_process.defaults`).”j§]”(j±ŒThe ”…””}”(j¶jSojÇjgnhNjÆNubj’)”}”(j¦Œ :option:`H`”j§]”j˜)”}”(j¦j]oj§]”j±ŒH”…””}”(j¶j_ojÇjgnhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j[oubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jioŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶j‡MujÄj‘hj“njÆKj¶jSoubj±Œ option tells ”…””}”(j¶jSojÇjgnhNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j~ojÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSoubj±Œ[ to translate GAMIT h-files in the day directory to GLOBK binary h-files and put them into ”…””}”(j¶jSojÇjgnhNjÆNubj˜)”}”(j¦Œ :file:`glbf/`”j§]”j±Œglbf/”…””}”(j¶jojÇjgnhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jSoubj±Œ; ”…””}”(j¶jSojÇjgnhNjÆNubj’)”}”(j¦Œ :option:`G`”j§]”j˜)”}”(j¦j§oj§]”j±ŒG”…””}”(j¶j©ojÇjgnhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j¥oubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j³oŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒG”ujÄj‘hj“njÆKj¶jSoubj±Œ indicates that ”…””}”(j¶jSojÇjgnhNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jÉojÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSoubj±Œ is to be run (you can use ”…””}”(j¶jSojÇjgnhNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jÛojÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSoubj±Œ5 just to do the h-file translation if you wish); and ”…””}”(j¶jSojÇjgnhNjÆNubj’)”}”(j¦Œ :option:`T`”j§]”j˜)”}”(j¦jïoj§]”j±ŒT”…””}”(j¶jñojÇjgnhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jíoubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jûoŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶j^IujÄj‘hj“njÆKj¶jSoubj±Œ< indicates that time series plots are to be generated using ”…””}”(j¶jSojÇjgnhNjÆNubjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶jpjÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSoubj±Œ (invoking first ”…””}”(j¶jSojÇjgnhNjÆNubjj)”}”(j¦Œ:program:`tssum`”j§]”j±Œtssum”…””}”(j¶j"pjÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSoubj±Œ1, the program that extracts coordinates from the ”…””}”(j¶jSojÇjgnhNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j4pjÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSoubj±Œ output ”…””}”(j¶jSojÇjgnhNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶jFpjÇjgnhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jSoubj±Œ file to produce ”…””}”(j¶jSojÇjgnhNjÆNubj˜)”}”(j¦Œ :file:`.pos`”j§]”j±Œ.pos”…””}”(j¶j[pjÇjgnhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jSoubj±ŒV files). Prior to Release 10.6, the coordinates could be extracted only with programs ”…””}”(j¶jSojÇjgnhNjÆNubjj)”}”(j¦Œ:program:`ensum`”j§]”j±Œensum”…””}”(j¶jppjÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSoubj±Œ and ”…””}”(j¶jSojÇjgnhNjÆNubjj)”}”(j¦Œ:program:`multibase`”j§]”j±Œ multibase”…””}”(j¶j‚pjÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSoubj±Œ to produce ”…””}”(j¶jSojÇjgnhNjÆNubj˜)”}”(j¦Œ :file:`mb`”j§]”j±Œmb”…””}”(j¶j”pjÇjgnhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jSoubj±Œ files and plotted with ”…””}”(j¶jSojÇjgnhNjÆNubjj)”}”(j¦Œ:program:`sh_plotcrd`”j§]”j±Œ sh_plotcrd”…””}”(j¶j©pjÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSoubj±Œ9. This option is still available in 10.7 with key letter ”…””}”(j¶jSojÇjgnhNjÆNubj’)”}”(j¦Œ :option:`E`”j§]”j˜)”}”(j¦j½pj§]”j±ŒE”…””}”(j¶j¿pjÇjgnhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j»pubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÉpŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶j:IujÄj‘hj“njÆKj¶jSoubj±Œí but will be deprecated in future releases. Finally, it is possible to combine the h-files you have created in the day directories with global or regional h-files generated by an external processing center (e.g. MIT or SOPAC), using the ”…””}”(j¶jSojÇjgnhNjÆNubj˜)”}”(j¦Œ:content:`hfnd`”j§]”j±Œhfnd”…””}”(j¶jÞpjÇjgnhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jSoubj±Œ token in the project ”…””}”(j¶jSojÇjgnhNjÆNubj˜)”}”(j¦Œ:file:`tables/process.defaults`”j§]”j±Œtables/process.defaults”…””}”(j¶jñpjÇjgnhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jSoubj±Œ (see ”…””}”(j¶jSojÇjgnhNjÆNubj’)”}”(j¦Œ%:numref:`intro_proc_process.defaults`”j§]”j˜)”}”(j¦jqj§]”j±Œintro_proc_process.defaults”…””}”(j¶j qjÇjgnhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jqubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jqŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_proc_process.defaults”ujÄj‘hj“njÆKj¶jSoubj±Œ).”…””}”(j¶jSojÇjgnhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“njÆKj¶j”njÇjgnubj`)”}”(j¦X :program:`sh_glred` uses the :option:`-netext` option with one or more GNSS (or other netext) codes to select which day directories to access for GAMIT h-files, appending a (lowercase) letter to the GLOBK binary h-file to distinguish among files in the :program:`globk` :file:`.gdl` list.”j§]”(jj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j4qjÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j0qubj±Œ uses the ”…””}”(j¶j0qjÇjgnhNjÆNubj’)”}”(j¦Œ:option:`-netext`”j§]”j˜)”}”(j¦jHqj§]”j±Œ-netext”…””}”(j¶jJqjÇjgnhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jFqubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jTqŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-netext”ujÄj‘hj“njÆKj¶j0qubj±ŒÏ option with one or more GNSS (or other netext) codes to select which day directories to access for GAMIT h-files, appending a (lowercase) letter to the GLOBK binary h-file to distinguish among files in the ”…””}”(j¶j0qjÇjgnhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jjqjÇjgnhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j0qubj±Œ ”…””}”(j¶j0qjÇjgnhNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶j|qjÇjgnhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j0qubj±Œ list.”…””}”(j¶j0qjÇjgnhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“njÆKj¶j”njÇjgnubej·}”(j¹]”(Œsh-glred”j’nej»]”j½]”(Œsh_glred”Œintro_proc_sh_glred”ejÀ]”jÂ]”ujÄh_j¶jgnjÇjgnhj“njÆKjÒ }”jqjˆnsjÔ }”j’njˆnsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j“nj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj“njNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jvnjjnj…njynuj_}”(Œrel”jvnŒdate”j…nujc}”je}”j’n]”jˆnasjg}”(jqj’njœqj™quji}”(jqˆjœq‰uj¹}”(j’nj”nj™qj”nujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ9Hyperlink target "intro-proc-sh-glred" is not referenced.”…””}”j¶jÇqsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÄqubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j“nŒline”KujÄjø ubajˆNj‰]”j‹NjÇjgnubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jâqsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jßqjÇjßqubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jñqjÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jßqjÇjßqubje)”}”(j¦Œ.. _intro_prod_combine:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-prod-combine”ujÄjdjÆKj¶jßqjÇjßqhŒF/chandler/home/floyd/public_html/gg/docs/source/intro/prod/combine.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒCombining h-files”j§]”j±ŒCombining h-files”…””}”(j¶jrjÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j rjÇjßqhj rjÆKubj`)”}”(j¦XêThere are several reasons why you may want to combine the h-files from your daily GAMIT processing with other h-files before generating a times series or velocity solution. If you have more than ~ 50 sites in a regional network, it is more efficient and just as accurate to process these in GAMIT networks of 30–50 sites and then combine them in GLOBK than to use a single large network (the GAMIT limit is 99 sites). Further, if you are processing a regional network and want to tie it rigorously to a larger regional or global reference frame, you can do so by combining your h-file(s) with those generated by MIT or SOPAC from their IGS processing or another analysis center's processing of regional continuous networks. Finally, to obtain more useful long-term statistics from your time series, to strengthen the reference frame for survey-mode observations, or to reduce the computational time for velocity solutions, you may wish to first combine the h-files from 5–30 days into a single h-file to be used in subsequent solutions. We discuss the pros and cons of these strategies in :numref:`intro_prod_weighting` and :numref:`intro_prod_refframe`, but their mechanical implementation is straightforward. For processing of a single day, :program:`sh_glred` combines the GAMIT processing from multiple GNSS or multiple subnets using the :option:`-netext` option and includes independently processed regional or global networks using the :option:`LA`, :option:`LB` or :option:`LC` options. Running :program:`sh_glred` for a single day with :option:`-globk_prefit COMB` specified will direct :program:`globk` to save a combined h-file for further processing. For multiple days, this option together with :option:`-ncomb` will aggregate the data over several days.”j§]”(j±XGThere are several reasons why you may want to combine the h-files from your daily GAMIT processing with other h-files before generating a times series or velocity solution. If you have more than ~ 50 sites in a regional network, it is more efficient and just as accurate to process these in GAMIT networks of 30–50 sites and then combine them in GLOBK than to use a single large network (the GAMIT limit is 99 sites). Further, if you are processing a regional network and want to tie it rigorously to a larger regional or global reference frame, you can do so by combining your h-file(s) with those generated by MIT or SOPAC from their IGS processing or another analysis center’s processing of regional continuous networks. Finally, to obtain more useful long-term statistics from your time series, to strengthen the reference frame for survey-mode observations, or to reduce the computational time for velocity solutions, you may wish to first combine the h-files from 5–30 days into a single h-file to be used in subsequent solutions. We discuss the pros and cons of these strategies in ”…””}”(j¶jrjÇjßqhNjÆNubj’)”}”(j¦Œ:numref:`intro_prod_weighting`”j§]”j˜)”}”(j¦j'rj§]”j±Œintro_prod_weighting”…””}”(j¶j)rjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶j%rubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j3rŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_prod_weighting”ujÄj‘hj rjÆKj¶jrubj±Œ and ”…””}”(j¶jrjÇjßqhNjÆNubj’)”}”(j¦Œ:numref:`intro_prod_refframe`”j§]”j˜)”}”(j¦jKrj§]”j±Œintro_prod_refframe”…””}”(j¶jMrjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jIrubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jWrŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_prod_refframe”ujÄj‘hj rjÆKj¶jrubj±ŒZ, but their mechanical implementation is straightforward. For processing of a single day, ”…””}”(j¶jrjÇjßqhNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jmrjÇjßqhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jrubj±ŒP combines the GAMIT processing from multiple GNSS or multiple subnets using the ”…””}”(j¶jrjÇjßqhNjÆNubj’)”}”(j¦Œ:option:`-netext`”j§]”j˜)”}”(j¦jrj§]”j±Œ-netext”…””}”(j¶jƒrjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jrubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jrŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-netext”ujÄj‘hj rjÆKj¶jrubj±ŒS option and includes independently processed regional or global networks using the ”…””}”(j¶jrjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LA`”j§]”j˜)”}”(j¦j¥rj§]”j±ŒLA”…””}”(j¶j§rjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j£rubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j±rŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLA”ujÄj‘hj rjÆKj¶jrubj±Œ, ”…””}”(j¶jrjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LB`”j§]”j˜)”}”(j¦jÉrj§]”j±ŒLB”…””}”(j¶jËrjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jÇrubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÕrŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLB”ujÄj‘hj rjÆKj¶jrubj±Œ or ”…””}”(j¶jrjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LC`”j§]”j˜)”}”(j¦jírj§]”j±ŒLC”…””}”(j¶jïrjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jërubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jùrŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLC”ujÄj‘hj rjÆKj¶jrubj±Œ options. Running ”…””}”(j¶jrjÇjßqhNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jsjÇjßqhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jrubj±Œ for a single day with ”…””}”(j¶jrjÇjßqhNjÆNubj’)”}”(j¦Œ:option:`-globk_prefit COMB`”j§]”j˜)”}”(j¦j#sj§]”j±Œ-globk_prefit COMB”…””}”(j¶j%sjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j!subaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j/sŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-globk_prefit COMB”ujÄj‘hj rjÆKj¶jrubj±Œ specified will direct ”…””}”(j¶jrjÇjßqhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jEsjÇjßqhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jrubj±Œ` to save a combined h-file for further processing. For multiple days, this option together with ”…””}”(j¶jrjÇjßqhNjÆNubj’)”}”(j¦Œ:option:`-ncomb`”j§]”j˜)”}”(j¦jYsj§]”j±Œ-ncomb”…””}”(j¶j[sjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jWsubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jesŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-ncomb”ujÄj‘hj rjÆKj¶jrubj±Œ+ will aggregate the data over several days.”…””}”(j¶jrjÇjßqhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj rjÆKj¶j rjÇjßqubj`)”}”(j¦XÂ:program:`sh_glred` allows you to automatically download and/or link in h-files from an external source. If the :option:`F` option is specified, h-files implied by the :option:`-net` option will be downloaded from MIT or SOPAC into the primary h-file directory (specified by :content:`glfpth` in :file:`process.defaults` and nominally :file:`glbf/`). Alternatively, you can collect the h-files in advance in the directory specified by :content:`hfnd` in :file:`process.defaults` and then set the :option:`LA`, :option:`LB`, and/or :option:`LC` options to link these files into :file:`glbf/`. :option:`LA` refers to ascii h-files (requiring :program:`htoglb` translation) of the form :file:`h{}{}?.{}{}` (e.g. SOPAC network files), :option:`LB` to binary h-files of the form :file:`h{}{
}{}????_{}{}.gl?` (with :file:`.glx` given precedence over :file:`.glr`), and :option:`LC` to binary h-files of the form :file:`H{}{}{
}_{}{}.GLX` (e.g., MIT combined h-files). For example, to use local processing in combination with MIT global h-files previously downloaded onto your system, the command to generate a 30-day time series for experiment "emed" would be”j§]”(jj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j…sjÇjßqhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jsubj±Œ] allows you to automatically download and/or link in h-files from an external source. If the ”…””}”(j¶jsjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`F`”j§]”j˜)”}”(j¦j™sj§]”j±ŒF”…””}”(j¶j›sjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j—subaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j¥sŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶jÖLujÄj‘hj rjÆKj¶jsubj±Œ- option is specified, h-files implied by the ”…””}”(j¶jsjÇjßqhNjÆNubj’)”}”(j¦Œ:option:`-net`”j§]”j˜)”}”(j¦j¼sj§]”j±Œ-net”…””}”(j¶j¾sjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jºsubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÈsŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-net”ujÄj‘hj rjÆKj¶jsubj±Œ] option will be downloaded from MIT or SOPAC into the primary h-file directory (specified by ”…””}”(j¶jsjÇjßqhNjÆNubj˜)”}”(j¦Œ:content:`glfpth`”j§]”j±Œglfpth”…””}”(j¶jÞsjÇjßqhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jsubj±Œ in ”…””}”(j¶jsjÇjßqhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jñsjÇjßqhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œ and nominally ”…””}”(j¶jsjÇjßqhNjÆNubj˜)”}”(j¦Œ :file:`glbf/`”j§]”j±Œglbf/”…””}”(j¶jtjÇjßqhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±ŒW). Alternatively, you can collect the h-files in advance in the directory specified by ”…””}”(j¶jsjÇjßqhNjÆNubj˜)”}”(j¦Œ:content:`hfnd`”j§]”j±Œhfnd”…””}”(j¶jtjÇjßqhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jsubj±Œ in ”…””}”j¶jssbj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶j.tjÇjßqhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œ and then set the ”…””}”(j¶jsjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LA`”j§]”j˜)”}”(j¦jEtj§]”j±ŒLA”…””}”(j¶jGtjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jCtubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jQtŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLA”ujÄj‘hj rjÆKj¶jsubj±Œ, ”…””}”(j¶jsjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LB`”j§]”j˜)”}”(j¦jitj§]”j±ŒLB”…””}”(j¶jktjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jgtubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jutŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLB”ujÄj‘hj rjÆKj¶jsubj±Œ , and/or ”…””}”(j¶jsjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LC`”j§]”j˜)”}”(j¦jtj§]”j±ŒLC”…””}”(j¶jtjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j‹tubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j™tŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLC”ujÄj‘hj rjÆKj¶jsubj±Œ" options to link these files into ”…””}”(j¶jsjÇjßqhNjÆNubj˜)”}”(j¦Œ :file:`glbf/`”j§]”j±Œglbf/”…””}”(j¶j¯tjÇjßqhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œ. ”…””}”(j¶jsjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LA`”j§]”j˜)”}”(j¦jÆtj§]”j±ŒLA”…””}”(j¶jÈtjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jÄtubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÒtŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLA”ujÄj‘hj rjÆKj¶jsubj±Œ$ refers to ascii h-files (requiring ”…””}”(j¶jsjÇjßqhNjÆNubjj)”}”(j¦Œ:program:`htoglb`”j§]”j±Œhtoglb”…””}”(j¶jètjÇjßqhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jsubj±Œ translation) of the form ”…””}”(j¶jsjÇjßqhNjÆNubj˜)”}”(j¦Œ':file:`h{}{}?.{}{}`”j§]”(j±Œh”…””}”(j¶jútjÇjßqhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jujÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jútubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jujÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jútubj±Œ?.”…””}”(j¶jútjÇjßqhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j"ujÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jútubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j0ujÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jútubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œ (e.g. SOPAC network files), ”…””}”(j¶jsjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LB`”j§]”j˜)”}”(j¦jMuj§]”j±ŒLB”…””}”(j¶jOujÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jKuubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jYuŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLB”ujÄj‘hj rjÆKj¶jsubj±Œ to binary h-files of the form ”…””}”(j¶jsjÇjßqhNjÆNubj˜)”}”(j¦Œ3:file:`h{}{
}{}????_{}{}.gl?`”j§]”(j±Œh”…””}”(j¶joujÇjßqhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jwujÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jouubj )”}”(j¦Œ
”j§]”j±Œ
”…””}”(j¶j…ujÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jouubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j“ujÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jouubj±Œ????_”…””}”(j¶joujÇjßqhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j¥ujÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jouubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j³ujÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jouubj±Œ.gl?”…””}”(j¶joujÇjßqhNjÆNubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œ (with ”…””}”(j¶jsjÇjßqhNjÆNubj˜)”}”(j¦Œ :file:`.glx`”j§]”j±Œ.glx”…””}”(j¶jÒujÇjßqhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œ given precedence over ”…””}”(j¶jsjÇjßqhNjÆNubj˜)”}”(j¦Œ :file:`.glr`”j§]”j±Œ.glr”…””}”(j¶jçujÇjßqhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œ), and ”…””}”(j¶jsjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LC`”j§]”j˜)”}”(j¦jþuj§]”j±ŒLC”…””}”(j¶jvjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jüuubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j vŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLC”ujÄj‘hj rjÆKj¶jsubj±Œ to binary h-files of the form ”…””}”j¶jssbj˜)”}”(j¦Œ/:file:`H{}{}{
}_{}{}.GLX`”j§]”(j±ŒH”…””}”(j¶j vjÇjßqhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j(vjÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j vubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j6vjÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j vubj )”}”(j¦Œ
”j§]”j±Œ
”…””}”(j¶jDvjÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j vubj±Œ_”…””}”(j¶j vjÇjßqhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jVvjÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j vubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jdvjÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j vubj±Œ.GLX”…””}”(j¶j vjÇjßqhNjÆNubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œâ (e.g., MIT combined h-files). For example, to use local processing in combination with MIT global h-files previously downloaded onto your system, the command to generate a 30-day time series for experiment “emed†would be”…””}”(j¶jsjÇjßqhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj rjÆKj¶j rjÇjßqubj)”}”(j¦ŒA$ sh_glred -expt emed -s 2009 121 2009 150 -net MIT -opt H LC G T”j§]”j±ŒA$ sh_glred -expt emed -s 2009 121 2009 150 -net MIT -opt H LC G T”…””}”j¶j‰vsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj rjÆKj¶j rjÇjßqubj`)”}”(j¦XÖSince :program:`sh_glred` will look for all binary h-files in the :file:`glbf/` directory, created previously when you generated the time series, you can leave out the :option:`-net`, :option:`H`, and :option:`LA` options when combining the files. This feature is particularly useful if the days you want to aggregate are not continuous (e.g. from a survey) and you have used the :option:`-local` option in the :program:`sh_glred` command that generated the time series.”j§]”(j±ŒSince ”…””}”(j¶j™vjÇjßqhNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j¡vjÇjßqhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j™vubj±Œ) will look for all binary h-files in the ”…””}”(j¶j™vjÇjßqhNjÆNubj˜)”}”(j¦Œ :file:`glbf/`”j§]”j±Œglbf/”…””}”(j¶j³vjÇjßqhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j™vubj±ŒY directory, created previously when you generated the time series, you can leave out the ”…””}”(j¶j™vjÇjßqhNjÆNubj’)”}”(j¦Œ:option:`-net`”j§]”j˜)”}”(j¦jÊvj§]”j±Œ-net”…””}”(j¶jÌvjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jÈvubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jÖvŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-net”ujÄj‘hj rjÆKj¶j™vubj±Œ, ”…””}”(j¶j™vjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`H`”j§]”j˜)”}”(j¦jîvj§]”j±ŒH”…””}”(j¶jðvjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jìvubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”júvŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶j‡MujÄj‘hj rjÆKj¶j™vubj±Œ, and ”…””}”(j¶j™vjÇjßqhNjÆNubj’)”}”(j¦Œ :option:`LA`”j§]”j˜)”}”(j¦jwj§]”j±ŒLA”…””}”(j¶jwjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jwubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jwŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒLA”ujÄj‘hj rjÆKj¶j™vubj±Œ§ options when combining the files. This feature is particularly useful if the days you want to aggregate are not continuous (e.g. from a survey) and you have used the ”…””}”(j¶j™vjÇjßqhNjÆNubj’)”}”(j¦Œ:option:`-local`”j§]”j˜)”}”(j¦j5wj§]”j±Œ-local”…””}”(j¶j7wjÇjßqhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j3wubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jAwŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-local”ujÄj‘hj rjÆKj¶j™vubj±Œ option in the ”…””}”(j¶j™vjÇjßqhNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jWwjÇjßqhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j™vubj±Œ( command that generated the time series.”…””}”(j¶j™vjÇjßqhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj rjÆKj¶j rjÇjßqubj`)”}”(j¦XEIf you are combining data over a span that is long enough that the error in the *a priori* velocity of any of your sites is large enough to cause an error in position, you should estimate velocities in the combination; however, it's generally better to make the span of the combination short enough that this is not an issue.”j§]”(j±ŒPIf you are combining data over a span that is long enough that the error in the ”…””}”(j¶jowjÇjßqhNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jwwjÇjßqhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jowubj±Œí velocity of any of your sites is large enough to cause an error in position, you should estimate velocities in the combination; however, it’s generally better to make the span of the combination short enough that this is not an issue.”…””}”(j¶jowjÇjßqhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj rjÆKj¶j rjÇjßqubej·}”(j¹]”(Œcombining-h-files”j rej»]”j½]”(Œcombining h-files”Œintro_prod_combine”ejÀ]”jÂ]”ujÄh_j¶jßqjÇjßqhj rjÆKjÒ }”j•wjrsjÔ }”j rjrsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j rj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj rjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jîqjâqjýqjñquj_}”(Œrel”jîqŒdate”jýqujc}”je}”j r]”jrasjg}”(j•wj rj”wj‘wuji}”(j•wˆj”w‰uj¹}”(j rj rj‘wj rujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ8Hyperlink target "intro-prod-combine" is not referenced.”…””}”j¶j¿wsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j¼wubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j rŒline”KujÄjø ubajˆNj‰]”j‹NjÇjßqubj j£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jÚwsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j×wjÇj×wubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jéwjÇj×whNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j×wjÇj×wubje)”}”(j¦Œ.. _intro_prod_editing:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-prod-editing”ujÄjdjÆKj¶j×wjÇj×whŒF/chandler/home/floyd/public_html/gg/docs/source/intro/prod/editing.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ Data Editing”j§]”j±Œ Data Editing”…””}”(j¶jxjÇj×whNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jxjÇj×whjxjÆKubj`)”}”(j¦X½Your solutions will be corrupted if you include data that are statistical outliers. For a time series from independent h-files, an error in one component of one site's coordinates will not affect any other site (and may have minimal effect on the other components), but as soon as you combine h-files with common parameters, whether multiple networks on a single day or the results from more than one day, the different estimates of the common parameter will clash, raising chi-square and distorting the solution. There are two ways you can remove outliers: using the :content:`rename` command of the :content:`eq_file` and using the :content:`sig_neu` command directly in the :program:`globk` command file. In the :content:`rename` command, if you designate the extent as :content:`_XCL` the site will always be excluded; with :content:`_XPS` the site will be excluded from any solution of more than one day but will still appear in daily time series; e.g.”j§]”(j±X:Your solutions will be corrupted if you include data that are statistical outliers. For a time series from independent h-files, an error in one component of one site’s coordinates will not affect any other site (and may have minimal effect on the other components), but as soon as you combine h-files with common parameters, whether multiple networks on a single day or the results from more than one day, the different estimates of the common parameter will clash, raising chi-square and distorting the solution. There are two ways you can remove outliers: using the ”…””}”(j¶jxjÇj×whNjÆNubj˜•)”}”(j¦Œ:content:`rename`”j§]”j±Œrename”…””}”(j¶jxjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jxubj±Œ command of the ”…””}”(j¶jxjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`eq_file`”j§]”j±Œeq_file”…””}”(j¶j0xjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jxubj±Œ and using the ”…””}”(j¶jxjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`sig_neu`”j§]”j±Œsig_neu”…””}”(j¶jCxjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jxubj±Œ command directly in the ”…””}”(j¶jxjÇj×whNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jVxjÇj×whNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jxubj±Œ command file. In the ”…””}”(j¶jxjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`rename`”j§]”j±Œrename”…””}”(j¶jhxjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jxubj±Œ) command, if you designate the extent as ”…””}”(j¶jxjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`_XCL`”j§]”j±Œ_XCL”…””}”(j¶j{xjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jxubj±Œ( the site will always be excluded; with ”…””}”(j¶jxjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`_XPS`”j§]”j±Œ_XPS”…””}”(j¶jŽxjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jxubj±Œr the site will be excluded from any solution of more than one day but will still appear in daily time series; e.g.”…””}”(j¶jxjÇj×whNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjxjÆKj¶jxjÇj×wubj)”}”(j¦ŒCrename MIT algo_gps algo_xcl 1997 5 14 0 0 1997 5 17 24 0”j§]”j±ŒCrename MIT algo_gps algo_xcl 1997 5 14 0 0 1997 5 17 24 0”…””}”j¶j§xsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjxjÆKj¶jxjÇj×wubj`)”}”(j¦Xwill remove from the solution the observations of ALGO in any h-files containing the characters :content:`MIT` between 14 and 17 May 1997. Note that the date span specified must completely encompass the start time of the first h-file and the end time of the last h-file. The h-file selector entry and/or the dates may be omitted for a more expansive exclusion. With the :content:`sig_neu` command you can effectively remove the effect of an error in a particular component by adding sufficient noise that it has negligible weight, e.g.”j§]”(j±Œ`will remove from the solution the observations of ALGO in any h-files containing the characters ”…””}”(j¶j·xjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`MIT`”j§]”j±ŒMIT”…””}”(j¶j¿xjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j·xubj±X between 14 and 17 May 1997. Note that the date span specified must completely encompass the start time of the first h-file and the end time of the last h-file. The h-file selector entry and/or the dates may be omitted for a more expansive exclusion. With the ”…””}”(j¶j·xjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`sig_neu`”j§]”j±Œsig_neu”…””}”(j¶jÒxjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j·xubj±Œ“ command you can effectively remove the effect of an error in a particular component by adding sufficient noise that it has negligible weight, e.g.”…””}”(j¶j·xjÇj×whNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjxjÆKj¶jxjÇj×wubj)”}”(j¦ŒDsig_neu MIT algo_gps 0 0 .5 1997 5 14 0 0 1997 5 18 0 0”j§]”j±ŒDsig_neu MIT algo_gps 0 0 .5 1997 5 14 0 0 1997 5 18 0 0”…””}”j¶jëxsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjxjÆKj¶jxjÇj×wubj`)”}”(j¦Œ®would reduce the effect of an error in height by adding :math:`0.25 \text{m}^2` in quadrature to the variance of the height component as estimated from the h-files specified.”j§]”(j±Œ8would reduce the effect of an error in height by adding ”…””}”(j¶jûxjÇj×whNjÆNubjO )”}”(j¦Œ:math:`0.25 \text{m}^2`”j§]”j±Œ0.25 \text{m}^2”…””}”(j¶jyjÇj×whNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jûxubj±Œ_ in quadrature to the variance of the height component as estimated from the h-files specified.”…””}”(j¶jûxjÇj×whNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjxjÆKj¶jxjÇj×wubj`)”}”(j¦X“Which of these approaches you choose is a matter of taste and could depend on the tools you use for editing. For continuous data, when you can afford to remove many outliers without weakening the solution, using the :content:`nsigma` option of the :program:`tsfit` program (see Chapter 4 of the `GLOBK Reference Manual `_) to automatically generate :content:`_XPS` commands, or the MATLAB-based interactive program `tsview `_ to generate :content:`_XPS` commands with the click of a mouse, are quite convenient. For survey-mode date, when every observation counts and you often want to down-weight heights but not horizontal components or only one horizontal component, :content:`sig_neu` commands are more convenient. The GAMIT utility :program:`grw` can be used to generate :content:`sig_neu` commands with only a few key-strokes.”j§]”(j±ŒØWhich of these approaches you choose is a matter of taste and could depend on the tools you use for editing. For continuous data, when you can afford to remove many outliers without weakening the solution, using the ”…””}”(j¶jyjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`nsigma`”j§]”j±Œnsigma”…””}”(j¶j#yjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jyubj±Œ option of the ”…””}”(j¶jyjÇj×whNjÆNubjj)”}”(j¦Œ:program:`tsfit`”j§]”j±Œtsfit”…””}”(j¶j6yjÇj×whNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jyubj±Œ program (see Chapter 4 of the ”…””}”(j¶jyjÇj×whNjÆNubj÷ )”}”(j¦ŒG`GLOBK Reference Manual `_”j§]”j±ŒGLOBK Reference Manual”…””}”(j¶jHyjÇj×whNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGLOBK Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GLOBK_Ref.pdf”ujÄjö j¶jyubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œglobk-reference-manual”aj»]”j½]”Œglobk reference manual”ajÀ]”jÂ]”Œrefuri”jXyujÄjdj Kj¶jyubj±Œ) to automatically generate ”…””}”(j¶jyjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`_XPS`”j§]”j±Œ_XPS”…””}”(j¶jjyjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jyubj±Œ3 commands, or the MATLAB-based interactive program ”…””}”(j¶jyjÇj×whNjÆNubj÷ )”}”(j¦Œ0`tsview `_”j§]”j±Œtsview”…””}”(j¶j}yjÇj×whNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œtsview”j Œ$http://geoweb.mit.edu/~tah/GGMatlab/”ujÄjö j¶jyubje)”}”(j¦Œ' ”j§]”j·}”(j¹]”Œtsview”aj»]”j½]”Œtsview”ajÀ]”jÂ]”Œrefuri”jyujÄjdj Kj¶jyubj±Œ to generate ”…””}”(j¶jyjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`_XPS`”j§]”j±Œ_XPS”…””}”(j¶jŸyjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jyubj±ŒÙ commands with the click of a mouse, are quite convenient. For survey-mode date, when every observation counts and you often want to down-weight heights but not horizontal components or only one horizontal component, ”…””}”(j¶jyjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`sig_neu`”j§]”j±Œsig_neu”…””}”(j¶j²yjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jyubj±Œ1 commands are more convenient. The GAMIT utility ”…””}”(j¶jyjÇj×whNjÆNubjj)”}”(j¦Œ:program:`grw`”j§]”j±Œgrw”…””}”(j¶jÅyjÇj×whNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jyubj±Œ can be used to generate ”…””}”(j¶jyjÇj×whNjÆNubj˜)”}”(j¦Œ:content:`sig_neu`”j§]”j±Œsig_neu”…””}”(j¶j×yjÇj×whNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jyubj±Œ& commands with only a few key-strokes.”…””}”(j¶jyjÇj×whNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjxjÆKj¶jxjÇj×wubej·}”(j¹]”(Œ data-editing”jxej»]”j½]”(Œ data editing”Œintro_prod_editing”ejÀ]”jÂ]”ujÄh_j¶j×wjÇj×whjxjÆKjÒ }”jöyjøwsjÔ }”jxjøwsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jxj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjxjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jæwjÚwjõwjéwuj_}”(Œrel”jæwŒdate”jõwujc}”je}”jx]”jøwasjg}”(jöyjxjõyjòyjbyj_yj—yj”yuji}”(jöyˆjõy‰jbyˆj—yˆuj¹}”(jxjxjòyjxj_yjYyj”yjŽyujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ8Hyperlink target "intro-prod-editing" is not referenced.”…””}”j¶j zsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jzubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jxŒline”KujÄjø ubajˆNj‰]”j‹NjÇj×wubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j;zsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j8zjÇj8zubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jJzjÇj8zhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j8zjÇj8zubje)”}”(j¦Œ.. _intro_prod:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ intro-prod”ujÄjdjÆKj¶j8zjÇj8zhŒD/chandler/home/floyd/public_html/gg/docs/source/intro/prod/index.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ*Generating Time Series and Velocity Fields”j§]”j±Œ*Generating Time Series and Velocity Fields”…””}”(j¶jhzjÇj8zhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jezjÇj8zhjdzjÆKubjí)”}”(j¦hoj§]”jò)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j¶jjü]”(NŒintro/prod/combine”†”NŒintro/prod/editing”†”NŒintro/prod/weighting”†”NŒintro/prod/refframe”†”NŒintro/prod/ts_vels”†”ejþ]”(jƒzj…zj‡zj‰zj‹zejJÿÿÿÿjNj‰jˆj‰jKj‰j]”ujÄjñhjdzjÆKj¶jvzubaj·}”(j¹]”j»]”j aj½]”jÀ]”jÂ]”ujÄjìj¶jezjÇj8zhjdzjÆNubj`)”}”(j¦XìWhen input to GLOBK as quasi-observations, h-files can be considered either individually (:program:`glred`) to generate time series or as a group (:program:`globk`) to estimate positions and velocities. In either case the most important decisions facing the analyst are how to edit and weight the data and how to define and realize the reference frame. In making these decisions, you need to consider what stations to include explicitly, how to treat the orbits and Earth orientation parameters (EOP), and practical constraints on computation speed and data storage. In this chapter we discuss strategies you might use to achieve your analysis objectives with the tools available in the GLOBK suite of programs. The computation of multi-year solutions may be carried out conveniently in a directory (e.g. :file:`vsoln/`) parallel to the directories used for each survey or year of continuous data. At this same level, you may want to create an additional :file:`tables/` directory containing files common to all the years and the velocity solutions. If you carry out a series of multi-year analyses, then command files in additional processing directories (:file:`asoln/`, :file:`bsoln/`, etc.) can use the same path (:file:`../tables/`) to these common files.”j§]”(j±ŒZWhen input to GLOBK as quasi-observations, h-files can be considered either individually (”…””}”(j¶j•zjÇj8zhNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jzjÇj8zhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j•zubj±Œ)) to generate time series or as a group (”…””}”(j¶j•zjÇj8zhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j¯zjÇj8zhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j•zubj±X‚) to estimate positions and velocities. In either case the most important decisions facing the analyst are how to edit and weight the data and how to define and realize the reference frame. In making these decisions, you need to consider what stations to include explicitly, how to treat the orbits and Earth orientation parameters (EOP), and practical constraints on computation speed and data storage. In this chapter we discuss strategies you might use to achieve your analysis objectives with the tools available in the GLOBK suite of programs. The computation of multi-year solutions may be carried out conveniently in a directory (e.g. ”…””}”(j¶j•zjÇj8zhNjÆNubj˜)”}”(j¦Œ:file:`vsoln/`”j§]”j±Œvsoln/”…””}”(j¶jÁzjÇj8zhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j•zubj±Œˆ) parallel to the directories used for each survey or year of continuous data. At this same level, you may want to create an additional ”…””}”(j¶j•zjÇj8zhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jÖzjÇj8zhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j•zubj±Œ» directory containing files common to all the years and the velocity solutions. If you carry out a series of multi-year analyses, then command files in additional processing directories (”…””}”(j¶j•zjÇj8zhNjÆNubj˜)”}”(j¦Œ:file:`asoln/`”j§]”j±Œasoln/”…””}”(j¶jëzjÇj8zhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j•zubj±Œ, ”…””}”(j¶j•zjÇj8zhNjÆNubj˜)”}”(j¦Œ:file:`bsoln/`”j§]”j±Œbsoln/”…””}”(j¶j{jÇj8zhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j•zubj±Œ, etc.) can use the same path (”…””}”(j¶j•zjÇj8zhNjÆNubj˜)”}”(j¦Œ:file:`../tables/`”j§]”j±Œ ../tables/”…””}”(j¶j{jÇj8zhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j•zubj±Œ) to these common files.”…””}”(j¶j•zjÇj8zhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjdzjÆKj¶jezjÇj8zubej·}”(j¹]”(Œ*generating-time-series-and-velocity-fields”jczej»]”j½]”(Œ*generating time series and velocity fields”Œ intro_prod”ejÀ]”jÂ]”ujÄh_j¶j8zjÇj8zhjdzjÆKjÒ }”j6{jYzsjÔ }”jczjYzsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jdzj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjdzjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jGzj;zjVzjJzuj_}”(Œrel”jGzŒdate”jVzujc}”je}”jcz]”jYzasjg}”(j6{jczj5{j2{uji}”(j6{ˆj5{‰uj¹}”(jczjezj2{jezujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ0Hyperlink target "intro-prod" is not referenced.”…””}”j¶j`{sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j]{ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jdzŒline”KujÄjø ubajˆNj‰]”j‹NjÇj8zubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j{{sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jx{jÇjx{ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jŠ{jÇjx{hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jx{jÇjx{ubje)”}”(j¦Œ.. _intro_prod_refframe:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-prod-refframe”ujÄjdjÆKj¶jx{jÇjx{hŒG/chandler/home/floyd/public_html/gg/docs/source/intro/prod/refframe.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒRealizing a Reference Frame”j§]”j±ŒRealizing a Reference Frame”…””}”(j¶j¨{jÇjx{hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j¥{jÇjx{hj¤{jÆKubj`)”}”(j¦X‹Although the GPS satellites provide a natural dynamic frame for ground-based geodesy, the doubly differenced phase observations (or equivalently, undifferenced phase with clocks estimated or provided) do not tie a ground station to the orbital constellation at the millimeter level we require for scientific studies. Rather, we define and realize a precise terrestrial frame by applying constraints to one or more sites in our network. GLOBK allows two approaches. The simplest, used also in GAMIT, is to apply in the :program:`globk` command file tight *a priori* uncertainties on the coordinates (positions and velocities) of one or more sites, e.g.”j§]”(j±XAlthough the GPS satellites provide a natural dynamic frame for ground-based geodesy, the doubly differenced phase observations (or equivalently, undifferenced phase with clocks estimated or provided) do not tie a ground station to the orbital constellation at the millimeter level we require for scientific studies. Rather, we define and realize a precise terrestrial frame by applying constraints to one or more sites in our network. GLOBK allows two approaches. The simplest, used also in GAMIT, is to apply in the ”…””}”(j¶j¶{jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j¾{jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¶{ubj±Œ command file tight ”…””}”(j¶j¶{jÇjx{hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jÐ{jÇjx{hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j¶{ubj±ŒW uncertainties on the coordinates (positions and velocities) of one or more sites, e.g.”…””}”(j¶j¶{jÇjx{hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤{jÆKj¶j¥{jÇjx{ubj)”}”(j¦Œsapr_neu all 1 1 1 .1 .1 .1 apr_neu algo .001 .001 .003 .001 .001 .003 apr_neu drao .002 .002 .002 .003 .003 .010”j§]”j±Œsapr_neu all 1 1 1 .1 .1 .1 apr_neu algo .001 .001 .003 .001 .001 .003 apr_neu drao .002 .002 .002 .003 .003 .010”…””}”j¶jè{sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhj¤{jÆK j¶j¥{jÇjx{ubj`)”}”(j¦ŒÍThis "finite constraints" approach is rarely used in GLOBK, however, because it can distort the network if the assigned constraints are not correct for the *a priori* coordinates and data in your solution.”j§]”(j±Œ This “finite constraints†approach is rarely used in GLOBK, however, because it can distort the network if the assigned constraints are not correct for the ”…””}”(j¶jø{jÇjx{hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j|jÇjx{hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jø{ubj±Œ' coordinates and data in your solution.”…””}”(j¶jø{jÇjx{hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤{jÆKj¶j¥{jÇjx{ubj`)”}”(j¦XhA more rigorous approach to frame realization is through "generalized constraints", in which you minimize the adjustments of coordinates of the frame-defining sites while estimating translation, rotation, and sometimes scale (Helmert parameters). With this approach, all of the reference sites are free to adjust (hence revealing bad data or coordinates) and any frame realized with a particular set of reference sites will differ from a frame realized with another set only in translation, rotation (and scale), with no internal distortion. You enact this approach by keeping the constraint in :program:`globk` free”j§]”(j±XWA more rigorous approach to frame realization is through “generalized constraintsâ€, in which you minimize the adjustments of coordinates of the frame-defining sites while estimating translation, rotation, and sometimes scale (Helmert parameters). With this approach, all of the reference sites are free to adjust (hence revealing bad data or coordinates) and any frame realized with a particular set of reference sites will differ from a frame realized with another set only in translation, rotation (and scale), with no internal distortion. You enact this approach by keeping the constraint in ”…””}”(j¶j|jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j |jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j|ubj±Œ free”…””}”(j¶j|jÇjx{hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤{jÆKj¶j¥{jÇjx{ubj)”}”(j¦Œ÷ apr_neu all 1 1 1 .1 .1 .1 # EOP loose if estimating rotation in glorg apr_wob 10 10 10 10 apr_ut1 10 10 mar_wob 3650 3650 365 365 mar_ut1 365 365 # EOP tight if estimating only translation in glorg x apr_wob .25 .25 .1 .1 x apr_ut1 .25 .1”j§]”j±Œ÷ apr_neu all 1 1 1 .1 .1 .1 # EOP loose if estimating rotation in glorg apr_wob 10 10 10 10 apr_ut1 10 10 mar_wob 3650 3650 365 365 mar_ut1 365 365 # EOP tight if estimating only translation in glorg x apr_wob .25 .25 .1 .1 x apr_ut1 .25 .1”…””}”j¶j8|sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhj¤{jÆKj¶j¥{jÇjx{ubj`)”}”(j¦Œ`and invoking :program:`glorg` to apply generalized constraints ("stabilization" in GLOBK jargon)”j§]”(j±Œ and invoking ”…””}”(j¶jH|jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jP|jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jH|ubj±ŒG to apply generalized constraints (“stabilization†in GLOBK jargon)”…””}”(j¶jH|jÇjx{hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤{jÆK#j¶j¥{jÇjx{ubj)”}”(j¦Œ  pos_org xtran ytran ztran xrot yrot zrot rate_org xtran ytran ztran xrot yrot zrot # translation-only x pos_org xtran ytran ztran x rate_org xtran ytran ztran”j§]”j±Œ  pos_org xtran ytran ztran xrot yrot zrot rate_org xtran ytran ztran xrot yrot zrot # translation-only x pos_org xtran ytran ztran x rate_org xtran ytran ztran”…””}”j¶jh|sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhj¤{jÆK%j¶j¥{jÇjx{ubj`)”}”(j¦XªEstimating both translation and rotation in :program:`glorg` is necessary for global and large regional networks and preferred for any network over ~ 50 km in extent. (The scale parameter can usually be omitted—but see the discussion in :cite:t:`Dong_et_al_1998`.) However, estimating rotation in addition to translation is robust only if you have at least six stabilization sites with a good geometric distribution. If there is only one site at the outer edge of the network (i.e. with a long "lever arm"), all of its error will go into the combination of rotation parameters in its direction. When this happens, both the uncertainty and residual of that site will be very small, there will be insufficient redundancy to provide stability to the network, and the stabilization statistics will be less meaningful. When you estimate translation only, you can get by with fewer stabilization sites and the geometry is much less important.”j§]”(j±Œ,Estimating both translation and rotation in ”…””}”(j¶jx|jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j€|jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jx|ubj±Œ³ is necessary for global and large regional networks and preferred for any network over ~ 50 km in extent. (The scale parameter can usually be omitted—but see the discussion in ”…””}”(j¶jx|jÇjx{hNjÆNubj’)”}”(j¦Œ:cite:t:`Dong_et_al_1998`”j§]”j)”}”(j¦j”|j§]”j±ŒDong_et_al_1998”…””}”(j¶j–|jÇjx{hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶j’|ubaj·}”(j¹]”Œid1”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j |Œreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒDong_et_al_1998”ujÄj‘hj¤{jÆK-j¶jx|ubj±X¦.) However, estimating rotation in addition to translation is robust only if you have at least six stabilization sites with a good geometric distribution. If there is only one site at the outer edge of the network (i.e. with a long “lever armâ€), all of its error will go into the combination of rotation parameters in its direction. When this happens, both the uncertainty and residual of that site will be very small, there will be insufficient redundancy to provide stability to the network, and the stabilization statistics will be less meaningful. When you estimate translation only, you can get by with fewer stabilization sites and the geometry is much less important.”…””}”(j¶jx|jÇjx{hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤{jÆK-j¶j¥{jÇjx{ubj`)”}”(j¦Xy The simplest and most robust approach to frame realization, for all but the smallest networks, is to incorporate into your solution 10 or more sites whose coordinates are included with small uncertainties in the :file:`.apr` file from the most recent International Terrestrial Reference Frame (ITRF) or its current IGS realization. The GLOBK template command files are set up to use :file:`igb14_comb.apr`, which is the second IGS realization of ITRF2014 plus the addition of older, no longer used sites from :file:`itrf14.apr`. The :file:`igb14_comb.eq` file that accompanies this :file:`.apr` file has :content:`rename` commands the are consistent with the 8-character site names in :file:`igb14_comb.apr` (or :file:`itrf14.apr`). In your solutions you can realize this frame either by including data from all of the chosen reference sites in your GAMIT processing, run in :content:`BASELINE` mode with IGS orbits fixed, or by including in your GAMIT processing 3–4 IGS sites (not necessarily reference sites) that will tie your h-file to an h-file generated by MIT or SOPAC from global processing. To be completely rigorous in this latter case, you should include orbit estimation in your GAMIT run (:content:`RELAX` mode) and allow the global h-file to determine the orbit. However, in practice with current IGS orbits, you can keep them fixed in the regional solution (:content:`BASELINE` mode in GAMIT) and allow them to adjust implicitly (in the global solution) by omitting the :content:`apr_svs` command in :program:`globk`. Whether orbits are estimated implicitly or explicitly for the global network, you need to include a fully global h-file (e.g. MIT GLX or all of the SOPAC "igs" h-files), though you do not have to explicitly estimate the coordinates of all the sites. The principle here is that the global h-file(s) includes all of the information from processing the phase data whether or not the parameters (orbital or site coordinates) are explicitly estimated. Thus you can explicitly estimate (:content:`use_site`) only the sites you intend to use in :program:`glorg` for stabilization or tectonic frame realization (:content:`plate` command of :program:`glorg`) or which are otherwise important scientifically for your study, thus saving considerable computation time compared with estimating explicitly the orbits and the coordinates of 300+ sites in the global h-files. Using externally generated GLOBK h-files gives you access to a large number of stations without the computational burden of running GAMIT yourself with a large network. The potential disadvantage is that the models you have used may not match those used by the external processing center (some matter more than others) and there is some burden imposed in downloading and storing the files (15–20 Mb per day) on your system. The script :program:`sh_get_hfiles`, invoked directly or via :program:`sh_glred` facilitates downloading the files.”j§]”(j±ŒÔThe simplest and most robust approach to frame realization, for all but the smallest networks, is to incorporate into your solution 10 or more sites whose coordinates are included with small uncertainties in the ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jÄ|jÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¼|ubj±ŒŸ file from the most recent International Terrestrial Reference Frame (ITRF) or its current IGS realization. The GLOBK template command files are set up to use ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:file:`igb14_comb.apr`”j§]”j±Œigb14_comb.apr”…””}”(j¶jÙ|jÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¼|ubj±Œh, which is the second IGS realization of ITRF2014 plus the addition of older, no longer used sites from ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:file:`itrf14.apr`”j§]”j±Œ itrf14.apr”…””}”(j¶jî|jÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¼|ubj±Œ. The ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:file:`igb14_comb.eq`”j§]”j±Œ igb14_comb.eq”…””}”(j¶j}jÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¼|ubj±Œ file that accompanies this ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶j}jÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¼|ubj±Œ file has ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`rename`”j§]”j±Œrename”…””}”(j¶j-}jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¼|ubj±Œ@ commands the are consistent with the 8-character site names in ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:file:`igb14_comb.apr`”j§]”j±Œigb14_comb.apr”…””}”(j¶j@}jÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¼|ubj±Œ (or ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:file:`itrf14.apr`”j§]”j±Œ itrf14.apr”…””}”(j¶jU}jÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¼|ubj±Œ‘). In your solutions you can realize this frame either by including data from all of the chosen reference sites in your GAMIT processing, run in ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`BASELINE`”j§]”j±ŒBASELINE”…””}”(j¶jj}jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¼|ubj±X7 mode with IGS orbits fixed, or by including in your GAMIT processing 3–4 IGS sites (not necessarily reference sites) that will tie your h-file to an h-file generated by MIT or SOPAC from global processing. To be completely rigorous in this latter case, you should include orbit estimation in your GAMIT run (”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`RELAX`”j§]”j±ŒRELAX”…””}”(j¶j}}jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¼|ubj±Œ› mode) and allow the global h-file to determine the orbit. However, in practice with current IGS orbits, you can keep them fixed in the regional solution (”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`BASELINE`”j§]”j±ŒBASELINE”…””}”(j¶j}jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¼|ubj±Œ] mode in GAMIT) and allow them to adjust implicitly (in the global solution) by omitting the ”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`apr_svs`”j§]”j±Œapr_svs”…””}”(j¶j£}jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¼|ubj±Œ command in ”…””}”(j¶j¼|jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j¶}jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¼|ubj±Xç. Whether orbits are estimated implicitly or explicitly for the global network, you need to include a fully global h-file (e.g. MIT GLX or all of the SOPAC “igs†h-files), though you do not have to explicitly estimate the coordinates of all the sites. The principle here is that the global h-file(s) includes all of the information from processing the phase data whether or not the parameters (orbital or site coordinates) are explicitly estimated. Thus you can explicitly estimate (”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`use_site`”j§]”j±Œuse_site”…””}”(j¶jÈ}jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¼|ubj±Œ&) only the sites you intend to use in ”…””}”(j¶j¼|jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jÛ}jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¼|ubj±Œ2 for stabilization or tectonic frame realization (”…””}”(j¶j¼|jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`plate`”j§]”j±Œplate”…””}”(j¶jí}jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¼|ubj±Œ command of ”…””}”(j¶j¼|jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j~jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¼|ubj±X‰) or which are otherwise important scientifically for your study, thus saving considerable computation time compared with estimating explicitly the orbits and the coordinates of 300+ sites in the global h-files. Using externally generated GLOBK h-files gives you access to a large number of stations without the computational burden of running GAMIT yourself with a large network. The potential disadvantage is that the models you have used may not match those used by the external processing center (some matter more than others) and there is some burden imposed in downloading and storing the files (15–20 Mb per day) on your system. The script ”…””}”(j¶j¼|jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`sh_get_hfiles`”j§]”j±Œ sh_get_hfiles”…””}”(j¶j~jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¼|ubj±Œ, invoked directly or via ”…””}”(j¶j¼|jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j$~jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¼|ubj±Œ# facilitates downloading the files.”…””}”(j¶j¼|jÇjx{hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤{jÆK4j¶j¥{jÇjx{ubj`)”}”(j¦XTIf you have a small network with only one or two (or perhaps no) sites with good *a priori* coordinates, you may be able to realize an adequate reference frame by fixing or tightly constraining one site. This works because the uncertainties and errors in "absolute" coordinates (relative to the satellites) map into uncertainties and errors in relative coordinates (your primary interest) roughly reduced by a factor of the satellite altitude (20,000 km) to the baseline length. So, for example, a 1 m uncertainty (or error) in the coordinates of a constrained site induces an uncertainty (or error) of only ~ 1 mm over a 20 km baseline. (The actual reduction depends on session length and geometry, but for short baselines you have considerable latitude in setting the *a priori* constraint.) Although you can apply the constraints with the :content:`apr_neu` command in :program:`globk`, as noted above, you may want to invoke :program:`glorg` for other reasons and prefer to leave the :program:`globk` constraints loose and apply the constraint using the :content:`force` or :content:`constrain` commands:”j§]”(j±ŒQIf you have a small network with only one or two (or perhaps no) sites with good ”…””}”(j¶j<~jÇjx{hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jD~jÇjx{hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j<~ubj±X« coordinates, you may be able to realize an adequate reference frame by fixing or tightly constraining one site. This works because the uncertainties and errors in “absolute†coordinates (relative to the satellites) map into uncertainties and errors in relative coordinates (your primary interest) roughly reduced by a factor of the satellite altitude (20,000 km) to the baseline length. So, for example, a 1 m uncertainty (or error) in the coordinates of a constrained site induces an uncertainty (or error) of only ~ 1 mm over a 20 km baseline. (The actual reduction depends on session length and geometry, but for short baselines you have considerable latitude in setting the ”…””}”(j¶j<~jÇjx{hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶jV~jÇjx{hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j<~ubj±Œ> constraint.) Although you can apply the constraints with the ”…””}”(j¶j<~jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`apr_neu`”j§]”j±Œapr_neu”…””}”(j¶jh~jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j<~ubj±Œ command in ”…””}”(j¶j<~jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j{~jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j<~ubj±Œ), as noted above, you may want to invoke ”…””}”(j¶j<~jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j~jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j<~ubj±Œ+ for other reasons and prefer to leave the ”…””}”(j¶j<~jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jŸ~jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j<~ubj±Œ6 constraints loose and apply the constraint using the ”…””}”(j¶j<~jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`force`”j§]”j±Œforce”…””}”(j¶j±~jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j<~ubj±Œ or ”…””}”(j¶j<~jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`constrain`”j§]”j±Œ constrain”…””}”(j¶jÄ~jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j<~ubj±Œ commands:”…””}”(j¶j<~jÇjx{hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤{jÆKAj¶j¥{jÇjx{ubj)”}”(j¦Œ­constrain algo npos 0. .001 constrain algo epos 0. .001 constrain algo upos 0. .003 constrain algo ndot 0. .001 constrain algo edot 0. .001 constrain algo udot 0. .003”j§]”j±Œ­constrain algo npos 0. .001 constrain algo epos 0. .001 constrain algo upos 0. .003 constrain algo ndot 0. .001 constrain algo edot 0. .001 constrain algo udot 0. .003”…””}”j¶jÝ~sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhj¤{jÆKGj¶j¥{jÇjx{ubj`)”}”(j¦XêWhen generating time series and velocity solutions used to evaluate the quality of the data and your analysis approach, the theoretical definition of the reference frame is not important. It is usually best to carry out these steps in the no-net-rotation (NNR) frame of the ITRF (and strictly speaking, you should use this frame if you are not estimating orbits since it is consistent with the EOPs). Eventually, however, you will want to view the velocities in a frame that is natural for geophysical interpretation, and that is usually with respect to a stable tectonic block near your network. If you want to use the realization of a major plate as determined from the ITRF data set (e.g. :cite:t:`Altamimi_et_al_2012`), then it is easy to do so simply by substituting in :program:`glorg` (not necessarily in :program:`globk`) one of the rotated ITRF apr files provided in :file:`~/gg/tables/` (e.g. :file:`igb14_comb_eura.apr`). The quality of the stabilization should be identical to one carried out with :file:`igb14_comb.apr` (NNR) since the relative motions of the sites has not been changed. If you want to realize a plate or smaller rigid block from your own solution, then you can do so using the :content:`plate` command of :program:`glorg`, e.g.”j§]”(j±X´When generating time series and velocity solutions used to evaluate the quality of the data and your analysis approach, the theoretical definition of the reference frame is not important. It is usually best to carry out these steps in the no-net-rotation (NNR) frame of the ITRF (and strictly speaking, you should use this frame if you are not estimating orbits since it is consistent with the EOPs). Eventually, however, you will want to view the velocities in a frame that is natural for geophysical interpretation, and that is usually with respect to a stable tectonic block near your network. If you want to use the realization of a major plate as determined from the ITRF data set (e.g. ”…””}”(j¶jí~jÇjx{hNjÆNubj’)”}”(j¦Œ:cite:t:`Altamimi_et_al_2012`”j§]”j)”}”(j¦j÷~j§]”j±ŒAltamimi_et_al_2012”…””}”(j¶jù~jÇjx{hNjÆNubaj·}”(j¹]”j»]”(j£Œcite”Œcite-t”ej½]”jÀ]”jÂ]”ujÄj*j¶jõ~ubaj·}”(j¹]”Œid2”aj»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jŒreftype”j…Œ refexplicit”‰Œrefwarn”‰j¶ŒAltamimi_et_al_2012”ujÄj‘hj¤{jÆKPj¶jí~ubj±Œ6), then it is easy to do so simply by substituting in ”…””}”(j¶jí~jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jjÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jí~ubj±Œ (not necessarily in ”…””}”(j¶jí~jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j+jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jí~ubj±Œ0) one of the rotated ITRF apr files provided in ”…””}”(j¶jí~jÇjx{hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶j=jÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jí~ubj±Œ (e.g. ”…””}”(j¶jí~jÇjx{hNjÆNubj˜)”}”(j¦Œ:file:`igb14_comb_eura.apr`”j§]”j±Œigb14_comb_eura.apr”…””}”(j¶jRjÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jí~ubj±ŒP). The quality of the stabilization should be identical to one carried out with ”…””}”(j¶jí~jÇjx{hNjÆNubj˜)”}”(j¦Œ:file:`igb14_comb.apr`”j§]”j±Œigb14_comb.apr”…””}”(j¶jgjÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jí~ubj±Œ° (NNR) since the relative motions of the sites has not been changed. If you want to realize a plate or smaller rigid block from your own solution, then you can do so using the ”…””}”(j¶jí~jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`plate`”j§]”j±Œplate”…””}”(j¶j|jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jí~ubj±Œ command of ”…””}”(j¶jí~jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jjÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jí~ubj±Œ, e.g.”…””}”(j¶jí~jÇjx{hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤{jÆKPj¶j¥{jÇjx{ubj)”}”(j¦Œ)plate noam algo nlib pie1 rcm5 brmu chur”j§]”j±Œ)plate noam algo nlib pie1 rcm5 brmu chur”…””}”j¶j§sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhj¤{jÆKWj¶j¥{jÇjx{ubj`)”}”(j¦XWith this command present, :program:`glorg` will estimate the rotation vector (Euler pole) for a block (spherical cap) containing these sites with respect to the stabilization frame. The :file:`.org` file print will contain the components and uncertainties of the rotation vector and will replace the velocity adjustments from the stabilization (i.e., with respect to the :file:`.apr` file) with residuals with respect to the plate prescribed to include that site (the velocity estimates themselves remain in the frame of the :file:`.apr` file). You can estimate any number of plates in a single solution so long as they are nearly independent and no one of them contains almost all of the sites used for stabilization (this will create a numerical instability). Running the script :program:`sh_org2vel` with the :program:`glorg` print file as input and the plate(s) specified with the names used in the :content:`plate` command will produce velocity summary file(s) with the motions of all sites in the solution with respect to each of the plates.”j§]”(j±ŒWith this command present, ”…””}”(j¶j·jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j¿jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j·ubj±Œ will estimate the rotation vector (Euler pole) for a block (spherical cap) containing these sites with respect to the stabilization frame. The ”…””}”(j¶j·jÇjx{hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶jÑjÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j·ubj±Œ­ file print will contain the components and uncertainties of the rotation vector and will replace the velocity adjustments from the stabilization (i.e., with respect to the ”…””}”(j¶j·jÇjx{hNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jæjÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j·ubj±ŒŽ file) with residuals with respect to the plate prescribed to include that site (the velocity estimates themselves remain in the frame of the ”…””}”(j¶j·jÇjx{hNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jûjÇjx{hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j·ubj±Œô file). You can estimate any number of plates in a single solution so long as they are nearly independent and no one of them contains almost all of the sites used for stabilization (this will create a numerical instability). Running the script ”…””}”(j¶j·jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`sh_org2vel`”j§]”j±Œ sh_org2vel”…””}”(j¶j€jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j·ubj±Œ with the ”…””}”(j¶j·jÇjx{hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j"€jÇjx{hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j·ubj±ŒK print file as input and the plate(s) specified with the names used in the ”…””}”(j¶j·jÇjx{hNjÆNubj˜)”}”(j¦Œ:content:`plate`”j§]”j±Œplate”…””}”(j¶j4€jÇjx{hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j·ubj±Œ€ command will produce velocity summary file(s) with the motions of all sites in the solution with respect to each of the plates.”…””}”(j¶j·jÇjx{hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤{jÆK[j¶j¥{jÇjx{ubej·}”(j¹]”(Œrealizing-a-reference-frame”j£{ej»]”j½]”(Œrealizing a reference frame”Œintro_prod_refframe”ejÀ]”jÂ]”ujÄh_j¶jx{jÇjx{hj¤{jÆKjÒ }”jS€j™{sjÔ }”j£{j™{subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j¤{j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj¤{jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j‡{j{{j–{jŠ{uj_}”(Œrel”j‡{Œdate”j–{ujc}”je}”j£{]”j™{asjg}”(jS€j£{jR€jO€uji}”(jS€ˆjR€‰uj¹}”(j£{j¥{jO€j¥{j§|j’|j jõ~ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ9Hyperlink target "intro-prod-refframe" is not referenced.”…””}”j¶j}€sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jz€ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j¤{Œline”KujÄjø ubajˆNj‰]”j‹NjÇjx{ubj j£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j˜€sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j•€jÇj•€ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j§€jÇj•€hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j•€jÇj•€ubje)”}”(j¦Œ.. _intro_prod_ts_vels:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-prod-ts-vels”ujÄjdjÆKj¶j•€jÇj•€hŒF/chandler/home/floyd/public_html/gg/docs/source/intro/prod/ts_vels.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ-Generating Time Series and Velocity Solutions”j§]”j±Œ-Generating Time Series and Velocity Solutions”…””}”(j¶jÅ€jÇj•€hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j€jÇj•€hjÁ€jÆKubj`)”}”(j¦XÍTo generate time series or estimate velocities from several years of data, you need to run :program:`glred` or :program:`globk` directly rather than using :program:`sh_glred`. As with creating irregular combined h-files, you can create the :file:`.gdl` file using the :command:`ls` command from the directory you intend to use for the multi-year analysis. For example, for a multiyear analysis in :file:`pnw/vsoln/` using combined h-files from individual years,”j§]”(j±Œ[To generate time series or estimate velocities from several years of data, you need to run ”…””}”(j¶jÓ€jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jÛ€jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓ€ubj±Œ or ”…””}”(j¶jÓ€jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jí€jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓ€ubj±Œ directly rather than using ”…””}”(j¶jÓ€jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jÿ€jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓ€ubj±ŒB. As with creating irregular combined h-files, you can create the ”…””}”(j¶jÓ€jÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶jjÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÓ€ubj±Œ file using the ”…””}”(j¶jÓ€jÇj•€hNjÆNubjj)”}”(j¦Œ :command:`ls`”j§]”j±Œls”…””}”(j¶j&jÇj•€hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jÓ€ubj±Œt command from the directory you intend to use for the multi-year analysis. For example, for a multiyear analysis in ”…””}”(j¶jÓ€jÇj•€hNjÆNubj˜)”}”(j¦Œ:file:`pnw/vsoln/`”j§]”j±Œ pnw/vsoln/”…””}”(j¶j8jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÓ€ubj±Œ. using combined h-files from individual years,”…””}”(j¶jÓ€jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆKj¶j€jÇj•€ubj)”}”(j¦Œ&$ ls ../pnw??/gsoln/*GLX > pnw_all.gdl”j§]”j±Œ&$ ls ../pnw??/gsoln/*GLX > pnw_all.gdl”…””}”j¶jSsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÁ€jÆK j¶j€jÇj•€ubj`)”}”(j¦Œ(or, if you have not aggregated the data,”j§]”j±Œ(or, if you have not aggregated the data,”…””}”(j¶jcjÇj•€hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆKj¶j€jÇj•€ubj)”}”(j¦Œ($ cat ../pnw??/gsoln/*.gdl > pnw_all.gdl”j§]”j±Œ($ cat ../pnw??/gsoln/*.gdl > pnw_all.gdl”…””}”j¶jqsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÁ€jÆKj¶j€jÇj•€ubj`)”}”(j¦X¼using :command:`cat` with the :file:`.gdl` files produced by :program:`sh_glred`, rather than :command:`ls` with the :file:`.glx` and :file:`.GLX` files in :file:`glbf/` avoids having to add the :content:`+` signs for multiple files within a day when running :program:`glred` for the long-term time series. (When running :program:`globk` to get velocities all files are combined regardless of whether the :content:`+` signs are present or not.)”j§]”(j±Œusing ”…””}”(j¶jjÇj•€hNjÆNubjj)”}”(j¦Œ:command:`cat`”j§]”j±Œcat”…””}”(j¶j‰jÇj•€hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ with the ”…””}”(j¶jjÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶j›jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ files produced by ”…””}”(j¶jjÇj•€hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j°jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ, rather than ”…””}”(j¶jjÇj•€hNjÆNubjj)”}”(j¦Œ :command:`ls`”j§]”j±Œls”…””}”(j¶jÂjÇj•€hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ with the ”…””}”j¶jsbj˜)”}”(j¦Œ :file:`.glx`”j§]”j±Œ.glx”…””}”(j¶jÔjÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ and ”…””}”(j¶jjÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.GLX`”j§]”j±Œ.GLX”…””}”(j¶jéjÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ files in ”…””}”(j¶jjÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`glbf/`”j§]”j±Œglbf/”…””}”(j¶jþjÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ avoids having to add the ”…””}”(j¶jjÇj•€hNjÆNubj˜)”}”(j¦Œ :content:`+`”j§]”j±Œ+”…””}”(j¶j‚jÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jubj±Œ4 signs for multiple files within a day when running ”…””}”(j¶jjÇj•€hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j&‚jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ. for the long-term time series. (When running ”…””}”(j¶jjÇj•€hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j8‚jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±ŒD to get velocities all files are combined regardless of whether the ”…””}”(j¶jjÇj•€hNjÆNubj˜)”}”(j¦Œ :content:`+`”j§]”j±Œ+”…””}”(j¶jJ‚jÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jubj±Œ signs are present or not.)”…””}”(j¶jjÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆKj¶j€jÇj•€ubj`)”}”(j¦XYour first step should always be to generate time series so that you can evaluate the statistics of your data and determine if there are any outliers that will distort the velocity solution. To run :program:`glred` directly to produce a time series from this file, set (uncomment e.g.”j§]”(j±ŒÆYour first step should always be to generate time series so that you can evaluate the statistics of your data and determine if there are any outliers that will distort the velocity solution. To run ”…””}”(j¶jc‚jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jk‚jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jc‚ubj±ŒF directly to produce a time series from this file, set (uncomment e.g.”…””}”(j¶jc‚jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆKj¶j€jÇj•€ubj)”}”(j¦ŒD$ glred 6 glred.prt glred.log pnw_all.gdl globk.cmd >& glred_rep.out”j§]”j±ŒD$ glred 6 glred.prt glred.log pnw_all.gdl globk.cmd >& glred_rep.out”…””}”j¶jƒ‚sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÁ€jÆKj¶j€jÇj•€ubj`)”}”(j¦XThe solutions for all h-files, obtained independently, are written into a single print file (specified by :content:`prt_opt` for finite constraints using :program:`globk`, :content:`org_opt` for generalized constraints using :program:`glorg`) so you can plot the results with”j§]”(j±ŒjThe solutions for all h-files, obtained independently, are written into a single print file (specified by ”…””}”(j¶j“‚jÇj•€hNjÆNubj˜)”}”(j¦Œ:content:`prt_opt`”j§]”j±Œprt_opt”…””}”(j¶j›‚jÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j“‚ubj±Œ for finite constraints using ”…””}”(j¶j“‚jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j®‚jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j“‚ubj±Œ, ”…””}”(j¶j“‚jÇj•€hNjÆNubj˜)”}”(j¦Œ:content:`org_opt`”j§]”j±Œorg_opt”…””}”(j¶jÀ‚jÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j“‚ubj±Œ# for generalized constraints using ”…””}”(j¶j“‚jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jÓ‚jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j“‚ubj±Œ") so you can plot the results with”…””}”(j¶j“‚jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆKj¶j€jÇj•€ubj)”}”(j¦Œ&$ sh_plot_pos -f glred*.org -r -t NONE”j§]”j±Œ&$ sh_plot_pos -f glred*.org -r -t NONE”…””}”j¶jë‚sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÁ€jÆK j¶j€jÇj•€ubj`)”}”(j¦X!(Alternatively you can create/save residual :file:`.pos` files for inspection and repeated plotting by running :program:`tssum` first and then :program:`sh_plot_pos` with :option:`*.pos` instead of :option:`*.org` for the input files.) The first check of the solution for each epoch is the quality of the stabilization. You can get a summary of the statistics by :command:`grep`'ing on :content:`POS STAT` in the print file. The NRMS values for the stabilization should be near unity in all three components, and the WRMS 1–2 mm in horizontal and 3–10 mm in vertical (potentially higher if vertical was down-weighted more than the default factor of 10). Check to make sure that no epoch has too few sites in the stabilization. If you find any problems, look at the solution itself for that epoch, noting which sites were removed from the stabilization and/or have large adjustments in the position summary. Next look at the histograms of nrms and wrms generated by :program:`sh_plot_pos` to see if the distribution of scatters among your sites is approximately Gaussian with the median nrms ~ 1.0. Finally, unless you have a network of hundreds of sites (in which case you are probably too experienced to need this chapter), you should view the time series for every site to be included in your solution, whether or not it is of direct scientific interest. Look for outliers at individual epochs and sites with unusually high nrms (> 1.5–2.0, depending on how you have weighted the data). If a large number of sites have outliers at a single epoch, review the GAMIT processing and the stabilization. Once you have identified any problematic position estimates and created rename or :content:`sig_neu` commands to remove them, you should repeat the time series to verify that your entries accomplished what you intended.”j§]”(j±Œ,(Alternatively you can create/save residual ”…””}”(j¶jû‚jÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.pos`”j§]”j±Œ.pos”…””}”(j¶jƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jû‚ubj±Œ7 files for inspection and repeated plotting by running ”…””}”(j¶jû‚jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`tssum`”j§]”j±Œtssum”…””}”(j¶jƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jû‚ubj±Œ first and then ”…””}”(j¶jû‚jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶j*ƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jû‚ubj±Œ with ”…””}”(j¶jû‚jÇj•€•hNjÆNubj’)”}”(j¦Œ:option:`*.pos`”j§]”j˜)”}”(j¦j>ƒj§]”j±Œ*.pos”…””}”(j¶j@ƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j<ƒubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”jJƒŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ*.pos”ujÄj‘hjÁ€jÆK$j¶jû‚ubj±Œ instead of ”…””}”(j¶jû‚jÇj•€hNjÆNubj’)”}”(j¦Œ:option:`*.org`”j§]”j˜)”}”(j¦jbƒj§]”j±Œ*.org”…””}”(j¶jdƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j`ƒubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”jnƒŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ*.org”ujÄj‘hjÁ€jÆK$j¶jû‚ubj±Œ– for the input files.) The first check of the solution for each epoch is the quality of the stabilization. You can get a summary of the statistics by ”…””}”(j¶jû‚jÇj•€hNjÆNubjj)”}”(j¦Œ:command:`grep`”j§]”j±Œgrep”…””}”(j¶j„ƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jû‚ubj±Œ ’ing on ”…””}”(j¶jû‚jÇj•€hNjÆNubj˜)”}”(j¦Œ:content:`POS STAT`”j§]”j±ŒPOS STAT”…””}”(j¶j–ƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jû‚ubj±X4 in the print file. The NRMS values for the stabilization should be near unity in all three components, and the WRMS 1–2 mm in horizontal and 3–10 mm in vertical (potentially higher if vertical was down-weighted more than the default factor of 10). Check to make sure that no epoch has too few sites in the stabilization. If you find any problems, look at the solution itself for that epoch, noting which sites were removed from the stabilization and/or have large adjustments in the position summary. Next look at the histograms of nrms and wrms generated by ”…””}”(j¶jû‚jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶j©ƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jû‚ubj±X¹ to see if the distribution of scatters among your sites is approximately Gaussian with the median nrms ~ 1.0. Finally, unless you have a network of hundreds of sites (in which case you are probably too experienced to need this chapter), you should view the time series for every site to be included in your solution, whether or not it is of direct scientific interest. Look for outliers at individual epochs and sites with unusually high nrms (> 1.5–2.0, depending on how you have weighted the data). If a large number of sites have outliers at a single epoch, review the GAMIT processing and the stabilization. Once you have identified any problematic position estimates and created rename or ”…””}”(j¶jû‚jÇj•€hNjÆNubj˜)”}”(j¦Œ:content:`sig_neu`”j§]”j±Œsig_neu”…””}”(j¶j»ƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jû‚ubj±Œw commands to remove them, you should repeat the time series to verify that your entries accomplished what you intended.”…””}”(j¶jû‚jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆK$j¶j€jÇj•€ubj`)”}”(j¦Œ‰Once you are satisfied with your time series, you can run :program:`globk` with the same :file:`.gdl` file to obtain a velocity estimate:”j§]”(j±Œ:Once you are satisfied with your time series, you can run ”…””}”(j¶jÔƒjÇj•€hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j܃jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÔƒubj±Œ with the same ”…””}”(j¶jÔƒjÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶jîƒjÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÔƒubj±Œ$ file to obtain a velocity estimate:”…””}”(j¶jÔƒjÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆK0j¶j€jÇj•€ubj)”}”(j¦ŒK$ globk 6 globk.prt globk.log. pnw_all.gdl globk..cmd VEL >&! glred_vel.out”j§]”j±ŒK$ globk 6 globk.prt globk.log. pnw_all.gdl globk..cmd VEL >&! glred_vel.out”…””}”j¶j „sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÁ€jÆK2j¶j€jÇj•€ubj`)”}”(j¦Œ}where the :option:`VEL` option invoked with the template :file:`globk.cmd` file will turn on velocity estimates and printout:”j§]”(j±Œ where the ”…””}”(j¶j„jÇj•€hNjÆNubj’)”}”(j¦Œ :option:`VEL`”j§]”j˜)”}”(j¦j#„j§]”j±ŒVEL”…””}”(j¶j%„jÇj•€hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j!„ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”j/„Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒVEL”ujÄj‘hjÁ€jÆK6j¶j„ubj±Œ" option invoked with the template ”…””}”(j¶j„jÇj•€hNjÆNubj˜)”}”(j¦Œ:file:`globk.cmd`”j§]”j±Œ globk.cmd”…””}”(j¶jE„jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j„ubj±Œ3 file will turn on velocity estimates and printout:”…””}”(j¶j„jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆK6j¶j€jÇj•€ubj)”}”(j¦Œ8apr_neu all 10 10 10 1 1 1 org_opt PSUM VSUM GDLF CMDS”j§]”j±Œ8apr_neu all 10 10 10 1 1 1 org_opt PSUM VSUM GDLF CMDS”…””}”j¶j`„sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjÁ€jÆK8j¶j€jÇj•€ubj`)”}”(j¦Œuand :file:`glorg.cmd`, invoked from within :file:`globk.cmd` includes stabilization for velocity as well as position:”j§]”(j±Œand ”…””}”(j¶jp„jÇj•€hNjÆNubj˜)”}”(j¦Œ:file:`glorg.cmd`”j§]”j±Œ glorg.cmd”…””}”(j¶jx„jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jp„ubj±Œ, invoked from within ”…””}”(j¶jp„jÇj•€hNjÆNubj˜)”}”(j¦Œ:file:`globk.cmd`”j§]”j±Œ globk.cmd”…””}”(j¶j„jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jp„ubj±Œ9 includes stabilization for velocity as well as position:”…””}”(j¶jp„jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆK=j¶j€jÇj•€ubj)”}”(j¦ŒŠ* Set parameters to estimate in stabilization pos_org xtran ytran ztran xrot yrot zrot rate_org xtran ytran ztran xrot yrot zrot”j§]”j±ŒŠ* Set parameters to estimate in stabilization pos_org xtran ytran ztran xrot yrot zrot rate_org xtran ytran ztran xrot yrot zrot”…””}”j¶j¨„sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjÁ€jÆK?j¶j€jÇj•€ubj`)”}”(j¦XThe :file:`.org` file output will contain stabilization information and a summary table for velocities as well as positions. Also, the experiment list will now contain all of the files used and the computed chi-square increments as each successive h-file is added to the solution:”j§]”(j±ŒThe ”…””}”(j¶j¸„jÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶jÀ„jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¸„ubj±X file output will contain stabilization information and a summary table for velocities as well as positions. Also, the experiment list will now contain all of the files used and the computed chi-square increments as each successive h-file is added to the solution:”…””}”(j¶j¸„jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆKEj¶j€jÇj•€ubj)”}”(j¦X¶EXPERIMENT LIST from vel.srt # Name SCALE Diag PPM Forw Chi2 Back Chi2 Status 1 H950820_PNW.GLX 1.000 0.000 0.115 -1.000 USED 2 H970607_PNW.GLX 1.000 0.000 0.220 -1.000 USED 3 H980813_PNW.GLX 1.000 0.000 0.234 -1.000 USED 5 H990516_PNW.GLX 1.000 0.000 0.184 -1.000 USED 6 H010719_PNW.GLX 1.000 0.000 0.295 -1.000 USED”j§]”j±X¶EXPERIMENT LIST from vel.srt # Name SCALE Diag PPM Forw Chi2 Back Chi2 Status 1 H950820_PNW.GLX 1.000 0.000 0.115 -1.000 USED 2 H970607_PNW.GLX 1.000 0.000 0.220 -1.000 USED 3 H980813_PNW.GLX 1.000 0.000 0.234 -1.000 USED 5 H990516_PNW.GLX 1.000 0.000 0.184 -1.000 USED 6 H010719_PNW.GLX 1.000 0.000 0.295 -1.000 USED”…””}”j¶jÛ„sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjÁ€jÆKHj¶j€jÇj•€ubj`)”}”(j¦XVWith a weighting of the coordinates estimates such that the uncertainties from each (combined) h-file are ~ 1 mm horizontal and ~ 5 mm vertical, the chi-square increments are typically less than 0.5 for regional data alone and 0.4 to 1.0 for global data. If an h-file is based on a poor GAMIT solution or there is a model incompatibility with previous h-files, the chi-square increment will be anomalous. When this occurs, you will need to return to the time series to see which sites show outliers that would create an incompatibility. A common example is a wrong antenna height for a station, which will show up as a height anomaly in the time series. How much chi-square is increased by a problem at one site will depend both on the size of the error and how many sites are in the solution. Very high chi-square values can result if you have two sites in the solution with the same name but at different locations. To guard against this problem, you should run :program:`glist` before you start the processing (see Section 5.1 of the `GLOBK Reference Manual `_).”j§]”(j±XÄWith a weighting of the coordinates estimates such that the uncertainties from each (combined) h-file are ~ 1 mm horizontal and ~ 5 mm vertical, the chi-square increments are typically less than 0.5 for regional data alone and 0.4 to 1.0 for global data. If an h-file is based on a poor GAMIT solution or there is a model incompatibility with previous h-files, the chi-square increment will be anomalous. When this occurs, you will need to return to the time series to see which sites show outliers that would create an incompatibility. A common example is a wrong antenna height for a station, which will show up as a height anomaly in the time series. How much chi-square is increased by a problem at one site will depend both on the size of the error and how many sites are in the solution. Very high chi-square values can result if you have two sites in the solution with the same name but at different locations. To guard against this problem, you should run ”…””}”(j¶jë„jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`glist`”j§]”j±Œglist”…””}”(j¶jó„jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jë„ubj±Œ9 before you start the processing (see Section 5.1 of the ”…””}”(j¶jë„jÇj•€hNjÆNubj÷ )”}”(j¦ŒG`GLOBK Reference Manual `_”j§]”j±ŒGLOBK Reference Manual”…””}”(j¶j…jÇj•€hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGLOBK Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GLOBK_Ref.pdf”ujÄjö j¶jë„ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œglobk-reference-manual”aj»]”j½]”Œglobk reference manual”ajÀ]”jÂ]”Œrefuri”j…ujÄjdj Kj¶jë„ubj±Œ).”…””}”(j¶jë„jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆKRj¶j€jÇj•€ubj`)”}”(j¦ŒTo plot the velocities, use”j§]”j±ŒTo plot the velocities, use”…””}”(j¶j-…jÇj•€hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆKZj¶j€jÇj•€ubj)”}”(j¦Œ3$ sh_plotvel -f globk_vel.org -R244.5/251/40.5/46.5”j§]”j±Œ3$ sh_plotvel -f globk_vel.org -R244.5/251/40.5/46.5”…””}”j¶j;…sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÁ€jÆK\j¶j€jÇj•€ubj`)”}”(j¦X«where the :option:`-f` argument is the :file:`.prt`, :file:`.org`, or :file:`.vel` file from which the :content:`SUMMARY VELOCITY` is to be plotted, and the second command-line entry gives the longitude and latitude range for the plot using standard GMT commands. See the documentation at the top of the script (or type :console:`sh_plotvel -help`) for additional options for displaying site names, scaling the uncertainties, setting the confidence level for error ellipses, and adding topography, fault maps, and other geographic features. The scripts :program:`sh_map_calif`, :program:`sh_map_china`, and :program:`sh_map_elements` in :file:`~/gg/com/` may be helpful as templates.”j§]”(j±Œ where the ”…””}”(j¶jK…jÇj•€hNjÆNubj’)”}”(j¦Œ :option:`-f`”j§]”j˜)”}”(j¦jU…j§]”j±Œ-f”…””}”(j¶jW…jÇj•€hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jS…ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”j Œ refdomain”ja…Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-f”ujÄj‘hjÁ€jÆK`j¶jK…ubj±Œ argument is the ”…””}”(j¶jK…jÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.prt`”j§]”j±Œ.prt”…””}”(j¶jw…jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jK…ubj±Œ, ”…””}”(j¶jK…jÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶jŒ…jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jK…ubj±Œ, or ”…””}”(j¶jK…jÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.vel`”j§]”j±Œ.vel”…””}”(j¶j¡…jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jK…ubj±Œ file from which the ”…””}”(j¶jK…jÇj•€hNjÆNubj˜)”}”(j¦Œ:content:`SUMMARY VELOCITY`”j§]”j±ŒSUMMARY VELOCITY”…””}”(j¶j¶…jÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jK…ubj±Œ¾ is to be plotted, and the second command-line entry gives the longitude and latitude range for the plot using standard GMT commands. See the documentation at the top of the script (or type ”…””}”(j¶jK…jÇj•€hNjÆNubj˜)”}”(j¦Œ:console:`sh_plotvel -help`”j§]”j±Œsh_plotvel -help”…””}”(j¶jÉ…jÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶jK…ubj±ŒÎ) for additional options for displaying site names, scaling the uncertainties, setting the confidence level for error ellipses, and adding topography, fault maps, and other geographic features. The scripts ”…””}”(j¶jK…jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`sh_map_calif`”j§]”j±Œ sh_map_calif”…””}”(j¶jÜ…jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jK…ubj±Œ, ”…””}”j¶jK…sbjj)”}”(j¦Œ:program:`sh_map_china`”j§]”j±Œ sh_map_china”…””}”(j¶jî…jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jK…ubj±Œ, and ”…””}”(j¶jK…jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`sh_map_elements`”j§]”j±Œsh_map_elements”…””}”(j¶j†jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jK…ubj±Œ in ”…””}”(j¶jK…jÇj•€hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/com/`”j§]”j±Œ ~/gg/com/”…””}”(j¶j†jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jK…ubj±Œ may be helpful as templates.”…””}”(j¶jK…jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆK`j¶j€jÇj•€ubj`)”}”(j¦XºFor large networks, particularly those including continuous stations with discontinuities and non-linear motion due to earthquakes, the interactive Matlab-based programs :program:`tsview` and :program:`velview` can be powerful tools. Their use and installation ar documented on the GAMIT/GLOBK webpage (http://geoweb.mit.edu/~tah/GGMatlab/). As a further aid to handling large data sets, we have recently developed programs (:program:`tssum`, :program:`tsfit`) that allow "prototyping" of GLOBK solutions by manipulating time series to identify discontinuities and non-linear effects quickly (see Chapter 4 of the `GLOBK Reference Manual `_). It will often be the case that the set of stations you use for stabilization of the time series for editing purposes define a reference frame that is inherently weaker in your region of interest than the final velocity solution—either because the editing frame encompasses a larger region and hence is more affected by spatially correlated errors, or because the number of well-known stations available for stabilization of individual h-files is much less than the total number of stations in the solution. The time series that best represents your final velocity solution is one that is stabilized with all of the stations in the solution. Thus, after you obtain this solution, you should rerun :program:`glred` with an enlarged :content:`stab_site` list and an :file:`.apr` file generated from the velocity solution. To get the :file:`.apr` file, use :program:`sh_exglk`, and to generate a :content:`stab_site` list to include all sites with position and velocity uncertainties below a specified level program :program:`org2stab`.”j§]”(j±ŒªFor large networks, particularly those including continuous stations with discontinuities and non-linear motion due to earthquakes, the interactive Matlab-based programs ”…””}”(j¶j-†jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`tsview`”j§]”j±Œtsview”…””}”(j¶j5†jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j-†ubj±Œ and ”…””}”(j¶j-†jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`velview`”j§]”j±Œvelview”…””}”(j¶jG†jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j-†ubj±Œ] can be powerful tools. Their use and installation ar documented on the GAMIT/GLOBK webpage (”…””}”(j¶j-†jÇj•€hNjÆNubj÷ )”}”(j¦Œ$http://geoweb.mit.edu/~tah/GGMatlab/”j§]”j±Œ$http://geoweb.mit.edu/~tah/GGMatlab/”…””}”(j¶jY†jÇj•€hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j[†ujÄjö j¶j-†ubj±ŒV). As a further aid to handling large data sets, we have recently developed programs (”…””}”(j¶j-†jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`tssum`”j§]”j±Œtssum”…””}”(j¶jl†jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j-†ubj±Œ, ”…””}”(j¶j-†jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`tsfit`”j§]”j±Œtsfit”…””}”(j¶j~†jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j-†ubj±ŒŸ) that allow “prototyping†of GLOBK solutions by manipulating time series to identify discontinuities and non-linear effects quickly (see Chapter 4 of the ”…””}”(j¶j-†jÇj•€hNjÆNubj÷ )”}”(j¦ŒG`GLOBK Reference Manual `_”j§]”j±ŒGLOBK Reference Manual”…””}”(j¶j†jÇj•€hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGLOBK Reference Manual”j Œ+http://geoweb.mit.edu/gg/docs/GLOBK_Ref.pdf”ujÄjö j¶j-†ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œid1”aj»]”j½]”jÀ]”Œglobk reference manual”ajÂ]”Œrefuri”j †ujÄjdj Kj¶j-†ubj±X½). It will often be the case that the set of stations you use for stabilization of the time series for editing purposes define a reference frame that is inherently weaker in your region of interest than the final velocity solution—either because the editing frame encompasses a larger region and hence is more affected by spatially correlated errors, or because the number of well-known stations available for stabilization of individual h-files is much less than the total number of stations in the solution. The time series that best represents your final velocity solution is one that is stabilized with all of the stations in the solution. Thus, after you obtain this solution, you should rerun ”…””}”(j¶j-†jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶j²†jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j-†ubj±Œ with an enlarged ”…””}”(j¶j-†jÇj•€hNjÆNubj˜)”}”(j¦Œ:content:`stab_site`”j§]”j±Œ stab_site”…””}”(j¶jĆjÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j-†ubj±Œ list and an ”…””}”(j¶j-†jÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶j׆jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j-†ubj±Œ7 file generated from the velocity solution. To get the ”…””}”(j¶j-†jÇj•€hNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jì†jÇj•€hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j-†ubj±Œ file, use ”…””}”(j¶j-†jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`sh_exglk`”j§]”j±Œsh_exglk”…””}”(j¶j‡jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j-†ubj±Œ, and to generate a ”…””}”(j¶j-†jÇj•€hNjÆNubj˜)”}”(j¦Œ:content:`stab_site`”j§]”j±Œ stab_site”…””}”(j¶j‡jÇj•€hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j-†ubj±Œd list to include all sites with position and velocity uncertainties below a specified level program ”…””}”(j¶j-†jÇj•€hNjÆNubjj)”}”(j¦Œ:program:`org2stab`”j§]”j±Œorg2stab”…””}”(j¶j&‡jÇj•€hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j-†ubj±Œ.”…””}”(j¶j-†jÇj•€hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÁ€jÆKdj¶j€jÇj•€ubej·}”(j¹]”(Œ-generating-time-series-and-velocity-solutions”jÀ€ej»]”j½]”(Œ-generating time series and velocity solutions”Œintro_prod_ts_vels”ejÀ]”jÂ]”ujÄh_j¶j•€jÇj•€hjÁ€jÆKjÒ }”jD‡j¶€sjÔ }”jÀ€j¶€subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jÁ€j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjÁ€jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j¤€j˜€j³€j§€uj_}”(Œrel”j¤€Œdate”j³€ujc}”je}”jÀ€]”j¶€asjg}”(jD‡jÀ€jC‡j@‡j…j…uji}”(jD‡ˆjC‡‰j…ˆuj¹}”(jÀ€j€j@‡j€j…j…j§†j¡†ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”jù )”}”(j¦hoj§]”j`)”}”(j¦Œ9Duplicate explicit target name: "globk reference manual".”j§]”j±Œ=Duplicate explicit target name: “globk reference manualâ€.”…””}”(j¶jm‡jÇj•€hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jj‡ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j§†aŒlevel”KŒtype”jŒsource”jÁ€Œline”KujÄjø j¶j€jÇj•€hjÁ€jÆKjubaj†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ8Hyperlink target "intro-prod-ts-vels" is not referenced.”…””}”j¶j‰‡sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j†‡ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jÁ€Œline”KujÄjø ubajˆNj‰]”j‹NjÇj•€ubjïj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j¤‡sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¡‡jÇj¡‡ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j³‡jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¡‡jÇj¡‡ubje)”}”(j¦Œ.. _intro_prod_weighting:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒintro-prod-weighting”ujÄjdjÆKj¶j¡‡jÇj¡‡hŒH/chandler/home/floyd/public_html/gg/docs/source/intro/prod/weighting.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ.Weighting the Data for Realistic Uncertainties”j§]”j±Œ.Weighting the Data for Realistic Uncertainties”…””}”(j¶jчjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j·jÇj¡‡hj͇jÆKubj`)”}”(j¦XJAs noted in :numref:`intro_gnss_model`, the dominant errors in GPS observations are not random, but rather have correlation times ranging from a few minutes (multipath, water vapor) to days or months (station motions due to monument instability and atmospheric, hydrological, and ocean loading; non-gravitational forces on the satellites). Ignoring these correlations will result in uncertainties that are too optimistic, mildly so for observations of a few days, more strongly so for continuous data. In this section we assume that you understand the theoretical and empirical basis for various approaches, and we describe how to implement them in GLOBK. (For some theoretical background see the "Error Analysis" presentation from a recent workshop under the "Workshops" menu item on the `GAMIT/GLOBK web site `_.)”j§]”(j±Œ As noted in ”…””}”(j¶j߇jÇj¡‡hNjÆNubj’)”}”(j¦Œ:numref:`intro_gnss_model`”j§]”j˜)”}”(j¦jé‡j§]”j±Œintro_gnss_model”…””}”(j¶jë‡jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jç‡ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jïŒ refdomain”jõ‡Œreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_gnss_model”ujÄj‘hj͇jÆKj¶j߇ubj±X÷, the dominant errors in GPS observations are not random, but rather have correlation times ranging from a few minutes (multipath, water vapor) to days or months (station motions due to monument instability and atmospheric, hydrological, and ocean loading; non-gravitational forces on the satellites). Ignoring these correlations will result in uncertainties that are too optimistic, mildly so for observations of a few days, more strongly so for continuous data. In this section we assume that you understand the theoretical and empirical basis for various approaches, and we describe how to implement them in GLOBK. (For some theoretical background see the “Error Analysis†presentation from a recent workshop under the “Workshops†menu item on the ”…””}”(j¶j߇jÇj¡‡hNjÆNubj÷ )”}”(j¦Œ3`GAMIT/GLOBK web site `_”j§]”j±ŒGAMIT/GLOBK web site”…””}”(j¶j ˆjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT/GLOBK web site”j Œhttp://geoweb.mit.edu/gg/”ujÄjö j¶j߇ubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œgamit-globk-web-site”aj»]”j½]”Œgamit/globk web site”ajÀ]”jÂ]”Œrefuri”jˆujÄjdj Kj¶j߇ubj±Œ.)”…””}”(j¶j߇jÇj¡‡hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj͇jÆKj¶j·jÇj¡‡ubj`)”}”(j¦XBStudies of long-term GPS coordinate time series have shown that the noise over periods of a few days is nearly white but increases steadily for longer periods. With continuous data we can analyze the time series and, based on the character of the noise over periods of weeks to years, infer the noise at the long periods relevant to estimating the error in site velocities or long-term decay following an earthquake. A Kalman filter such as :program:`globk` cannot without significant complication realize all possible error models (in particular a "flicker noise" model that best fits most GPS time series), but it can easily realize the two "end-member" models—white noise and a random walk—that together allow us to achieve meaningful short-term statistics for data editing and realistic uncertainties for estimated velocities.”j§]”(j±X¹Studies of long-term GPS coordinate time series have shown that the noise over periods of a few days is nearly white but increases steadily for longer periods. With continuous data we can analyze the time series and, based on the character of the noise over periods of weeks to years, infer the noise at the long periods relevant to estimating the error in site velocities or long-term decay following an earthquake. A Kalman filter such as ”…””}”(j¶j3ˆjÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j;ˆjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j3ˆubj±X cannot without significant complication realize all possible error models (in particular a “flicker noise†model that best fits most GPS time series), but it can easily realize the two “end-member†models—white noise and a random walk—that together allow us to achieve meaningful short-term statistics for data editing and realistic uncertainties for estimated velocities.”…””}”(j¶j3ˆjÇj¡‡hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj͇jÆK j¶j·jÇj¡‡ubj`)”}”(j¦XTThe :math:`\chi^2` (chi-square) increments (:content:`chii`) computed by :program:`globk` when h-files are combined reflect the inconsistency in the coordinate estimates from the current solution and the estimates from the new h-file and can usually be seen in the time series. If the data from all sites are properly weighted for their short-term scatter, the nrms of the time series and the chi-square increments should be ~ 1.0. Chi-square increments less than 1 will occur when there is little redundancy or if you have down-weighted the data to allow for more realistic velocity estimates. Values greater than one will occur if the sigmas on the h-files are too small or there are uncompensated outliers among the coordinate estimates. **These must be found using the time series and corrected as described in** :numref:`intro_prod_editing`\ **.**”j§]”(j±ŒThe ”…””}”(j¶jSˆjÇj¡‡hNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶j[ˆjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jSˆubj±Œ (chi-square) increments (”…””}”(j¶jSˆjÇj¡‡hNjÆNubj˜)”}”(j¦Œ:content:`chii`”j§]”j±Œchii”…””}”(j¶jmˆjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jSˆubj±Œ) computed by ”…””}”(j¶jSˆjÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j€ˆjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jSˆubj±XŒ when h-files are combined reflect the inconsistency in the coordinate estimates from the current solution and the estimates from the new h-file and can usually be seen in the time series. If the data from all sites are properly weighted for their short-term scatter, the nrms of the time series and the chi-square increments should be ~ 1.0. Chi-square increments less than 1 will occur when there is little redundancy or if you have down-weighted the data to allow for more realistic velocity estimates. Values greater than one will occur if the sigmas on the h-files are too small or there are uncompensated outliers among the coordinate estimates. ”…””}”(j¶jSˆjÇj¡‡hNjÆNubj>)”}”(j¦ŒK**These must be found using the time series and corrected as described in**”j§]”j±ŒGThese must be found using the time series and corrected as described in”…””}”(j¶j’ˆjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjœ>j¶jSˆubj±Œ ”…””}”(j¶jSˆjÇj¡‡hNjÆNubj’)”}”(j¦Œ:numref:`intro_prod_editing`”j§]”j˜)”}”(j¦j¦ˆj§]”j±Œintro_prod_editing”…””}”(j¶j¨ˆjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶j¤ˆubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jïŒ refdomain”j²ˆŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_prod_editing”ujÄj‘hj͇jÆKj¶jSˆubj±Œ ”…””}”(j¶jSˆjÇj¡‡hNjÆNubj>)”}”(j¦Œ**.**”j§]”j±Œ.”…””}”(j¶jȈjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjœ>j¶jSˆubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj͇jÆKj¶j·jÇj¡‡ubj`)”}”(j¦Xw We have noted earlier that the weighting of the phase data in GAMIT is such that the coordinate uncertainties in daily h-files are mildly pessimistic compared to the daily scatter, so you should expect chi-square values of 0.3 to 1.0 when you stack these files in :program:`globk`. If you combine many days together, however, the h-file uncertainties will get smaller, by the square root of the number of days combined, and the chi-square values increase linearly with the number of days. You can compensate for this by adding white noise to the coordinate estimates using the :content:`sig_neu` command. The values to be added can be determined from the short-term scatter in the time series. Adding white noise for a uniform network of continuous stations is, strictly speaking, not necessary since the true uncertainty in velocity estimates will be dominated by the long-period noise added using :content:`mar_neu` (random-walk) command, but it can be useful in editing by establishing a more realistic ratio between the uncertainties within an h-file that has a combination of continuous and survey-mode data. For example, if some position estimates in the h-file are based on thirty 24-hr sessions and others on two 24-hr sessions, the position uncertainties on the h-file for the 30-day sites will be a factor of four smaller than the 2-day sites even though their true uncertainties are nearly the same because of the dominance of correlated noise. To take an example, suppose the formal uncertainty and scatter in horizontal coordinates for all sites from a 24-hr session is 1.0 mm. In the combined h-file, the uncertainty for the 30-day site will be 0.2 mm and for the 2-day site 0.7 mm. If we add quadratically 0.75 mm of white noise to the horizontal coordinates of all sites on the h-files (:content:`sig_neu all .00075 .00075 0`), then the uncertainties used in the solution will become 0.8 mm for the 30-day sites and 1.0 mm for the 2-day site, more closely reflecting their scatter (and hence contribution to :math:`\chi^2`). You may also want to add white noise for individual stations that show a higher level of short-term scatter than is reflected in their uncertainties—that is a higher nrms in the daily time series. Use of the :content:`sig_neu` command for reweighting is preferred over the variance factor used with h-files in the :file:`.gdl` list since an elevated noise level is usually associated with only a subset of sites in the h-file. An exception would be when you have h-files generated from GAMIT solutions using different sampling times, in which case the variance factor is useful to balance the weight with other h-files in your solution.”j§]”(j±XWe have noted earlier that the weighting of the phase data in GAMIT is such that the coordinate uncertainties in daily h-files are mildly pessimistic compared to the daily scatter, so you should expect chi-square values of 0.3 to 1.0 when you stack these files in ”…””}”(j¶j܈jÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jäˆjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j܈ubj±X). If you combine many days together, however, the h-file uncertainties will get smaller, by the square root of the number of days combined, and the chi-square values increase linearly with the number of days. You can compensate for this by adding white noise to the coordinate estimates using the ”…””}”(j¶j܈jÇj¡‡hNjÆNubj˜)”}”(j¦Œ:content:`sig_neu`”j§]”j±Œsig_neu”…””}”(j¶jöˆjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j܈ubj±X0 command. The values to be added can be determined from the short-term scatter in the time series. Adding white noise for a uniform network of continuous stations is, strictly speaking, not necessary since the true uncertainty in velocity estimates will be dominated by the long-period noise added using ”…””}”(j¶j܈jÇj¡‡hNjÆNubj˜)”}”(j¦Œ:content:`mar_neu`”j§]”j±Œmar_neu”…””}”(j¶j ‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j܈ubj±Xv (random-walk) command, but it can be useful in editing by establishing a more realistic ratio between the uncertainties within an h-file that has a combination of continuous and survey-mode data. For example, if some position estimates in the h-file are based on thirty 24-hr sessions and others on two 24-hr sessions, the position uncertainties on the h-file for the 30-day sites will be a factor of four smaller than the 2-day sites even though their true uncertainties are nearly the same because of the dominance of correlated noise. To take an example, suppose the formal uncertainty and scatter in horizontal coordinates for all sites from a 24-hr session is 1.0 mm. In the combined h-file, the uncertainty for the 30-day site will be 0.2 mm and for the 2-day site 0.7 mm. If we add quadratically 0.75 mm of white noise to the horizontal coordinates of all sites on the h-files (”…””}”(j¶j܈jÇj¡‡hNjÆNubj˜)”}”(j¦Œ&:content:`sig_neu all .00075 .00075 0`”j§]”j±Œsig_neu all .00075 .00075 0”…””}”(j¶j‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j܈ubj±Œ·), then the uncertainties used in the solution will become 0.8 mm for the 30-day sites and 1.0 mm for the 2-day site, more closely reflecting their scatter (and hence contribution to ”…””}”(j¶j܈jÇj¡‡hNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶j/‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶j܈ubj±ŒÕ). You may also want to add white noise for individual stations that show a higher level of short-term scatter than is reflected in their uncertainties—that is a higher nrms in the daily time series. Use of the ”…””}”(j¶j܈jÇj¡‡hNjÆNubj˜)”}”(j¦Œ:content:`sig_neu`”j§]”j±Œsig_neu”…””}”(j¶jA‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j܈ubj±ŒX command for reweighting is preferred over the variance factor used with h-files in the ”…””}”(j¶j܈jÇj¡‡hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶jT‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j܈ubj±X6 list since an elevated noise level is usually associated with only a subset of sites in the h-file. An exception would be when you have h-files generated from GAMIT solutions using different sampling times, in which case the variance factor is useful to balance the weight with other h-files in your solution.”…””}”(j¶j܈jÇj¡‡hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj͇jÆKj¶j·jÇj¡‡ubj`)”}”(j¦X¦The primary way we account for the long-period noise that most influences velocity estimates is by adding a random walk to the error model used by :program:`globk`. For sites with ~ 100 or more position estimates, the appropriate value of the random walk for each component can be determined using the First-Order Gauss-Markov Extrapolation ("FOGMEx") or "realistic sigma" algorithm described by Herring [2003] and Floyd and Herring [2020], and in the "Error Analysis" presentations from the workshops. The algorithm uses the scatter in the time series for all possible averaging times (e.g. 1 day to 600 days for a 1200-day time series) to determine how the time series statistics depart from white noise. If the noise is white, the rms should decrease as the square root of the averaging time, and the nrms stay the same. In practice, however for GPS time series, the rms decreases much more slowly with averaging time, and nrms increases (since the formal uncertainty decreases). By fitting nrms (actually :math:`\chi^2`) versus averaging time to an exponential function (expected for a first-order Gauss-Markov process) and evaluating this function for infinite averaging time, the algorithm determines both the scale factor to be applied to the white-noise velocity sigma to get a more realistic sigma and the value of the random walk that will produce this sigma in the :program:`globk` solution. To get the :content:`mar_neu` commands, run”j§]”(j±Œ“The primary way we account for the long-period noise that most influences velocity estimates is by adding a random walk to the error model used by ”…””}”(j¶jo‰jÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jw‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jo‰ubj±XZ. For sites with ~ 100 or more position estimates, the appropriate value of the random walk for each component can be determined using the First-Order Gauss-Markov Extrapolation (“FOGMExâ€) or “realistic sigma†algorithm described by Herring [2003] and Floyd and Herring [2020], and in the “Error Analysis†presentations from the workshops. The algorithm uses the scatter in the time series for all possible averaging times (e.g. 1 day to 600 days for a 1200-day time series) to determine how the time series statistics depart from white noise. If the noise is white, the rms should decrease as the square root of the averaging time, and the nrms stay the same. In practice, however for GPS time series, the rms decreases much more slowly with averaging time, and nrms increases (since the formal uncertainty decreases). By fitting nrms (actually ”…””}”(j¶jo‰jÇj¡‡hNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶j‰‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶jo‰ubj±Xa) versus averaging time to an exponential function (expected for a first-order Gauss-Markov process) and evaluating this function for infinite averaging time, the algorithm determines both the scale factor to be applied to the white-noise velocity sigma to get a more realistic sigma and the value of the random walk that will produce this sigma in the ”…””}”(j¶jo‰jÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j›‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jo‰ubj±Œ solution. To get the ”…””}”(j¶jo‰jÇj¡‡hNjÆNubj˜)”}”(j¦Œ:content:`mar_neu`”j§]”j±Œmar_neu”…””}”(j¶j­‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jo‰ubj±Œ commands, run”…””}”(j¶jo‰jÇj¡‡hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj͇jÆK"j¶j·jÇj¡‡ubj)”}”(j¦Œ$ sh_gen_stats -ts SUM.tsfit”j§]”j±Œ$ sh_gen_stats -ts SUM.tsfit”…””}”j¶jƉsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj͇jÆK*j¶j·jÇj¡‡ubj`)”}”(j¦Œƒwhere :file:`SUM.tsfit` is the output of an :program:`sh_plot_pos` run invoking :program:`tsfit` (or :program:`tsfit` directly); or”j§]”(j±Œwhere ”…””}”(j¶jÖ‰jÇj¡‡hNjÆNubj˜)”}”(j¦Œ:file:`SUM.tsfit`”j§]”j±Œ SUM.tsfit”…””}”(j¶jÞ‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÖ‰ubj±Œ is the output of an ”…””}”(j¶jÖ‰jÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶jó‰jÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÖ‰ubj±Œ run invoking ”…””}”(j¶jÖ‰jÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`tsfit`”j§]”j±Œtsfit”…””}”(j¶jŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÖ‰ubj±Œ (or ”…””}”(j¶jÖ‰jÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`tsfit`”j§]”j±Œtsfit”…””}”(j¶jŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÖ‰ubj±Œ directly); or”…””}”(j¶jÖ‰jÇj¡‡hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj͇jÆK.j¶j·jÇj¡‡ubj)”}”(j¦Œ$ sh_gen_stats -ir va[root].ens”j§]”j±Œ$ sh_gen_stats -ir va[root].ens”…””}”j¶j/Šsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj͇jÆK1j¶j·jÇj¡‡ubj`)”}”(j¦Xqwhere :option:`{[root]}` is an identifier of your choosing and the input file has the name :file:`va[root].ens`, obtained by renaming the :file:`VAL` file from running :program:`sh_plotcrd` (or :program:`ensum` or :program:`enfit` directly). You can also invoke the FOGMEx algorithm from within :program:`tsview` by selecting "Realistic Sigma". For sites with fewer than ~ 100 estimates, the values you use for the random walk will necessarily be less precise, so you might use, for example, the median value from :program:`sh_gen_stats` for the network or an "eyeball" estimate of long-period systematics in the time series.”j§]”(j±Œwhere ”…””}”(j¶j?ŠjÇj¡‡hNjÆNubj’)”}”(j¦Œ:option:`{[root]}`”j§]”j˜)”}”(j¦jIŠj§]”j±Œ{[root]}”…””}”(j¶jKŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jGŠubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jïŒ refdomain”jUŠŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ{[root]}”ujÄj‘hj͇jÆK5j¶j?Šubj±ŒC is an identifier of your choosing and the input file has the name ”…””}”(j¶j?ŠjÇj¡‡hNjÆNubj˜)”}”(j¦Œ:file:`va[root].ens`”j§]”j±Œ va[root].ens”…””}”(j¶jkŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?Šubj±Œ, obtained by renaming the ”…””}”(j¶j?ŠjÇj¡‡hNjÆNubj˜)”}”(j¦Œ :file:`VAL`”j§]”j±ŒVAL”…””}”(j¶j€ŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?Šubj±Œ file from running ”…””}”(j¶j?ŠjÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`sh_plotcrd`”j§]”j±Œ sh_plotcrd”…””}”(j¶j•ŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j?Šubj±Œ (or ”…””}”(j¶j?ŠjÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`ensum`”j§]”j±Œensum”…””}”(j¶j§ŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j?Šubj±Œ or ”…””}”(j¶j?ŠjÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`enfit`”j§]”j±Œenfit”…””}”(j¶j¹ŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j?Šubj±ŒA directly). You can also invoke the FOGMEx algorithm from within ”…””}”(j¶j?ŠjÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`tsview`”j§]”j±Œtsview”…””}”(j¶jËŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j?Šubj±ŒÎ by selecting “Realistic Sigmaâ€. For sites with fewer than ~ 100 estimates, the values you use for the random walk will necessarily be less precise, so you might use, for example, the median value from ”…””}”(j¶j?ŠjÇj¡‡hNjÆNubjj)”}”(j¦Œ:program:`sh_gen_stats`”j§]”j±Œ sh_gen_stats”…””}”(j¶jÝŠjÇj¡‡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j?Šubj±Œ\ for the network or an “eyeball†estimate of long-period systematics in the time series.”…””}”(j¶j?ŠjÇj¡‡hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj͇jÆK5j¶j·jÇj¡‡ubej·}”(j¹]”(Œ.weighting-the-data-for-realistic-uncertainties”j̇ej»]”j½]”(Œ.weighting the data for realistic uncertainties”Œintro_prod_weighting”ejÀ]”jÂ]”ujÄh_j¶j¡‡jÇj¡‡hj͇jÆKjÒ }”jûŠj‡sjÔ 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This must be an absoute path. [Default pwd] ”j§]”(je)”}”(j¦Œ:option:`-dir`”j§]”j’)”}”(j¦j3j§]”j˜)”}”(j¦j3j§]”j±Œ-dir”…””}”(j¶j8jÇjshNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j5ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jüŒ refdomain”jBŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-dir”ujÄj‘hjŸjÆK4j¶j1ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK4j¶j-ubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒmExperiment directory or root directory for experiment processing. This must be an absoute path. [Default pwd]”j§]”j±ŒmExperiment directory or root directory for experiment processing. This must be an absoute path. [Default pwd]”…””}”(j¶j]jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK3j¶jZubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j-ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK4j¶j*ubaj·}”(j¹]”j)aj»]”j½]”Œman_sh_gamit_dir”ajÀ]”jÂ]”ujÄj ej¶jšjÇjshjŸjÆNjÒ }”j{jsjÔ }”j)jsubje)”}”(j¦Œ.. _man_sh_gamit_d:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-d”ujÄjdjÆK:j¶jšjÇjshjŸubj e)”}”(j¦hoj§]”je)”}”(j¦ŒZ:option:`-d` yr days where yr and days are the data to be processed e.g. 1997 153 156 178 ”j§]”(je)”}”(j¦Œ:option:`-d` yr days”j§]”(j’)”}”(j¦Œ :option:`-d`”j§]”j˜)”}”(j¦j˜j§]”j±Œ-d”…””}”(j¶jšjÇjshNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j–ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jüŒ refdomain”j¤Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-d”ujÄj‘hjŸjÆK9j¶j’ubj±Œ yr days”…””}”(j¶j’jÇjshNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK9j¶jŽubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒDwhere yr and days are the data to be processed e.g. 1997 153 156 178”j§]”j±ŒDwhere yr and days are the data to be processed e.g. 1997 153 156 178”…””}”(j¶jÃjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK9j¶jÀubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jŽubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK9j¶j‹ubaj·}”(j¹]”jŠaj»]”j½]”Œman_sh_gamit_d”ajÀ]”jÂ]”ujÄj ej¶jšjÇjshjŸjÆNjÒ }”jáj€sjÔ }”jŠj€subje)”}”(j¦Œ.. _man_sh_gamit_s:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-s”ujÄjdjÆK?j¶jšjÇjshjŸubj e)”}”(j¦hoj§]”je)”}”(j¦ŒW-s yr d1 d2 where d1 is start day and d2 is stop day to be processed e.g. 1997 153 178 ”j§]”(je)”}”(j¦Œ -s yr d1 d2”j§]”j±Œ -s yr d1 d2”…””}”(j¶jøjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK>j¶jôubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒJwhere d1 is start day and d2 is stop day to be processed e.g. 1997 153 178”j§]”j±ŒJwhere d1 is start day and d2 is stop day to be processed e.g. 1997 153 178”…””}”(j¶j ‘jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK>j¶j‘ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jôubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK>j¶jñubaj·}”(j¹]”jðaj»]”j½]”Œman_sh_gamit_s”ajÀ]”jÂ]”ujÄj ej¶jšjÇjshjŸjÆNjÒ }”j'‘jæsjÔ }”jðjæsubje)”}”(j¦Œ.. _man_sh_gamit_r:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-r”ujÄjdjÆKDj¶jšjÇjshjŸubj©Œ option_list”“”)”}”(j¦hoj§]”j©Œoption_list_item”“”)”}”(j¦hoj§]”(j©Œ option_group”“”)”}”(j¦hoj§]”j©Œoption”“”)”}”(j¦Œ-r day”j§]”(j©Œ option_string”“”)”}”(j¦Œ-r”j§]”j±Œ-r”…””}”j¶jN‘sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶jH‘ubj©Œoption_argument”“”)”}”(j¦Œday”j§]”j±Œday”…””}”(j¶j^‘jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”Œ ”ujÄj\‘j¶jH‘ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jC‘ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶j>‘ubj©Œ description”“”)”}”(j¦Œ1where day is number of days before current date. ”j§]”j`)”}”(j¦Œ0where day is number of days before current date.”j§]”j±Œ0where day is number of days before current date.”…””}”(j¶j€‘jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKCj¶j|‘ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶j>‘ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j9‘jÇjshjŸjÆNubaj·}”(j¹]”j6‘aj»]”j½]”Œman_sh_gamit_r”ajÀ]”jÂ]”ujÄj7‘hjŸjÆKBj¶jšjÇjsjÒ }”jž‘j,‘sjÔ }”j6‘j,‘subje)”}”(j¦Œ.. _man_sh_gamit_gnss:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-gnss”ujÄjdjÆKIj¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-gnss”j§]”(jM‘)”}”(j¦Œ-g”j§]”j±Œ-g”…””}”j¶j»‘sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j·‘ubj]‘)”}”(j¦Œnss”j§]”j±Œnss”…””}”(j¶jÉ‘jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶j·‘ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶j´‘ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶j±‘ubj{‘)”}”(j¦ŒGNSS ( G R C E J I) default G ”j§]”j`)”}”(j¦ŒGNSS ( G R C E J I) default G”j§]”j±ŒGNSS ( G R C E J I) default G”…””}”(j¶jè‘jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKHj¶jä‘ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶j±‘ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j®‘jÇjshjŸjÆNubaj·}”(j¹]”j­‘aj»]”j½]”Œman_sh_gamit_gnss”ajÀ]”jÂ]”ujÄj7‘hjŸjÆKGj¶jšjÇjsjÒ }”j’j£‘sjÔ }”j­‘j£‘subje)”}”(j¦Œ.. _man_sh_gamit_lfreq:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-lfreq”ujÄjdjÆKNj¶jšjÇjshjŸubj e)”}”(j¦hoj§]”je)”}”(j¦ŒÔ-lfreq # Lower frequency selection depending on GNSS e.g., # = 5 for G L5; 6, 7 or 8 for E L6, L7 or L8; 5 or 7 for C L5 or L7 Options couples to GNSS selection. (Default, not specified and GAMIT selection used ”j§]”(je)”}”(j¦Œ-lfreq #”j§]”j±Œ-lfreq #”…””}”(j¶j’jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆKNj¶j’ubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒÊLower frequency selection depending on GNSS e.g., # = 5 for G L5; 6, 7 or 8 for E L6, L7 or L8; 5 or 7 for C L5 or L7 Options couples to GNSS selection. (Default, not specified and GAMIT selection used”j§]”j±ŒÊLower frequency selection depending on GNSS e.g., # = 5 for G L5; 6, 7 or 8 for E L6, L7 or L8; 5 or 7 for C L5 or L7 Options couples to GNSS selection. (Default, not specified and GAMIT selection used”…””}”(j¶j.’jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKMj¶j+’ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j’ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆKNj¶j’ubaj·}”(j¹]”j’aj»]”j½]”Œman_sh_gamit_lfreq”ajÀ]”jÂ]”ujÄj ej¶jšjÇjshjŸjÆNjÒ }”jL’j ’sjÔ }”j’j ’subje)”}”(j¦Œ.. _man_sh_gamit_expt:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-expt”ujÄjdjÆKTj¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-expt”j§]”(jM‘)”}”(j¦Œ-e”j§]”j±Œ-e”…””}”j¶ji’sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶je’ubj]‘)”}”(j¦Œxpt”j§]”j±Œxpt”…””}”(j¶jw’jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶je’ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jb’ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶j_’ubj{‘)”}”(j¦ŒP4 char name of experiment/s to run. (list of expts can be used). [Default expt] ”j§]”j`)”}”(j¦ŒO4 char name of experiment/s to run. (list of expts can be used). [Default expt]”j§]”j±ŒO4 char name of experiment/s to run. (list of expts can be used). [Default expt]”…””}”(j¶j–’jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKSj¶j’’ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶j_’ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j\’jÇjshjŸjÆNubaj·}”(j¹]”j[’aj»]”j½]”Œman_sh_gamit_expt”ajÀ]”jÂ]”ujÄj7‘hjŸjÆKRj¶jšjÇjsjÒ }”j´’jQ’sjÔ }”j[’jQ’subje)”}”(j¦Œ.. _man_sh_gamit_orbit:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-orbit”ujÄjdjÆKYj¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-orbit”j§]”(jM‘)”}”(j¦Œ-o”j§]”j±Œ-o”…””}”j¶jÑ’sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶jÍ’ubj]‘)”}”(j¦Œrbit”j§]”j±Œrbit”…””}”(j¶jß’jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶jÍ’ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jÊ’ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jÇ’ubj{‘)”}”(j¦XType of orbit to use. (igsf igsr igsu codf code codm codr emrf esaf gfzf gfzm grgm jaxm jplf mitf ngsf siof sior siou tumm wuhm [Default igsf] See sh_get_orbits for description. Optional second argument gives the day-of-year for the orbit if not the same as processing day ”j§]”j`)”}”(j¦XType of orbit to use. (igsf igsr igsu codf code codm codr emrf esaf gfzf gfzm grgm jaxm jplf mitf ngsf siof sior siou tumm wuhm [Default igsf] See sh_get_orbits for description. Optional second argument gives the day-of-year for the orbit if not the same as processing day”j§]”j±XType of orbit to use. (igsf igsr igsu codf code codm codr emrf esaf gfzf gfzm grgm jaxm jplf mitf ngsf siof sior siou tumm wuhm [Default igsf] See sh_get_orbits for description. Optional second argument gives the day-of-year for the orbit if not the same as processing day”…””}”(j¶jþ’jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKXj¶jú’ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jÇ’ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶jÄ’jÇjshjŸjÆNubaj·}”(j¹]”jÃ’aj»]”j½]”Œman_sh_gamit_orbit”ajÀ]”jÂ]”ujÄj7‘hjŸjÆKWj¶jšjÇjsjÒ }”j“j¹’sjÔ }”jÃ’j¹’subje)”}”(j¦Œ.. _man_sh_gamit_orbt:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-orbt”ujÄjdjÆKaj¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-orbt”j§]”(jM‘)”}”(j¦Œ-o”j§]”j±Œ-o”…””}”j¶j9“sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j5“ubj]‘)”}”(j¦Œrbt”j§]”j±Œrbt”…””}”(j¶jG“jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶j5“ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶j2“ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶j/“ubj{‘)”}”(j¦Œˆ4 char ID for g-files. Specify only to use a non-conventional, locally generated g-file [Default is lowercase of downloaded orbit type] ”j§]”j`)”}”(j¦Œ‡4 char ID for g-files. Specify only to use a non-conventional, locally generated g-file [Default is lowercase of downloaded orbit type]”j§]”j±Œ‡4 char ID for g-files. Specify only to use a non-conventional, locally generated g-file [Default is lowercase of downloaded orbit type]”…””}”(j¶jf“jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK`j¶jb“ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶j/“ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j,“jÇjshjŸjÆNubaj·}”(j¹]”j+“aj»]”j½]”Œman_sh_gamit_orbt”ajÀ]”jÂ]”ujÄj7‘hjŸjÆK_j¶jšjÇjsjÒ }”j„“j!“sjÔ }”j+“j!“subje)”}”(j¦Œ.. _man_sh_gamit_srm_param:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-srm-param”ujÄjdjÆKgj¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ -srp_param”j§]”(jM‘)”}”(j¦Œ-s”j§]”j±Œ-s”…””}”j¶j¡“sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j“ubj]‘)”}”(j¦Œrp_param”j§]”j±Œrp_param”…””}”(j¶j¯“jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶j“ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jš“ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶j—“ubj{‘)”}”(j¦ŒµRadiation-pressure parameters to estimate in the fit to the input orbit (default allpr) (See :program:`sh_sp3fit` for other options and interaction with radiation model in sestbl.) ”j§]”j`)”}”(j¦Œ´Radiation-pressure parameters to estimate in the fit to the input orbit (default allpr) (See :program:`sh_sp3fit` for other options and interaction with radiation model in sestbl.)”j§]”(j±Œ]Radiation-pressure parameters to estimate in the fit to the input orbit (default allpr) (See ”…””}”(j¶jΓjÇjshNjÆNubjj)”}”(j¦Œ:program:`sh_sp3fit`”j§]”j±Œ sh_sp3fit”…””}”(j¶jÖ“jÇjshNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jΓubj±ŒC for other options and interaction with radiation model in sestbl.)”…””}”(j¶jΓjÇjshNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKfj¶jÊ“ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶j—“ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j”“jÇjshjŸjÆNubaj·}”(j¹]”j““aj»]”j½]”Œman_sh_gamit_srm_param”ajÀ]”jÂ]”ujÄj7‘hjŸjÆKej¶jšjÇjsjÒ }”jþ“j‰“sjÔ }”j““j‰“subje)”}”(j¦Œ.. _man_sh_gamit_eops:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-eops”ujÄjdjÆKmj¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-eops”j§]”(jM‘)”}”(j¦Œ-e”j§]”j±Œ-e”…””}”j¶j”sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j”ubj]‘)”}”(j¦Œops”j§]”j±Œops”…””}”(j¶j)”jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶j”ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶j”ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶j”ubj{‘)”}”(j¦ŒAName of EOP series to use. (bull_b, bull_a, etc.) [Default usno] ”j§]”j`)”}”(j¦Œ@Name of EOP series to use. (bull_b, bull_a, etc.) [Default usno]”j§]”j±Œ@Name of EOP series to use. (bull_b, bull_a, etc.) [Default usno]”…””}”(j¶jH”jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKlj¶jD”ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶j”ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j”jÇjshjŸjÆNubaj·}”(j¹]”j ”aj»]”j½]”Œman_sh_gamit_eops”ajÀ]”jÂ]”ujÄj7‘hjŸjÆKkj¶jšjÇjsjÒ }”jf”j”sjÔ }”j ”j”subje)”}”(j¦Œ.. _man_sh_gamit_localeop:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-localeop”ujÄjdjÆKsj¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ -localeop”j§]”(jM‘)”}”(j¦Œ-l”j§]”j±Œ-l”…””}”j¶jƒ”sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j”ubj]‘)”}”(j¦Œocaleop”j§]”j±Œocaleop”…””}”(j¶j‘”jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶j”ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶j|”ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jy”ubj{‘)”}”(j¦ŒqUse a local copy of EOP tables (series used is defined by -eops). No ftp update will be attempted. [Default off] ”j§]”j`)”}”(j¦ŒpUse a local copy of EOP tables (series used is defined by -eops). No ftp update will be attempted. [Default off]”j§]”j±ŒpUse a local copy of EOP tables (series used is defined by -eops). No ftp update will be attempted. [Default off]”…””}”(j¶j°”jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKrj¶j¬”ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jy”ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶jv”jÇjshjŸjÆNubaj·}”(j¹]”ju”aj»]”j½]”Œman_sh_gamit_localeop”ajÀ]”jÂ]”ujÄj7‘hjŸjÆKqj¶jšjÇjsjÒ }”jΔjk”sjÔ }”ju”jk”subje)”}”(j¦Œ.. _man_sh_gamit_remakex:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-remakex”ujÄjdjÆKyj¶jšjÇjshjŸubj e)”}”(j¦hoj§]”je)”}”(j¦ŒÆ-remakex Y/C/N Y - Remake x-files without checking. C - Remake x-file if orbit and session.info are incompatable and all RINEX available [Default C] N - Don't remake x-files under any circumstances ”j§]”(je)”}”(j¦Œ-remakex Y/C/N”j§]”j±Œ-remakex Y/C/N”…””}”(j¶jå”jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆKzj¶já”ubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ¶Y - Remake x-files without checking. C - Remake x-file if orbit and session.info are incompatable and all RINEX available [Default C] N - Don't remake x-files under any circumstances”j§]”j±Œ¸Y - Remake x-files without checking. C - Remake x-file if orbit and session.info are incompatable and all RINEX available [Default C] N - Don’t remake x-files under any circumstances”…””}”(j¶jö”jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKxj¶jó”ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶já”ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆKzj¶jÞ”ubaj·}”(j¹]”jÝ”aj»]”j½]”Œman_sh_gamit_remakex”ajÀ]”jÂ]”ujÄj ej¶jšjÇjshjŸjÆNjÒ }”j•jÓ”sjÔ }”jÝ”jÓ”subje)”}”(j¦Œ.. _man_sh_gamit_remakek:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-remakek”ujÄjdjÆK€j¶jšjÇjshjŸubj e)”}”(j¦hoj§]”je)”}”(j¦Œ¨-renamek Y/C/N Y - Remove existing k-files and remake C - Do not remake k-files unless missing or X-files remade (default) N - Do not remake k-files -- stop if missing ”j§]”(je)”}”(j¦Œ-renamek Y/C/N”j§]”j±Œ-renamek Y/C/N”…””}”(j¶j+•jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆKj¶j'•ubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ˜Y - Remove existing k-files and remake C - Do not remake k-files unless missing or X-files remade (default) N - Do not remake k-files -- stop if missing”j§]”j±Œ™Y - Remove existing k-files and remake C - Do not remake k-files unless missing or X-files remade (default) N - Do not remake k-files – stop if missing”…””}”(j¶j<•jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKj¶j9•ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j'•ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆKj¶j$•ubaj·}”(j¹]”j#•aj»]”j½]”Œman_sh_gamit_remakek”ajÀ]”jÂ]”ujÄj ej¶jšjÇjshjŸjÆNjÒ }”jZ•j•sjÔ }”j#•j•subje)”}”(j¦Œ.. _man_sh_gamit_remakej:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-remakej”ujÄjdjÆK‡j¶jšjÇjshjŸubj e)”}”(j¦hoj§]”je)”}”(j¦Œ†-remakej Y/N Y - Remake j-file (default) N - Do not remake j-file (used with epoch-by-epoch j-files for SA with mismatched time tags) ”j§]”(je)”}”(j¦Œ -remakej Y/N”j§]”j±Œ -remakej Y/N”…””}”(j¶jq•jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK‡j¶jm•ubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒxY - Remake j-file (default) N - Do not remake j-file (used with epoch-by-epoch j-files for SA with mismatched time tags)”j§]”j±ŒxY - Remake j-file (default) N - Do not remake j-file (used with epoch-by-epoch j-files for SA with mismatched time tags)”…””}”(j¶j‚•jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK†j¶j•ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jm•ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK‡j¶jj•ubaj·}”(j¹]”ji•aj»]”j½]”Œman_sh_gamit_remakej”ajÀ]”jÂ]”ujÄj ej¶jšjÇjshjŸjÆNjÒ }”j •j_•sjÔ }”ji•j_•subje)”}”(j¦Œ.. _man_sh_gamit_remakeg:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-remakeg”ujÄjdjÆKj¶jšjÇjshjŸubj e)”}”(j¦hoj§]”je)”}”(j¦Œ‰-remakeg Y/N Y - Remake g-file (default, unless usr g-file) N - Do not remake if it exists. Showld be used when processing sub-networks ”j§]”(je)”}”(j¦Œ -remakeg Y/N”j§]”j±Œ -remakeg Y/N”…””}”(j¶j·•jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆKj¶j³•ubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ{Y - Remake g-file (default, unless usr g-file) N - Do not remake if it exists. Showld be used when processing sub-networks”j§]”j±Œ{Y - Remake g-file (default, unless usr g-file) N - Do not remake if it exists. Showld be used when processing sub-networks”…””}”(j¶jÈ•jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKŒj¶jÅ•ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j³•ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆKj¶j°•ubaj·}”(j¹]”j¯•aj»]”j½]”Œman_sh_gamit_remakeg”ajÀ]”jÂ]”ujÄj ej¶jšjÇjshjŸjÆNjÒ }”jæ•j¥•sjÔ }”j¯•j¥•subje)”}”(j¦Œ.. _man_sh_gamit_netext:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-netext”ujÄjdjÆK“j¶jšjÇjshjŸubj e)”}”(j¦hoj§]”je)”}”(j¦Œ¨-netext char Add network suffix to day directories (default if -gnss not in the command line is none (day number only): otherwise use the GNSS code, e.g., 301G) ”j§]”(je)”}”(j¦Œ -netext char”j§]”j±Œ -netext char”…””}”(j¶jý•jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK’j¶jù•ubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒšAdd network suffix to day directories (default if -gnss not in the command line is none (day number only): otherwise use the GNSS code, e.g., 301G)”j§]”j±ŒšAdd network suffix to day directories (default if -gnss not in the command line is none (day number only): otherwise use the GNSS code, e.g., 301G)”…””}”(j¶j–jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK’j¶j –ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jù•ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK’j¶jö•ubaj·}”(j¹]”jõ•aj»]”j½]”Œman_sh_gamit_netext”ajÀ]”jÂ]”ujÄj ej¶jšjÇjshjŸjÆNjÒ }”j,–jë•sjÔ }”jõ•jë•subje)”}”(j¦Œ.. _man_sh_gamit_yrext:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-yrext”ujÄjdjÆK˜j¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-yrext”j§]”(jM‘)”}”(j¦Œ-y”j§]”j±Œ-y”…””}”j¶jI–sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶jE–ubj]‘)”}”(j¦Œrext”j§]”j±Œrext”…””}”(j¶jW–jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶jE–ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jB–ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶j?–ubj{‘)”}”(j¦Œ0Add year prefix to day directories. Ie 1997_053 ”j§]”j`)”}”(j¦Œ/Add year prefix to day directories. Ie 1997_053”j§]”j±Œ/Add year prefix to day directories. 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sampling interval, number of epochs, start time (default 30 2880 0 0) ”j§]”j`)”}”(j¦ŒOSession - sampling interval, number of epochs, start time (default 30 2880 0 0)”j§]”j±ŒOSession - sampling interval, number of epochs, start time (default 30 2880 0 0)”…””}”(j¶jÀ—jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK¦j¶j¼—ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶j‰—ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j†—jÇjshjŸjÆNubaj·}”(j¹]”j…—aj»]”j½]”Œman_sh_gamit_sessinfo”ajÀ]”jÂ]”ujÄj7‘hjŸjÆK¥j¶jšjÇjsjÒ }”jÞ—j{—sjÔ }”j…—j{—subje)”}”(j¦Œ.. _man_sh_gamit_rx_doy_plus:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-rx-doy-plus”ujÄjdjÆK¬j¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ -rx_doy_plus”j§]”(jM‘)”}”(j¦Œ-r”j§]”j±Œ-r”…””}”j¶jû—sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j÷—ubj]‘)”}”(j¦Œ x_doy_plus”j§]”j±Œ x_doy_plus”…””}”(j¶j ˜jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶j÷—ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jô—ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jñ—ubj{‘)”}”(j¦ŒLSearch RINEX file names this many days into the future for current-day data ”j§]”j`)”}”(j¦ŒKSearch RINEX file names this many days into the future for current-day data”j§]”j±ŒKSearch RINEX file names this many days into the future for current-day data”…””}”(j¶j(˜jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK«j¶j$˜ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jñ—ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶jî—jÇjshjŸjÆNubaj·}”(j¹]”jí—aj»]”j½]”Œman_sh_gamit_rx_doy_plus”ajÀ]”jÂ]”ujÄj7‘hjŸjÆKªj¶jšjÇjsjÒ }”jF˜jã—sjÔ }”jí—jã—subje)”}”(j¦Œ.. _man_sh_gamit_rx_doy_minus:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-rx-doy-minus”ujÄjdjÆK±j¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ -rx_doy_minus”j§]”(jM‘)”}”(j¦Œ-r”j§]”j±Œ-r”…””}”j¶jc˜sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j_˜ubj]‘)”}”(j¦Œ x_doy_minus”j§]”j±Œ x_doy_minus”…””}”(j¶jq˜jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶j_˜ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶j\˜ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jY˜ubj{‘)”}”(j¦ŒJSearch RINEX file names this many days into the past for current-day data ”j§]”j`)”}”(j¦ŒISearch RINEX file names this many days into the past for current-day data”j§]”j±ŒISearch RINEX file names this many days into the past for current-day data”…””}”(j¶j˜jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK°j¶jŒ˜ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jY˜ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶jV˜jÇjshjŸjÆNubaj·}”(j¹]”jU˜aj»]”j½]”Œman_sh_gamit_rx_doy_minus”ajÀ]”jÂ]”ujÄj7‘hjŸjÆK¯j¶jšjÇjsjÒ }”j®˜jK˜sjÔ }”jU˜jK˜subje)”}”(j¦Œ.. _man_sh_gamit_minspan:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-minspan”ujÄjdjÆK¶j¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-minspan”j§]”(jM‘)”}”(j¦Œ-m”j§]”j±Œ-m”…””}”j¶j˘sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶jǘubj]‘)”}”(j¦Œinspan”j§]”j±Œinspan”…””}”(j¶jÙ˜jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶jǘubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jĘubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jÁ˜ubj{‘)”}”(j¦ŒFMinimum span of data in rinex files in hours [Default is 0.1 (6 min)] ”j§]”j`)”}”(j¦ŒEMinimum span of data in rinex files in hours [Default is 0.1 (6 min)]”j§]”j±ŒEMinimum span of data in rinex files in hours [Default is 0.1 (6 min)]”…””}”(j¶jø˜jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKµj¶jô˜ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jÁ˜ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j¾˜jÇjshjŸjÆNubaj·}”(j¹]”j½˜aj»]”j½]”Œman_sh_gamit_minspan”ajÀ]”jÂ]”ujÄj7‘hjŸjÆK´j¶jšjÇjsjÒ }”j™j³˜sjÔ }”j½˜j³˜subje)”}”(j¦Œ.. _man_sh_gamit_mailto:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒman-sh-gamit-mailto”ujÄjdjÆK»j¶jšjÇjshjŸubj8‘)”}”(j¦hoj§]”(j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-mailto”j§]”(jM‘)”}”(j¦Œ-m”j§]”j±Œ-m”…””}”j¶j3™sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j/™ubj]‘)”}”(j¦Œailto”j§]”j±Œailto”…””}”(j¶jA™jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶j/™ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶j,™ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶j)™ubj{‘)”}”(j¦ŒLName of user and machine to send results summary (e.g. example@example.com) ”j§]”j`)”}”(j¦ŒKName of user and machine to send results summary (e.g. example@example.com)”j§]”(j±Œ7Name of user and machine to send results summary (e.g. ”…””}”(j¶j`™jÇjshNjÆNubj÷ )”}”(j¦Œexample@example.com”j§]”j±Œexample@example.com”…””}”(j¶jh™jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”Œmailto:example@example.com”ujÄjö j¶j`™ubj±Œ)”…””}”(j¶j`™jÇjshNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKºj¶j\™ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶j)™ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j&™jÇjshjŸjÆNubj=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-snrres”j§]”(jM‘)”}”(j¦Œ-s”j§]”j±Œ-s”…””}”j¶j˜™sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j”™ubj]‘)”}”(j¦Œnrres”j§]”j±Œnrres”…””}”(j¶j¦™jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶j”™ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶j‘™ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jŽ™ubj{‘)”}”(j¦ŒRCalculate theoretical phase residuals from SNR. (requires raw data or rinex W/SNR)”j§]”j`)”}”(j¦jÙj§]”j±ŒRCalculate theoretical phase residuals from SNR. (requires raw data or rinex W/SNR)”…””}”(j¶jÅ™jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK¼j¶jÁ™ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jŽ™ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j&™jÇjshjŸjÆNubj=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-noacc”j§]”(jM‘)”}”(j¦Œ-n”j§]”j±Œ-n”…””}”j¶jè™sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶jä™ubj]‘)”}”(j¦Œoacc”j§]”j±Œoacc”…””}”(j¶jö™jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶jä™ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶já™ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jÞ™ubj{‘)”}”(j¦ŒTDo not exclude satellites base on accuracy codes in the .sp3 file. [Default exclude]”j§]”j`)”}”(j¦jšj§]”j±ŒTDo not exclude satellites base on accuracy codes in the .sp3 file. [Default exclude]”…””}”(j¶jšjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK½j¶jšubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jÞ™ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j&™jÇjshjŸjÆNubej·}”(j¹]”j%™aj»]”j½]”Œman_sh_gamit_mailto”ajÀ]”jÂ]”ujÄj7‘hjŸjÆK¹j¶jšjÇjsjÒ }”j2šj™sjÔ }”j%™j™subj`)”}”(j¦XÑ-ofit val Maximum orbit misfit allowed when fitting GMAIT orbit model to .SP3 file. [Default 0.1 m] -xsite list List of sites to be excluded from the processing. [format site:yyyy_ddd-yyyy_ddd OR site] -copt opts Types of files to be compressed in the day directory. [Default: x k ao D] -aopt opts Types of files to be archived under -archivepth . [Default: null] -dopt opts Types of files to be deleted from the day directory. [Default: c]”j§]”j±XÑ-ofit val Maximum orbit misfit allowed when fitting GMAIT orbit model to .SP3 file. [Default 0.1 m] -xsite list List of sites to be excluded from the processing. [format site:yyyy_ddd-yyyy_ddd OR site] -copt opts Types of files to be compressed in the day directory. [Default: x k ao D] -aopt opts Types of files to be archived under -archivepth . [Default: null] -dopt opts Types of files to be deleted from the day directory. [Default: c]”…””}”(j¶j7šjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆK¾j¶jšjÇjsubj©Œ block_quote”“”)”}”(j¦ŒÑPossible d-, c-, and a- opts: D, H, ao, ac, as, b, c, d, e, g, h, i, j, k, l, m, met, o, p, ps, q, t, x, z, all Note: all for -dopt will also remove the day directories, so pairs logically with -aopt H h q as”j§]”j`)”}”(j¦ŒÑPossible d-, c-, and a- opts: D, H, ao, ac, as, b, c, d, e, g, h, i, j, k, l, m, met, o, p, ps, q, t, x, z, all Note: all for -dopt will also remove the day directories, so pairs logically with -aopt H h q as”j§]”j±ŒÑPossible d-, c-, and a- opts: D, H, ao, ac, as, b, c, d, e, g, h, i, j, k, l, m, met, o, p, ps, q, t, x, z, all Note: all for -dopt will also remove the day directories, so pairs logically with -aopt H h q as”…””}”(j¶jKšjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÃj¶jGšubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjEšhjŸjÆKÃj¶jšjÇjsubj8‘)”}”(j¦hoj§]”(j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-topt”j§]”(jM‘)”}”(j¦Œ-t”j§]”j±Œ-t”…””}”j¶jlšsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶jhšubj]‘)”}”(j¦Œopt”j§]”j±Œopt”…””}”(j¶jzšjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶jhšubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶ješubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jbšubj{‘)”}”(j¦Œóopts Defines the list of table files to be relinked if they already exist [Default = none] none all nutabl. soltab. luntab. gdetic.dat guess_rcvant.dat leap.sec svnav.dat svs_exclude.dat tform.dat antmod.dat rcvant.dat dcb.dat core pole ut1”j§]”j`)”}”(j¦Œóopts Defines the list of table files to be relinked if they already exist [Default = none] none all nutabl. soltab. luntab. gdetic.dat guess_rcvant.dat leap.sec svnav.dat svs_exclude.dat tform.dat antmod.dat rcvant.dat dcb.dat core pole ut1”j§]”j±Œóopts Defines the list of table files to be relinked if they already exist [Default = none] none all nutabl. soltab. luntab. gdetic.dat guess_rcvant.dat leap.sec svnav.dat svs_exclude.dat tform.dat antmod.dat rcvant.dat dcb.dat core pole ut1”…””}”(j¶j™šjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÅj¶j•šubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jbšubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j_šjÇjshjŸjÆNubj=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-c”j§]”jM‘)”}”(j¦j»šj§]”j±Œ-c”…””}”j¶j½šsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶j¹šubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶j¶šubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶j³šubj{‘)”}”(j¦Œ>Do not compress RINEX files when done [Default is to compress]”j§]”j`)”}”(j¦jØšj§]”j±Œ>Do not compress RINEX files when done [Default is to compress]”…””}”(j¶jÚšjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÉj¶jÖšubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶j³šubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j_šjÇjshjŸjÆNubj=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-h”j§]”jM‘)”}”(j¦jûšj§]”j±Œ-h”…””}”j¶jýšsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶jùšubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jöšubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jóšubj{‘)”}”(j¦Œ3Use Hatanaka RINEX compress algorithm. [Default No]”j§]”j`)”}”(j¦j›j§]”j±Œ3Use Hatanaka RINEX compress algorithm. [Default No]”…””}”(j¶j›jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÊj¶j›ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jóšubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j_šjÇjshjŸjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj7‘hjŸjÆKÅj¶jšjÇjsubj`)”}”(j¦X¤-archivepth dir Directory where files are to be archived [Default $procdir/archive] -xver char 1-character x-file version (6th character of x-file). [Default is single-digit year] -noftp Use this option if no ftp download connections are available. -met Link in RINEX met files from ../met [Default off] -ion [opts] Download IONEX files to ../ionex and link [Default igsg if no argument given]”j§]”j±X¤-archivepth dir Directory where files are to be archived [Default $procdir/archive] -xver char 1-character x-file version (6th character of x-file). [Default is single-digit year] -noftp Use this option if no ftp download connections are available. -met Link in RINEX met files from ../met [Default off] -ion [opts] Download IONEX files to ../ionex and link [Default igsg if no argument given]”…””}”(j¶j9›jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKËj¶jšjÇjsubjFš)”}”(j¦ŒFAutomatically switced on if "Ion model = GMAP" given in tables/sestbl.”j§]”j`)”}”(j¦jI›j§]”j±ŒJAutomatically switced on if “Ion model = GMAP†given in tables/sestbl.”…””}”(j¶jK›jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÐj¶jG›ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjEšhjŸjÆKÐj¶jšjÇjsubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ -ftp_prog”j§]”(jM‘)”}”(j¦Œ-f”j§]”j±Œ-f”…””}”j¶jk›sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶jg›ubj]‘)”}”(j¦Œtp_prog”j§]”j±Œtp_prog”…””}”(j¶jy›jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶jg›ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jd›ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶ja›ubj{‘)”}”(j¦Œ2Name of ftp program: ftp or ncftp [default is ftp]”j§]”j`)”}”(j¦j–›j§]”j±Œ2Name of ftp program: ftp or ncftp [default is ftp]”…””}”(j¶j˜›jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÑj¶j”›ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶ja›ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶j^›jÇjshjŸjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj7‘hjŸjÆKÑj¶jšjÇjsubj`)”}”(j¦XÑ-rinex_ftpsites List of ftp sites to be searched for rinex files [default sopac cddis and unavco] -subdir creates a temporary subdirectory to speed up uncompress when there are many rinex files in directory -aprfile Name of xyz coordinate .apr file to be used. [Default is itrf2000.apr] -xcheck Y/N Do not ftp rinex file if the xfile exists already [Default N] -noprocess opt Use this option if gamit processing should be avoided. [Default ftp].”j§]”j±XÑ-rinex_ftpsites List of ftp sites to be searched for rinex files [default sopac cddis and unavco] -subdir creates a temporary subdirectory to speed up uncompress when there are many rinex files in directory -aprfile Name of xyz coordinate .apr file to be used. [Default is itrf2000.apr] -xcheck Y/N Do not ftp rinex file if the xfile exists already [Default N] -noprocess opt Use this option if gamit processing should be avoided. [Default ftp].”…””}”(j¶j·›jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÒj¶jšjÇjsubjFš)”}”(j¦Œ†Possible: ftp - ftp rinex, eop, brdc, orbits. preproc - ftp + preprocess sites updating station.info and lfile if necessary.”j§]”j e)”}”(j¦hoj§]”je)”}”(j¦Œ|Possible: ftp - ftp rinex, eop, brdc, orbits. preproc - ftp + preprocess sites updating station.info and lfile if necessary.”j§]”(je)”}”(j¦Œ-Possible: ftp - ftp rinex, eop, brdc, orbits.”j§]”j±Œ-Possible: ftp - ftp rinex, eop, brdc, orbits.”…””}”(j¶jЛjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK×j¶jÌ›ubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒNpreproc - ftp + preprocess sites updating station.info and lfile if necessary.”j§]”j±ŒNpreproc - ftp + preprocess sites updating station.info and lfile if necessary.”…””}”(j¶já›jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKØj¶jÞ›ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jÌ›ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjŸjÆK×j¶jÉ›ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶jÅ›ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjEšhjŸjÆK×j¶jšjÇjsubj`)”}”(j¦ŒË-update_l (Y/N) Use this option to stop the l-file being updated by the .apr file [Default = Y] -no_lf_upd Do NOT update the master tables l-file (lfile.) when large coordinate adjustment occur - EVER.”j§]”j±ŒË-update_l (Y/N) Use this option to stop the l-file being updated by the .apr file [Default = Y] -no_lf_upd Do NOT update the master tables l-file (lfile.) when large coordinate adjustment occur - EVER.”…””}”(j¶jœjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÙj¶jšjÇjsubjFš)”}”(j¦ŒT[Default - update tables/lfile. if Update tolerance specified in sestbl. is exceeded”j§]”j`)”}”(j¦jœj§]”j±ŒT[Default - update tables/lfile. if Update tolerance specified in sestbl. is exceeded”…””}”(j¶jœjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÛj¶jœubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjEšhjŸjÆKÛj¶jšjÇjsubj`)”}”(j¦X-fixed_rx_list Link ONLY rinex files for sites listed in sites.defaults [Default = N] -sd file Name of sites.defaults file to use [Default = $procdir/tables/sites.defaults] -metutil N/Z Output Zenith wet delay and precipitable water using zenith hydrostatic delays [Default N]”j§]”j±X-fixed_rx_list Link ONLY rinex files for sites listed in sites.defaults [Default = N] -sd file Name of sites.defaults file to use [Default = $procdir/tables/sites.defaults] -metutil N/Z Output Zenith wet delay and precipitable water using zenith hydrostatic delays [Default N]”…””}”(j¶j,œjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKÜj¶jšjÇjsubjFš)”}”(j¦ŒWZ - Use GAMIT z-files to provide zenith hydrostatic delays (o-file interval is assumed)”j§]”j`)”}”(j¦j<œj§]”j±ŒWZ - Use GAMIT z-files to provide zenith hydrostatic delays (o-file interval is assumed)”…””}”(j¶j>œjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKßj¶j:œubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjEšhjŸjÆKßj¶jšjÇjsubj8‘)”}”(j¦hoj§]”j=‘)”}”(j¦hoj§]”(jB‘)”}”(j¦hoj§]”jG‘)”}”(j¦Œ-jclock”j§]”(jM‘)”}”(j¦Œ-j”j§]”j±Œ-j”…””}”j¶j^œsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjL‘j¶jZœubj]‘)”}”(j¦Œclock”j§]”j±Œclock”…””}”(j¶jlœjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œ delimiter”houjÄj\‘j¶jZœubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjF‘j¶jWœubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjA‘j¶jTœubj{‘)”}”(j¦ŒnSource for j-file clocks: sp3 or brdc; brdc the default for now for GPS, forced to sp3 for non-GPS processing ”j§]”j`)”}”(j¦ŒmSource for j-file clocks: sp3 or brdc; brdc the default for now for GPS, forced to sp3 for non-GPS processing”j§]”j±ŒmSource for j-file clocks: sp3 or brdc; brdc the default for now for GPS, forced to sp3 for non-GPS processing”…””}”(j¶j‹œjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjŸjÆKàj¶j‡œubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjz‘j¶jTœubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj<‘j¶jQœjÇjshjŸjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj7‘hjŸjÆKàj¶jšjÇjsubej·}”(j¹]”Œusage”aj»]”j½]”Œusage”ajÀ]”jÂ]”ujÄh_j¶jºjÇjshjŸjÆK)ubej·}”(j¹]”Œ#script-to-automate-gamit-processing”aj»]”j½]”Œ#script to automate gamit processing”ajÀ]”jÂ]”ujÄh_j¶j jÇjshjŸjÆK ubej·}”(j¹]”(Œsh-gamit”jžej»]”j½]”(Œsh_gamit”Œ man_sh_gamit”ejÀ]”jÂ]”ujÄh_j¶jsjÇjshjŸjÆKjÒ }”jÁœj”sjÔ }”jžj”subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jŸj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjŸjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j‚jvj‘j…uj_}”(Œrel”j‚Œdate”j‘ujc}”je}”(jž]”j”aj)]”jajŠ]”j€ajð]”jæaj6‘]”j,‘aj­‘]”j£‘aj’]”j ’aj[’]”jQ’ajÃ’]”j¹’aj+“]”j!“aj““]”j‰“aj ”]”j”aju”]”jk”ajÝ”]”jÓ”aj#•]”j•aji•]”j_•aj¯•]”j¥•ajõ•]”jë•aj;–]”j1–aj£–]”j™–aj —]”j—aj…—]”j{—ají—]”jã—ajU˜]”jK˜aj½˜]”j³˜aj%™]”j™aujg}”(jÁœjžjÀœj½œj¸œjµœjnjkj—j”j°œj­œj{j)jájŠj'‘jðjž‘j6‘j’j­‘jL’j’j´’j[’j“jÃ’j„“j+“jþ“j““jf”j ”jΔju”j•jÝ”jZ•j#•j •ji•jæ•j¯•j,–jõ•j”–j;–jü–j£–jv—j —jÞ—j…—jF˜jí—j®˜jU˜j™j½˜j2šj%™uji}”(jÁœˆjÀœ‰j¸œ‰jn‰j—‰j°œ‰j{ˆjáˆj'‘ˆjž‘ˆj’ˆjL’ˆj´’ˆj“ˆj„“ˆjþ“ˆjf”ˆjΔˆj•ˆjZ•ˆj •ˆj效j,–ˆj”–ˆjü–ˆjv—ˆjÞ—ˆjF˜ˆj®˜ˆj™ˆj2šˆuj¹}”(jžj j½œj jµœjºjkj Žj”jqj­œjšj)j*jŠj‹jðjñj6‘j9‘j­‘j®‘j’j’j[’j\’jÃ’jÄ’j+“j,“j““j”“j ”j”ju”jv”jÝ”jÞ”j#•j$•ji•jj•j¯•j°•jõ•jö•j;–j<–j£–j¤–j —j —j…—j†—jí—jî—jU˜jV˜j½˜j¾˜j%™j&™ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”(jù )”}”(j¦hoj§]”j`)”}”(j¦Œ;Option list ends without a blank line; unexpected unindent.”j§]”j±Œ;Option list ends without a blank line; unexpected unindent.”…””}”(j¶jjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”ŒWARNING”Œline”K¾Œsource”jŸujÄjø j¶jšjÇjshjŸjÆK½ubjù )”}”(j¦hoj§]”j`)”}”(j¦ŒUnexpected indentation.”j§]”j±ŒUnexpected indentation.”…””}”(j¶jjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”ŒERROR”Œsource”jŸŒline”KÃujÄjø j¶jšjÇjshjŸjÆKÂubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ;Block quote ends without a blank line; unexpected unindent.”j§]”j±Œ;Block quote ends without a blank line; unexpected unindent.”…””}”(j¶j;jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j8ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒline”KÅŒsource”jŸujÄjø j¶jšjÇjshjŸjÆNubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ;Option list ends without a blank line; unexpected unindent.”j§]”j±Œ;Option list ends without a blank line; unexpected unindent.”…””}”(j¶jVjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jSubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒline”KËŒsource”jŸujÄjø j¶jšjÇjshjŸjÆKÊubjù )”}”(j¦hoj§]”j`)”}”(j¦ŒUnexpected indentation.”j§]”j±ŒUnexpected indentation.”…””}”(j¶jqjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jnubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”j5Œsource”jŸŒline”KÐujÄjø j¶jšjÇjshjŸjÆKÏubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ;Block quote ends without a blank line; unexpected unindent.”j§]”j±Œ;Block quote ends without a blank line; unexpected unindent.”…””}”(j¶jŒjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j‰ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒline”KÑŒsource”jŸujÄjø j¶jšjÇjshjŸjÆNubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ;Option list ends without a blank line; unexpected unindent.”j§]”j±Œ;Option list ends without a blank line; unexpected unindent.”…””}”(j¶j§jÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j¤ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒline”KÒŒsource”jŸujÄjø j¶jšjÇjshjŸjÆKÑubjù )”}”(j¦hoj§]”j`)”}”(j¦ŒUnexpected indentation.”j§]”j±ŒUnexpected indentation.”…””}”(j¶jÂjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j¿ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”j5Œsource”jŸŒline”K×ujÄjø j¶jšjÇjshjŸjÆKÖubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ;Block quote ends without a blank line; unexpected unindent.”j§]”j±Œ;Block quote ends without a blank line; unexpected unindent.”…””}”(j¶jÝjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÚubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒline”KÙŒsource”jŸujÄjø j¶jšjÇjshNjÆNubjù )”}”(j¦hoj§]”j`)”}”(j¦ŒUnexpected indentation.”j§]”j±ŒUnexpected indentation.”…””}”(j¶jøjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jõubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”j5Œsource”jŸŒline”KÛujÄjø j¶jšjÇjshjŸjÆKÚubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ;Block quote ends without a blank line; unexpected unindent.”j§]”j±Œ;Block quote ends without a blank line; unexpected unindent.”…””}”(j¶jžjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jžubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒline”KÜŒsource”jŸujÄjø j¶jšjÇjshjŸjÆNubjù )”}”(j¦hoj§]”j`)”}”(j¦ŒUnexpected indentation.”j§]”j±ŒUnexpected indentation.”…””}”(j¶j.žjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j+žubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”j5Œsource”jŸŒline”KßujÄjø j¶jšjÇjshjŸjÆKÞubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ;Block quote ends without a blank line; unexpected unindent.”j§]”j±Œ;Block quote ends without a blank line; unexpected unindent.”…””}”(j¶jIžjÇjshNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jFžubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒline”KàŒsource”jŸujÄjø j¶jšjÇjshjŸjÆNubej†]”(jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ2Hyperlink target "man-sh-gamit" is not referenced.”…””}”j¶ježsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jbžubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”KujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ6Hyperlink target "man-sh-gamit-dir" is not referenced.”…””}”j¶jžsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j|žubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”K4ujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ4Hyperlink target "man-sh-gamit-d" is not referenced.”…””}”j¶j™žsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j–žubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”K:ujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ4Hyperlink target "man-sh-gamit-s" is not referenced.”…””}”j¶j³žsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j°žubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”K?ujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ4Hyperlink target "man-sh-gamit-r" is not referenced.”…””}”j¶jÍžsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÊžubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”KDujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ7Hyperlink target "man-sh-gamit-gnss" is not referenced.”…””}”j¶jçžsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jäžubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”KIujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ8Hyperlink target "man-sh-gamit-lfreq" is not referenced.”…””}”j¶jŸsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jþžubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”KNujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ7Hyperlink target "man-sh-gamit-expt" is not referenced.”…””}”j¶jŸsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jŸubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”KTujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ8Hyperlink target "man-sh-gamit-orbit" is not referenced.”…””}”j¶j5Ÿsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j2Ÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”KYujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ7Hyperlink target "man-sh-gamit-orbt" is not referenced.”…””}”j¶jOŸsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jLŸubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”KaujÄjø ubjù )”}”(j¦ho•#j§]”j`)”}”(j¦hoj§]”j±ŒHyperlink target "man-sh-gamit-rx-doy-plus" is not referenced.”…””}”j¶j¡ sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jž ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”K¬ujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ?Hyperlink target "man-sh-gamit-rx-doy-minus" is not referenced.”…””}”j¶j» sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j¸ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”K±ujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ:Hyperlink target "man-sh-gamit-minspan" is not referenced.”…””}”j¶jÕ sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÒ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”K¶ujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ9Hyperlink target "man-sh-gamit-mailto" is not referenced.”…””}”j¶jï sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jì ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŸŒline”K»ujÄjø ubejˆNj‰]”j‹NjÇjsubjûj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j ¡sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¡jÇj¡ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j¡jÇj¡hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¡jÇj¡ubje)”}”(j¦Œ.. _qsg_additional_software:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒqsg-additional-software”ujÄjdjÆKj¶j¡jÇj¡hŒF/chandler/home/floyd/public_html/gg/docs/source/quickstart/addl_sw.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒAdditional Software”j§]”j±ŒAdditional Software”…””}”(j¶j7¡jÇj¡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j4¡jÇj¡hj3¡jÆKubj`)”}”(j¦X£There are several additional programs that users may find useful, if not necessary, to install before running GAMIT/GLOBK. The major addition is `GMT `_, which is required for any GAMIT/GLOBK scripts that produce plots, e.g. :program:`sh_plot_pos`, :program:`sh_plotvel`, etc. You can install GMT for Debian-based Linux distributions such as Ubuntu from the main repository, e.g.”j§]”(j±Œ‘There are several additional programs that users may find useful, if not necessary, to install before running GAMIT/GLOBK. The major addition is ”…””}”(j¶jE¡jÇj¡hNjÆNubj÷ )”}”(j¦Œ/`GMT `_”j§]”j±ŒGMT”…””}”(j¶jM¡jÇj¡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGMT”j Œ&https://www.generic-mapping-tools.org/”ujÄjö j¶jE¡ubje)”}”(j¦Œ) ”j§]”j·}”(j¹]”Œgmt”aj»]”j½]”Œgmt”ajÀ]”jÂ]”Œrefuri”j]¡ujÄjdj Kj¶jE¡ubj±ŒI, which is required for any GAMIT/GLOBK scripts that produce plots, e.g. ”…””}”(j¶jE¡jÇj¡hNjÆNubjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶jo¡jÇj¡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jE¡ubj±Œ, ”…””}”(j¶jE¡jÇj¡hNjÆNubjj)”}”(j¦Œ:program:`sh_plotvel`”j§]”j±Œ sh_plotvel”…””}”(j¶j¡jÇj¡hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jE¡ubj±Œm, etc. You can install GMT for Debian-based Linux distributions such as Ubuntu from the main repository, e.g.”…””}”(j¶jE¡jÇj¡hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj3¡jÆKj¶j4¡jÇj¡ubj)”}”(j¦Œ($ sudo apt install gmt gmt-dcw gmt-gshhg”j§]”j±Œ($ sudo apt install gmt gmt-dcw gmt-gshhg”…””}”j¶j™¡sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj3¡jÆK j¶j4¡jÇj¡ubj`)”}”(j¦ŒQor from a community repository for RPM-based distributions such as openSUSE, e.g.”j§]”j±ŒQor from a community repository for RPM-based distributions such as openSUSE, e.g.”…””}”(j¶j©¡jÇj¡hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj3¡jÆKj¶j4¡jÇj¡ubj)”}”(j¦Œy$ sudo zypper ar -f http://download.opensuse.org/repositories/home:/beyerle:/IAC/openSUSE_Leap_15.1/home:beyerle:IAC.repo”j§]”j±Œy$ sudo zypper ar -f http://download.opensuse.org/repositories/home:/beyerle:/IAC/openSUSE_Leap_15.1/home:beyerle:IAC.repo”…””}”j¶j·¡sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj3¡jÆKj¶j4¡jÇj¡ubej·}”(j¹]”(Œadditional-software”j2¡ej»]”j½]”(Œadditional software”Œqsg_additional_software”ejÀ]”jÂ]”ujÄh_j¶j¡jÇj¡hj3¡jÆKjÒ }”jÍ¡j(¡sjÔ }”j2¡j(¡subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j3¡j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj3¡jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j¡j ¡j%¡j¡uj_}”(Œrel”j¡Œdate”j%¡ujc}”je}”j2¡]”j(¡asjg}”(jÍ¡j2¡jÌ¡jÉ¡jg¡jd¡uji}”(jÍ¡ˆjÌ¡‰jg¡ˆuj¹}”(j2¡j4¡jÉ¡j4¡jd¡j^¡ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ=Hyperlink target "qsg-additional-software" is not referenced.”…””}”j¶j÷¡sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jô¡ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j3¡Œline”KujÄjø ubajˆNj‰]”j‹NjÇj¡ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j¢sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¢jÇj¢ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j!¢jÇj¢hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j¢jÇj¢ubje)”}”(j¦Œ.. _qsg_compilation:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒqsg-compilation”ujÄjdjÆKj¶j¢jÇj¢hŒJ/chandler/home/floyd/public_html/gg/docs/source/quickstart/compilation.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ Compilation”j§]”j±Œ Compilation”…””}”(j¶j?¢jÇj¢hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j<¢jÇj¢hj;¢jÆKubj`)”}”(j¦XWe provide a script, :program:`install_software`, to compile GAMIT/GLOBK. You can download this file from the same server as the source code or extract it from the :file:`com.\ |rel|\ .tar.gz` file before running it, e.g. from your :file:`{}` directory:”j§]”(j±ŒWe provide a script, ”…””}”(j¶jM¢jÇj¢hNjÆNubjj)”}”(j¦Œ:program:`install_software`”j§]”j±Œinstall_software”…””}”(j¶jU¢jÇj¢hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jM¢ubj±Œt, to compile GAMIT/GLOBK. You can download this file from the same server as the source code or extract it from the ”…””}”(j¶jM¢jÇj¢hNjÆNubj˜)”}”(j¦Œ:file:`com.\ |rel|\ .tar.gz`”j§]”j±Œcom.|rel|.tar.gz”…””}”(j¶jg¢jÇj¢hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jM¢ubj±Œ( file before running it, e.g. from your ”…””}”(j¶jM¢jÇj¢hNjÆNubj˜)”}”(j¦Œ:file:`{}`”j§]”j )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j€¢jÇj¢hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j|¢ubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jM¢ubj±Œ directory:”…””}”(j¶jM¢jÇj¢hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj;¢jÆKj¶j<¢jÇj¢ubj)”}”(j¦ŒG$ tar xfzv com.10.71.tar.gz com/install_software $ com/install_software”j§]”j±ŒG$ tar xfzv com.10.71.tar.gz com/install_software $ com/install_software”…””}”j¶j¡¢sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj;¢jÆK j¶j<¢jÇj¢ubj`)”}”(j¦Œ±If you downloaded a copy of :program:`install_software` directly from our server you will need to make it executable before running, e.g. from your :file:`{}` directory:”j§]”(j±ŒIf you downloaded a copy of ”…””}”(j¶j±¢jÇj¢hNjÆNubjj)”}”(j¦Œ:program:`install_software`”j§]”j±Œinstall_software”…””}”(j¶j¹¢jÇj¢hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j±¢ubj±Œ] directly from our server you will need to make it executable before running, e.g. from your ”…””}”(j¶j±¢jÇj¢hNjÆNubj˜)”}”(j¦Œ:file:`{}`”j§]”j )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jÏ¢jÇj¢hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jË¢ubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j±¢ubj±Œ directory:”…””}”(j¶j±¢jÇj¢hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj;¢jÆKj¶j<¢jÇj¢ubj)”}”(j¦Œ$ chmod +x install_software”j§]”j±Œ$ chmod +x install_software”…””}”j¶jð¢sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj;¢jÆKj¶j<¢jÇj¢ubj`)”}”(j¦XZEither way, read carefully the questions the script asks and provide the information it requires. If the X11 libraries and headers cannot be found automatically, you will need to stop the compilation and edit :file:`libraries/Makefile.config` (in your :file:`{}` directory) before re-running :program:`install_software`. Specifically, you will need to edit the :content:`X11LIBPATH` and :content:`X11INCPATH` lines near the top of the file; typical locations for the required files for common operating systems are provided, so you may only need to uncomment the relevant lines, e.g. for macOS:”j§]”(j±ŒÑEither way, read carefully the questions the script asks and provide the information it requires. If the X11 libraries and headers cannot be found automatically, you will need to stop the compilation and edit ”…””}”(j¶j£jÇj¢hNjÆNubj˜)”}”(j¦Œ!:file:`libraries/Makefile.config`”j§]”j±Œlibraries/Makefile.config”…””}”(j¶j£jÇj¢hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£ubj±Œ (in your ”…””}”(j¶j£jÇj¢hNjÆNubj˜)”}”(j¦Œ:file:`{}`”j§]”j )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j!£jÇj¢hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j£ubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£ubj±Œ directory) before re-running ”…””}”(j¶j£jÇj¢hNjÆNubjj)”}”(j¦Œ:program:`install_software`”j§]”j±Œinstall_software”…””}”(j¶j<£jÇj¢hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j£ubj±Œ*. Specifically, you will need to edit the ”…””}”(j¶j£jÇj¢hNjÆNubj˜)”}”(j¦Œ:content:`X11LIBPATH`”j§]”j±Œ X11LIBPATH”…””}”(j¶jN£jÇj¢hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j£ubj±Œ and ”…””}”(j¶j£jÇj¢hNjÆNubj˜)”}”(j¦Œ:content:`X11INCPATH`”j§]”j±Œ X11INCPATH”…””}”(j¶ja£jÇj¢hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j£ubj±Œº lines near the top of the file; typical locations for the required files for common operating systems are provided, so you may only need to uncomment the relevant lines, e.g. for macOS:”…””}”(j¶j£jÇj¢hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj;¢jÆKj¶j<¢jÇj¢ubj)”}”(j¦Œ3X11LIBPATH /usr/X11/lib X11INCPATH /usr/X11/include”j§]”j±Œ3X11LIBPATH /usr/X11/lib X11INCPATH /usr/X11/include”…””}”j¶jz£sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhj;¢jÆKj¶j<¢jÇj¢ubj`)”}”(j¦Œ½Once the :program:`install_software` script completes successfully, you will see instructions to set up environment variables to run GAMIT/GLOBK, which is the last step of the installation.”j§]”(j±Œ Once the ”…””}”(j¶jŠ£jÇj¢hNjÆNubjj)”}”(j¦Œ:program:`install_software`”j§]”j±Œinstall_software”…””}”(j¶j’£jÇj¢hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jŠ£ubj±Œ™ script completes successfully, you will see instructions to set up environment variables to run GAMIT/GLOBK, which is the last step of the installation.”…””}”(j¶jŠ£jÇj¢hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj;¢jÆKj¶j<¢jÇj¢ubej·}”(j¹]”(Œ compilation”j:¢ej»]”j½]”(Œ compilation”Œqsg_compilation”ejÀ]”jÂ]”ujÄh_j¶j¢jÇj¢hj;¢jÆKjÒ }”j°£j0¢sjÔ }”j:¢j0¢subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j;¢j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj;¢jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j¢j¢j-¢j!¢uj_}”(Œrel”j¢Œdate”j-¢ujc}”je}”j:¢]”j0¢asjg}”(j°£j:¢j¯£j¬£uji}”(j°£ˆj¯£‰uj¹}”(j:¢j<¢j¬£j<¢ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ5Hyperlink target "qsg-compilation" is not referenced.”…””}”j¶jÚ£sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j×£ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j;¢Œline”KujÄjø ubajˆNj‰]”j‹NjÇj¢ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jõ£sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jò£jÇjò£ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j¤jÇjò£hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jò£jÇjò£ubje)”}”(j¦Œ.. _qsg_download:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ qsg-download”ujÄjdjÆKj¶jò£jÇjò£hŒG/chandler/home/floyd/public_html/gg/docs/source/quickstart/download.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒDownloading Source Code”j§]”j±ŒDownloading Source Code”…””}”(j¶j"¤jÇjò£hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j¤jÇjò£hj¤jÆKubj`)”}”(j¦ŒêGAMIT/GLOBK requires a license to run, which is granted to an institution, not individuals; all current members of a licensed institution are permitted to run GAMIT/GLOBK. See http://geoweb.mit.edu/gg/license.php for more information.”j§]”(j±Œ°GAMIT/GLOBK requires a license to run, which is granted to an institution, not individuals; all current members of a licensed institution are permitted to run GAMIT/GLOBK. See ”…””}”(j¶j0¤jÇjò£hNjÆNubj÷ )”}”(j¦Œ$http://geoweb.mit.edu/gg/license.php”j§]”j±Œ$http://geoweb.mit.edu/gg/license.php”…””}”(j¶j8¤jÇjò£hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j:¤ujÄjö j¶j0¤ubj±Œ for more information.”…””}”(j¶j0¤jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆKj¶j¤jÇjò£ubj`)”}”(j¦Œ´Once you have obtained the license information, download at least the following files (|release| is the current version) from our server, as described in the instructions received:”j§]”(j±ŒWOnce you have obtained the license information, download at least the following files (”…””}”(j¶jQ¤jÇjò£hNjÆNubj±Œ10.71”…””}”(j¶jQ¤jÇjò£hNjÆNubj±ŒT is the current version) from our server, as described in the instructions received:”…””}”(j¶jQ¤jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆK j¶j¤jÇjò£ubj“)”}”(j¦hoj§]”(j˜)”}”(j¦Œcom.\ |release|.tar.gz”j§]”j`)”}”(j¦jl¤j§]”(j±Œcom. ”…””}”(j¶jn¤jÇjò£hNjÆNubj±Œ10.71”…””}”(j¶jn¤jÇjò£hNjÆNubj±Œ.tar.gz”…””}”(j¶jn¤jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆK j¶jj¤ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jg¤jÇjò£hj¤jÆNubj˜)”}”(j¦Œgamit.\ |release|.tar.gz”j§]”j`)”}”(j¦j‹¤j§]”(j±Œgamit. ”…””}”(j¶j¤jÇjò£hNjÆNubj±Œ10.71”…””}”(j¶j¤jÇjò£hNjÆNubj±Œ.tar.gz”…””}”(j¶j¤jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆK j¶j‰¤ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jg¤jÇjò£hj¤jÆNubj˜)”}”(j¦Œhelp.\ |release|.tar.gz”j§]”j`)”}”(j¦jª¤j§]”(j±Œhelp. ”…””}”(j¶j¬¤jÇjò£hNjÆNubj±Œ10.71”…””}”(j¶j¬¤jÇjò£hNjÆNubj±Œ.tar.gz”…””}”(j¶j¬¤jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆKj¶j¨¤ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jg¤jÇjò£hj¤jÆNubj˜)”}”(j¦Œkf.\ |release|.tar.gz”j§]”j`)”}”(j¦jɤj§]”(j±Œkf. ”…””}”(j¶jˤjÇjò£hNjÆNubj±Œ10.71”…””}”(j¶jˤjÇjò£hNjÆNubj±Œ.tar.gz”…””}”(j¶jˤjÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆKj¶jǤubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jg¤jÇjò£hj¤jÆNubj˜)”}”(j¦Œlibraries.\ |release|.tar.gz”j§]”j`)”}”(j¦jè¤j§]”(j±Œ libraries. ”…””}”(j¶jê¤jÇjò£hNjÆNubj±Œ10.71”…””}”(j¶jê¤jÇjò£hNjÆNubj±Œ.tar.gz”…””}”(j¶jê¤jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆKj¶jæ¤ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jg¤jÇjò£hj¤jÆNubj˜)”}”(j¦Œtables.\ |release|.tar.gz”j§]”j`)”}”(j¦j¥j§]”(j±Œ tables. ”…””}”(j¶j ¥jÇjò£hNjÆNubj±Œ10.71”…””}”(j¶j ¥jÇjò£hNjÆNubj±Œ.tar.gz”…””}”(j¶j ¥jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆKj¶j¥ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jg¤jÇjò£hj¤jÆNubj˜)”}”(j¦Œ test_install.\ |release|.tar.gz ”j§]”j`)”}”(j¦Œtest_install.\ |release|.tar.gz”j§]”(j±Œtest_install. ”…””}”(j¶j(¥jÇjò£hNjÆNubj±Œ10.71”…””}”(j¶j(¥jÇjò£hNjÆNubj±Œ.tar.gz”…””}”(j¶j(¥jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆKj¶j$¥ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jg¤jÇjò£hj¤jÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj¤jÆK j¶j¤jÇjò£ubj`)”}”(j¦ŒÑand any :file:`incremental_updates.{}.tar.gz` files, where :file:`{}` is the calendar date of the latest updates. You can use :command:`curl` or :command:`wget` from the command line, e.g.:”j§]”(j±Œand any ”…””}”(j¶jJ¥jÇjò£hNjÆNubj˜)”}”(j¦Œ/:file:`incremental_updates.{}.tar.gz`”j§]”(j±Œincremental_updates.”…””}”(j¶jR¥jÇjò£hNjÆNubj )”}”(j¦Œ ”j§]”j±Œ ”…””}”(j¶jZ¥jÇjò£hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jR¥ubj±Œ.tar.gz”…””}”(j¶jR¥jÇjò£hNjÆNubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jJ¥ubj±Œ files, where ”…””}”(j¶jJ¥jÇjò£hNjÆNubj˜)”}”(j¦Œ:file:`{}`”j§]”j )”}”(j¦Œ ”j§]”j±Œ ”…””}”(j¶j}¥jÇjò£hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jy¥ubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jJ¥ubj±Œ9 is the calendar date of the latest updates. You can use ”…””}”(j¶jJ¥jÇjò£hNjÆNubjj)”}”(j¦Œ:command:`curl`”j§]”j±Œcurl”…””}”(j¶j˜¥jÇjò£hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jJ¥ubj±Œ or ”…””}”(j¶jJ¥jÇjò£hNjÆNubjj)”}”(j¦Œ:command:`wget`”j§]”j±Œwget”…””}”(j¶jª¥jÇjò£hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jJ¥ubj±Œ from the command line, e.g.:”…””}”(j¶jJ¥jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆKj¶j¤jÇjò£ubj)”}”(j¦Œv$ curl -k -R -O -u : '/source/{com,gamit,help,kf,libraries,tables,test_install}.10.71.tar.gz'”j§]”j±Œv$ curl -k -R -O -u : '/source/{com,gamit,help,kf,libraries,tables,test_install}.10.71.tar.gz'”…””}”j¶jÂ¥sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj¤jÆKj¶j¤jÇjò£ubj`)”}”(j¦Œthen:”j§]”j±Œthen:”…””}”(j¶jÒ¥jÇjò£hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆKj¶j¤jÇjò£ubj)”}”(j¦Œ]$ curl -k -R -O -u : /source/incremental_updates.01.tar.gz”j§]”j±Œ]$ curl -k -R -O -u : /source/incremental_updates.01.tar.gz”…””}”j¶jà¥sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj¤jÆKj¶j¤jÇjò£ubj`)”}”(j¦Œor:”j§]”j±Œor:”…””}”(j¶jð¥jÇjò£hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆK"j¶j¤jÇjò£ubj)”}”(j¦ŒÉ$ wget --no-check-certificate -N --user= --password= /source/{com,gamit,help,kf,libraries,tables,test_install}.10.71.tar.gz /source/incremental_updates.01.tar.gz”j§]”j±ŒÉ$ wget --no-check-certificate -N --user= --password= /source/{com,gamit,help,kf,libraries,tables,test_install}.10.71.tar.gz /source/incremental_updates.01.tar.gz”…””}”j¶jþ¥sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj¤jÆK$j¶j¤jÇjò£ubj`)”}”(j¦XKwhere :console:`` must be replaced by our server address and directory, :console:`` by the username and :console:`` by the password provided in the instructions received, and :console:`` and :console:`` by the current (four-digit) year and (two-digit) month, respectively. You may also access the distribution via a web browser but you must use our \https:// URL. Most browsers nowadays block FTP connections and you may therefore be prompted to open an alternative program, for example Finder on a Mac, if you enter the old \ftp:// URL into a browser.”j§]”(j±Œwhere ”…””}”(j¶j¦jÇjò£hNjÆNubj˜)”}”(j¦Œ:console:``”j§]”j±Œ”…””}”(j¶j¦jÇjò£hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j¦ubj±Œ7 must be replaced by our server address and directory, ”…””}”(j¶j¦jÇjò£hNjÆNubj˜)”}”(j¦Œ:console:``”j§]”j±Œ ”…””}”(j¶j)¦jÇjò£hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j¦ubj±Œ by the username and ”…””}”(j¶j¦jÇjò£hNjÆNubj˜)”}”(j¦Œ:console:``”j§]”j±Œ ”…””}”(j¶j<¦jÇjò£hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j¦ubj±Œ< by the password provided in the instructions received, and ”…””}”(j¶j¦jÇjò£hNjÆNubj˜)”}”(j¦Œ:console:``”j§]”j±Œ”…””}”(j¶jO¦jÇjò£hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j¦ubj±Œ and ”…””}”(j¶j¦jÇjò£hNjÆNubj˜)”}”(j¦Œ:console:``”j§]”j±Œ”…””}”(j¶jb¦jÇjò£hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j¦ubj±X^ by the current (four-digit) year and (two-digit) month, respectively. You may also access the distribution via a web browser but you must use our https:// URL. Most browsers nowadays block FTP connections and you may therefore be prompted to open an alternative program, for example Finder on a Mac, if you enter the old ftp:// URL into a browser.”…””}”(j¶j¦jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆK)j¶j¤jÇjò£ubj`)”}”(j¦X>The incremental updates contain sometimes critical updates to source code and tables, and should be downloaded on at least a monthly basis. Failure to keep GAMIT/GLOBK updated will result in errors and other issues. Updates can be compiled in exactly the same way as described in the :doc:`compilation` section, below.”j§]”(j±XThe incremental updates contain sometimes critical updates to source code and tables, and should be downloaded on at least a monthly basis. Failure to keep GAMIT/GLOBK updated will result in errors and other issues. Updates can be compiled in exactly the same way as described in the ”…””}”(j¶j{¦jÇjò£hNjÆNubj’)”}”(j¦Œ:doc:`compilation`”j§]”j)”}”(j¦j…¦j§]”j±Œ compilation”…””}”(j¶j‡¦jÇjò£hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶jƒ¦ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j‘¦Œreftype”Œdoc”Œ refexplicit”‰Œrefwarn”ˆj¶Œ compilation”ujÄj‘hj¤jÆK-j¶j{¦ubj±Œ section, below.”…””}”(j¶j{¦jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆK-j¶j¤jÇjò£ubj`)”}”(j¦X5Before downloading these files, we recommend choosing where you wish to install GAMIT/GLOBK by creating a main source directory. Examples include :file:`src/gg/|rel|/` or :file:`gamit-globk/|rel|/` in your home directory. In the following sections we refer to your chosen main directory as :file:`{}`.”j§]”(j±Œ’Before downloading these files, we recommend choosing where you wish to install GAMIT/GLOBK by creating a main source directory. Examples include ”…””}”(j¶j­¦jÇjò£hNjÆNubj˜)”}”(j¦Œ:file:`src/gg/|rel|/`”j§]”j±Œ src/gg/|rel|/”…””}”(j¶jµ¦jÇjò£hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­¦ubj±Œ or ”…””}”(j¶j­¦jÇjò£hNjÆNubj˜)”}”(j¦Œ:file:`gamit-globk/|rel|/`”j§]”j±Œgamit-globk/|rel|/”…””}”(j¶jʦjÇjò£hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­¦ubj±Œ] in your home directory. In the following sections we refer to your chosen main directory as ”…””}”(j¶j­¦jÇjò£hNjÆNubj˜)”}”(j¦Œ:file:`{}`”j§]”j )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶jã¦jÇjò£hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶jߦubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j­¦ubj±Œ.”…””}”(j¶j­¦jÇjò£hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¤jÆK1j¶j¤jÇjò£ubej·}”(j¹]”(Œdownloading-source-code”j¤ej»]”j½]”(Œdownloading source code”Œ qsg_download”ejÀ]”jÂ]”ujÄh_j¶jò£jÇjò£hj¤jÆKjÒ }”j §j¤sjÔ }”j¤j¤subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j¤j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj¤jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j¤jõ£j¤j¤uj_}”(Œrel”j¤Œdate”j¤ujc}”je}”j¤]”j¤asjg}”(j §j¤j §j§uji}”(j §ˆj §‰uj¹}”(j¤j¤j§j¤ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ2Hyperlink target "qsg-download" is not referenced.”…””}”j¶j4§sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j1§ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j¤Œline”KujÄjø ubajˆNj‰]”j‹NjÇjò£ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jO§sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jL§jÇjL§ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j^§jÇjL§hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jL§jÇjL§ubje)”}”(j¦Œ.. _qsg_intro:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ qsg-intro”ujÄjdjÆKj¶jL§jÇjL§hŒD/chandler/home/floyd/public_html/gg/docs/source/quickstart/intro.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ Introduction”j§]”j±Œ Introduction”…””}”(j¶j|§jÇjL§hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jy§jÇjL§hjx§jÆKubj`)”}”(j¦XØThis Quick Start Guide provides basic instructions for first-time users getting started with GAMIT/GLOBK. We describe the :doc:`download `, :doc:`compilation ` and :doc:`test ` processes, beyond which we refer users to our main technical documents (:doc:`/intro/index` and the more detailed reference manuals for `GAMIT `_ and `GLOBK `_).”j§]”(j±ŒzThis Quick Start Guide provides basic instructions for first-time users getting started with GAMIT/GLOBK. We describe the ”…””}”(j¶jŠ§jÇjL§hNjÆNubj’)”}”(j¦Œ:doc:`download `”j§]”j)”}”(j¦j”§j§]”j±Œdownload”…””}”(j¶j–§jÇjL§hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶j’§ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j §Œreftype”Œdoc”Œ refexplicit”ˆŒrefwarn”ˆj¶Œdownload”ujÄj‘hjx§jÆKj¶jŠ§ubj±Œ, ”…””}”(j¶jŠ§jÇjL§hNjÆNubj’)”}”(j¦Œ :doc:`compilation `”j§]”j)”}”(j¦j¸§j§]”j±Œ compilation”…””}”(j¶jº§jÇjL§hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶j¶§ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jħŒreftype”Œdoc”Œ refexplicit”ˆŒrefwarn”ˆj¶Œ compilation”ujÄj‘hjx§jÆKj¶jŠ§ubj±Œ and ”…””}”(j¶jŠ§jÇjL§hNjÆNubj’)”}”(j¦Œ!:doc:`test `”j§]”j)”}”(j¦jܧj§]”j±Œtest”…””}”(j¶jÞ§jÇjL§hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶jÚ§ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j觌reftype”Œdoc”Œ refexplicit”ˆŒrefwarn”ˆj¶Œ/test_install/index”ujÄj‘hjx§jÆKj¶jŠ§ubj±ŒI processes, beyond which we refer users to our main technical documents (”…””}”(j¶jŠ§jÇjL§hNjÆNubj’)”}”(j¦Œ:doc:`/intro/index`”j§]”j)”}”(j¦j¨j§]”j±Œ /intro/index”…””}”(j¶j¨jÇjL§hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶jþ§ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j ¨Œreftype”Œdoc”Œ refexplicit”‰Œrefwarn”ˆj¶Œ /intro/index”ujÄj‘hjx§jÆKj¶jŠ§ubj±Œ- and the more detailed reference manuals for ”…””}”(j¶jŠ§jÇjL§hNjÆNubj÷ )”}”(j¦Œ6`GAMIT `_”j§]”j±ŒGAMIT”…””}”(j¶j"¨jÇjL§hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT”j Œ+http://geoweb.mit.edu/gg/docs/GAMIT_Ref.pdf”ujÄjö j¶jŠ§ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œgamit”aj»]”j½]”Œgamit”ajÀ]”jÂ]”Œrefuri”j2¨ujÄjdj Kj¶jŠ§ubj±Œ and ”…””}”j¶jŠ§sbj÷ )”}”(j¦Œ6`GLOBK `_”j§]”j±ŒGLOBK”…””}”(j¶jD¨jÇjL§hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGLOBK”j Œ+http://geoweb.mit.edu/gg/docs/GLOBK_Ref.pdf”ujÄjö j¶jŠ§ubje)”}”(j¦Œ. ”j§]”j·}”(j¹]”Œglobk”aj»]”j½]”Œglobk”ajÀ]”jÂ]”Œrefuri”jT¨ujÄjdj Kj¶jŠ§ubj±Œ).”…””}”(j¶jŠ§jÇjL§hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjx§jÆKj¶jy§jÇjL§ubj`)”}”(j¦ŒrThis information is compiled through experience with first-time users of GAMIT/GLOBK from workshops and elsewhere.”j§]”j±ŒrThis information is compiled through experience with first-time users of GAMIT/GLOBK from workshops and elsewhere.”…””}”(j¶jl¨jÇjL§hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjx§jÆK j¶jy§jÇjL§ubj`)”}”(j¦ŒÿThe :doc:`prereq` section provides details separated by the type of operating system (:ref:`Linux `, :ref:`macOS ` and :ref:`Windows `). The rest of the compilation and testing process is common to all operating systems.”j§]”(j±ŒThe ”…””}”(j¶jz¨jÇjL§hNjÆNubj’)”}”(j¦Œ :doc:`prereq`”j§]”j)”}”(j¦j„¨j§]”j±Œprereq”…””}”(j¶j†¨jÇjL§hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶j‚¨ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j¨Œreftype”Œdoc”Œ refexplicit”‰Œrefwarn”ˆj¶Œprereq”ujÄj‘hjx§jÆK j¶jz¨ubj±ŒE section provides details separated by the type of operating system (”…””}”(j¶jz¨jÇjL§hNjÆNubj’)”}”(j¦Œ:ref:`Linux `”j§]”j)”}”(j¦j¨¨j§]”j±ŒLinux”…””}”(j¶jª¨jÇjL§hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-ref”ej½]”jÀ]”jÂ]”ujÄj*j¶j¦¨ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j´¨Œreftype”Œref”Œ refexplicit”ˆŒrefwarn”ˆj¶Œ qsg_linux”ujÄj‘hjx§jÆK j¶jz¨ubj±Œ, ”…””}”(j¶jz¨jÇjL§hNjÆNubj’)”}”(j¦Œ:ref:`macOS `”j§]”j)”}”(j¦j̨j§]”j±ŒmacOS”…””}”(j¶jΨjÇjL§hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-ref”ej½]”jÀ]”jÂ]”ujÄj*j¶jʨubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jبŒreftype”Œref”Œ refexplicit”ˆŒrefwarn”ˆj¶Œ qsg_macos”ujÄj‘hjx§jÆK j¶jz¨ubj±Œ and ”…””}”(j¶jz¨jÇjL§hNjÆNubj’)”}”(j¦Œ:ref:`Windows `”j§]”j)”}”(j¦jð¨j§]”j±ŒWindows”…””}”(j¶jò¨jÇjL§hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-ref”ej½]”jÀ]”jÂ]”ujÄj*j¶jî¨ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”jü¨Œreftype”Œref”Œ refexplicit”ˆŒrefwarn”ˆj¶Œ qsg_windows”ujÄj‘hjx§jÆK j¶jz¨ubj±ŒV). The rest of the compilation and testing process is common to all operating systems.”…””}”(j¶jz¨jÇjL§hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjx§jÆK j¶jy§jÇjL§ubj )”}”(j¦Œ­Clickable web links to the many documents and software mentioned are embedded in this document for reference. Hover the cursor over any underlined text to click on the link.”j§]”j±Œ­Clickable web links to the many documents and software mentioned are embedded in this document for reference. Hover the cursor over any underlined text to click on the link.”…””}”j¶j©sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0ujÄjj¶jy§jÇjL§hjx§jÆKubej·}”(j¹]”(Œ introduction”jw§ej»]”j½]”(Œ introduction”Œ qsg_intro”ejÀ]”jÂ]”ujÄh_j¶jL§jÇjL§hjx§jÆKjÒ }”j,©jm§sjÔ }”jw§jm§subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jx§j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjx§jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j[§jO§jj§j^§uj_}”(Œrel”j[§Œdate”jj§ujc}”je}”jw§]”jm§asjg}”(j,©jw§j+©j(©j<¨j9¨j^¨j[¨uji}”(j,©ˆj+©‰j<¨ˆj^¨ˆuj¹}”(jw§jy§j(©jy§j9¨j3¨j[¨jU¨ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ/Hyperlink target "qsg-intro" is not referenced.”…””}”j¶jV©sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jS©ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jx§Œline”KujÄjø ubajˆNj‰]”j‹NjÇjL§ubjðj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jq©sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jn©jÇjn©ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j€©jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jn©jÇjn©ubje)”}”(j¦Œ.. _qsg_prereq:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ qsg-prereq”ujÄjdjÆKj¶jn©jÇjn©hŒE/chandler/home/floyd/public_html/gg/docs/source/quickstart/prereq.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ Prerequisites”j§]”j±Œ Prerequisites”…””}”(j¶jž©jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j›©jÇjn©hjš©jÆKubj`)”}”(j¦ŒáGAMIT/GLOBK requires a few other programs to be installed before compiling the source code and running the software to its full capacity. These prerequisites are also listed on our website at http://geoweb.mit.edu/gg/pre.php.”j§]”(j±ŒÀGAMIT/GLOBK requires a few other programs to be installed before compiling the source code and running the software to its full capacity. These prerequisites are also listed on our website at ”…””}”(j¶j¬©jÇjn©hNjÆNubj÷ )”}”(j¦Œ http://geoweb.mit.edu/gg/pre.php”j§]”j±Œ http://geoweb.mit.edu/gg/pre.php”…””}”(j¶j´©jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j¶©ujÄjö j¶j¬©ubj±Œ.”…””}”(j¶j¬©jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKj¶j›©jÇjn©ubj`)”}”(j¦ŒIn addition to a basic Unix- or Linux-based operating system, there are four fundamental requirements for installing GAMIT/GLOBK on any system:”j§]”j±ŒIn addition to a basic Unix- or Linux-based operating system, there are four fundamental requirements for installing GAMIT/GLOBK on any system:”…””}”(j¶jÍ©jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK j¶j›©jÇjn©ubj“)”}”(j¦hoj§]”(j˜)”}”(j¦Œa Fortran compiler;”j§]”j`)”}”(j¦jà©j§]”j±Œa Fortran compiler;”…””}”(j¶jâ©jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK j¶jÞ©ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÛ©jÇjn©hjš©jÆNubj˜)”}”(j¦Œ a C compiler;”j§]”j`)”}”(j¦j÷©j§]”j±Œ a C compiler;”…””}”(j¶jù©jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK j¶jõ©ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÛ©jÇjn©hjš©jÆNubj˜)”}”(j¦ŒžX11 libraries and headers, specifically: * an X11 library (libX11.a, libX11.so, libX11.dylib, libX11.la or libX11.dll.a); and * an X11 header file (Xlib.h). ”j§]”(j`)”}”(j¦Œ(X11 libraries and headers, specifically:”j§]”j±Œ(X11 libraries and headers, specifically:”…””}”(j¶jªjÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK j¶j ªubj“)”}”(j¦hoj§]”(j˜)”}”(j¦ŒRan X11 library (libX11.a, libX11.so, libX11.dylib, libX11.la or libX11.dll.a); and”j§]”j`)”}”(j¦j#ªj§]”j±ŒRan X11 library (libX11.a, libX11.so, libX11.dylib, libX11.la or libX11.dll.a); and”…””}”(j¶j%ªjÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKj¶j!ªubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jªubj˜)”}”(j¦Œan X11 header file (Xlib.h). ”j§]”j`)”}”(j¦Œan X11 header file (Xlib.h).”j§]”j±Œan X11 header file (Xlib.h).”…””}”(j¶j<ªjÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKj¶j8ªubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jªubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hjš©jÆKj¶j ªubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÛ©jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hjš©jÆK j¶j›©jÇjn©ubj`)”}”(j¦Œ^Many operating systems will have some or all of these installed by default but others may not.”j§]”j±Œ^Many operating systems will have some or all of these installed by default but others may not.”…””}”(j¶jbªjÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKj¶j›©jÇjn©ubj`)”}”(j¦X…Below are details about what to expect from our experience with various operating systems. Once you have completed the steps described for your system, below, download the source code provided on our server, via FTP or secure HTTP, and install GAMIT/GLOBK. Further information is available in the :doc:`download` section and on the main `GAMIT/GLOBK web page `_.”j§]”(j±X)Below are details about what to expect from our experience with various operating systems. Once you have completed the steps described for your system, below, download the source code provided on our server, via FTP or secure HTTP, and install GAMIT/GLOBK. Further information is available in the ”…””}”(j¶jpªjÇjn©hNjÆNubj’)”}”(j¦Œ:doc:`download`”j§]”j)”}”(j¦jzªj§]”j±Œdownload”…””}”(j¶j|ªjÇjn©hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶jxªubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jðŒ refdomain”j†ªŒreftype”Œdoc”Œ refexplicit”‰Œrefwarn”ˆj¶Œdownload”ujÄj‘hjš©jÆKj¶jpªubj±Œ section and on the main ”…””}”(j¶jpªjÇjn©hNjÆNubj÷ )”}”(j¦Œ3`GAMIT/GLOBK web page `_”j§]”j±ŒGAMIT/GLOBK web page”…””}”(j¶jœªjÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGAMIT/GLOBK web page”j Œhttp://geoweb.mit.edu/gg/”ujÄjö j¶jpªubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œgamit-globk-web-page”aj»]”j½]”Œgamit/globk web page”ajÀ]”jÂ]”Œrefuri”j¬ªujÄjdj Kj¶jpªubj±Œ.”…””}”(j¶jpªjÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKj¶j›©jÇjn©ubje)”}”(j¦Œ.. _qsg_linux:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ qsg-linux”ujÄjdjÆKj¶j›©jÇjn©hjš©ubje)”}”(j¦Œ.. _qsg_debian:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ qsg-debian”ujÄjdjÆKj¶j›©jÇjn©hjš©jÒ }”Œ qsg_linux”jĪsjÔ }”jΪjĪsubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒDebian-Based Linux”j§]”j±ŒDebian-Based Linux”…””}”(j¶jàªjÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jݪjÇjn©hjš©jÆKubj`)”}”(j¦X*Debian-based Linux distributions include the common `Ubuntu `_ operating system. Install the prerequisite programs, including any dependencies and others that we have found to be missing in the core distribution but must be installed, i.e. (requires administrative privileges):”j§]”(j±Œ4Debian-based Linux distributions include the common ”…””}”(j¶jîªjÇjn©hNjÆNubj÷ )”}”(j¦Œ`Ubuntu `_”j§]”j±ŒUbuntu”…””}”(j¶jöªjÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒUbuntu”j Œhttps://ubuntu.com/”ujÄjö j¶jîªubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œubuntu”aj»]”j½]”jÀ]”Œubuntu”ajÂ]”Œrefuri”j«ujÄjdj Kj¶jîªubj±Œ× operating system. Install the prerequisite programs, including any dependencies and others that we have found to be missing in the core distribution but must be installed, i.e. (requires administrative privileges):”…””}”(j¶jîªjÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK j¶jݪjÇjn©ubj)”}”(j¦Œ<$ sudo apt install gfortran make libx11-dev csh tcsh bc curl”j§]”j±Œ<$ sudo apt install gfortran make libx11-dev csh tcsh bc curl”…””}”j¶j«sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjš©jÆK#j¶jݪjÇjn©ubje)”}”(j¦Œ .. _qsg_rpm:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒqsg-rpm”ujÄjdjÆK,j¶jݪjÇjn©hjš©ubej·}”(j¹]”(Œdebian-based-linux”jÙªjΪej»]”j½]”(Œdebian-based linux”Œ qsg_debian”jÛªejÀ]”jÂ]”ujÄh_j¶j›©jÇjn©hjš©jÆKjÒ }”(j?«jϪjÛªjĪujÔ }”(jÙªjϪjΪjĪuubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒRPM-Based Linux”j§]”j±ŒRPM-Based Linux”…””}”(j¶jG«jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jD«jÇjn©hjš©jÆK+ubj`)”}”(j¦XqRPM-based Linux distributions include `Fedora `_, `CentOS `_ and `openSUSE `_ operating systems. Install the prerequisite programs, including any dependencies and others that we have found to be missing in the core distribution but must be installed, i.e. (requires administrative privileges):”j§]”(j±Œ&RPM-based Linux distributions include ”…””}”(j¶jU«jÇjn©hNjÆNubj÷ )”}”(j¦Œ"`Fedora `_”j§]”j±ŒFedora”…””}”(j¶j]«jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒFedora”j Œhttps://getfedora.org/”ujÄjö j¶jU«ubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œfedora”aj»]”j½]”Œfedora”ajÀ]”jÂ]”Œrefuri”jm«ujÄjdj Kj¶jU«ubj±Œ, ”…””}”(j¶jU«jÇjn©hNjÆNubj÷ )”}”(j¦Œ#`CentOS `_”j§]”j±ŒCentOS”…””}”(j¶j«jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒCentOS”j Œhttps://www.centos.org/”ujÄjö j¶jU«ubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œcentos”aj»]”j½]”Œcentos”ajÀ]”jÂ]”Œrefuri”j«ujÄjdj Kj¶jU«ubj±Œ and ”…””}”(j¶jU«jÇjn©hNjÆNubj÷ )”}”(j¦Œ'`openSUSE `_”j§]”j±ŒopenSUSE”…””}”(j¶j¡«jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒopenSUSE”j Œhttps://www.opensuse.org/”ujÄjö j¶jU«ubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œopensuse”aj»]”j½]”jÀ]”Œopensuse”ajÂ]”Œrefuri”j±«ujÄjdj Kj¶jU«ubj±ŒØ operating systems. Install the prerequisite programs, including any dependencies and others that we have found to be missing in the core distribution but must be installed, i.e. (requires administrative privileges):”…””}”(j¶jU«jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK-j¶jD«jÇjn©ubj)”}”(j¦ŒD$ sudo zypper install gcc-fortran libX11-devel csh tcsh ftp hostname”j§]”j±ŒD$ sudo zypper install gcc-fortran libX11-devel csh tcsh ftp hostname”…””}”j¶jÉ«sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjš©jÆK0j¶jD«jÇjn©ubje)”}”(j¦Œ.. _qsg_macos:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ qsg-macos”ujÄjdjÆK9j¶jD«jÇjn©hjš©ubej·}”(j¹]”(Œrpm-based-linux”j8«ej»]”j½]”(Œrpm-based linux”Œqsg_rpm”ejÀ]”jÂ]”ujÄh_j¶j›©jÇjn©hjš©jÆK+jÒ }”jê«j.«sjÔ }”j8«j.«subj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒmacOS”j§]”j±ŒmacOS”…””}”(j¶jò«jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jï«jÇjn©hjš©jÆK8ubj`)”}”(j¦ŒÕmacOS (previously Mac OS X) requires the installation of Command Line Tools for Xcode, a Fortran compiler and XQuartz. The simplest way to install Command Line Tools for Xcode is to open a Terminal window and run:”j§]”j±ŒÕmacOS (previously Mac OS X) requires the installation of Command Line Tools for Xcode, a Fortran compiler and XQuartz. The simplest way to install Command Line Tools for Xcode is to open a Terminal window and run:”…””}”(j¶j¬jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK:j¶jï«jÇjn©ubj)”}”(j¦Œ$ xcode-select --install”j§]”j±Œ$ xcode-select --install”…””}”j¶j¬sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjš©jÆK=j¶jï«jÇjn©ubj`)”}”(j¦XÖThis will download and install core command line programs, including a C compiler, and any dependencies. A Fortran compiler is not included but you may install gfortran from a standard installer (:file:`.dmg`) file available from the `GCC Wiki web page `_. Install the X Windows libraries and headers with `XQuartz `_, which is available for download as a standard installer (:file:`.dmg`) file.”j§]”(j±ŒÄThis will download and install core command line programs, including a C compiler, and any dependencies. A Fortran compiler is not included but you may install gfortran from a standard installer (”…””}”(j¶j¬jÇjn©hNjÆNubj˜)”}”(j¦Œ :file:`.dmg`”j§]”j±Œ.dmg”…””}”(j¶j&¬jÇjn©hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¬ubj±Œ) file available from the ”…””}”(j¶j¬jÇjn©hNjÆNubj÷ )”}”(j¦ŒF`GCC Wiki web page `_”j§]”j±ŒGCC Wiki web page”…””}”(j¶j;¬jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGCC Wiki web page”j Œ/https://gcc.gnu.org/wiki/GFortranBinaries#MacOS”ujÄjö j¶j¬ubje)”}”(j¦Œ2 ”j§]”j·}”(j¹]”Œgcc-wiki-web-page”aj»]”j½]”Œgcc wiki web page”ajÀ]”jÂ]”Œrefuri”jK¬ujÄjdj Kj¶j¬ubj±Œ3. Install the X Windows libraries and headers with ”…””}”(j¶j¬jÇjn©hNjÆNubj÷ )”}”(j¦Œ%`XQuartz `_”j§]”j±ŒXQuartz”…””}”(j¶j]¬jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒXQuartz”j Œhttps://www.xquartz.org/”ujÄjö j¶j¬ubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œxquartz”aj»]”j½]”Œxquartz”ajÀ]”jÂ]”Œrefuri”jm¬ujÄjdj Kj¶j¬ubj±Œ;, which is available for download as a standard installer (”…””}”(j¶j¬jÇjn©hNjÆNubj˜)”}”(j¦Œ :file:`.dmg`”j§]”j±Œ.dmg”…””}”(j¶j¬jÇjn©hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¬ubj±Œ) file.”…””}”(j¶j¬jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKAj¶jï«jÇjn©ubje)”}”(j¦Œ.. _qsg_windows:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ qsg-windows”ujÄjdjÆKJj¶jï«jÇjn©hjš©ubej·}”(j¹]”(Œmacos”jã«ej»]”j½]”(Œmacos”Œ qsg_macos”ejÀ]”jÂ]”ujÄh_j¶j›©jÇjn©hjš©jÆK8jÒ }”j«¬jÙ«sjÔ }”jã«jÙ«subj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒWindows”j§]”j±ŒWindows”…””}”(j¶j³¬jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j°¬jÇjn©hjš©jÆKIubj`)”}”(j¦XžRecent releases of Windows 10 and above may install and run the `Windows Subsystem for Linux `_. See the `Microsoft Docs installation guide `_ for details. Once complete, install required packages following the instructions for Linux distributions, above, e.g. for :ref:`qsg_debian` if you install and use the `Ubuntu `_ or `Debian `_ package, or for :ref:`qsg_rpm` if you install and use the `openSUSE `_ package.”j§]”(j±Œ@Recent releases of Windows 10 and above may install and run the ”…””}”(j¶jÁ¬jÇjn©hNjÆNubj÷ )”}”(j¦ŒS`Windows Subsystem for Linux `_”j§]”j±ŒWindows Subsystem for Linux”…””}”(j¶jɬjÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒWindows Subsystem for Linux”j Œ2https://docs.microsoft.com/en-us/windows/wsl/about”ujÄjö j¶jÁ¬ubje)”}”(j¦Œ5 ”j§]”j·}”(j¹]”Œwindows-subsystem-for-linux”aj»]”j½]”Œwindows subsystem for linux”ajÀ]”jÂ]”Œrefuri”jÙ¬ujÄjdj Kj¶jÁ¬ubj±Œ . See the ”…””}”(j¶jÁ¬jÇjn©hNjÆNubj÷ )”}”(j¦Œa`Microsoft Docs installation guide `_”j§]”j±Œ!Microsoft Docs installation guide”…””}”(j¶jë¬jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ!Microsoft Docs installation guide”j Œ:https://docs.microsoft.com/en-us/windows/wsl/install-win10”ujÄjö j¶jÁ¬ubje)”}”(j¦Œ= ”j§]”j·}”(j¹]”Œ!microsoft-docs-installation-guide”aj»]”j½]”Œ!microsoft docs installation guide”ajÀ]”jÂ]”Œrefuri”jû¬ujÄjdj Kj¶jÁ¬ubj±Œ{ for details. Once complete, install required packages following the instructions for Linux distributions, above, e.g. for ”…””}”(j¶jÁ¬jÇjn©hNjÆNubj’)”}”(j¦Œ:ref:`qsg_debian`”j§]”j)”}”(j¦j­j§]”j±Œ qsg_debian”…””}”(j¶j­jÇjn©hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-ref”ej½]”jÀ]”jÂ]”ujÄj*j¶j ­ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jðŒ refdomain”j­Œreftype”Œref”Œ refexplicit”‰Œrefwarn”ˆj¶Œ qsg_debian”ujÄj‘hjš©jÆKKj¶jÁ¬ubj±Œ if you install and use the ”…””}”(j¶jÁ¬jÇjn©hNjÆNubj÷ )”}”(j¦Œ:`Ubuntu `_”j§]”j±ŒUbuntu”…””}”(j¶j1­jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒUbuntu”j Œ.https://apps.microsoft.com/detail/9pdxgncfsczv”ujÄjö j¶jÁ¬ubje)”}”(j¦Œ1 ”j§]”j·}”(j¹]”Œid1”aj»]”j½]”jÀ]”j«ajÂ]”Œrefuri”jA­ujÄjdj Kj¶jÁ¬ubj±Œ or ”…””}”(j¶jÁ¬jÇjn©hNjÆNubj÷ )”}”(j¦Œ:`Debian `_”j§]”j±ŒDebian”…””}”(j¶jR­jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒDebian”j Œ.https://apps.microsoft.com/detail/9msvkqc78pk6”ujÄjö j¶jÁ¬ubje)”}”(j¦Œ1 ”j§]”j·}”(j¹]”Œdebian”aj»]”j½]”Œdebian”ajÀ]”jÂ]”Œrefuri”jb­ujÄjdj Kj¶jÁ¬ubj±Œ package, or for ”…””}”(j¶jÁ¬jÇjn©hNjÆNubj’)”}”(j¦Œ:ref:`qsg_rpm`”j§]”j)”}”(j¦jv­j§]”j±Œqsg_rpm”…””}”(j¶jx­jÇjn©hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-ref”ej½]”jÀ]”jÂ]”ujÄj*j¶jt­ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jðŒ refdomain”j‚­Œreftype”Œref”Œ refexplicit”‰Œrefwarn”ˆj¶Œqsg_rpm”ujÄj‘hjš©jÆKKj¶jÁ¬ubj±Œ if you install and use the ”…””}”j¶jÁ¬sbj÷ )”}”(j¦Œ<`openSUSE `_”j§]”j±ŒopenSUSE”…””}”(j¶j˜­jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒopenSUSE”j Œ.https://apps.microsoft.com/detail/9mssk2zxxn11”ujÄjö j¶jÁ¬ubje)”}”(j¦Œ1 ”j§]”j·}”(j¹]”Œid2”aj»]”j½]”jÀ]”j¼«ajÂ]”Œrefuri”j¨­ujÄjdj Kj¶jÁ¬ubj±Œ package.”…””}”(j¶jÁ¬jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKKj¶j°¬jÇjn©ubj`)”}”(j¦XìOtherwise we recommend installing a virtual machine (e.g. `VirtualBox `_ or `VMWare Workstation Player `_), which requires the installation of a regular Linux distribution (e.g. `Ubuntu `_ to run via the virtual machine. GAMIT/GLOBK may then be installed and run on this virtual machine operating system, again following the instructions for the relevant Linux distribution, above.”j§]”(j±Œ:Otherwise we recommend installing a virtual machine (e.g. ”…””}”(j¶j¿­jÇjn©hNjÆNubj÷ )”}”(j¦Œ+`VirtualBox `_”j§]”j±Œ VirtualBox”…””}”(j¶jÇ­jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ VirtualBox”j Œhttps://www.virtualbox.org/”ujÄjö j¶j¿­ubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œ virtualbox”aj»]”j½]”Œ virtualbox”ajÀ]”jÂ]”Œrefuri”j×­ujÄjdj Kj¶j¿­ubj±Œ or ”…””}”(j¶j¿­jÇjn©hNjÆNubj÷ )”}”(j¦ŒG`VMWare Workstation Player `_”j§]”j±ŒVMWare Workstation Player”…””}”(j¶jé­jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒVMWare Workstation Player”j Œ(https://www.vmware.com/go/downloadplayer”ujÄjö j¶j¿­ubje)”}”(j¦Œ+ ”j§]”j·}”(j¹]”Œvmware-workstation-player”aj»]”j½]”Œvmware workstation player”ajÀ]”jÂ]”Œrefuri”jù­ujÄjdj Kj¶j¿­ubj±ŒI), which requires the installation of a regular Linux distribution (e.g. ”…””}”(j¶j¿­jÇjn©hNjÆNubj÷ )”}”(j¦Œ2`Ubuntu `_”•j§]”j±ŒUbuntu”…””}”(j¶j ®jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒUbuntu”j Œ&http://www.ubuntu.com/download/desktop”ujÄjö j¶j¿­ubje)”}”(j¦Œ) ”j§]”j·}”(j¹]”Œid3”aj»]”j½]”jÀ]”Œubuntu”ajÂ]”Œrefuri”j®ujÄjdj Kj¶j¿­ubj±ŒÁ to run via the virtual machine. GAMIT/GLOBK may then be installed and run on this virtual machine operating system, again following the instructions for the relevant Linux distribution, above.”…””}”(j¶j¿­jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKOj¶j°¬jÇjn©ubj`)”}”(j¦XdPreviously we had preferred to use `Cygwin `_, which is a Linux emulator for Windows, for installing and running GAMIT/GLOBK. To install Cygwin, download and run :download:`setup-x86.exe ` (for 32-bit computers) or :download:`setup-x86_64.exe ` (64-bit) to begin installation. Generally, the defaults shown throughout the installation process are adequate and need not be changed. There are, however, specific packages which are required in addition to the default Cygwin packages that are installed. These are at least:”j§]”(j±Œ#Previously we had preferred to use ”…””}”(j¶j3®jÇjn©hNjÆNubj÷ )”}”(j¦Œ`Cygwin `_”j§]”j±ŒCygwin”…””}”(j¶j;®jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒCygwin”j Œhttps://cygwin.com/”ujÄjö j¶j3®ubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œcygwin”aj»]”j½]”Œcygwin”ajÀ]”jÂ]”Œrefuri”jK®ujÄjdj Kj¶j3®ubj±Œu, which is a Linux emulator for Windows, for installing and running GAMIT/GLOBK. To install Cygwin, download and run ”…””}”(j¶j3®jÇjn©hNjÆNubj¡Œdownload_reference”“”)”}”(j¦Œ<:download:`setup-x86.exe `”j§]”j˜)”}”(j¦ja®j§]”j±Œ setup-x86.exe”…””}”(j¶jc®jÇjn©hNjÆNubaj·}”(j¹]”j»]”(j£Œdownload”ej½]”jÀ]”jÂ]”ujÄj—j¶j_®ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jðŒ refdomain”hoŒreftype”jm®Œ refexplicit”ˆŒrefwarn”‰j¶Œ https://cygwin.com/setup-x86.exe”j j|®ujÄj]®hjš©jÆKRj¶j3®ubj±Œ (for 32-bit computers) or ”…””}”(j¶j3®jÇjn©hNjÆNubj^®)”}”(j¦ŒB:download:`setup-x86_64.exe `”j§]”j˜)”}”(j¦jƒ®j§]”j±Œsetup-x86_64.exe”…””}”(j¶j…®jÇjn©hNjÆNubaj·}”(j¹]”j»]”(j£Œdownload”ej½]”jÀ]”jÂ]”ujÄj—j¶j®ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jðŒ refdomain”hoŒreftype”j®Œ refexplicit”ˆŒrefwarn”‰j¶Œ#https://cygwin.com/setup-x86_64.exe”j jž®ujÄj]®hjš©jÆKRj¶j3®ubj±X (64-bit) to begin installation. Generally, the defaults shown throughout the installation process are adequate and need not be changed. There are, however, specific packages which are required in addition to the default Cygwin packages that are installed. These are at least:”…””}”(j¶j3®jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKRj¶j°¬jÇjn©ubj“)”}”(j¦hoj§]”(j˜)”}”(j¦Œ“Devel/gcc-fortran (allowing the required dependencies to be installed will ensure the GCC core packages are also installed, including a C compiler)”j§]”j`)”}”(j¦j®®j§]”j±Œ“Devel/gcc-fortran (allowing the required dependencies to be installed will ensure the GCC core packages are also installed, including a C compiler)”…””}”(j¶j°®jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKXj¶j¬®ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j©®jÇjn©hjš©jÆNubj˜)”}”(j¦Œ Devel/make”j§]”j`)”}”(j¦jÅ®j§]”j±Œ Devel/make”…””}”(j¶jÇ®jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKYj¶jîubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j©®jÇjn©hjš©jÆNubj˜)”}”(j¦ŒMath/bc”j§]”j`)”}”(j¦jÜ®j§]”j±ŒMath/bc”…””}”(j¶jÞ®jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKZj¶jÚ®ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j©®jÇjn©hjš©jÆNubj˜)”}”(j¦Œ Shells/tcsh”j§]”j`)”}”(j¦jó®j§]”j±Œ Shells/tcsh”…””}”(j¶jõ®jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK[j¶jñ®ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j©®jÇjn©hjš©jÆNubj˜)”}”(j¦ŒX11/libX11-devel ”j§]”j`)”}”(j¦ŒX11/libX11-devel”j§]”j±ŒX11/libX11-devel”…””}”(j¶j ¯jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK\j¶j¯ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j©®jÇjn©hjš©jÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hjš©jÆKXj¶j°¬jÇjn©ubj`)”}”(j¦X;(One may search for the appropriate packages from the `Cygwin package search `_. Search for "libX11.*" and "Xlib.h" for the X11 libraries and header file, respectively, to find the appropriate package.) We also highly recommend installing the :file:`X11/xinit` package and its dependencies. This will provide an X Windows environment from which one can open and use, for example, Emacs for creating or editing text files. This is important given the different end-of-line characters between Windows and other systems (Unix, Linux and macOS).”j§]”(j±Œ6(One may search for the appropriate packages from the ”…””}”(j¶j&¯jÇjn©hNjÆNubj÷ )”}”(j¦Œ7`Cygwin package search `_”j§]”j±ŒCygwin package search”…””}”(j¶j.¯jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒCygwin package search”j Œhttps://cygwin.com/packages/”ujÄjö j¶j&¯ubje)”}”(j¦Œ ”j§]”j·}”(j¹]”Œcygwin-package-search”aj»]”j½]”Œcygwin package search”ajÀ]”jÂ]”Œrefuri”j>¯ujÄjdj Kj¶j&¯ubj±Œ¬. Search for “libX11.*†and “Xlib.h†for the X11 libraries and header file, respectively, to find the appropriate package.) We also highly recommend installing the ”…””}”(j¶j&¯jÇjn©hNjÆNubj˜)”}”(j¦Œ:file:`X11/xinit`”j§]”j±Œ X11/xinit”…””}”(j¶jP¯jÇjn©hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&¯ubj±X package and its dependencies. This will provide an X Windows environment from which one can open and use, for example, Emacs for creating or editing text files. This is important given the different end-of-line characters between Windows and other systems (Unix, Linux and macOS).”…””}”(j¶j&¯jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK^j¶j°¬jÇjn©ubje)”}”(j¦Œ.. _qsg_dc_access:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ qsg-dc-access”ujÄjdjÆKij¶j°¬jÇjn©hjš©ubej·}”(j¹]”(Œwindows”j¤¬ej»]”j½]”(Œwindows”Œ qsg_windows”ejÀ]”jÂ]”ujÄh_j¶j›©jÇjn©hjš©jÆKIjÒ }”j|¯jš¬sjÔ }”j¤¬jš¬subj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒOAccess to the CDDIS, EarthScope (Formerly UNAVCO) and SOPAC Global Data Centers”j§]”j±ŒOAccess to the CDDIS, EarthScope (Formerly UNAVCO) and SOPAC Global Data Centers”…””}”(j¶j„¯jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j¯jÇjn©hjš©jÆKhubj`)”}”(j¦X3Access to the CDDIS global data server via anonymous FTP was discontinued after 31 October 2020. CDDIS now needs to be accessed via authenticated secure HTTP or anonymous secure FTP. Several of our scripts which download data for use during GNSS data processing have been updated to accommodate this change.”j§]”j±X3Access to the CDDIS global data server via anonymous FTP was discontinued after 31 October 2020. CDDIS now needs to be accessed via authenticated secure HTTP or anonymous secure FTP. Several of our scripts which download data for use during GNSS data processing have been updated to accommodate this change.”…””}”(j¶j’¯jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKjj¶j¯jÇjn©ubj`)”}”(j¦X$We recommend you register to use authenticated secure HTTP by creating a NASA Earthdata account at https://urs.earthdata.nasa.gov/. Then you must include this information in a :file:`.netrc` file (note the dot at the beginning of the file name) in your home directory with the following line:”j§]”(j±ŒcWe recommend you register to use authenticated secure HTTP by creating a NASA Earthdata account at ”…””}”(j¶j ¯jÇjn©hNjÆNubj÷ )”}”(j¦Œhttps://urs.earthdata.nasa.gov/”j§]”j±Œhttps://urs.earthdata.nasa.gov/”…””}”(j¶j¨¯jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jª¯ujÄjö j¶j ¯ubj±Œ.. Then you must include this information in a ”…””}”(j¶j ¯jÇjn©hNjÆNubj˜)”}”(j¦Œ:file:`.netrc`”j§]”j±Œ.netrc”…””}”(j¶j»¯jÇjn©hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ¯ubj±Œf file (note the dot at the beginning of the file name) in your home directory with the following line:”…””}”(j¶j ¯jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKnj¶j¯jÇjn©ubj)”}”(j¦ŒCmachine urs.earthdata.nasa.gov login password ”j§]”j±ŒCmachine urs.earthdata.nasa.gov login password ”…””}”j¶jÖ¯sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjš©jÆKqj¶j¯jÇjn©ubj`)”}”(j¦Xéwhere :content:`` is replaced by your Earthdata username and :content:`` is replaced by your Earthdata password. (Do not use quotation marks or brackets around your :content:`` or :content:`` in this line in :file:`.netrc`.) If you do not wish to create an Earthdata account, you may still access the CDDIS archive via anonymous secure FTP but this requires your system to have :command:`curl` version ≥ 7.11.0 or :command:`wget` version ≥ 1.18.”j§]”(j±Œwhere ”…””}”(j¶jæ¯jÇjn©hNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ ”…””}”(j¶jî¯jÇjn©hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jæ¯ubj±Œ, is replaced by your Earthdata username and ”…””}”(j¶jæ¯jÇjn©hNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ ”…””}”(j¶j°jÇjn©hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jæ¯ubj±Œ] is replaced by your Earthdata password. (Do not use quotation marks or brackets around your ”…””}”(j¶jæ¯jÇjn©hNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ ”…””}”(j¶j°jÇjn©hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jæ¯ubj±Œ or ”…””}”(j¶jæ¯jÇjn©hNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ ”…””}”(j¶j'°jÇjn©hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jæ¯ubj±Œ in this line in ”…””}”(j¶jæ¯jÇjn©hNjÆNubj˜)”}”(j¦Œ:file:`.netrc`”j§]”j±Œ.netrc”…””}”(j¶j:°jÇjn©hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæ¯ubj±Œœ.) If you do not wish to create an Earthdata account, you may still access the CDDIS archive via anonymous secure FTP but this requires your system to have ”…””}”(j¶jæ¯jÇjn©hNjÆNubjj)”}”(j¦Œ:command:`curl`”j§]”j±Œcurl”…””}”(j¶jO°jÇjn©hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jæ¯ubj±Œ version ≥ 7.11.0 or ”…””}”(j¶jæ¯jÇjn©hNjÆNubjj)”}”(j¦Œ:command:`wget`”j§]”j±Œwget”…””}”(j¶ja°jÇjn©hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jæ¯ubj±Œ version ≥ 1.18.”…””}”(j¶jæ¯jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKuj¶j¯jÇjn©ubj`)”}”(j¦Œ¶We also recommend adding a similar line in a :file:`.netrc` file in your home directory to provide the CDDIS secure FTP server and the SOPAC server with the information they request:”j§]”(j±Œ-We also recommend adding a similar line in a ”…””}”(j¶jy°jÇjn©hNjÆNubj˜)”}”(j¦Œ:file:`.netrc`”j§]”j±Œ.netrc”…””}”(j¶j°jÇjn©hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jy°ubj±Œ{ file in your home directory to provide the CDDIS secure FTP server and the SOPAC server with the information they request:”…””}”(j¶jy°jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKyj¶j¯jÇjn©ubj)”}”(j¦Œ{machine gdc.cddis.eosdis.nasa.gov login anonymous password machine garner.ucsd.edu login anonymous password ”j§]”j±Œ{machine gdc.cddis.eosdis.nasa.gov login anonymous password machine garner.ucsd.edu login anonymous password ”…””}”j¶jœ°sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒtext”j(}”ujÄjhjš©jÆK{j¶j¯jÇjn©ubj`)”}”(j¦Œrwhere :content:`` is replaced by your email address (again, without quotation marks or brackets around it).”j§]”(j±Œwhere ”…””}”(j¶j¬°jÇjn©hNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ”…””}”(j¶j´°jÇjn©hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¬°ubj±ŒZ is replaced by your email address (again, without quotation marks or brackets around it).”…””}”(j¶j¬°jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK€j¶j¯jÇjn©ubj`)”}”(j¦X‡We recommend installing the `EarthScope Command Line Interface (CLI) `_ to download data and products from EarthScope (formerly UNAVCO). You must have Python version 3.7 or above available on your operating system. We suggest installing the EarthScope CLI in a virtual environment in a hidden directory, e.g. :file:`.earthscope-cli`, in your home directory and adding :file:`$HOME/.earthscope-cli/bin` to your :envvar:`PATH` environment variable or linking the :program:`es` program to a directory you already have in your :envvar:`PATH`, e.g. :file:`~/gg/com/`, so GAMIT/GLOBK may run it, e.g.”j§]”(j±ŒWe recommend installing the ”…””}”(j¶jÍ°jÇjn©hNjÆNubj÷ )”}”(j¦Œ``EarthScope Command Line Interface (CLI) `_”j§]”j±Œ'EarthScope Command Line Interface (CLI)”…””}”(j¶jÕ°jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ'EarthScope Command Line Interface (CLI)”j Œ3https://gitlab.com/earthscope/public/earthscope-cli”ujÄjö j¶jÍ°ubje)”}”(j¦Œ6 ”j§]”j·}”(j¹]”Œ%earthscope-command-line-interface-cli”aj»]”j½]”Œ'earthscope command line interface (cli)”ajÀ]”jÂ]”Œrefuri”jå°ujÄjdj Kj¶jÍ°ubj±Œî to download data and products from EarthScope (formerly UNAVCO). You must have Python version 3.7 or above available on your operating system. We suggest installing the EarthScope CLI in a virtual environment in a hidden directory, e.g. ”…””}”(j¶jÍ°jÇjn©hNjÆNubj˜)”}”(j¦Œ:file:`.earthscope-cli`”j§]”j±Œ.earthscope-cli”…””}”(j¶j÷°jÇjn©hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÍ°ubj±Œ$, in your home directory and adding ”…””}”(j¶jÍ°jÇjn©hNjÆNubj˜)”}”(j¦Œ!:file:`$HOME/.earthscope-cli/bin`”j§]”j±Œ$HOME/.earthscope-cli/bin”…””}”(j¶j ±jÇjn©hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÍ°ubj±Œ to your ”…””}”(j¶jÍ°jÇjn©hNjÆNubj¡h‰“”)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jü]”((Œsingle”ŒPATH”Œindex-0”hoNt”(j,±Œenvironment variable; PATH”j.±hoNt”eujÄh‰j¶jÍ°ubje)”}”(j¦hoj§]”j·}”(j¹]”j.±aj»]”j½]”jÀ]”jÂ]”ujÄjdj¶jÍ°ubj’)”}”(j¦Œ:envvar:`PATH`”j§]”j˜)”}”(j¦j=±j§]”j±ŒPATH”…””}”(j¶j?±jÇjn©hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-envvar”ej½]”jÀ]”jÂ]”ujÄj—j¶j;±ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jðŒ refdomain”jI±Œreftype”Œenvvar”Œ refexplicit”‰Œrefwarn”‰j¶j-±ujÄj‘hjš©jÆK‚j¶jÍ°ubj±Œ% environment variable or linking the ”…””}”(j¶jÍ°jÇjn©hNjÆNubjj)”}”(j¦Œ :program:`es`”j§]”j±Œes”…””}”(j¶j^±jÇjn©hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÍ°ubj±Œ1 program to a directory you already have in your ”…””}”(j¶jÍ°jÇjn©hNjÆNubj!±)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jü]”((j,±ŒPATH”Œindex-1”hoNt”(j,±Œenvironment variable; PATH”j{±hoNt”eujÄh‰j¶jÍ°ubje)”}”(j¦hoj§]”j·}”(j¹]”j{±aj»]”j½]”jÀ]”jÂ]”ujÄjdj¶jÍ°ubj’)”}”(j¦Œ:envvar:`PATH`”j§]”j˜)”}”(j¦jŠ±j§]”j±ŒPATH”…””}”(j¶jŒ±jÇjn©hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-envvar”ej½]”jÀ]”jÂ]”ujÄj—j¶jˆ±ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jðŒ refdomain”j–±Œreftype”Œenvvar”Œ refexplicit”‰Œrefwarn”‰j¶jz±ujÄj‘hjš©jÆK‚j¶jÍ°ubj±Œ, e.g. ”…””}”(j¶jÍ°jÇjn©hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/com/`”j§]”j±Œ ~/gg/com/”…””}”(j¶j«±jÇjn©hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÍ°ubj±Œ!, so GAMIT/GLOBK may run it, e.g.”…””}”(j¶jÍ°jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆK‚j¶j¯jÇjn©ubj)”}”(j¦Œ«$ cd ~ $ mkdir .earthscope-cli $ python3 -m venv .earthscope-cli $ . .earthscope-cli/bin/activate $ pip install earthscope-cli $ ln -s ~/.earthscope-cli/bin/es ~/gg/com/es”j§]”j±Œ«$ cd ~ $ mkdir .earthscope-cli $ python3 -m venv .earthscope-cli $ . .earthscope-cli/bin/activate $ pip install earthscope-cli $ ln -s ~/.earthscope-cli/bin/es ~/gg/com/es”…””}”j¶jƱsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjš©jÆK†j¶j¯jÇjn©ubj`)”}”(j¦XSee https://cddis.nasa.gov/Data_and_Derived_Products/CDDIS_Archive_Access.html (CDDIS), https://www.unavco.org/data/gps-gnss/file-server/file-server-access-examples.html (EarthScope, formerly UNAVCO) and http://garner.ucsd.edu/ (SOPAC) for more information.”j§]”(j±ŒSee ”…””}”(j¶jÖ±jÇjn©hNjÆNubj÷ )”}”(j¦ŒJhttps://cddis.nasa.gov/Data_and_Derived_Products/CDDIS_Archive_Access.html”j§]”j±ŒJhttps://cddis.nasa.gov/Data_and_Derived_Products/CDDIS_Archive_Access.html”…””}”(j¶jÞ±jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jà±ujÄjö j¶jÖ±ubj±Œ (CDDIS), ”…””}”(j¶jÖ±jÇjn©hNjÆNubj÷ )”}”(j¦ŒQhttps://www.unavco.org/data/gps-gnss/file-server/file-server-access-examples.html”j§]”j±ŒQhttps://www.unavco.org/data/gps-gnss/file-server/file-server-access-examples.html”…””}”(j¶jñ±jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jó±ujÄjö j¶jÖ±ubj±Œ# (EarthScope, formerly UNAVCO) and ”…””}”(j¶jÖ±jÇjn©hNjÆNubj÷ )”}”(j¦Œhttp://garner.ucsd.edu/”j§]”j±Œhttp://garner.ucsd.edu/”…””}”(j¶j²jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j²ujÄjö j¶jÖ±ubj±Œ (SOPAC) for more information.”…””}”(j¶jÖ±jÇjn©hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjš©jÆKj¶j¯jÇjn©ubej·}”(j¹]”(ŒLaccess-to-the-cddis-earthscope-formerly-unavco-and-sopac-global-data-centers”ju¯ej»]”j½]”(ŒOaccess to the cddis, earthscope (formerly unavco) and sopac global data centers”Œ qsg_dc_access”ejÀ]”jÂ]”ujÄh_j¶j›©jÇjn©hjš©jÆKhjÒ }”j#²jk¯sjÔ }”ju¯jk¯subej·}”(j¹]”(Œ prerequisites”j™©ej»]”j½]”(Œ prerequisites”Œ qsg_prereq”ejÀ]”jÂ]”ujÄh_j¶jn©jÇjn©hjš©jÆKjÒ }”j.²j©sjÔ }”j™©j©subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jš©j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjš©jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j}©jq©jŒ©j€©uj_}”(Œrel”j}©Œdate”jŒ©ujc}”je}”(j™©]”j©ajΪ]”jĪajÙª]”jϪaj8«]”j.«ajã«]”jÙ«aj¤¬]”jš¬aju¯]”jk¯aujg}”(j.²j™©j-²j*²j¶ªj³ªjÛªjΪj?«jÙªj>«j;«Œubuntu”Njê«j8«jé«jæ«jw«jt«j™«j–«Œopensuse”Nj«¬jã«jª¬j§¬jU¬jR¬jw¬jt¬j|¯j¤¬j{¯jx¯jã¬jà¬j­j­jl­ji­já­jÞ­j®j®jU®jR®jH¯jE¯j#²ju¯j"²j²jï°jì°uji}”(j.²ˆj-²‰j¶ªˆjÛªˆj?«ˆj>«‰jL²ˆj꫈j髉jw«ˆj™«ˆjM²ˆj«¬ˆjª¬‰jU¬ˆjw¬ˆj|¯ˆj{¯‰j㬈j­ˆjl­ˆjá­ˆj®ˆjU®ˆjH¯ˆj#²ˆj"²‰jï°ˆuj¹}”(j™©j›©j*²j›©j³ªj­ªjΪjݪjÙªjݪj;«jݪj «j«j8«jD«jæ«jD«jt«jn«j–«j«j¸«j²«jã«jï«j§¬jï«jR¬jL¬jt¬jn¬j¤¬j°¬jx¯j°¬jà¬jÚ¬j­jü¬jH­jB­ji­jc­j¯­j©­jÞ­jØ­j®jú­j"®j®jR®jL®jE¯j?¯ju¯j¯j²j¯jì°jæ°j.±j2±j{±j±ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”(jù )”}”(j¦hoj§]”j`)”}”(j¦Œ)Duplicate explicit target name: "ubuntu".”j§]”j±Œ-Duplicate explicit target name: “ubuntuâ€.”…””}”(j¶j_²jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j\²ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jH­aŒlevel”KŒtype”jŒsource”jš©Œline”KujÄjø j¶j°¬jÇjn©hjš©jÆKMubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ+Duplicate explicit target name: "opensuse".”j§]”j±Œ/Duplicate explicit target name: “opensuseâ€.”…””}”(j¶jz²jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jw²ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j¯­aŒlevel”KŒtype”jŒsource”jš©Œline”KujÄjø j¶j°¬jÇjn©hjš©jÆKMubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ)Duplicate explicit target name: "ubuntu".”j§]”j±Œ-Duplicate explicit target name: “ubuntuâ€.”…””}”(j¶j•²jÇjn©hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j’²ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j"®aŒlevel”KŒtype”jŒsource”jš©Œline”KujÄjø j¶j°¬jÇjn©hjš©jÆKPubej†]”(jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ0Hyperlink target "qsg-prereq" is not referenced.”…””}”j¶j±²sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j®²ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jš©Œline”KujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ/Hyperlink target "qsg-linux" is not referenced.”…””}”j¶j˲sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jȲubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jš©Œline”KujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ0Hyperlink target "qsg-debian" is not referenced.”…””}”j¶jå²sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jâ²ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jš©Œline”KujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ-Hyperlink target "qsg-rpm" is not referenced.”…””}”j¶jÿ²sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jü²ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jš©Œline”K,ujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ/Hyperlink target "qsg-macos" is not referenced.”…””}”j¶j³sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j³ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jš©Œline”K9ujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ1Hyperlink target "qsg-windows" is not referenced.”…””}”j¶j3³sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j0³ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jš©Œline”KJujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ3Hyperlink target "qsg-dc-access" is not referenced.”…””}”j¶jM³sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jJ³ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jš©Œline”KiujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ-Hyperlink target "index-0" is not referenced.”…””}”j¶jg³sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jd³ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jš©Œline”K‚ujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ-Hyperlink target "index-1" is not referenced.”…””}”j¶j³sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j~³ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jš©Œline”K‚ujÄjø ubejˆNj‰]”j‹NjÇjn©ubj÷j£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jœ³sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j™³jÇj™³ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j«³jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j™³jÇj™³ubj`)”}”(j¦Œ"Release Notes for GAMIT/GLOBK 10.5”j§]”j±Œ"Release Notes for GAMIT/GLOBK 10.5”…””}”(j¶jº³jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hŒ@/chandler/home/floyd/public_html/gg/docs/source/relnote/10.5.rst”jÆKj¶j™³jÇj™³ubj`)”}”(j¦Œ#Last updated by rwk 12 August 2014”j§]”j±Œ#Last updated by rwk 12 August 2014”…””}”(j¶jɳjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKj¶j™³jÇj™³ubj©Œ transition”“”)”}”(j¦ŒF----------------------------------------------------------------------”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj׳hjȳjÆKj¶j™³jÇj™³ubj`)”}”(j¦ŒŸRelease 10.41 consolidates incremental updates made since release 10.40 of November 2010 and adds several new features not included in the incremental updates.”j§]”j±ŒŸRelease 10.41 consolidates incremental updates made since release 10.40 of November 2010 and adds several new features not included in the incremental updates.”…””}”(j¶jã³jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKj¶j™³jÇj™³ubj`)”}”(j¦X-We have provided and will keep up-to-date, ITRF2008 coordinates sites in prior releases of the ITRF as well as new sites that have been and will be added for IGS processing. The primary file, in the ITRF2008 NNR frame is itrf08_comb.apr; and there are secondary files, itrf08_comb_[plate].apr, created by rotating this file to the frames of the major plates using the Euler poles estimated by Altamimi et al. [J. Geophys. Res., 117, B07402, doi:10.1029/2011JB008930,2012]. (Note that the plate-referenced files that we created 2012-01-06 and put into incremental_updates/tables were based on preliminary vectors that changed in the final publication, so users who downloaded these should replace them by the current files.) These files should always be used in conjunc- tion with the rename file itrf08_comb.eq to assure that the 8-character site name assigned to your data matches the coordinates for the appropri- ate period. See 'apr_and_eq_files.txt' in the download documentation directory for a complete explanation of how the combined files were constructed.”j§]”j±X1We have provided and will keep up-to-date, ITRF2008 coordinates sites in prior releases of the ITRF as well as new sites that have been and will be added for IGS processing. The primary file, in the ITRF2008 NNR frame is itrf08_comb.apr; and there are secondary files, itrf08_comb_[plate].apr, created by rotating this file to the frames of the major plates using the Euler poles estimated by Altamimi et al. [J. Geophys. Res., 117, B07402, doi:10.1029/2011JB008930,2012]. (Note that the plate-referenced files that we created 2012-01-06 and put into incremental_updates/tables were based on preliminary vectors that changed in the final publication, so users who downloaded these should replace them by the current files.) These files should always be used in conjunc- tion with the rename file itrf08_comb.eq to assure that the 8-character site name assigned to your data matches the coordinates for the appropri- ate period. See ‘apr_and_eq_files.txt’ in the download documentation directory for a complete explanation of how the combined files were constructed.”…””}”(j¶jñ³jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK j¶j™³jÇj™³ubj`)”}”(j¦X2There are improved templates in ~/gg/tables for GLOBK runs: globk_comb.cmd, glorg_comb.cmd, globk_long.cmd, glorg_long.cmd. These reflect current best practice and take advantage of the 'option' feature of the globk, glorg, and sh_glred command lines so that the same command file can be used for both repeatabilities and velocity solutions without editing the file itself. The standard southern California example has been reworked to use these file and should now be easier to execute and to use as a template for your own processing. Also, there is a new detailed recipe for processing and analyzing survey-mode (sGPS) measurements, 'sGPS_recipe.txt', to be found in the documents directory of the download site and also on the web as part of the presentations from the recent workshop held at UNAVCO (Boulder13).”j§]”j±X:There are improved templates in ~/gg/tables for GLOBK runs: globk_comb.cmd, glorg_comb.cmd, globk_long.cmd, glorg_long.cmd. These reflect current best practice and take advantage of the ‘option’ feature of the globk, glorg, and sh_glred command lines so that the same command file can be used for both repeatabilities and velocity solutions without editing the file itself. The standard southern California example has been reworked to use these file and should now be easier to execute and to use as a template for your own processing. Also, there is a new detailed recipe for processing and analyzing survey-mode (sGPS) measurements, ‘sGPS_recipe.txt’, to be found in the documents directory of the download site and also on the web as part of the presentations from the recent workshop held at UNAVCO (Boulder13).”…””}”(j¶jÿ³jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKj¶j™³jÇj™³ubj`)”}”(j¦XÀThe GPT/GMF models for zenith hydrostatic delay and mapping functions have been replaced by the new GPT2 model (Lager et al., Geophys. Res. Lett., ) which is based on a more refined numerical weather model, includes semi-annual as well as annual variations, has better spatial resolution, and accounts better for height differences through a seasonally dependent lapse rate. In the new model both the ZHD and mapping funtions are derived from a table, gpt.grid, automatically linked into the experiment and day directories from ~/gg/tables. If you specify GPT or GMT in your sestbl. and have gpt.grid in ~/gg/tables, you will automatically get GPT2 (the old GPT is invoked only if gpt.grid is missing).”j§]”j±XÀThe GPT/GMF models for zenith hydrostatic delay and mapping functions have been replaced by the new GPT2 model (Lager et al., Geophys. Res. Lett., ) which is based on a more refined numerical weather model, includes semi-annual as well as annual variations, has better spatial resolution, and accounts better for height differences through a seasonally dependent lapse rate. In the new model both the ZHD and mapping funtions are derived from a table, gpt.grid, automatically linked into the experiment and day directories from ~/gg/tables. If you specify GPT or GMT in your sestbl. and have gpt.grid in ~/gg/tables, you will automatically get GPT2 (the old GPT is invoked only if gpt.grid is missing).”…””}”(j¶j ´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK*j¶j™³jÇj™³ubj`)”}”(j¦XLGLOBK now has the ability to remove non-tidal atmospheric loading (ATML) based on the average of the day given in the h-file. Since GLOBK can not yet read an grid file to apply the ATML corrections directly, if you want to investigate their effects, the best strategy is to apply the ATML in GAMIT and then optionally retain or remove the corrections using the new command -appload_mod in the GLOBK commaand file. The preferred ATML files for GAMIT are those that have been filtered to remove sub-daily terms (atmfilt_cm.YYYY). In principle, the sub-daily thermal tides should be applied in GAMIT, but none of the current models, including a time-dependent recently developed by Ray and Ponte, has been shown to reproduce accurately the tidal loading, so the present recommendation of the IGS for the next reprocessing is to omit these terms.”j§]”j±XLGLOBK now has the ability to remove non-tidal atmospheric loading (ATML) based on the average of the day given in the h-file. Since GLOBK can not yet read an grid file to apply the ATML corrections directly, if you want to investigate their effects, the best strategy is to apply the ATML in GAMIT and then optionally retain or remove the corrections using the new command -appload_mod in the GLOBK commaand file. The preferred ATML files for GAMIT are those that have been filtered to remove sub-daily terms (atmfilt_cm.YYYY). In principle, the sub-daily thermal tides should be applied in GAMIT, but none of the current models, including a time-dependent recently developed by Ray and Ponte, has been shown to reproduce accurately the tidal loading, so the present recommendation of the IGS for the next reprocessing is to omit these terms.”…””}”(j¶j´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK5j¶j™³jÇj™³ubj`)”}”(j¦X@Liz Petrie of the University of Newcastle has coded a model in ARC for the accelerations on the GPS satellites due to antenna radiation and Earth radiation. These models are invoked by setting 'Earth radiation model = NCEL1', now default in the sestbl. and 'fixdrv'. As part of this modification, we have reworked many of the subroutines in ARC to be more modular, added (backward-compatible) models to the ARC batch file, and coded sh_get_orbits and sh_sp3fit to read the orbital models from from a sestbl. This latter change assures that the orbital models used for creating g- and t-files from sp3 files will be consistent with the models used for the data processing. For sh_gamit processsing, the sestbl. in ../tables is automatically linked into the /igs directory. If the sestbl is absent, hard-wired models will be used.”j§]”j±XHLiz Petrie of the University of Newcastle has coded a model in ARC for the accelerations on the GPS satellites due to antenna radiation and Earth radiation. These models are invoked by setting ‘Earth radiation model = NCEL1’, now default in the sestbl. and ‘fixdrv’. As part of this modification, we have reworked many of the subroutines in ARC to be more modular, added (backward-compatible) models to the ARC batch file, and coded sh_get_orbits and sh_sp3fit to read the orbital models from from a sestbl. This latter change assures that the orbital models used for creating g- and t-files from sp3 files will be consistent with the models used for the data processing. For sh_gamit processsing, the sestbl. in ../tables is automatically linked into the /igs directory. If the sestbl is absent, hard-wired models will be used.”…””}”(j¶j)´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKCj¶j™³jÇj™³ubj`)”}”(j¦X"Three model conventions have been updated to be consistent with those used by the IGS: mean pole and short-period EOP are changed from IERS 1996 to IERS 2010, and the gravity field from EGM96 to EGM08. These changes are important for EOP estimation but have neglible effect on positioning.”j§]”j±X"Three model conventions have been updated to be consistent with those used by the IGS: mean pole and short-period EOP are changed from IERS 1996 to IERS 2010, and the gravity field from EGM96 to EGM08. These changes are important for EOP estimation but have neglible effect on positioning.”…””}”(j¶j7´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKPj¶j™³jÇj™³ubj`)”}”(j¦XíA new script sh_plot_pos will read PBO-style pos files rather than _mb files for plotting time series. GLOBK now generates the 'PBO' lines in the print files automatically (no need to use PBOP in the print options). We have retained sh_plotcrd and the use of _mb files for this release, but they will eventually go away. The Python script ts_plot.py, introduced in Release 10.40 to read pos files will also be abandoned because it required too many non-standard Python libraries (see below).”j§]”j±XñA new script sh_plot_pos will read PBO-style pos files rather than _mb files for plotting time series. GLOBK now generates the ‘PBO’ lines in the print files automatically (no need to use PBOP in the print options). We have retained sh_plotcrd and the use of _mb files for this release, but they will eventually go away. The Python script ts_plot.py, introduced in Release 10.40 to read pos files will also be abandoned because it required too many non-standard Python libraries (see below).”…””}”(j¶jE´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKVj¶j™³jÇj™³ubj`)”}”(j¦XÕThe new script sh_plot_elmean, together with additions to the autcln summary files allow plotting of mean residuals over several days as a function of elevation angle or satellite nadir angle, providing more diagnostics for bad antenna models or tracking environments. These can be used instead of or in conjuction with the individual-day sky plots and phase vs elevation plots produced by sh_oneway from the autcln DPH files when '-pres ELEV' specified with sh_gamit.”j§]”j±XÙThe new script sh_plot_elmean, together with additions to the autcln summary files allow plotting of mean residuals over several days as a function of elevation angle or satellite nadir angle, providing more diagnostics for bad antenna models or tracking environments. These can be used instead of or in conjuction with the individual-day sky plots and phase vs elevation plots produced by sh_oneway from the autcln DPH files when ‘-pres ELEV’ specified with sh_gamit.”…””}”(j¶jS´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK^j¶j™³jÇj™³ubj`)”}”(j¦XmKeeping an up-to-date svnav.dat and antmod.dat file is <> to correct processing. Failure to do so will often impose the wrong radiation- pressure model, SV antenna offset, and yaw model on the satellite. We will notify users any time these files are changed, but regular checking of the incremental_updates/README file is advised. Changes since 10.40 are:”j§]”j±XmKeeping an up-to-date svnav.dat and antmod.dat file is <> to correct processing. Failure to do so will often impose the wrong radiation- pressure model, SV antenna offset, and yaw model on the satellite. We will notify users any time these files are changed, but regular checking of the incremental_updates/README file is advised. Changes since 10.40 are:”…””}”(j¶ja´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKfj¶j™³jÇj™³ubjFš)”}”(j¦Xœ- Launch of SV 35 (Blk IIA) as PRN 1 (date: 110606) - Reassignment of PRN 1 to newly launched SV63 (Blk IIF) (110718) - Reassignment of PRN 30 from SV 31 to SV 35 (both Block IIA (110816) - Update the maximum yaw rates for Block II and Block IIA satellites using the weighted average values determined by JPL 1996-2008 (110824) - Reassignment of PRN 24 from SV 24 (Blk IIA) to SV 49 (Blk IIR-M) - Reassignment of PRN 24 from SV 49 (Blk IIR-M) to SV 32 (120315) - Reassignment of PRN 24 from SV 32 (Blk IIR) to SV 37 (Blk IIA) (120426) - Reassignment of PRN 24 from SV 37 (Blk IIA) to SV 49 (Blk IIR-M) (120806) - Launch of SV 65 (Blk IIF), replacing SV 49 (Blk IIR-M) as PRN 24 (121008) - Reassignment of PRN 27 from SV 27 (Blk IIA) to SV 49 (Blk IIR-M) (121018) - Reassignment of PRN 30 from SV 35 (Blk IIA) to SV 49 (Blk IIR-M) (130510) - Reassignment of PRN 27 from SV 49 (Blk IIR-M) to SV 66 (Blk IIF) (130516) ”j§]”j“)”}”(j¦hoj§]”(j˜)”}”(j¦Œ1Launch of SV 35 (Blk IIA) as PRN 1 (date: 110606)”j§]”j`)”}”(j¦jx´j§]”j±Œ1Launch of SV 35 (Blk IIA) as PRN 1 (date: 110606)”…””}”(j¶jz´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKkj¶jv´ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦ŒAReassignment of PRN 1 to newly launched SV63 (Blk IIF) (110718)”j§]”j`)”}”(j¦j´j§]”j±ŒAReassignment of PRN 1 to newly launched SV63 (Blk IIF) (110718)”…””}”(j¶j‘´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKlj¶j´ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦ŒDReassignment of PRN 30 from SV 31 to SV 35 (both Block IIA (110816)”j§]”j`)”}”(j¦j¦´j§]”j±ŒDReassignment of PRN 30 from SV 31 to SV 35 (both Block IIA (110816)”…””}”(j¶j¨´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKmj¶j¤´ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦Œ‹Update the maximum yaw rates for Block II and Block IIA satellites using the weighted average values determined by JPL 1996-2008 (110824)”j§]”j e)”}”(j¦hoj§]”je)”}”(j¦Œ‰Update the maximum yaw rates for Block II and Block IIA satellites using the weighted average values determined by JPL 1996-2008 (110824)”j§]”(je)”}”(j¦ŒBUpdate the maximum yaw rates for Block II and Block IIA satellites”j§]”j±ŒBUpdate the maximum yaw rates for Block II and Block IIA satellites”…””}”(j¶jÆ´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆKnj¶j´ubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒFusing the weighted average values determined by JPL 1996-2008 (110824)”j§]”j±ŒFusing the weighted average values determined by JPL 1996-2008 (110824)”…””}”(j¶j×´jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKoj¶jÔ´ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j´ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆKnj¶j¿´ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶j»´ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦Œ@Reassignment of PRN 24 from SV 24 (Blk IIA) to SV 49 (Blk IIR-M)”j§]”j`)”}”(j¦jÿ´j§]”j±Œ@Reassignment of PRN 24 from SV 24 (Blk IIA) to SV 49 (Blk IIR-M)”…””}”(j¶jµjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKpj¶jý´ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦Œ?Reassignment of PRN 24 from SV 49 (Blk IIR-M) to SV 32 (120315)”j§]”j`)”}”(j¦jµj§]”j±Œ?Reassignment of PRN 24 from SV 49 (Blk IIR-M) to SV 32 (120315)”…””}”(j¶jµjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKqj¶jµubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦ŒGReassignment of PRN 24 from SV 32 (Blk IIR) to SV 37 (Blk IIA) (120426)”j§]”j`)”}”(j¦j-µj§]”j±ŒGReassignment of PRN 24 from SV 32 (Blk IIR) to SV 37 (Blk IIA) (120426)”…””}”(j¶j/µjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKrj¶j+µubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦ŒIReassignment of PRN 24 from SV 37 (Blk IIA) to SV 49 (Blk IIR-M) (120806)”j§]”j`)”}”(j¦jDµj§]”j±ŒIReassignment of PRN 24 from SV 37 (Blk IIA) to SV 49 (Blk IIR-M) (120806)”…””}”(j¶jFµjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKsj¶jBµubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦ŒILaunch of SV 65 (Blk IIF), replacing SV 49 (Blk IIR-M) as PRN 24 (121008)”j§]”j`)”}”(j¦j[µj§]”j±ŒILaunch of SV 65 (Blk IIF), replacing SV 49 (Blk IIR-M) as PRN 24 (121008)”…””}”(j¶j]µjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKtj¶jYµubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦ŒJReassignment of PRN 27 from SV 27 (Blk IIA) to SV 49 (Blk IIR-M) (121018)”j§]”j`)”}”(j¦jrµj§]”j±ŒJReassignment of PRN 27 from SV 27 (Blk IIA) to SV 49 (Blk IIR-M) (121018)”…””}”(j¶jtµjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKuj¶jpµubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦ŒIReassignment of PRN 30 from SV 35 (Blk IIA) to SV 49 (Blk IIR-M) (130510)”j§]”j`)”}”(j¦j‰µj§]”j±ŒIReassignment of PRN 30 from SV 35 (Blk IIA) to SV 49 (Blk IIR-M) (130510)”…””}”(j¶j‹µjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKvj¶j‡µubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubj˜)”}”(j¦ŒKReassignment of PRN 27 from SV 49 (Blk IIR-M) to SV 66 (Blk IIF) (130516) ”j§]”j`)”}”(j¦ŒIReassignment of PRN 27 from SV 49 (Blk IIR-M) to SV 66 (Blk IIF) (130516)”j§]”j±ŒIReassignment of PRN 27 from SV 49 (Blk IIR-M) to SV 66 (Blk IIF) (130516)”…””}”(j¶j¢µjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKwj¶jžµubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶js´ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåŒ-”ujÄj’hjȳjÆKkj¶jo´ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjEšhjȳjÆKkj¶j™³jÇj™³ubj`)”}”(j¦ŒOther changes and commments:”j§]”j±ŒOther changes and commments:”…””}”(j¶jõjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKzj¶j™³jÇj™³ubj`)”}”(j¦Œ** 10.41 vs 10.40”j§]”j±Œ** 10.41 vs 10.40”…””}”(j¶jѵjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK|j¶j™³jÇj™³ubj`)”}”(j¦XNew receivers: TRIMBLE NETR3, R7 GNSS, and SPS852 ; LEICA GG02PLUS, GS08PLUS, GS09, GS12, GR25, and GS25; NOV OEM6; Ashtech PF500 and PF800;, NAVCOM SF-3040 SF-3050; Topcon TPSGR5; JAVAD TR_VS; SEPT POLARX4, POLARX4TR, and POLARXS; SOK GSR2700 RSX; SOUTH S82T GNSS and S82V GNSS; STONEX S9II GNSS; IFEN NX_NTR_303_D, NX_NTR_500_D, NX_NTR_600_D, SX_NSR_RT_200, SX_NSR_RT_300, SX_NSR_RT_400, SX_NSR_RT_401, SX_NSR_RT_402, SX_NSR_RT_700, and SX_NSR_RT_800. RNG FASA+, ITT 3750300, GEOMAX Zenith10, GEOMAX Zenith20 receivrs”j§]”j±XNew receivers: TRIMBLE NETR3, R7 GNSS, and SPS852 ; LEICA GG02PLUS, GS08PLUS, GS09, GS12, GR25, and GS25; NOV OEM6; Ashtech PF500 and PF800;, NAVCOM SF-3040 SF-3050; Topcon TPSGR5; JAVAD TR_VS; SEPT POLARX4, POLARX4TR, and POLARXS; SOK GSR2700 RSX; SOUTH S82T GNSS and S82V GNSS; STONEX S9II GNSS; IFEN NX_NTR_303_D, NX_NTR_500_D, NX_NTR_600_D, SX_NSR_RT_200, SX_NSR_RT_300, SX_NSR_RT_400, SX_NSR_RT_401, SX_NSR_RT_402, SX_NSR_RT_700, and SX_NSR_RT_800. RNG FASA+, ITT 3750300, GEOMAX Zenith10, GEOMAX Zenith20 receivrs”…””}”(j¶jßµjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK~j¶j™³jÇj™³ubj`)”}”(j¦XNew antennas: TRM_R6, TRM_R8. TRM55970,TRM59900.00, TRM59900.00, and TRMAG25; NOV533 (compact), NOV702_2.02 and NOV702_3.00; ASH701023.A and ASH70123.L1; LEIGS08, LEIGS12, LEIGG02PLUS, and LEIGS08PLUS;, NavCom NAV_ANT3001BR (AT1675-20W); JAV_TRIUMPH-1, JAVTRIUMPH_VS, JNSCR_C146-22-1 and four JPSREGANT; TPSHIPER_II, TPSHIPER_II+10, TPS NET-G3A, and TPSGR5; SEPCHOKE_MC; Navxperience NAX3G+C; Stonex STHS82_7224V3.0 and STXS9SA7224V3.0; Altus APSAPS-3; Rusnavgeoset RNG80971.00; ITT3750323; GeoMax GMXZENITH10 and GMXZENITH20.”j§]”j±XNew antennas: TRM_R6, TRM_R8. TRM55970,TRM59900.00, TRM59900.00, and TRMAG25; NOV533 (compact), NOV702_2.02 and NOV702_3.00; ASH701023.A and ASH70123.L1; LEIGS08, LEIGS12, LEIGG02PLUS, and LEIGS08PLUS;, NavCom NAV_ANT3001BR (AT1675-20W); JAV_TRIUMPH-1, JAVTRIUMPH_VS, JNSCR_C146-22-1 and four JPSREGANT; TPSHIPER_II, TPSHIPER_II+10, TPS NET-G3A, and TPSGR5; SEPCHOKE_MC; Navxperience NAX3G+C; Stonex STHS82_7224V3.0 and STXS9SA7224V3.0; Altus APSAPS-3; Rusnavgeoset RNG80971.00; ITT3750323; GeoMax GMXZENITH10 and GMXZENITH20.”…””}”(j¶jíµjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK†j¶j™³jÇj™³ubj`)”}”(j¦ŒiCorrect the values in hi.dat used to convert slant height to direct height for the TPSHIPER_PLUS antenna.”j§]”j±ŒiCorrect the values in hi.dat used to convert slant height to direct height for the TPSHIPER_PLUS antenna.”…””}”(j¶jûµjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKŽj¶j™³jÇj™³ubj`)”}”(j¦Œ˜Fix typos in hi.dat entries for SEN14R, SENS49R, SENS96, SENS96, SEN96R, TPS721, TRSXDS, and TRSLDR antennas; add dimensions for Leica LEIAR25 antennas.”j§]”j±Œ˜Fix typos in hi.dat entries for SEN14R, SENS49R, SENS96, SENS96, SEN96R, TPS721, TRSXDS, and TRSLDR antennas; add dimensions for Leica LEIAR25 antennas.”…””}”(j¶j ¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK‘j¶j™³jÇj™³ubj`)”}”(j¦ŒVUpdated Makefile.config.new (to be renamed to Makefile.config) for new Linux releases.”j§]”j±ŒVUpdated Makefile.config.new (to be renamed to Makefile.config) for new Linux releases.”…””}”(j¶j¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK”j¶j™³jÇj™³ubj`)”}”(j¦ŒÈCreating an earthquake file: The script sh_makeeqdef has been updated to use hypercenter locations from the EHB bulletin (via ISC) up to the end of 2008, and from the standard ISC bulleint thereafter.”j§]”j±ŒÈCreating an earthquake file: The script sh_makeeqdef has been updated to use hypercenter locations from the EHB bulletin (via ISC) up to the end of 2008, and from the standard ISC bulleint thereafter.”…””}”(j¶j%¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK—j¶j™³jÇj™³ubj`)”}”(j¦Œ:Update sh_get_hfiles for changes in the SOPAC archive ftp.”j§]”j±Œ:Update sh_get_hfiles for changes in the SOPAC archive ftp.”…””}”(j¶j3¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK›j¶j™³jÇj™³ubj`)”}”(j¦Œ6Fix bug in reading more than 36 SVs from a RINEX file.”j§]”j±Œ6Fix bug in reading more than 36 SVs from a RINEX file.”…””}”(j¶jA¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKj¶j™³jÇj™³ubj`)”}”(j¦Œ.Fix the p-file and h-file printout for SP EOP.”j§]”j±Œ.Fix the p-file and h-file printout for SP EOP.”…””}”(j¶jO¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKŸj¶j™³jÇj™³ubj`)”}”(j¦ŒvUpdate sh_get_orbits to use repro1 orbits when down loading igsf from CDDIS. These orbits are available week 730-1459.”j§]”j±ŒvUpdate sh_get_orbits to use repro1 orbits when down loading igsf from CDDIS. These orbits are available week 730-1459.”…””}”(j¶j]¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK¡j¶j™³jÇj™³ubj`)”}”(j¦Œ=Updated grdtab to remove S1/S2 tides from non-filtered grids.”j§]”j±Œ=Updated grdtab to remove S1/S2 tides from non-filtered grids.”…””}”(j¶jk¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK¤j¶j™³jÇj™³ubj`)”}”(j¦Œ•Change mapping of ietide for h-files: mean-pole-tide removed is now bit 4 (8), rather than bit 5 (16). Other minor changes to 'solve'; see sversn.f.”j§]”j±Œ™Change mapping of ietide for h-files: mean-pole-tide removed is now bit 4 (8), rather than bit 5 (16). Other minor changes to ‘solve’; see sversn.f.”…””}”(j¶jy¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK¦j¶j™³jÇj™³ubj`)”}”(j¦ŒÆconvertc: Updates to check reasonableness, allow more file types, fix bug in reading vel file created by velrot with longer lines, and reverse the order from lat/lon to lon/lat for GEO or GEP files.”j§]”j±ŒÆconvertc: Updates to check reasonableness, allow more file types, fix bug in reading vel file created by velrot with longer lines, and reverse the order from lat/lon to lon/lat for GEO or GEP files.”…””}”(j¶j‡¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK©j¶j™³jÇj™³ubj`)”}”(j¦Œ+sh_get_nav, sh_get_orbits: Add wget option.”j§]”j±Œ+sh_get_nav, sh_get_orbits: Add wget option.”…””}”(j¶j•¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK­j¶j™³jÇj™³ubj`)”}”(j¦ŒŸsh_PBS_gamit: changed "mailto" variable to "mail_to because" of some conflict/problem returning blank argument to -M option in qsub command, which stalls qsub.”j§]”j±Œ§sh_PBS_gamit: changed “mailto†variable to “mail_to because†of some conflict/problem returning blank argument to -M option in qsub command, which stalls qsub.”…””}”(j¶j£¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK¯j¶j™³jÇj™³ubj`)”}”(j¦ŒFsh_eq: Removed from /com since made obsolete by eq option of sh_exglk.”j§]”j±ŒFsh_eq: Removed from /com since made obsolete by eq option of sh_exglk.”…””}”(j¶j±¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK²j¶j™³jÇj™³ubj`)”}”(j¦Œesh_metutil/metutil: Increase dimensions for z-file entries to allow 10-second sampling over 24 hours.”j§]”j±Œesh_metutil/metutil: Increase dimensions for z-file entries to allow 10-second sampling over 24 hours.”…””}”(j¶j¿¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK´j¶j™³jÇj™³ubj`)”}”(j¦Œ¾sh_gamit: Add '-alpha off' and '+antalias' to ImageMagic convert to avoid transparency and pixelation in converting sky plot images from Postscript to gif; change default aprf to itrf08.apr.”j§]”j±ŒÆsh_gamit: Add ‘-alpha off’ and ‘+antalias’ to ImageMagic convert to avoid transparency and pixelation in converting sky plot images from Postscript to gif; change default aprf to itrf08.apr.”…””}”(j¶jͶjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK·j¶j™³jÇj™³ubj`)”}”(j¦ŒRUpdated hfupd.f and hfupd_ut.f to find renamed sites in station.info for updating.”j§]”j±ŒRUpdated hfupd.f and hfupd_ut.f to find renamed sites in station.info for updating.”…””}”(j¶jÛ¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK»j¶j™³jÇj™³ubj`)”}”(j¦Œ5Updated template sestbl. to fix typo for 'Mag field'.”j§]”j±Œ9Updated template sestbl. to fix typo for ‘Mag field’.”…””}”(j¶jé¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆK¾j¶j™³jÇj™³ubj`)”}”(j¦Œ>Updated read_pmu_inp.f to account for GPS-UTC time difference.”j§]”j±Œ>Updated read_pmu_inp.f to account for GPS-UTC time difference.”…””}”(j¶j÷¶jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÀj¶j™³jÇj™³ubj`)”}”(j¦Œ-Fixed format "errors" in tsfit.f and tssum.f.”j§]”j±Œ1Fixed format “errors†in tsfit.f and tssum.f.”…””}”(j¶j·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÂj¶j™³jÇj™³ubj`)”}”(j¦Œ9Fix bug in computng average hydrological load for h-file.”j§]”j±Œ9Fix bug in computng average hydrological load for h-file.”…””}”(j¶j·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÄj¶j™³jÇj™³ubj`)”}”(j¦Œ!Added displace folder to updates.”j§]”j±Œ!Added displace folder to updates.”…””}”(j¶j!·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÆj¶j™³jÇj™³ubj`)”}”(j¦ŒLAllow by-passing uncompress when downloading RINEX files: /com/sh_get_rinex.”j§]”j±ŒLAllow by-passing uncompress when downloading RINEX files: /com/sh_get_rinex.”…””}”(j¶j/·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÈj¶j™³jÇj™³ubj`)”}”(j¦Œ»Fixed bug in grdtab reading OSO list files with slightly different formats; correct comments for order of tokens on the grdtab command line. Copy from gamit/grdtab: grdtab, get_otl_list.”j§]”j±Œ»Fixed bug in grdtab reading OSO list files with slightly different formats; correct comments for order of tokens on the grdtab command line. Copy from gamit/grdtab: grdtab, get_otl_list.”…””}”(j¶j=·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÊj¶j™³jÇj™³ubj`)”}”(j¦Œ9Added "GCR APTOL" warning to email summary from sh_gamit.”j§]”j±Œ=Added “GCR APTOL†warning to email summary from sh_gamit.”…””}”(j¶jK·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÎj¶j™³jÇj™³ubj`)”}”(j¦Œ«sh_get_orbits/sh_sp3fit/ngstot: GLONASS SVS can be can be present (but are ignored); add ESA finals (ESAF) as an orbit option; fix bug with SV id is blank rather than 'G'.”j§]”j±Œ¯sh_get_orbits/sh_sp3fit/ngstot: GLONASS SVS can be can be present (but are ignored); add ESA finals (ESAF) as an orbit option; fix bug with SV id is blank rather than ‘G’.”…””}”(j¶jY·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÐj¶j™³jÇj™³ubj`)”}”(j¦ŒÔsh_glred: add options to select the command file and to input a prefix string for the globk OPTION command; add ability to search for binary files with extent 'glb') (PBO, e.g.); fix problem with 'word too long'.”j§]”j±ŒÜsh_glred: add options to select the command file and to input a prefix string for the globk OPTION command; add ability to search for binary files with extent ‘glb’) (PBO, e.g.); fix problem with ‘word too long’.”…””}”(j¶jg·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÔj¶j™³jÇj™³ubj`)”}”(j¦Œ¸Changes to better handle CYGWIN installations. Copy com/unimake and libraries/Makefile.config.new (and rename to Makefile.config after checking for compatibility with local settings).”j§]”j±Œ¸Changes to better handle CYGWIN installations. Copy com/unimake and libraries/Makefile.config.new (and rename to Makefile.config after checking for compatibility with local settings).”…””}”(j¶ju·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKØj¶j™³jÇj™³ubj`)”}”(j¦ŒPUpdated sh_link_rinex and sh_PBS_gamit to use -expt option for links and copies.”j§]”j±ŒPUpdated sh_link_rinex and sh_PBS_gamit to use -expt option for links and copies.”…””}”(j¶jƒ·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÜj¶j™³jÇj™³ubj`)”}”(j¦ŒbUpdated sh_get_rinex to allow >1000 site downloads. Error with Word too long in original version.”j§]”j±ŒbUpdated sh_get_rinex to allow >1000 site downloads. Error with Word too long in original version.”…””}”(j¶j‘·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKßj¶j™³jÇj™³ubj`)”}”(j¦ŒˆUpdate globk/autcln to implement new features (see help files) and updated pole tide definitions. Makefile.generic in gen_util updated.”j§]”j±ŒˆUpdate globk/autcln to implement new features (see help files) and updated pole tide definitions. Makefile.generic in gen_util updated.”…””}”(j¶jŸ·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKâj¶j™³jÇj™³ubj`)”}”(j¦ŒŒNew script to compare a list of RINEX files with one or more station.info files to check for station.info.completeness, /com/sh_stinfo_list.”j§]”j±ŒŒNew script to compare a list of RINEX files with one or more station.info files to check for station.info.completeness, /com/sh_stinfo_list.”…””}”(j¶j­·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKåj¶j™³jÇj™³ubj`)”}”(j¦ŒlChanged the USNO ftp command in gg/tables/ftp_info to use passive transfer; necessary since 1 February 2012.”j§]”j±ŒlChanged the USNO ftp command in gg/tables/ftp_info to use passive transfer; necessary since 1 February 2012.”…””}”(j¶j»·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKèj¶j™³jÇj™³ubj`)”}”(j¦Œ‡Updated kf/ctogobs/proc_phsfin.f to output mean residuals by elevation in 1-deg bins. ELMEAN lines. Bins with no data list 99.9 values.”j§]”j±Œ‡Updated kf/ctogobs/proc_phsfin.f to output mean residuals by elevation in 1-deg bins. ELMEAN lines. Bins with no data list 99.9 values.”…””}”(j¶jÉ·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKëj¶j™³jÇj™³ubj`)”}”(j¦ŒEUpdated frame_to_fra.f with help option and plate to use the feature.”j§]”j±ŒEUpdated frame_to_fra.f with help option and plate to use the feature.”…””}”(j¶j×·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKîj¶j™³jÇj™³ubj`)”}”(j¦Œ`Allow automatic uncompressing of bzip2 files. Copy from com: sh_crx2rnx, sh_get_rinex, sh_gamit.”j§]”j±Œ`Allow automatic uncompressing of bzip2 files. Copy from com: sh_crx2rnx, sh_get_rinex, sh_gamit.”…””}”(j¶jå·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKðj¶j™³jÇj™³ubj`)”}”(j¦ŒIFix bug in getting the average atmospheric loading value into the h-file.”j§]”j±ŒIFix bug in getting the average atmospheric loading value into the h-file.”…””}”(j¶jó·jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKój¶j™³jÇj™³ubj`)”}”(j¦Œ;Update 'profile' utility to handle changed vel-file format.”j§]”j±Œ?Update ‘profile’ utility to handle changed vel-file format.”…””}”(j¶j¸jÇj™³•hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKõj¶j™³jÇj™³ubj`)”}”(j¦Œ Corrected "find" commands in install_software with trailing slashes to follow linked directories successfully when verifying or searching for libX11 and Xlib.h.”j§]”j±Œ¤Corrected “find†commands in install_software with trailing slashes to follow linked directories successfully when verifying or searching for libX11 and Xlib.h.”…””}”(j¶j¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKøj¶j™³jÇj™³ubj`)”}”(j¦Œ:Allow reading of ANTEX files with 0.5-degree grid spacing.”j§]”j±Œ:Allow reading of ANTEX files with 0.5-degree grid spacing.”…””}”(j¶j¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKûj¶j™³jÇj™³ubj`)”}”(j¦Œ5Allow processing from c-files to check model changes.”j§]”j±Œ5Allow processing from c-files to check model changes.”…””}”(j¶j+¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKýj¶j™³jÇj™³ubj`)”}”(j¦Œ†Read met values from a RINEX met file using free-format (work-around for improperly written RINEX v2 files). gamit/model/read_metrnx.”j§]”j±Œ†Read met values from a RINEX met file using free-format (work-around for improperly written RINEX v2 files). gamit/model/read_metrnx.”…””}”(j¶j9¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆKÿj¶j™³jÇj™³ubj`)”}”(j¦ŒOAdded NONE command file name feature to tsfit.f (in help but not implemented) .”j§]”j±ŒOAdded NONE command file name feature to tsfit.f (in help but not implemented) .”…””}”(j¶jG¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ\Change to model/read_metrnx.f to allow reading of mis-formatted RINEX met files from Matera.”j§]”j±Œ\Change to model/read_metrnx.f to allow reading of mis-formatted RINEX met files from Matera.”…””}”(j¶jU¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦X2TRACK: Added new relative humidity option to GPT; fixed bug in velocity apriori coordinates; updated help file; new script sh_track_to_kml; account for model differences between L1 and L2; fix bug in reading the last epoch of an IONEX file; trap better bad clocks and data; add support for C2 range data.”j§]”j±X2TRACK: Added new relative humidity option to GPT; fixed bug in velocity apriori coordinates; updated help file; new script sh_track_to_kml; account for model differences between L1 and L2; fix bug in reading the last epoch of an IONEX file; trap better bad clocks and data; add support for C2 range data.”…””}”(j¶jc¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒntrackRT: TRACK updates plus fixed timing problem with trackRT and BNC2.5; updated handle BNC 2.6 feed format.”j§]”j±ŒntrackRT: TRACK updates plus fixed timing problem with trackRT and BNC2.5; updated handle BNC 2.6 feed format.”…””}”(j¶jq¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM j¶j™³jÇj™³ubj`)”}”(j¦Œ¡Update DLAPACK routines to current versions to avoid a bug effective with gfortran 4.6 when run with optimization (now default unless -mno-align-double is sset).”j§]”j±Œ¡Update DLAPACK routines to current versions to avoid a bug effective with gfortran 4.6 when run with optimization (now default unless -mno-align-double is sset).”…””}”(j¶j¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ@Fix bug in kf/svpos/svdiff.f when more than 12-channels of data.”j§]”j±Œ@Fix bug in kf/svpos/svdiff.f when more than 12-channels of data.”…””}”(j¶j¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ¢sh_upd_stnfo/mtinf: Fix bug with in and out station.info files with rx files; fix -rxo option; increase dimensions to work with current SOPAC station.info files.”j§]”j±Œ¢sh_upd_stnfo/mtinf: Fix bug with in and out station.info files with rx files; fix -rxo option; increase dimensions to work with current SOPAC station.info files.”…””}”(j¶j›¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj e)”}”(j¦hoj§]”je)”}”(j¦Œ‘sh_setup: Change to copy in whatever is linked was station.info in ~/gg/tables, now nominally station.info.mit. Rename station.info.sopac.newfmt”j§]”(je)”}”(j¦ŒBsh_setup: Change to copy in whatever is linked was station.info in”j§]”j±ŒBsh_setup: Change to copy in whatever is linked was station.info in”…””}”(j¶j°¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆMj¶j¬¸ubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒN~/gg/tables, now nominally station.info.mit. Rename station.info.sopac.newfmt”j§]”j±ŒN~/gg/tables, now nominally station.info.mit. Rename station.info.sopac.newfmt”…””}”(j¶jÁ¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j¾¸ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j¬¸ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆMj¶j©¸ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶j™³jÇj™³hjȳjÆNubj`)”}”(j¦Œto station.info.sopac.”j§]”j±Œto station.info.sopac.”…””}”(j¶já¸jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œsh_makeeqdef: New script to create globk earthquake file from ”…””}”(j¶j‰¹jÇj™³hNjÆNubj÷ )”}”(j¦Œhttp://neic.usgs.gov/”j§]”j±Œhttp://neic.usgs.gov/”…””}”(j¶j‘¹jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j“¹ujÄjö j¶j‰¹ubj±Œ catalog.”…””}”(j¶j‰¹jÇj™³hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM6j¶j™³jÇj™³ubj`)”}”(j¦ŒTThe command 'reset' in the eq_file will reset all of the input site extents to _GPS.”j§]”j±ŒXThe command ‘reset’ in the eq_file will reset all of the input site extents to _GPS.”…””}”(j¶jª¹jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM9j¶j™³jÇj™³ubj`)”}”(j¦XAdded a white-noise process to the mar_scale command so that some process noise can be applied between to h-files at the same time, useful if they were generated with differeent scales, e.g., ITRF2005 for IGS repro1 and ITRF2008 for data processed using itrf08_comb.apr.”j§]”j±XAdded a white-noise process to the mar_scale command so that some process noise can be applied between to h-files at the same time, useful if they were generated with differeent scales, e.g., ITRF2005 for IGS repro1 and ITRF2008 for data processed using itrf08_comb.apr.”…””}”(j¶j¸¹jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM<j¶j™³jÇj™³ubj`)”}”(j¦Œ9Allow 'getrel' to work with newer GLOBK velocity formats.”j§]”j±Œ=Allow ‘getrel’ to work with newer GLOBK velocity formats.”…””}”(j¶jƹjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMAj¶j™³jÇj™³ubj`)”}”(j¦ŒuUpdated kf/utils/stinf_to_rename.f to handle current scheme of using only a 4-character ID for the initial site name.”j§]”j±ŒuUpdated kf/utils/stinf_to_rename.f to handle current scheme of using only a 4-character ID for the initial site name.”…””}”(j¶jÔ¹jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMCj¶j™³jÇj™³ubj`)”}”(j¦Œ;Fix serious bug in ARC affecting the SV yaw during eclipse.”j§]”j±Œ;Fix serious bug in ARC affecting the SV yaw during eclipse.”…””}”(j¶jâ¹jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMFj¶j™³jÇj™³ubj`)”}”(j¦ŒžFix bug in failing to use C2 when both C2 and P2 indicated with the RINEX header but P2 zero for SVs that have C2. Copy gamit/lib/rrinex.f. Kogan/King 110420”j§]”j±ŒžFix bug in failing to use C2 when both C2 and P2 indicated with the RINEX header but P2 zero for SVs that have C2. Copy gamit/lib/rrinex.f. Kogan/King 110420”…””}”(j¶jð¹jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMHj¶j™³jÇj™³ubj`)”}”(j¦XKFix bug in failure to apply center-of-mass correction (CMC) for ocean tide models when translating sp3 files to t-files; fix bug in writing MIT sp3 files. Add 'status' message for CMC corrections in both ngstot and ttongs. Copy from gamit/orbits: oversn.f, ngstot.f, rsp3hd.f, ttongs.f, wsp3hd.f, and sdtrit.f. Kogan/King 110414”j§]”j±XOFix bug in failure to apply center-of-mass correction (CMC) for ocean tide models when translating sp3 files to t-files; fix bug in writing MIT sp3 files. Add ‘status’ message for CMC corrections in both ngstot and ttongs. Copy from gamit/orbits: oversn.f, ngstot.f, rsp3hd.f, ttongs.f, wsp3hd.f, and sdtrit.f. Kogan/King 110414”…””}”(j¶jþ¹jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMLj¶j™³jÇj™³ubj`)”}”(j¦Œ-Fix bogus header in ANTEX file. King 110322”j§]”j±Œ-Fix bogus header in ANTEX file. King 110322”…””}”(j¶j ºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMRj¶j™³jÇj™³ubj`)”}”(j¦ŒûAllow use of IERS2010 model for short-period EOP (Ray model still default). Copy cversn.f, pmut1_oceans.f, and Makefile.generic from /libraries/comlib; lversn.f and srotat.f from gamit/lib; fversn.f and mdmake.f from gamit/fixdrv. Herring/King 110223”j§]”j±ŒûAllow use of IERS2010 model for short-period EOP (Ray model still default). Copy cversn.f, pmut1_oceans.f, and Makefile.generic from /libraries/comlib; lversn.f and srotat.f from gamit/lib; fversn.f and mdmake.f from gamit/fixdrv. Herring/King 110223”…””}”(j¶jºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMTj¶j™³jÇj™³ubj`)”}”(j¦ŒYFix htoglb bug in making ephemeris file (occurs only with Intel compiler). Herring 110202”j§]”j±ŒYFix htoglb bug in making ephemeris file (occurs only with Intel compiler). Herring 110202”…””}”(j¶j(ºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMXj¶j™³jÇj™³ubj`)”}”(j¦ŒTChange default setting in sh_plotvel to be compatible with GMT4. Ferhat/King 110119”j§]”j±ŒTChange default setting in sh_plotvel to be compatible with GMT4. Ferhat/King 110119”…””}”(j¶j6ºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMZj¶j™³jÇj™³ubj`)”}”(j¦ŒcFix problem with setting day-loop span in sh_gamit with some operating systems. Shimada/King 110117”j§]”j±ŒcFix problem with setting day-loop span in sh_gamit with some operating systems. Shimada/King 110117”…””}”(j¶jDºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM\j¶j™³jÇj™³ubj`)”}”(j¦X°Copy into /tables itrf08.apr, IGS08_101117.apr (current IGS) (from IGS08.ssc), and IGS08_101117.eq (GLOBK rename, from soln_IGS08.snx) files. The eq fiile has names matching those in both itrf08.apr and IGS08_101117.apr; note, however, that the IGS files may have discontinuities later than those accounted for in itrf08.apr, and that the IGS08 apr file will not include coordinates for early segments used in ITRF2008. King 110106”j§]”j±X°Copy into /tables itrf08.apr, IGS08_101117.apr (current IGS) (from IGS08.ssc), and IGS08_101117.eq (GLOBK rename, from soln_IGS08.snx) files. The eq fiile has names matching those in both itrf08.apr and IGS08_101117.apr; note, however, that the IGS files may have discontinuities later than those accounted for in itrf08.apr, and that the IGS08 apr file will not include coordinates for early segments used in ITRF2008. King 110106”…””}”(j¶jRºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM^j¶j™³jÇj™³ubj`)”}”(j¦Œ_Allow sh_find_data to work over a year boundary. Copy from /com. Shimada/McClusky/King 110106”j§]”j±Œ_Allow sh_find_data to work over a year boundary. Copy from /com. Shimada/McClusky/King 110106”…””}”(j¶j`ºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMej¶j™³jÇj™³ubj`)”}”(j¦Œ–Add the 2011 lunisolar tables to incremental_updates/tables/. (luntab and soltab were in the 10.4 distribution, but nutabl. was missing). King 110104”j§]”j±Œ–Add the 2011 lunisolar tables to incremental_updates/tables/. (luntab and soltab were in the 10.4 distribution, but nutabl. was missing). King 110104”…””}”(j¶jnºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMgj¶j™³jÇj™³ubj`)”}”(j¦ŒXRemove bogus test on t-file year > 2010. Copy gamit/fixdrv/armake.f. King 110101/110103”j§]”j±ŒXRemove bogus test on t-file year > 2010. Copy gamit/fixdrv/armake.f. King 110101/110103”…””}”(j¶j|ºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMjj¶j™³jÇj™³ubj`)”}”(j¦Œ/Allow more up to 20 observables in RINEX files.”j§]”j±Œ/Allow more up to 20 observables in RINEX files.”…””}”(j¶jŠºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMlj¶j™³jÇj™³ubj`)”}”(j¦Œ@Updated glist to output of sites by time all on one (long) line.”j§]”j±Œ@Updated glist to output of sites by time all on one (long) line.”…””}”(j¶j˜ºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMnj¶j™³jÇj™³ubj e)”}”(j¦hoj§]”je)”}”(j¦ŒŸUpdated treatment of coordinates in renames globk (fixed problem with XCL renames with earthquakes that have been previously applied). Khandler/eq_name_chng.f ”j§]”(je)”}”(j¦ŒbUpdated treatment of coordinates in renames globk (fixed problem with XCL renames with earthquakes”j§]”j±ŒbUpdated treatment of coordinates in renames globk (fixed problem with XCL renames with earthquakes”…””}”(j¶j­ºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆMqj¶j©ºubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ;that have been previously applied). Khandler/eq_name_chng.f”j§]”j±Œ;that have been previously applied). Khandler/eq_name_chng.f”…””}”(j¶j¾ºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMqj¶j»ºubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j©ºubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆMqj¶j¦ºubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶j™³jÇj™³hjȳjÆNubj`)”}”(j¦ŒNCorrect a bug in sh_gamit when linking IONEX files with multiple experiments.”j§]”j±ŒNCorrect a bug in sh_gamit when linking IONEX files with multiple experiments.”…””}”(j¶jÞºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMsj¶j™³jÇj™³ubj`)”}”(j¦ŒJAdd slant heights for the TRM39105.00 (Zephyr w/o ground plane) to hi.dat.”j§]”j±ŒJAdd slant heights for the TRM39105.00 (Zephyr w/o ground plane) to hi.dat.”…””}”(j¶jìºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMuj¶j™³jÇj™³ubj`)”}”(j¦ŒFCorrect the echo of the atmospheric tidal loading model in the p-file.”j§]”j±ŒFCorrect the echo of the atmospheric tidal loading model in the p-file.”…””}”(j¶júºjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMwj¶j™³jÇj™³ubj`)”}”(j¦Œ** 10.4 vs 10.35”j§]”j±Œ** 10.4 vs 10.35”…””}”(j¶j»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMzj¶j™³jÇj™³ubj`)”}”(j¦Œ‘Introduction of a real-time kinematic module, trackRT. See help/trackRT.hlp for a complete description including instructions for installation.”j§]”j±Œ‘Introduction of a real-time kinematic module, trackRT. See help/trackRT.hlp for a complete description including instructions for installation.”…””}”(j¶j»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM|j¶j™³jÇj™³ubj`)”}”(j¦XŽChanges to the code and svnav.dat to use an appropriate radiation-pressure model and antenna offset for Block IIF satellites (only PN 25 thus far). If you need to combine new processing with MIT or SOPAC global h-files that used the old models set ' apr_svs prn_12 100 100 100 10 10 10 0R ' to unlink the radiation pressure models. Both MIT and SOPAC will rerun these days to remove the problem.”j§]”j±X’Changes to the code and svnav.dat to use an appropriate radiation-pressure model and antenna offset for Block IIF satellites (only PN 25 thus far). If you need to combine new processing with MIT or SOPAC global h-files that used the old models set ‘ apr_svs prn_12 100 100 100 10 10 10 0R ‘ to unlink the radiation pressure models. Both MIT and SOPAC will rerun these days to remove the problem.”…””}”(j¶j$»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦X˜Two new programs, tscon and tsfit, are available for prototyping GLOBK solutions. They allow you to convert PBO, REASON, and other time series to GLOBK formats and to generate in an iterative but rapid fashion appropriate models for discontinuities and earthquakes in continuous time series prior to making long globk runs. See Chapter 4 of the GLOBK Reference Manual and the help files for tscon and tsfit.”j§]”j±X˜Two new programs, tscon and tsfit, are available for prototyping GLOBK solutions. They allow you to convert PBO, REASON, and other time series to GLOBK formats and to generate in an iterative but rapid fashion appropriate models for discontinuities and earthquakes in continuous time series prior to making long globk runs. See Chapter 4 of the GLOBK Reference Manual and the help files for tscon and tsfit.”…””}”(j¶j2»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM†j¶j™³jÇj™³ubj`)”}”(j¦Œ’There is a new example, better designed for instruction on setting up processing with new data and incorporating a multi-year solution with GLOBK.”j§]”j±Œ’There is a new example, better designed for instruction on setting up processing with new data and incorporating a multi-year solution with GLOBK.”…””}”(j¶j@»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMŒj¶j™³jÇj™³ubj`)”}”(j¦X8The c-file and h-file formats have changed. C-files from prior releases cannot be used, but the code remains compatible with older GAMIT (ascii) and GLOBK (binary) h-files. The impetus for this change was to better document models used in the processing, particularly for receiver and satellite antenna models.”j§]”j±X8The c-file and h-file formats have changed. C-files from prior releases cannot be used, but the code remains compatible with older GAMIT (ascii) and GLOBK (binary) h-files. The impetus for this change was to better document models used in the processing, particularly for receiver and satellite antenna models.”…””}”(j¶jN»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦X Higher-order ionospheric (HOI) corrections (2nd and 3rd order, but not bending) are available in GAMIT, as described by Petrie et al. [J. Geophys. Res., 115, B03417, doi:10.1029/2009jb006677, 2010]. Using these terms requires downloading daily IONEX files containing total electron content (TEC) at 2-hr intervals from CODE into the [expt]/ionex directory and linking these into the day directory using '-ion' in the sh_gamit command file. To apply the effects in processing, set 'Ion model = GMAP' and 'Mag field = ITRF11' in the sestbl. See the new Chapter 8 of the GAMIT Reference Manual for more details. Thanks to Liz Petrie of Newcastle U (UK) for most of the work on this, and to Andrzej Araszkiewicz the Military U of Technology (Poland) for important contributions.”j§]”j±XHigher-order ionospheric (HOI) corrections (2nd and 3rd order, but not bending) are available in GAMIT, as described by Petrie et al. [J. Geophys. Res., 115, B03417, doi:10.1029/2009jb006677, 2010]. Using these terms requires downloading daily IONEX files containing total electron content (TEC) at 2-hr intervals from CODE into the [expt]/ionex directory and linking these into the day directory using ‘-ion’ in the sh_gamit command file. To apply the effects in processing, set ‘Ion model = GMAP’ and ‘Mag field = ITRF11’ in the sestbl. See the new Chapter 8 of the GAMIT Reference Manual for more details. Thanks to Liz Petrie of Newcastle U (UK) for most of the work on this, and to Andrzej Araszkiewicz the Military U of Technology (Poland) for important contributions.”…””}”(j¶j\»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM•j¶j™³jÇj™³ubj`)”}”(j¦ŒñThe procedure for creating and keeping an updated station.info file has been better documented and enhanced by changes to sh_upd_stnfo. See the description on p. 27 of the Introduction to GAMIT/GLOBK manual, or the README of the new example.”j§]”j±ŒñThe procedure for creating and keeping an updated station.info file has been better documented and enhanced by changes to sh_upd_stnfo. See the description on p. 27 of the Introduction to GAMIT/GLOBK manual, or the README of the new example.”…””}”(j¶jj»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¡j¶j™³jÇj™³ubj`)”}”(j¦XuGLOBK will now accept multiple eq_files, allowing you to configure separate files for earthquakes, breaks, and editing (_XPS, XCL). If an eq_file entry uses the 'break' command rather than the 'rename' command, globk will assign the extent. A new RENM print option causes the full rename list to be output. glist now also allows for multiple eq_files, separated by colons.”j§]”j±X}GLOBK will now accept multiple eq_files, allowing you to configure separate files for earthquakes, breaks, and editing (_XPS, XCL). If an eq_file entry uses the ‘break’ command rather than the ‘rename’ command, globk will assign the extent. A new RENM print option causes the full rename list to be output. glist now also allows for multiple eq_files, separated by colons.”…””}”(j¶jx»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¦j¶j™³jÇj™³ubj`)”}”(j¦X9We are now providing in the GRIDS directory on everest.mit.edu atmospheric loading files that have been filtered to remove the diurnal and semi-diurnal thermal tides (S1, S2) using the procedure described by Tregoning and Watson (J. Geophys. Res., 14, B09403, doi:10.1029/2009JB006344, 2009). These can be used in conjunction with atl.grid (also on everest) comprising the IERS standard S1,S2 tides (Ponte and Ray, Geophys. Res. Lett.,29, 2153, doi:10.1029/ 2002GL016340, 2002) by renaming the filtered files (atmfilt_cm.YYYY) to the standard name for unfiltered files (atmdisp_cm.YYYY) in gg/tables, and setting 'Use atl.grid = Y' and 'Tides applied = 63' in the sestbl. Based on feedback from users, we hope to eventually discontinue distribution of the unfiltered grids. Note that earlier versions of the filtered files, from either ANU or MIT, were written incorrectly; further, there was a bug in the 'model' routine that read the sub-daily ATL from the u-file, causing the north and up components to be reversed. Any use of ATL should use the new grids and Release 10.4.”j§]”j±XEWe are now providing in the GRIDS directory on everest.mit.edu atmospheric loading files that have been filtered to remove the diurnal and semi-diurnal thermal tides (S1, S2) using the procedure described by Tregoning and Watson (J. Geophys. Res., 14, B09403, doi:10.1029/2009JB006344, 2009). These can be used in conjunction with atl.grid (also on everest) comprising the IERS standard S1,S2 tides (Ponte and Ray, Geophys. Res. Lett.,29, 2153, doi:10.1029/ 2002GL016340, 2002) by renaming the filtered files (atmfilt_cm.YYYY) to the standard name for unfiltered files (atmdisp_cm.YYYY) in gg/tables, and setting ‘Use atl.grid = Y’ and ‘Tides applied = 63’ in the sestbl. Based on feedback from users, we hope to eventually discontinue distribution of the unfiltered grids. Note that earlier versions of the filtered files, from either ANU or MIT, were written incorrectly; further, there was a bug in the ‘model’ routine that read the sub-daily ATL from the u-file, causing the north and up components to be reversed. Any use of ATL should use the new grids and Release 10.4.”…””}”(j¶j†»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¬j¶j™³jÇj™³ubj`)”}”(j¦XšThere is a new plotting script, ts_plot.py, that reads PBO-style time- series files (.pos), created by tscon or tssum, rather than the mb_-files created by ensum. We plan to transition to the .pos format eventually since it is more complete and flexible, but this will happen slowly and only when we're sure that users can easily install all of the libraries needed to run ts_plot.py: Python V2.7 ( http://www.python.org/download/ ); Numpy ( http://new.scipy.org/download.html ), optionally scipy; matplotlib ( http://sourceforge.net/projects/matplotlib/files/matplotlib/matplotlib-1.0/ ) and egenix-mx-base-3.1.3 ( http://www.egenix.com/products/python/mxBase/ ).”j§]”(j±Œ‡There is a new plotting script, ts_plot.py, that reads PBO-style time- series files (.pos), created by tscon or tssum, rather than the ”…””}”(j¶j”»jÇj™³hNjÆNubj©Œ problematic”“”)”}”(j¦Œmb_”j§]”j±Œmb_”…””}”j¶jž»sbaj·}”(j¹]”Œid2”aj»]”j½]”jÀ]”jÂ]”Œrefid”Œid1”ujÄjœ»j¶j”»jÇj™³hNjÆNubj±X -files created by ensum. We plan to transition to the .pos format eventually since it is more complete and flexible, but this will happen slowly and only when we’re sure that users can easily install all of the libraries needed to run ts_plot.py: Python V2.7 ( ”…””}”(j¶j”»jÇj™³hNjÆNubj÷ )”}”(j¦Œhttp://www.python.org/download/”j§]”j±Œhttp://www.python.org/download/”…””}”(j¶j³»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jµ»ujÄjö j¶j”»ubj±Œ ); Numpy ( ”…””}”(j¶j”»jÇj™³hNjÆNubj÷ )”}”(j¦Œ"http://new.scipy.org/download.html”j§]”j±Œ"http://new.scipy.org/download.html”…””}”(j¶jÆ»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jÈ»ujÄjö j¶j”»ubj±Œ# ), optionally scipy; matplotlib ( ”…””}”(j¶j”»jÇj™³hNjÆNubj÷ )”}”(j¦ŒKhttp://sourceforge.net/projects/matplotlib/files/matplotlib/matplotlib-1.0/”j§]”j±ŒKhttp://sourceforge.net/projects/matplotlib/files/matplotlib/matplotlib-1.0/”…””}”(j¶jÙ»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jÛ»ujÄjö j¶j”»ubj±Œ ) and egenix-mx-base-3.1.3 ( ”…””}”(j¶j”»jÇj™³hNjÆNubj÷ )”}”(j¦Œ-http://www.egenix.com/products/python/mxBase/”j§]”j±Œ-http://www.egenix.com/products/python/mxBase/”…””}”(j¶jì»jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jî»ujÄjö j¶j”»ubj±Œ ).”…””}”(j¶j”»jÇj™³hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM»j¶j™³jÇj™³ubj`)”}”(j¦Œ¦Changes to tsview to enhance performance when viewing and editing large numbers of time series; recording of the reasons for edits when creating entries for eq_files.”j§]”j±Œ¦Changes to tsview to enhance performance when viewing and editing large numbers of time series; recording of the reasons for edits when creating entries for eq_files.”…””}”(j¶j¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÅj¶j™³jÇj™³ubj`)”}”(j¦ŒÆThere are updates to autcln and solve to better handle single-frequency data. The default in autcln now requires the user to include 'L1only' in the autcln.cmd file to process single-frequency data.”j§]”j±ŒÊThere are updates to autcln and solve to better handle single-frequency data. The default in autcln now requires the user to include ‘L1only’ in the autcln.cmd file to process single-frequency data.”…””}”(j¶j¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÉj¶j™³jÇj™³ubj`)”}”(j¦X÷Pseudorange resolution of wide-lane ambiguities (LC_AUTCLN) is now recommended for networks larger than 50 km and data from January 1994 (except with codeless receivers), the date from which empirically determined differential code biases (DCB) for each SV have been determined (dcb.dat) by AIUB. A new algorithm, implemented for Release 10.34, is more robust than the earlier one and gives some weight to the ionsophere-constrained phase WL. The defaults controls should work well for most networks with recent data, but you may want to test increasing the 'ion constraint' value (from the default .01 to .02) under maximum ionspheric conditions (2000-2002), or decreasing the value (to .005) for old data under minimum ionospheric conditions (1994-1998).”j§]”j±XûPseudorange resolution of wide-lane ambiguities (LC_AUTCLN) is now recommended for networks larger than 50 km and data from January 1994 (except with codeless receivers), the date from which empirically determined differential code biases (DCB) for each SV have been determined (dcb.dat) by AIUB. A new algorithm, implemented for Release 10.34, is more robust than the earlier one and gives some weight to the ionsophere-constrained phase WL. The defaults controls should work well for most networks with recent data, but you may want to test increasing the ‘ion constraint’ value (from the default .01 to .02) under maximum ionspheric conditions (2000-2002), or decreasing the value (to .005) for old data under minimum ionospheric conditions (1994-1998).”…””}”(j¶j!¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÍj¶j™³jÇj™³ubj`)”}”(j¦X;There are now IGS RINEX files with as many as 11 obervables, requiring an update of the code (rrxhed and rrinex in gamit/lib) and remaking the executables with MAXOBT=11 in gamit/includes/makex.h. IGS ANTEX files begining with igs05_1499.atx have more comment lines than we originally coded (50). Set MAXTXT=1000 in gamit/includes/dimpar.h. and remake gamit. Prior to an October 2008 incremental update to 10.34, failure to make this change will result in a cryptic failure in suggesting a misnamed receiver or antenna. Release 10.4 will recognize ANTEX Version 1.4.”j§]”j±X;There are now IGS RINEX files with as many as 11 obervables, requiring an update of the code (rrxhed and rrinex in gamit/lib) and remaking the executables with MAXOBT=11 in gamit/includes/makex.h. IGS ANTEX files begining with igs05_1499.atx have more comment lines than we originally coded (50). Set MAXTXT=1000 in gamit/includes/dimpar.h. and remake gamit. Prior to an October 2008 incremental update to 10.34, failure to make this change will result in a cryptic failure in suggesting a misnamed receiver or antenna. Release 10.4 will recognize ANTEX Version 1.4.”…””}”(j¶j/¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMØj¶j™³jÇj™³ubj`)”}”(j¦Œ¾Fix a bug in time argument for GPT; affects the annual signal in heights at the level of 0.2-1.0 mm. Thanks to Francois Fund (ESGT) for catching this and Paul Tregoning (ANU) for testing it.”j§]”j±Œ¾Fix a bug in time argument for GPT; affects the annual signal in heights at the level of 0.2-1.0 mm. Thanks to Francois Fund (ESGT) for catching this and Paul Tregoning (ANU) for testing it.”…””}”(j¶j=¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMáj¶j™³jÇj™³ubj`)”}”(j¦X1Fix bugs and deficiencies in sh_upd_stnfo/mstinf to obtain a better match of entries with RINEX files and to avoid multiple entries continuous stations when not needed. Add the ability to get a station list from sites.defaults and/or the /rinex directory, and the ability to use wildcards to get multiple IGS log files. Fix bug in distinguishing between Receiver Type' and 'Receiver SN', and 'Antenna Type' and 'Antenna SN' in reading station.info files (thanks to Olivier Charade (INSU/CNRS), allow more complete updating of station.info entries mid-session.”j§]”j±X?Fix bugs and deficiencies in sh_upd_stnfo/mstinf to obtain a better match of entries with RINEX files and to avoid multiple entries continuous stations when not needed. Add the ability to get a station list from sites.defaults and/or the /rinex directory, and the ability to use wildcards to get multiple IGS log files. Fix bug in distinguishing between Receiver Type’ and ‘Receiver SN’, and ‘Antenna Type’ and ‘Antenna SN’ in reading station.info files (thanks to Olivier Charade (INSU/CNRS), allow more complete updating of station.info entries mid-session.”…””}”(j¶jK¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMåj¶j™³jÇj™³ubj`)”}”(j¦XLFix two bugs in fixdrv, both introduced in 10.35: 1) full-solution observable erroneously set when quick_pre observable = LC (allowed for backward compatibility) rather than LC_ONLY (preferred); 2) check on too-tight a priori coordinate constraints failed in sh_sigelv. Thanks to Liz Petrie (Newcastle) for catching both of these.”j§]”j±XLFix two bugs in fixdrv, both introduced in 10.35: 1) full-solution observable erroneously set when quick_pre observable = LC (allowed for backward compatibility) rather than LC_ONLY (preferred); 2) check on too-tight a priori coordinate constraints failed in sh_sigelv. Thanks to Liz Petrie (Newcastle) for catching both of these.”…””}”(j¶jY¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMîj¶j™³jÇj™³ubj`)”}”(j¦XFix bug in sh_get_nav when the day number has leading zeroes, needed for CDDIS downloads with tscsh (one line of code missed in fixes applied to most scripts for 10.35 release). Thanks to S Shimada of NIED for the catch and Mark Murray for additional cleanup.”j§]”j±XFix bug in sh_get_nav when the day number has leading zeroes, needed for CDDIS downloads with tscsh (one line of code missed in fixes applied to most scripts for 10.35 release). Thanks to S Shimada of NIED for the catch and Mark Murray for additional cleanup.”…””}”(j¶jg¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMôj¶j™³jÇj™³ubj`)”}”(j¦Œ™Fix bug in kf/glfor/get_max_glbd.f that resulted in wrong dimension for the partial derivative array when earthquakes logs and/or apr_rot commands used.”j§]”j±Œ™Fix bug in kf/glfor/get_max_glbd.f that resulted in wrong dimension for the partial derivative array when earthquakes logs and/or apr_rot commands used.”…””}”(j¶ju¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMùj¶j™³jÇj™³ubj`)”}”(j¦Œ:Updates to 'track' to account for millisecond range jumps.”j§]”j±Œ>Updates to ‘track’ to account for millisecond range jumps.”…””}”(j¶jƒ¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMýj¶j™³jÇj™³ubj`)”}”(j¦Œ±Fix bug in creating station.info entries with sh_upd_stnfo when the compiler option for floating point is not real*8. Thanks to Mark Murray (New Mexico Tech) for catching this.”j§]”j±Œ±Fix bug in creating station.info entries with sh_upd_stnfo when the compiler option for floating point is not real*8. Thanks to Mark Murray (New Mexico Tech) for catching this.”…””}”(j¶j‘¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÿj¶j™³jÇj™³ubj`)”}”(j¦ŒPFix bug in utility org2stab to get a stablization list from a velocity solution.”j§]”j±ŒPFix bug in utility org2stab to get a stablization list from a velocity solution.”…””}”(j¶jŸ¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ?Fix bug in sorting median process-noise values in sh_gen_stats.”j§]”j±Œ?Fix bug in sorting median process-noise values in sh_gen_stats.”…””}”(j¶j­¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒECorrect a bug in sh_update_eop after detecting an invalid EOP series.”j§]”j±ŒECorrect a bug in sh_update_eop after detecting an invalid EOP series.”…””}”(j¶j»¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ.Fix failure to link binary for utility ne2azel”j§]”j±Œ.Fix failure to link binary for utility ne2azel”…””}”(j¶jɼjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM j¶j™³jÇj™³ubj`)”}”(j¦Œ´Add gradients to the output file of sh_metutil; trap an empty z-file from having no good observations at a site. Copy gamit/utils/metutil. Thanks to Mark Murray (New Mexico Tech).”j§]”j±Œ´Add gradients to the output file of sh_metutil; trap an empty z-file from having no good observations at a site. Copy gamit/utils/metutil. Thanks to Mark Murray (New Mexico Tech).”…””}”(j¶j×¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM j¶j™³jÇj™³ubj`)”}”(j¦Œ•Modify sh_get_met to work with either Z or gz files, and for multiple days; update the met directories for CDDIS. Thanks to Kalev Rannat (Tallin U).”j§]”j±Œ•Modify sh_get_met to work with either Z or gz files, and for multiple days; update the met directories for CDDIS. Thanks to Kalev Rannat (Tallin U).”…””}”(j¶jå¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦X Add ~60 receivers and ~10 antennas to rcvant.dat. Update to current IGS ANTEX file (igs05_1597.atx) and create igs05_1597_plus.atx by adding PCV models from NGS for 8 antennas not in the IGS file. Correct misspellings or official changes for 6 receivers or antennas.”j§]”j±X Add ~60 receivers and ~10 antennas to rcvant.dat. Update to current IGS ANTEX file (igs05_1597.atx) and create igs05_1597_plus.atx by adding PCV models from NGS for 8 antennas not in the IGS file. Correct misspellings or official changes for 6 receivers or antennas.”…””}”(j¶jó¼jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ×Changes to unimake and Makefile.config to facilitate installation under CYGWIN. See the notes 'CYGWIN' under updates/documentation. Thanks to Semi Ergintav (TUBITAK) and George Vergos (AUTH) for notes and testing.”j§]”j±ŒÛChanges to unimake and Makefile.config to facilitate installation under CYGWIN. See the notes ‘CYGWIN’ under updates/documentation. Thanks to Semi Ergintav (TUBITAK) and George Vergos (AUTH) for notes and testing.”…””}”(j¶j½jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒôAdd to sh_gamit the ability to invoke sh_metutil to get ZWD and PW (met-file) from an input z-file and o-file, and to archive, compress, or delete z- and met-files at the end of the run. Add script sh_met2pbo to concatenate multiple met-files.”j§]”j±ŒôAdd to sh_gamit the ability to invoke sh_metutil to get ZWD and PW (met-file) from an input z-file and o-file, and to archive, compress, or delete z- and met-files at the end of the run. Add script sh_met2pbo to concatenate multiple met-files.”…””}”(j¶j½jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ5Fix header entries and format in writing SP3-C files.”j§]”j±Œ5Fix header entries and format in writing SP3-C files.”…””}”(j¶j½jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM!j¶j™³jÇj™³ubj`)”}”(j¦Œ¥Update Hatanaka RINEX compression routines to version 4.0.4, fixing function name conflict with getline in gcc 4.4 and cleaning handling of line-feed at end of file.”j§]”j±Œ¥Update Hatanaka RINEX compression routines to version 4.0.4, fixing function name conflict with getline in gcc 4.4 and cleaning handling of line-feed at end of file.”…””}”(j¶j+½jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM#j¶j™³jÇj™³ubj`)”}”(j¦Œ1Add output lines in Euler-pole utility conveuler.”j§]”j±Œ1Add output lines in Euler-pole utility conveuler.”…””}”(j¶j9½jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM'j¶j™³jÇj™³ubj`)”}”(j¦Œ_Modify format in utility confpol to convert N,E sigmas and correlations to confidence ellipses.”j§]”j±Œ_Modify format in utility confpol to convert N,E sigmas and correlations to confidence ellipses.”…””}”(j¶jG½jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM)j¶j™³jÇj™³ubj`)”}”(j¦ŒpNew utility check_siteid to compare 4-character IDs from glist and several external formats to detect conflicts.”j§]”j±ŒpNew utility check_siteid to compare 4-character IDs from glist and several external formats to detect conflicts.”…””}”(j¶jU½jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM,j¶j™³jÇj™³ubj`)”}”(j¦Œ 7 characters.”j§]”j±Œ5Fix bug in sh_org2vel when plate name > 7 characters.”…””}”(j¶jr¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMjj¶j™³jÇj™³ubj`)”}”(j¦Œ&Fix bug in sh_oneway for GMT formating”j§]”j±Œ&Fix bug in sh_oneway for GMT formating”…””}”(j¶j€¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMlj¶j™³jÇj™³ubj`)”}”(j¦Œ7Fix bug in creating x-files with Topcon firmware > 3.0.”j§]”j±Œ7Fix bug in creating x-files with Topcon firmware > 3.0.”…””}”(j¶jŽ¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMnj¶j™³jÇj™³ubj`)”}”(j¦ŒªFix bug in assignment of number of zenith or gradient parameters from an input interval (one too few in recent releases). Thanks to Ian Thomas of Newcastle for the catch.”j§]”j±ŒªFix bug in assignment of number of zenith or gradient parameters from an input interval (one too few in recent releases). Thanks to Ian Thomas of Newcastle for the catch.”…””}”(j¶jœ¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMpj¶j™³jÇj™³ubj`)”}”(j¦ŒhFix bug in sh_sp3fit, which incorrectly used IGS92 rather than EGM96 gravity field for the final t-file.”j§]”j±ŒhFix bug in sh_sp3fit, which incorrectly used IGS92 rather than EGM96 gravity field for the final t-file.”…””}”(j¶jª¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMtj¶j™³jÇj™³ubj`)”}”(j¦ŒŠNew 'fixdrv' option: Allow skipping of the loose solution ('skip loose = y') to avoid poorly conditioned matrix with very short baselines.”j§]”j±Œ’New ‘fixdrv’ option: Allow skipping of the loose solution (‘skip loose = y’) to avoid poorly conditioned matrix with very short baselines.”…””}”(j¶j¸¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMwj¶j™³jÇj™³ubj`)”}”(j¦ŒrAllow of VMF1 ZHD with GMF; works now if UFL first 'met source' option and either map.grid or map.list is present.”j§]”j±ŒvAllow of VMF1 ZHD with GMF; works now if UFL first ‘met source’ option and either map.grid or map.list is present.”…””}”(j¶jƾjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMzj¶j™³jÇj™³ubj`)”}”(j¦Œ:Fix bug in reading ANTEX files with more than 50 comments.”j§]”j±Œ:Fix bug in reading ANTEX files with more than 50 comments.”…””}”(j¶jÔ¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM}j¶j™³jÇj™³ubj`)”}”(j¦ŒÓThe command-line coordinate conversion program (a replacement for 'tform' in most cases) has been updated to output longitudes as either -180 to +180 or 0 to 360 and to fix a bug in outputting spherical l-files.”j§]”j±Œ×The command-line coordinate conversion program (a replacement for ‘tform’ in most cases) has been updated to output longitudes as either -180 to +180 or 0 to 360 and to fix a bug in outputting spherical l-files.”…””}”(j¶jâ¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒoAdd to sh_gamit summary the names of sites removed from processing by the minxf control in processing.defaults.”j§]”j±ŒoAdd to sh_gamit summary the names of sites removed from processing by the minxf control in processing.defaults.”…””}”(j¶jð¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMƒj¶j™³jÇj™³ubj`)”}”(j¦ŒªCleanup of 'solve': changes in the information written to the q-file by, remove some screen print; initialize 'avgload' variable; remove obsolete single-difference code.”j§]”j±Œ²Cleanup of ‘solve’: changes in the information written to the q-file by, remove some screen print; initialize ‘avgload’ variable; remove obsolete single-difference code.”…””}”(j¶jþ¾jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM†j¶j™³jÇj™³ubj`)”}”(j¦Œ6Add site code to error messages in reading ANTEX files”j§]”j±Œ6Add site code to error messages in reading ANTEX files”…””}”(j¶j ¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMŠj¶j™³jÇj™³ubj`)”}”(j¦Œ2Support 'gz' with Hatanaka-compressed RINEX files.”j§]”j±Œ6Support ‘gz’ with Hatanaka-compressed RINEX files.”…””}”(j¶j¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMŒj¶j™³jÇj™³ubj`)”}”(j¦Œ¯tables: Updates to svnav.dat and antmod.dat for SV49/PN01; it is essential to make this update for data acquired after the launch (March 2009). Add luni-solar tables for 2009.”j§]”j±Œ¯tables: Updates to svnav.dat and antmod.dat for SV49/PN01; it is essential to make this update for data acquired after the launch (March 2009). Add luni-solar tables for 2009.”…””}”(j¶j(¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMŽj¶j™³jÇj™³ubj`)”}”(j¦X|New receivers: NOV4G2 (NOV OEM4-G2), LC123G (LEICA GX1230GG), LC902G (LEICA GMX902GG), LC1220 (LEICA GX1220), SEPX2E (SEPT POLARX2E), SEPX2C (SEPT POLARX2C), SEPAX1 (SEPT ASTERX1) SEPAX2 (SEPT ASTERX2), ALTPS3 (ALTUS APS-3), LEICA GRX1200+, LEICA GRX1200+GNSS, LEICA GX1210, LEICA GX1210+, LEICA GX1220+, LEICA GX1230+, LEICA GX1220+GNSS, LEICA GX1230+GNSS, NOVV3R (NOV OEMV3-RT2)”j§]”j±X|New receivers: NOV4G2 (NOV OEM4-G2), LC123G (LEICA GX1230GG), LC902G (LEICA GMX902GG), LC1220 (LEICA GX1220), SEPX2E (SEPT POLARX2E), SEPX2C (SEPT POLARX2C), SEPAX1 (SEPT ASTERX1) SEPAX2 (SEPT ASTERX2), ALTPS3 (ALTUS APS-3), LEICA GRX1200+, LEICA GRX1200+GNSS, LEICA GX1210, LEICA GX1210+, LEICA GX1220+, LEICA GX1230+, LEICA GX1220+GNSS, LEICA GX1230+GNSS, NOVV3R (NOV OEMV3-RT2)”…””}”(j¶j6¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM’j¶j™³jÇj™³ubj`)”}”(j¦XNew Antennas: TPSG3A (TPSG3_A1),TR5980 (TRM59800.00), SOKGSR (SOK_GSR2700ISX), AER167 (AERAT1675_29, NOV702 (NOV702), LEICA AX1201, LEIAX1203+GNSS, LEIATX1230+GNSS, SEP220 (SEP_POLANT+), SEP29S (EP_POLANT+_GG), TRMZGS (TRM57971.00). Correct typos in TOP72110 and SOK_RADIAN_IS entries.”j§]”j±XNew Antennas: TPSG3A (TPSG3_A1),TR5980 (TRM59800.00), SOKGSR (SOK_GSR2700ISX), AER167 (AERAT1675_29, NOV702 (NOV702), LEICA AX1201, LEIAX1203+GNSS, LEIATX1230+GNSS, SEP220 (SEP_POLANT+), SEP29S (EP_POLANT+_GG), TRMZGS (TRM57971.00). Correct typos in TOP72110 and SOK_RADIAN_IS entries.”…””}”(j¶jD¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM™j¶j™³jÇj™³ubj`)”}”(j¦Œ** 10.34 vs 10.33”j§]”j±Œ** 10.34 vs 10.33”…””}”(j¶jR¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMŸj¶j™³jÇj™³ubj`)”}”(j¦Œ®sh_gamit (and sh_get_orbits) allow the use of IGS ultra-rapid orbits that include predictions, facilitating near-realtime generating of coordinates or atmospheric parameters.”j§]”j±Œ®sh_gamit (and sh_get_orbits) allow the use of IGS ultra-rapid orbits that include predictions, facilitating near-realtime generating of coordinates or atmospheric parameters.”…””}”(j¶j`¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¡j¶j™³jÇj™³ubj`)”}”(j¦XòFix a serious bug in 'model' whereby the pole tide, if requested, was returned as zero or undefined. The effect is up to 2 mm in horizontal and 5 mm in heights for a global solution, less than 1 mm horizontal for interstation differences up several thousand km. The problem is avoided if you omit the pole tide in GAMIT and set 'app_ptid all' in GLOBK. (You cannot simply set the control in GLOBK because GLOBK will not apply the tide if the h-file indicates that it has been applied in GAMIT.)”j§]”j±XúFix a serious bug in ‘model’ whereby the pole tide, if requested, was returned as zero or undefined. The effect is up to 2 mm in horizontal and 5 mm in heights for a global solution, less than 1 mm horizontal for interstation differences up several thousand km. The problem is avoided if you omit the pole tide in GAMIT and set ‘app_ptid all’ in GLOBK. (You cannot simply set the control in GLOBK because GLOBK will not apply the tide if the h-file indicates that it has been applied in GAMIT.)”…””}”(j¶jn¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¥j¶j™³jÇj™³ubj`)”}”(j¦XÎtables: Fix error in svnav.dat in setting start dates for PN29/SV57 and PN07/SV48, both erroneously set for 2007 10 20 instead of their actual launch dates. There is no problem with the PN29 error since the previous SV having this PN was dead by 2007 10 20 (day 293), but for PN07, using the old files will result in errors for the period between day 293 and the demise of the old PN07 on day 345. Thanks to Sigrun Hreinsdottir of U. Arizona for catching this.”j§]”j±XÎtables: Fix error in svnav.dat in setting start dates for PN29/SV57 and PN07/SV48, both erroneously set for 2007 10 20 instead of their actual launch dates. There is no problem with the PN29 error since the previous SV having this PN was dead by 2007 10 20 (day 293), but for PN07, using the old files will result in errors for the period between day 293 and the demise of the old PN07 on day 345. Thanks to Sigrun Hreinsdottir of U. Arizona for catching this.”…””}”(j¶j|¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¬j¶j™³jÇj™³ubj`)”}”(j¦Œ?Add percentage of ambiguities resolved to sh_gamit summary file”j§]”j±Œ?Add percentage of ambiguities resolved to sh_gamit summary file”…””}”(j¶jŠ¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM´j¶j™³jÇj™³ubj e)”}”(j¦hoj§]”(je)”}”(j¦ŒjNew receivers: SOK GSR2600, JPS EGGDT, SEPT POLARX2E, TPSHIPER_LITE TPS-HIPER-GGD (same as TPS HIPER-GD).”j§]”(je)”}”(j¦ŒDNew receivers: SOK GSR2600, JPS EGGDT, SEPT POLARX2E, TPSHIPER_LITE”j§]”j±ŒDNew receivers: SOK GSR2600, JPS EGGDT, SEPT POLARX2E, TPSHIPER_LITE”…””}”(j¶jŸ¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆM¶j¶j›¿ubj3e)”}”(j¦hoj§]”j`•)”}”(j¦Œ%TPS-HIPER-GGD (same as TPS HIPER-GD).”j§]”j±Œ%TPS-HIPER-GGD (same as TPS HIPER-GD).”…””}”(j¶j°¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM·j¶j­¿ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j›¿ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆM¶j¶j˜¿ubje)”}”(j¦ŒŸNew antennas: Micropulse WAAS 2225NW, TRM41249USCG; fix name of TPSCR.G3 to conform with IGS standard. Correct SLAGP to SLHGP for ASH700228A,B,C in hi.dat. ”j§]”(je)”}”(j¦ŒMNew antennas: Micropulse WAAS 2225NW, TRM41249USCG; fix name of TPSCR.G3 to”j§]”j±ŒMNew antennas: Micropulse WAAS 2225NW, TRM41249USCG; fix name of TPSCR.G3 to”…””}”(j¶jοjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆMºj¶jÊ¿ubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒPconform with IGS standard. Correct SLAGP to SLHGP for ASH700228A,B,C in hi.dat.”j§]”j±ŒPconform with IGS standard. Correct SLAGP to SLHGP for ASH700228A,B,C in hi.dat.”…””}”(j¶jß¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¹j¶jÜ¿ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jÊ¿ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆMºj¶j˜¿jÇj™³ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶j™³jÇj™³hjȳjÆNubj`)”}”(j¦Œ°Handle correctly site renames--either explicit for instrument changes or implicit for earthquakes---within a session ('model'): use only data from the longer of the two spans.”j§]”j±ŒµHandle correctly site renames–either explicit for instrument changes or implicit for earthquakes—within a session (‘model’): use only data from the longer of the two spans.”…””}”(j¶jÿ¿jÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¼j¶j™³jÇj™³ubj`)”}”(j¦ŒçThere is a new coordinate-conversion utility 'convertc' which will take as input a GLOBK apr-file (Cartesian) or a GLOBK velocity file or glist file (geodetic), and output an apr-file, velocity file, or KML file (for Google Earth).”j§]”j±ŒëThere is a new coordinate-conversion utility ‘convertc’ which will take as input a GLOBK apr-file (Cartesian) or a GLOBK velocity file or glist file (geodetic), and output an apr-file, velocity file, or KML file (for Google Earth).”…””}”(j¶j ÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÀj¶j™³jÇj™³ubj`)”}”(j¦Œèof the functions formerly performed by tform; Track: Fixes for milli-second clock resets that are not correctly accounted for in the RINEX files. Small bug fixes and some format changes. Increased size to allow 12-hrs of 2-Hz data.”j§]”j±Œèof the functions formerly performed by tform; Track: Fixes for milli-second clock resets that are not correctly accounted for in the RINEX files. Small bug fixes and some format changes. Increased size to allow 12-hrs of 2-Hz data.”…””}”(j¶jÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÅj¶j™³jÇj™³ubj`)”}”(j¦XPlate-referenced apr file for ITRF 2005: The files distributed with 10.33 were in error, having used the TIRF 2000 poles to rotate itrf05.apr to the major plates rather than the new poles from Altamimi et al. [2007]. The new files are correct, and also have site extents (_1Ps, 2PS, etc) corresponding to the GLOBK convention used in itrf05.apr and corresponding to the names used in itrf05.eq_rename. Corrected versions of itrf05_aust.apr, itrf05_pcfc.apr, itrf05_soam.apr, itrf_noam,apr, itrf05_eura.apr, and itrf_anta.apr.”j§]”j±XPlate-referenced apr file for ITRF 2005: The files distributed with 10.33 were in error, having used the TIRF 2000 poles to rotate itrf05.apr to the major plates rather than the new poles from Altamimi et al. [2007]. The new files are correct, and also have site extents (_1Ps, 2PS, etc) corresponding to the GLOBK convention used in itrf05.apr and corresponding to the names used in itrf05.eq_rename. Corrected versions of itrf05_aust.apr, itrf05_pcfc.apr, itrf05_soam.apr, itrf_noam,apr, itrf05_eura.apr, and itrf_anta.apr.”…””}”(j¶j)ÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÊj¶j™³jÇj™³ubj`)”}”(j¦Œ2Updated algoritm for clock estimation in 'autcln'.”j§]”j±Œ6Updated algoritm for clock estimation in ‘autcln’.”…””}”(j¶j7ÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÒj¶j™³jÇj™³ubj`)”}”(j¦Œ–Fix bug in setting DCBs for non-Trimble receivers when AS off. Occured only prior to DCB availability, so no effect except a rare * printed in x-file.”j§]”j±Œ–Fix bug in setting DCBs for non-Trimble receivers when AS off. Occured only prior to DCB availability, so no effect except a rare * printed in x-file.”…””}”(j¶jEÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÔj¶j™³jÇj™³ubj`)”}”(j¦Œ.Wild cards now allowed for all GLOBK commands.”j§]”j±Œ.Wild cards now allowed for all GLOBK commands.”…””}”(j¶jSÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM×j¶j™³jÇj™³ubj`)”}”(j¦Œ*Fix bug in making sky plots with sh_gamit.”j§]”j±Œ*Fix bug in making sky plots with sh_gamit.”…””}”(j¶jaÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÙj¶j™³jÇj™³ubj`)”}”(j¦Œ7New feature in sh_plotcrd to select stations by region.”j§]”j±Œ7New feature in sh_plotcrd to select stations by region.”…””}”(j¶joÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÛj¶j™³jÇj™³ubj`)”}”(j¦Œ?Fix bug in locating RINEX and h-files on the local file system.”j§]”j±Œ?Fix bug in locating RINEX and h-files on the local file system.”…””}”(j¶j}ÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÝj¶j™³jÇj™³ubj`)”}”(j¦ŒVIncrease the dimensions of MAXCHN to account for receivers with more than 20 channels.”j§]”j±ŒVIncrease the dimensions of MAXCHN to account for receivers with more than 20 channels.”…””}”(j¶j‹ÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMßj¶j™³jÇj™³ubj`)”}”(j¦ŒvChange in Apr., Unc., and Int. formats of globk/glorg print files to allow velocities of -999.99 m/yr (motion on ice).”j§]”j±ŒvChange in Apr., Unc., and Int. formats of globk/glorg print files to allow velocities of -999.99 m/yr (motion on ice).”…””}”(j¶j™ÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMáj¶j™³jÇj™³ubj`)”}”(j¦ŒŒFix a problem reading an integer elevation cutoff from the sestbl (should be used only with LC_HELP). Thanks to Rossana deMarco of CNR-IRPI.”j§]”j±ŒŒFix a problem reading an integer elevation cutoff from the sestbl (should be used only with LC_HELP). Thanks to Rossana deMarco of CNR-IRPI.”…””}”(j¶j§ÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMäj¶j™³jÇj™³ubj`)”}”(j¦X ZHD in 'model': There is a bug that causes a fatal when RNX UFL is the met heirarchy and the RINEX values are bogus. The bug is complicated by the presence of a redundant and unused file in the distribution. To fix the problem, copy /gamit/model/get_met_source.f and Makefile.generic, remove from your /gamit/model directory the file get_ion_source.f, Makefile, and model_lib.a; then regenerate the Makefile (unimake -m model from the /gamit level) and remake model. Thanks to Liz Petrie at U Newcastle for catching this.”j§]”j±XZHD in ‘model’: There is a bug that causes a fatal when RNX UFL is the met heirarchy and the RINEX values are bogus. The bug is complicated by the presence of a redundant and unused file in the distribution. To fix the problem, copy /gamit/model/get_met_source.f and Makefile.generic, remove from your /gamit/model directory the file get_ion_source.f, Makefile, and model_lib.a; then regenerate the Makefile (unimake -m model from the /gamit level) and remake model. Thanks to Liz Petrie at U Newcastle for catching this.”…””}”(j¶jµÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMçj¶j™³jÇj™³ubj`)”}”(j¦ŒO'yawtab': Fix bug in call to oversn.f, effect is only to miss version numbers.”j§]”j±ŒS‘yawtab’: Fix bug in call to oversn.f, effect is only to miss version numbers.”…””}”(j¶jÃÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMïj¶j™³jÇj™³ubj`)”}”(j¦ŒMMac OSX Intel: Fix inadvertent carriage return in /libraries/Makefile.config.”j§]”j±ŒMMac OSX Intel: Fix inadvertent carriage return in /libraries/Makefile.config.”…””}”(j¶jÑÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMñj¶j™³jÇj™³ubj`)”}”(j¦Œ** 10.33 vs 10.32”j§]”j±Œ** 10.33 vs 10.32”…””}”(j¶jßÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMôj¶j™³jÇj™³ubj`)”}”(j¦ŒiUpdate svnav.dat and antmod.dat (igs05_1461.atx) for SV55/PN15 (25 Oct 2007) and SV57/PN29 (21 Dec 2007).”j§]”j±ŒiUpdate svnav.dat and antmod.dat (igs05_1461.atx) for SV55/PN15 (25 Oct 2007) and SV57/PN29 (21 Dec 2007).”…””}”(j¶jíÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMöj¶j™³jÇj™³ubj`)”}”(j¦Œ Lunisolar tables for 2008; IAU 1980 nutations replaced by IAU 2000 nutations. H-files created with the old model will be automatically rotated to the new model.”j§]”j±Œ Lunisolar tables for 2008; IAU 1980 nutations replaced by IAU 2000 nutations. H-files created with the old model will be automatically rotated to the new model.”…””}”(j¶jûÀjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMùj¶j™³jÇj™³ubj`)”}”(j¦Œ\sestbl: Change 'Antenna model' to AZEL and 'SV antenna model' to ELEV to use absolute PCVs;”j§]”j±Œdsestbl: Change ‘Antenna model’ to AZEL and ‘SV antenna model’ to ELEV to use absolute PCVs;”…””}”(j¶j ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMýj¶j™³jÇj™³ubj`)”}”(j¦ŒSsittbl: Loosen suggested constraints to relect preference for ambiguity resolution.”j§]”j±ŒSsittbl: Loosen suggested constraints to relect preference for ambiguity resolution.”…””}”(j¶jÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒˆFix bug for OTL interpolation for sites between 0 longitude and the first grid point (0.25 deg for FES2004, 0.5 deg for other grids). 1”j§]”j±ŒˆFix bug for OTL interpolation for sites between 0 longitude and the first grid point (0.25 deg for FES2004, 0.5 deg for other grids). 1”…””}”(j¶j%ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒMFix bug in reading and using ATML or VMF1 values on the last day of the year.”j§]”j±ŒMFix bug in reading and using ATML or VMF1 values on the last day of the year.”…””}”(j¶j3ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ¤New receivers: LEICA GRX1200GGPRO, TPS NETG3, TPS MAXOR, TPS EUROCARD, NOV OEMV3 New antennas: LEIAT504GG, TRM4600, TRM41249USCG, NOV702GG, NOV702GL, NOV702 rev.4”j§]”j±Œ¤New receivers: LEICA GRX1200GGPRO, TPS NETG3, TPS MAXOR, TPS EUROCARD, NOV OEMV3 New antennas: LEIAT504GG, TRM4600, TRM41249USCG, NOV702GG, NOV702GL, NOV702 rev.4”…””}”(j¶jAÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ)Replace 'compress' but 'gzip' in scripts.”j§]”j±Œ1Replace ‘compress’ but ‘gzip’ in scripts.”…””}”(j¶jOÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM j¶j™³jÇj™³ubj`)”}”(j¦ŒpVelocity histograms (sh_velhist): Add capability to set a minimum as well as maximum sigma and a geographicbox.”j§]”j±ŒpVelocity histograms (sh_velhist): Add capability to set a minimum as well as maximum sigma and a geographicbox.”…””}”(j¶j]ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM j¶j™³jÇj™³ubj`)”}”(j¦ŒfEnhancements to facility cluster computer: In /com, sh_PBS_gamit, sh_gamit, sh_sp3fit, sh_get_orbits.”j§]”j±ŒfEnhancements to facility cluster computer: In /com, sh_PBS_gamit, sh_gamit, sh_sp3fit, sh_get_orbits.”…””}”(j¶jkÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒhAdd worst, best, median in calculating random walk for'real sigma' algorithm in sh_gen_stats, sh_enstat:”j§]”j±ŒlAdd worst, best, median in calculating random walk for’real sigma’ algorithm in sh_gen_stats, sh_enstat:”…””}”(j¶jyÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ`guess_rcvant.dat: Added missing carats (^) to entries for the TOPCON/TPS receivers and antennas.”j§]”j±Œ`guess_rcvant.dat: Added missing carats (^) to entries for the TOPCON/TPS receivers and antennas.”…””}”(j¶j‡ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒJTRACK: Fixed 10-hz epoch problem and reading gamit zenith delay estimates.”j§]”j±ŒJTRACK: Fixed 10-hz epoch problem and reading gamit zenith delay estimates.”…””}”(j¶j•ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ©sh_sp3fit: Fix bug reading sp3c files (old code wrong but works ok with g77 but not gfortran). Thanks to Demitry Balandin (Inst Geophysics Urals, RAS) for finding this.”j§]”j±Œ©sh_sp3fit: Fix bug reading sp3c files (old code wrong but works ok with g77 but not gfortran). Thanks to Demitry Balandin (Inst Geophysics Urals, RAS) for finding this.”…””}”(j¶j£ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ@Fix bug with merging station.info files (sh_upd_stnfo, mstinf2).”j§]”j±Œ@Fix bug with merging station.info files (sh_upd_stnfo, mstinf2).”…””}”(j¶j±ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒdNew RINEX compresssion routines provided by Yuki Hatanaka (GSI-Tsukuba) to handle RINEX Version 3.0.”j§]”j±ŒdNew RINEX compresssion routines provided by Yuki Hatanaka (GSI-Tsukuba) to handle RINEX Version 3.0.”…””}”(j¶j¿ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM j¶j™³jÇj™³ubj`)”}”(j¦ŒKFix header comments for sh_metutil (correct units for temperature and ZHD).”j§]”j±ŒKFix header comments for sh_metutil (correct units for temperature and ZHD).”…””}”(j¶jÍÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM#j¶j™³jÇj™³ubj`)”}”(j¦XˆUsing Az-El PCV corrections: There was an error in interpolating the ANTEX tables when both elevation- and azimuth-dependent corrections are used. On rare occasions, depending on the details of the model and distribution of observations, the bug could generate up to 10 mm error in heights and zenith delays, though usually the effect is negligible. Thanks to Wang Min of CEA for the catch.”j§]”j±XˆUsing Az-El PCV corrections: There was an error in interpolating the ANTEX tables when both elevation- and azimuth-dependent corrections are used. On rare occasions, depending on the details of the model and distribution of observations, the bug could generate up to 10 mm error in heights and zenith delays, though usually the effect is negligible. Thanks to Wang Min of CEA for the catch.”…””}”(j¶jÛÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM%j¶j™³jÇj™³ubj`)”}”(j¦X-Using GPT for a priori pressure and temperature. There was a bug in the time argument used to read the GPT model; the change in values, however, is very small and has a negigible effect on estimates of heights or zenith delays. Copy gamit/model/atmdel.f. Thanks to Peter Smythe of ANU for the catch.”j§]”j±X-Using GPT for a priori pressure and temperature. There was a bug in the time argument used to read the GPT model; the change in values, however, is very small and has a negigible effect on estimates of heights or zenith delays. Copy gamit/model/atmdel.f. Thanks to Peter Smythe of ANU for the catch.”…””}”(j¶jéÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM,j¶j™³jÇj™³ubj`)”}”(j¦Œ>Fixed problem with converting mutiple SINEX files with htoglb.”j§]”j±Œ>Fixed problem with converting mutiple SINEX files with htoglb.”…””}”(j¶j÷ÁjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM1j¶j™³jÇj™³ubj`)”}”(j¦ŒOsh_rx2apr (svpos); Fix problem using RINEX Version 1 (missing 'G' for SV name).”j§]”j±ŒSsh_rx2apr (svpos); Fix problem using RINEX Version 1 (missing ‘G’ for SV name).”…””}”(j¶jÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM3j¶j™³jÇj™³ubj`)”}”(j¦Œ9Change to autcln to improve postfit editing for old data.”j§]”j±Œ9Change to autcln to improve postfit editing for old data.”…””}”(j¶jÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM5j¶j™³jÇj™³ubj`)”}”(j¦Œ>Change the default gravity field for 'arc' to EGM96' (fixdrv).”j§]”j±ŒDChange the default gravity field for ‘arc’ to EGM96’ (fixdrv).”…””}”(j¶j!ÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM7j¶j™³jÇj™³ubj`)”}”(j¦Œ.Add gravity and nutation models to the h-file.”j§]”j±Œ.Add gravity and nutation models to the h-file.”…””}”(j¶j/ÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM9j¶j™³jÇj™³ubj`)”}”(j¦Œ0Fix bug in 'xtorx' with new-format station.info.”j§]”j±Œ4Fix bug in ‘xtorx’ with new-format station.info.”…””}”(j¶j=ÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM;j¶j™³jÇj™³ubj`)”}”(j¦Œ** 10.32 vs 10.31”j§]”j±Œ** 10.32 vs 10.31”…””}”(j¶jKÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM>j¶j™³jÇj™³ubj`)”}”(j¦XInstallation: 1) For the Intel compiler the link for libraries/comlib/execute_intel.f should point to execute_hp.f, not exectute_g77.f; 2) for OSX 8.8, Makefile.config updated to read 'OS_ID Darwin 5200 8800'; 3) for gfortran, restore a missing link for csubs.f in gamit/clean.”j§]”j±XInstallation: 1) For the Intel compiler the link for libraries/comlib/execute_intel.f should point to execute_hp.f, not exectute_g77.f; 2) for OSX 8.8, Makefile.config updated to read ‘OS_ID Darwin 5200 8800’; 3) for gfortran, restore a missing link for csubs.f in gamit/clean.”…””}”(j¶jYÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM@j¶j™³jÇj™³ubj`)”}”(j¦XAmbiguity resolution with LC_AUTCLN: changes in autcln will improve resolution of WLs signficantly, both before and after the introduction of DCBs (April 2001). Changes in solve will reduce or eliminate cases of failed inversions due to problems removing dependent biases.”j§]”j±XAmbiguity resolution with LC_AUTCLN: changes in autcln will improve resolution of WLs signficantly, both before and after the introduction of DCBs (April 2001). Changes in solve will reduce or eliminate cases of failed inversions due to problems removing dependent biases.”…””}”(j¶jgÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMEj¶j™³jÇj™³ubj`)”}”(j¦ŒðAmbiguity resolution with LC_HELP: WL resolution in the presence of high ionosphere is improved by rescaling the WL bias sigmas by the rms deviations for each baseline rather than by the overall nrms of the ionosphere-constrained solution.”j§]”j±ŒðAmbiguity resolution with LC_HELP: WL resolution in the presence of high ionosphere is improved by rescaling the WL bias sigmas by the rms deviations for each baseline rather than by the overall nrms of the ionosphere-constrained solution.”…””}”(j¶juÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMJj¶j™³jÇj™³ubj`)”}”(j¦XiNarrow-lane ambiguity resolution : With both LC_AUTCLN and LC_HELP, deviation-scaling of the NL sigmas is also implemented. The effect on resolution is not large, but the statistical summaries now printed in the q-file provide useful diagnostics for tuning ambuiguity resolution. (Changes also to sh_gamit to pick up the new print for the mailto summary file.”j§]”j±XiNarrow-lane ambiguity resolution : With both LC_AUTCLN and LC_HELP, deviation-scaling of the NL sigmas is also implemented. The effect on resolution is not large, but the statistical summaries now printed in the q-file provide useful diagnostics for tuning ambuiguity resolution. (Changes also to sh_gamit to pick up the new print for the mailto summary file.”…””}”(j¶jƒÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMNj¶j™³jÇj™³ubj`)”}”(j¦ŒDVMF1: Changes to allow multiple formats of VMF1 station-list files.”j§]”j±ŒDVMF1: Changes to allow multiple formats of VMF1 station-list files.”…””}”(j¶j‘ÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMTj¶j™³jÇj™³ubj`)”}”(j¦Œ„autcln.cmd: The template gg/tables had an extraneous blank before 'POST lc_autcln' that should be removed to use LC_AUTCLN in GAMIT.”j§]”j±Œˆautcln.cmd: The template gg/tables had an extraneous blank before ‘POST lc_autcln’ that should be removed to use LC_AUTCLN in GAMIT.”…””}”(j¶jŸÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMVj¶j™³jÇj™³ubj`)”}”(j¦ŒµMETUTIL: Fix two bugs using RINEX met files: 1) add correctly an extra value at the end to allow proper interpolation; 2) change temperature units to K. Copy gamit/utils/metutil.f.”j§]”j±ŒµMETUTIL: Fix two bugs using RINEX met files: 1) add correctly an extra value at the end to allow proper interpolation; 2) change temperature units to K. Copy gamit/utils/metutil.f.”…””}”(j¶j­ÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMYj¶j™³jÇj™³ubj`)”}”(j¦ŒâAshtech choke ring antennas: Bug in setting the aliases for these antennas for purposes of calculating direct height from slant height, results in a direct height error of about 1 mm for an antenna mounted 1 m above the mark.”j§]”j±ŒâAshtech choke ring antennas: Bug in setting the aliases for these antennas for purposes of calculating direct height from slant height, results in a direct height error of about 1 mm for an antenna mounted 1 m above the mark.”…””}”(j¶j»ÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM]j¶j™³jÇj™³ubj`)”}”(j¦Œ9New receviers: Added Leica GMX902 and Trimble R7 and R8.”j§]”j±Œ9New receviers: Added Leica GMX902 and Trimble R7 and R8.”…””}”(j¶jÉÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMaj¶j™³jÇj™³ubj`)”}”(j¦Œ”Creating new-style station.info: Add self-documentation for program gamit/hi/conv_stnfo) that converts an old-style to new-style station.info file.”j§]”j±Œ”Creating new-style station.info: Add self-documentation for program gamit/hi/conv_stnfo) that converts an old-style to new-style station.info file.”…””}”(j¶j×ÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMcj¶j™³jÇj™³ubj`)”}”(j¦Œsh_plotvel: Better diagnostics.”j§]”j±Œsh_plotvel: Better diagnostics.”…””}”(j¶jåÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMfj¶j™³jÇj™³ubj`)”}”(j¦Œ‹RINEX compression: Change sh_get_rinex to use sh_crx2rnx instead of sh_uncompress, and sh_uncomopress to use gunzip instead of uncompress.”j§]”j±Œ‹RINEX compression: Change sh_get_rinex to use sh_crx2rnx instead of sh_uncompress, and sh_uncomopress to use gunzip instead of uncompress.”…””}”(j¶jóÂjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMhj¶j™³jÇj™³ubj`)”}”(j¦Œ«GLORG: Output option (MIDP) which references solutions to the midpoint epoch of the combined data; should not be used when large stochastic position estimates are present.”j§]”j±Œ«GLORG: Output option (MIDP) which references solutions to the midpoint epoch of the combined data; should not be used when large stochastic position estimates are present.”…””}”(j¶jÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMkj¶j™³jÇj™³ubj`)”}”(j¦Œ** 10.31 vs 10.30”j§]”j±Œ** 10.31 vs 10.30”…””}”(j¶jÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMoj¶j™³jÇj™³ubj`)”}”(j¦ŒÒhi.dat: The ASHDMG antennas was misnamed ASHGD3; fixed errors in slant range dimensions for the ASHDMG, ROGSNR, and ROGRMA antennas. None of these errors will affect runs with DHARP as the height measurement.”j§]”j±ŒÒhi.dat: The ASHDMG antennas was misnamed ASHGD3; fixed errors in slant range dimensions for the ASHDMG, ROGSNR, and ROGRMA antennas. None of these errors will affect runs with DHARP as the height measurement.”…””}”(j¶jÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMqj¶j™³jÇj™³ubj`)”}”(j¦ŒqAtmospheric delay models: Fixed bug in GPT; made reading of a RINEX met file or a u-file ZHD (VMF1) more robust.”j§]”j±ŒqAtmospheric delay models: Fixed bug in GPT; made reading of a RINEX met file or a u-file ZHD (VMF1) more robust.”…””}”(j¶j+ÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMuj¶j™³jÇj™³ubj`)”}”(j¦Œ^Met utilities: Fixed problem with RINEX met files and improved interpolation for sh_met_util.”j§]”j±Œ^Met utilities: Fixed problem with RINEX met files and improved interpolation for sh_met_util.”…””}”(j¶j9ÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMxj¶j™³jÇj™³ubj`)”}”(j¦Œ»gcc/g77 3.4.x bug: Added a temporary patch to a lapack routine causing 'solve' to stall in an infinite loop when compiled with level 3 optimization with gcc/g77 3.4.x and possibly 2.95.”j§]”j±Œ¿gcc/g77 3.4.x bug: Added a temporary patch to a lapack routine causing ‘solve’ to stall in an infinite loop when compiled with level 3 optimization with gcc/g77 3.4.x and possibly 2.95.”…””}”(j¶jGÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM{j¶j™³jÇj™³ubj e)”}”(j¦hoj§]”je)”}”(j¦Œikf/track : Fixed problem reading RX files with internal comments with more than 12 lines rd_rinex_obs.f. ”j§]”(je)”}”(j¦Œkf/track”j§]”j±Œkf/track”…””}”(j¶j\ÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆM€j¶jXÃubj©Œ classifier”“”)”}”(j¦ŒMFixed problem reading RX files with internal comments with more than 12 lines”j§]”j±ŒMFixed problem reading RX files with internal comments with more than 12 lines”…””}”(j¶jlÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjjÃj¶jXÃhjȳubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œrd_rinex_obs.f.”j§]”j±Œrd_rinex_obs.f.”…””}”(j¶j}ÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM€j¶jzÃubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jXÃubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehjȳjÆM€j¶jUÃubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶j™³jÇj™³hjȳjÆNubj`)”}”(j¦ŒeDeleting eclipse data: Has not worked properly for some time, but now fixed in gamit/utils/autecl.f.”j§]”j±ŒeDeleting eclipse data: Has not worked properly for some time, but now fixed in gamit/utils/autecl.f.”…””}”(j¶jÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM‚j¶j™³jÇj™³ubj`)”}”(j¦ŒÔProblems compiling and using ocean loading with the HP f90 compiler.. Download the entire incrementals to get Makefile changes, system-dependent routines, and several GAMIT routines with uninitialized variables.”j§]”j±ŒÔProblems compiling and using ocean loading with the HP f90 compiler.. Download the entire incrementals to get Makefile changes, system-dependent routines, and several GAMIT routines with uninitialized variables.”…””}”(j¶j«ÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM…j¶j™³jÇj™³ubj`)”}”(j¦Œ.Initialization problem for 'idatum' in fixdrv.”j§]”j±Œ2Initialization problem for ‘idatum’ in fixdrv.”…””}”(j¶j¹ÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM‰j¶j™³jÇj™³ubj`)”}”(j¦Œ¥Sky plots not created by sh_gamit because sh_make_sky_gifs looks for 'autcln postfit' in the sestbl, but this command is no longer necessary; fixed sh_make_sky_gifs.”j§]”j±Œ©Sky plots not created by sh_gamit because sh_make_sky_gifs looks for ‘autcln postfit’ in the sestbl, but this command is no longer necessary; fixed sh_make_sky_gifs.”…””}”(j¶jÇÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM‹j¶j™³jÇj™³ubj`)”}”(j¦Œ]Fix intel compiler flags for 'solve'. Thanks to S. Shimada (NIED/Tsukuba) for catching this.”j§]”j±ŒaFix intel compiler flags for ‘solve’. Thanks to S. Shimada (NIED/Tsukuba) for catching this.”…””}”(j¶jÕÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMŽj¶j™³jÇj™³ubj`)”}”(j¦Œ¥SV-dependent data reweighting did not work with (default) 'AUTCLN Postfit = R' option. Copy gamit/fixdrv/bmake.f. Thanks to Wang Min (CEA/Beijing) for catching this.”j§]”j±Œ©SV-dependent data reweighting did not work with (default) ‘AUTCLN Postfit = R’ option. Copy gamit/fixdrv/bmake.f. Thanks to Wang Min (CEA/Beijing) for catching this.”…””}”(j¶jãÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒiAdd traps for # SVs on g-file or nav-file > maxsat. Copy gamit/fixdrv/satnmr.f and gamit/makexp/checke.f”j§]”j±ŒiAdd traps for # SVs on g-file or nav-file > maxsat. Copy gamit/fixdrv/satnmr.f and gamit/makexp/checke.f”…””}”(j¶jñÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM“j¶j™³jÇj™³ubj`)”}”(j¦Œxhi.dat: Correct entries for SLBCR for ROGSNR and ROGRMA. Thanks to Sigrun Hreinsdottir of U. Arizona for catching this.”j§]”j±Œxhi.dat: Correct entries for SLBCR for ROGSNR and ROGRMA. Thanks to Sigrun Hreinsdottir of U. Arizona for catching this.”…””}”(j¶jÿÃjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM–j¶j™³jÇj™³ubj`)”}”(j¦XtOS-dependent routine for HP: The HP requires a special version of libraries/comlib/systime.f so so we have re-introduced OS-dependent versions; also we need an HP version of kf/gen_util/execute.f. Copy cversn.f, Makefile.generic, and the systime_HHH.f version you need from /libraries/comlib; and Makefile.generic and the execute_HHH.f version you need from kf/gen_util.”j§]”j±XtOS-dependent routine for HP: The HP requires a special version of libraries/comlib/systime.f so so we have re-introduced OS-dependent versions; also we need an HP version of kf/gen_util/execute.f. Copy cversn.f, Makefile.generic, and the systime_HHH.f version you need from /libraries/comlib; and Makefile.generic and the execute_HHH.f version you need from kf/gen_util.”…””}”(j¶j ÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM™j¶j™³jÇj™³ubj`)”}”(j¦ŒVMAKEX problem opening and closing hi.dat. Copy makex.f and closem.f from gamit/makex.”j§]”j±ŒVMAKEX problem opening and closing hi.dat. Copy makex.f and closem.f from gamit/makex.”…””}”(j¶jÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMŸj¶j™³jÇj™³ubj`)”}”(j¦X‰svnav.dat: Update for PN12/SV58. Copy svnav.dat or svnav.dat.igs, depending on whether you want to maintain backward-compatibility or IGS-consistency for SV antenna offsets when using a relative PCVs (with absolute PCVs, these values are overridden by antmod.dat). Note that SOPAC used an old svnav.dat for processing of PRN 12 between 2006 12 15 and 2007 01 13, so if you are combining SOPAC H-files with your own processing, you must either exclude PRN 12 from your processing or allow the radiation-pressure parameters to adjust independently in the SOPAC and your own h-files. This is easily accomplish by 'apr_svs prn_12 100 100 100 10 10 10 0R'. As described in the 10.2 Release Notes, a similar situation pertains to PN22/SV22 as a result our error in listing its block number. Its radiation pressure parameters should be decoupled from all SOPAC or MIT H-files created between 1993 and 2003.”j§]”j±Xsvnav.dat: Update for PN12/SV58. Copy svnav.dat or svnav.dat.igs, depending on whether you want to maintain backward-compatibility or IGS-consistency for SV antenna offsets when using a relative PCVs (with absolute PCVs, these values are overridden by antmod.dat). Note that SOPAC used an old svnav.dat for processing of PRN 12 between 2006 12 15 and 2007 01 13, so if you are combining SOPAC H-files with your own processing, you must either exclude PRN 12 from your processing or allow the radiation-pressure parameters to adjust independently in the SOPAC and your own h-files. This is easily accomplish by ‘apr_svs prn_12 100 100 100 10 10 10 0R’. As described in the 10.2 Release Notes, a similar situation pertains to PN22/SV22 as a result our error in listing its block number. Its radiation pressure parameters should be decoupled from all SOPAC or MIT H-files created between 1993 and 2003.”…””}”(j¶j)ÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¡j¶j™³jÇj™³ubj`)”}”(j¦Œ_GLORG: Fixed I*8 declaration for memory allocation on 64-bit machines when plate estimate used.”j§]”j±Œ_GLORG: Fixed I*8 declaration for memory allocation on 64-bit machines when plate estimate used.”…””}”(j¶j7ÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM­j¶j™³jÇj™³ubj`)”}”(j¦Œ¨HTOGLB: Sinex routines changed to read and deconstrain center of mass and satellite anttena offset estimates. Added codes for IGS05_1404 antmod file to SMod_to_full.f.”j§]”j±Œ¨HTOGLB: Sinex routines changed to read and deconstrain center of mass and satellite anttena offset estimates. Added codes for IGS05_1404 antmod file to SMod_to_full.f.”…””}”(j¶jEÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM°j¶j™³jÇj™³ubj`)”}”(j¦ŒAsh_rx2apr: svpos/svdiff now work properly with the C2 observable.”j§]”j±ŒAsh_rx2apr: svpos/svdiff now work properly with the C2 observable.”…””}”(j¶jSÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM³j¶j™³jÇj™³ubj`)”}”(j¦X½Apriori coordinates: GAMIT/model now has the ability to use the full 8-character station name when reading a GLOBK-style L-file together with a GLOBK eq_file. The link scripts will now attempt to link into the day directory, via the [expt]/tables directory a file named 'eq_rename', which you may link (in [expt]/tables or gg/tables to a particular rename file. In the gg/tables directory distributed with 10.31, theeq_rename file is linked to a file derived from the steps documented for IGS stations by IGS Analysis Center Coordinator Remi Ferland (NRCan) and distributed as IGS-Discontinuities.snx. This file is incomplete even for IGS stations but may serve as a starting point for GAMIT users.”j§]”j±XÁApriori coordinates: GAMIT/model now has the ability to use the full 8-character station name when reading a GLOBK-style L-file together with a GLOBK eq_file. The link scripts will now attempt to link into the day directory, via the [expt]/tables directory a file named ‘eq_rename’, which you may link (in [expt]/tables or gg/tables to a particular rename file. In the gg/tables directory distributed with 10.31, theeq_rename file is linked to a file derived from the steps documented for IGS stations by IGS Analysis Center Coordinator Remi Ferland (NRCan) and distributed as IGS-Discontinuities.snx. This file is incomplete even for IGS stations but may serve as a starting point for GAMIT users.”…””}”(j¶jaÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMµj¶j™³jÇj™³ubj`)”}”(j¦XãTrapping bad a priori coordinates: If you overconstrain a station's coordinates in the GAMIT run, you will get an elevated nrms and degraded ambiguity resolution. There is now a test for this in 'solve', based on an adjustment more than twice the apiori constraint. The script sh_sigelv in the batch file now checks for the requisite lines in the q-file, and if a station has a large adjustment in the first ('p') solution, its constraints are relaxed for the final ('a') solution.”j§]”j±XñTrapping bad a priori coordinates: If you overconstrain a station’s coordinates in the GAMIT run, you will get an elevated nrms and degraded ambiguity resolution. There is now a test for this in ‘solve’, based on an adjustment more than twice the apiori constraint. The script sh_sigelv in the batch file now checks for the requisite lines in the q-file, and if a station has a large adjustment in the first (‘p’) solution, its constraints are relaxed for the final (‘a’) solution.”…””}”(j¶joÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM¿j¶j™³jÇj™³ubj`)”}”(j¦X N-file reweighting: Because the N-file is now always written (for trapping bad a priori coordinates), the sestbl command for invoking phase-error reweighting is changed from 'Use N-file = Y' to 'AUTCLN reweight = Y'. However, the old command will still work in 10.31.”j§]”j±XN-file reweighting: Because the N-file is now always written (for trapping bad a priori coordinates), the sestbl command for invoking phase-error reweighting is changed from ‘Use N-file = Y’ to ‘AUTCLN reweight = Y’. However, the old command will still work in 10.31.”…””}”(j¶j}ÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÆj¶j™³jÇj™³ubj`)”}”(j¦Œ** 10.30 vs 10.21”j§]”j±Œ** 10.30 vs 10.21”…””}”(j¶j‹ÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÌj¶j™³jÇj™³ubj`)”}”(j¦ŒÆSpeed of computation: New inversion routines have been added to SOLVE, improving the speed by about 30%. Note that gfortran will gain another 10% compared to g77, and the Intel compiler about 25%.”j§]”j±ŒÆSpeed of computation: New inversion routines have been added to SOLVE, improving the speed by about 30%. Note that gfortran will gain another 10% compared to g77, and the Intel compiler about 25%.”…””}”(j¶j™ÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÎj¶j™³jÇj™³ubj`)”}”(j¦Œùsh_gamit.log: All of the GAMIT batch file status, warning, and fatal messages are now written into the log file, and more traps have been added to stop the run once a fatal is encountered. This should make it easier to find the source of a failure.”j§]”j±Œùsh_gamit.log: All of the GAMIT batch file status, warning, and fatal messages are now written into the log file, and more traps have been added to stop the run once a fatal is encountered. This should make it easier to find the source of a failure.”…””}”(j¶j§ÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÒj¶j™³jÇj™³ubj`)”}”(j¦Œ£Fix logic to 'cfmrg' and 'solve' to allow more than 30 SVs. This change is necessary if you use the full complement of SVs currently distributed with IGS orbits.”j§]”j±Œ«Fix logic to ‘cfmrg’ and ‘solve’ to allow more than 30 SVs. This change is necessary if you use the full complement of SVs currently distributed with IGS orbits.”…””}”(j¶jµÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM×j¶j™³jÇj™³ubj`)”}”(j¦Œ‡Fix sh_gamit problem resulting in deleted rinex files when making Hatanaka compressed RINEX at the end of the run. Copy /com/sh_gamit.”j§]”j±Œ‡Fix sh_gamit problem resulting in deleted rinex files when making Hatanaka compressed RINEX at the end of the run. Copy /com/sh_gamit.”…””}”(j¶jÃÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÛj¶j™³jÇj™³ubj`)”}”(j¦Œ]Add aliases for JNS versions of Topcon 'zero-centered' antennas. Copy gamit/lib/ant_alias.f.”j§]”j±ŒaAdd aliases for JNS versions of Topcon ‘zero-centered’ antennas. Copy gamit/lib/ant_alias.f.”…””}”(j¶jÑÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÞj¶j™³jÇj™³ubj`)”}”(j¦XAUTCLN: Fixed problem with postfit editing bias flags, added additional calls to trim one way to remove bad data and fixed P1/P2 residual output, and changed default # of channels from 14 to 15 to accommadate newer receivers (also fixable by setting 'max_chan 15' in autcln.cmd.)”j§]”j±XAUTCLN: Fixed problem with postfit editing bias flags, added additional calls to trim one way to remove bad data and fixed P1/P2 residual output, and changed default # of channels from 14 to 15 to accommadate newer receivers (also fixable by setting ‘max_chan 15’ in autcln.cmd.)”…””}”(j¶jßÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMáj¶j™³jÇj™³ubj`)”}”(j¦X]MAKEXP: Fixed problem when a station.info entry begins later than the session start and on a separate day. Avoid problem when station.info has no entry for data in a RINEX file linked into the day directory but not used in the session: rstnfo now prints only a warning if called by makexp; if there is a true omission, makex will stop with a fatal.”j§]”j±X]MAKEXP: Fixed problem when a station.info entry begins later than the session start and on a separate day. Avoid problem when station.info has no entry for data in a RINEX file linked into the day directory but not used in the session: rstnfo now prints only a warning if called by makexp; if there is a true omission, makex will stop with a fatal.”…””}”(j¶jíÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMæj¶j™³jÇj™³ubj`)”}”(j¦XŸSOLVE: Fixed bug in printing observable/ambiguity type in q-file, Fix bugs when estimating a single zenith delay. Fix bug (introduced with incrementals of 060227) in assigning gradient apr values; thanks to Sunil Bisnath of CfA and Mathilde Vergnolle of U. Luxembourg. Fix a bug in reading the batch file and writing the q-file header when there are more than 50 sites; thanks to Kirill Palamartchouk of TU Crete.”j§]”j±XŸSOLVE: Fixed bug in printing observable/ambiguity type in q-file, Fix bugs when estimating a single zenith delay. Fix bug (introduced with incrementals of 060227) in assigning gradient apr values; thanks to Sunil Bisnath of CfA and Mathilde Vergnolle of U. Luxembourg. Fix a bug in reading the batch file and writing the q-file header when there are more than 50 sites; thanks to Kirill Palamartchouk of TU Crete.”…””}”(j¶jûÄjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMìj¶j™³jÇj™³ubj`)”}”(j¦ŒkGLORG: Added eq_dist option for estimates of logarithmic parameters; fix some bugs in earthquake reporting.”j§]”j±ŒkGLORG: Added eq_dist option for estimates of logarithmic parameters; fix some bugs in earthquake reporting.”…””}”(j¶j ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMój¶j™³jÇj™³ubj`)”}”(j¦ŒÂPlotting time series: The new print option PBOP in glorg will generate output lines in the format adopted by the U.S. Plate Boundary Observatory (PBO); plots are generated by new program tssum.”j§]”j±ŒÂPlotting time series: The new print option PBOP in glorg will generate output lines in the format adopted by the U.S. Plate Boundary Observatory (PBO); plots are generated by new program tssum.”…””}”(j¶jÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMöj¶j™³jÇj™³ubj`)”}”(j¦Œ+GLBTOSNX: Improved output of renamed sites.”j§]”j±Œ+GLBTOSNX: Improved output of renamed sites.”…””}”(j¶j%ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMúj¶j™³jÇj™³ubj`)”}”(j¦Œ…Allow true C2 observables by not changing 'C2' to 'P2' unless the data are earlier than 2004 (needed for Trimble serial P-code data).”j§]”j±ŒAllow true C2 observables by not changing ‘C2’ to ‘P2’ unless the data are earlier than 2004 (needed for Trimble serial P-code data).”…””}”(j¶j3ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMüj¶j™³jÇj™³ubj`)”}”(j¦Œjsh_merge_rinex: Now allows input of the sampling intervel. Thanks to Seiichi Shimada of NIED for the fix.”j§]”j±Œjsh_merge_rinex: Now allows input of the sampling intervel. Thanks to Seiichi Shimada of NIED for the fix.”…””}”(j¶jAÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMÿj¶j™³jÇj™³ubj`)”}”(j¦Œ¸sh_make_rinex: The script to run to run TEQC on raw data files to create RINEX had a bug that prevented mixing of Trimble data files with those from any other receiver type; now fixed.”j§]”j±Œ¸sh_make_rinex: The script to run to run TEQC on raw data files to create RINEX had a bug that prevented mixing of Trimble data files with those from any other receiver type; now fixed.”…””}”(j¶jOÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒáSP3-C files: Fix option (-u) in sh_sp3fit for excluding SVs, thanks to Wang Min of CEA Beijing. Fix problems when flags are needed, thanks to Mark Murray of New Mexico Tech. Fix bug in naming g-file with 2- or 3-day fits.”j§]”j±ŒáSP3-C files: Fix option (-u) in sh_sp3fit for excluding SVs, thanks to Wang Min of CEA Beijing. Fix problems when flags are needed, thanks to Mark Murray of New Mexico Tech. Fix bug in naming g-file with 2- or 3-day fits.”…””}”(j¶j]ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒþPCV models: Updated versions of the IGS01 relative and IGS05 absolute PCV models in gg/tables: igs_01_antex11.pcv and igs_05.atx. The igs_05.atx file has a model for the new PRN 17 (SVN 53) as well as revisions of additions for about 50 ground antennas.”j§]”j±ŒþPCV models: Updated versions of the IGS01 relative and IGS05 absolute PCV models in gg/tables: igs_01_antex11.pcv and igs_05.atx. The igs_05.atx file has a model for the new PRN 17 (SVN 53) as well as revisions of additions for about 50 ground antennas.”…””}”(j¶jkÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM j¶j™³jÇj™³ubj`)”}”(j¦ŒrTRACK: Updated to handle sp3c format and new IIRM satellites; small changes to better handle bad pseudorange data.”j§]”j±ŒrTRACK: Updated to handle sp3c format and new IIRM satellites; small changes to better handle bad pseudorange data.”…””}”(j¶jyÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦ŒŠFix non-working -u option (exclude SVs with unknown accuracy code) in sh_sp3fit. Thanks to Wang Min of CEA for the catch. McClusky 060306”j§]”j±ŒŠFix non-working -u option (exclude SVs with unknown accuracy code) in sh_sp3fit. Thanks to Wang Min of CEA for the catch. McClusky 060306”…””}”(j¶j‡ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ¦Missing data from Leica GRX1200: Fix omission of SVs in upper channels when an incorrect firmware version is used in station.info; thanks to Wang Min of CEA Beijing.”j§]”j±Œ¦Missing data from Leica GRX1200: Fix omission of SVs in upper channels when an incorrect firmware version is used in station.info; thanks to Wang Min of CEA Beijing.”…””}”(j¶j•ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ\sh_baseline: Allow turning off of error bars and setting the tick and labels of the y-axis.”j§]”j±Œ\sh_baseline: Allow turning off of error bars and setting the tick and labels of the y-axis.”…””}”(j¶j£ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ—sh_upd_stnfo: Fixed bug in updating station.info from a RINEX file when more than 12 SVs listed in an epoch line; thanks to A. Zubovitch of RAS Moscow.”j§]”j±Œ—sh_upd_stnfo: Fixed bug in updating station.info from a RINEX file when more than 12 SVs listed in an epoch line; thanks to A. Zubovitch of RAS Moscow.”…””}”(j¶j±ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆMj¶j™³jÇj™³ubj`)”}”(j¦Œ[Bogus antenna heights: Fix bug that set HI=0. when using hi.dat with a missing height code.”j§]”j±Œ[Bogus antenna heights: Fix bug that set HI=0. when using hi.dat with a missing height code.”…””}”(j¶j¿ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM j¶j™³jÇj™³ubj`)”}”(j¦Œ^unify_apr: Better handling of sites when they appear multiple times in pos_mode and vel_mode.”j§]”j±Œ^unify_apr: Better handling of sites when they appear multiple times in pos_mode and vel_mode.”…””}”(j¶jÍÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM#j¶j™³jÇj™³ubj`)”}”(j¦ŒMmerge_apr: New program to merge two a priori files with no duplicate entries.”j§]”j±ŒMmerge_apr: New program to merge two a priori files with no duplicate entries.”…””}”(j¶jÛÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM&j¶j™³jÇj™³ubj`)”}”(j¦ŒxFix non-POSIX standard calls to 'head' and 'tail' command in > 100 scripts (old form does not work with Fedora Core 5).”j§]”j±Œ€Fix non-POSIX standard calls to ‘head’ and ‘tail’ command in > 100 scripts (old form does not work with Fedora Core 5).”…””}”(j¶jéÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM(j¶j™³jÇj™³ubj`)”}”(j¦Œ®Use gzip/gunzip instead of compress/uncompress in locating and creating RINEX files. (Still more scripts to change for this.) Copy from /com: sh_find_data and sh_make_rinex.”j§]”j±Œ®Use gzip/gunzip instead of compress/uncompress in locating and creating RINEX files. (Still more scripts to change for this.) Copy from /com: sh_find_data and sh_make_rinex.”…””}”(j¶j÷ÅjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjȳjÆM+j¶j™³jÇj™³ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jȳj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjȳjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j¨³jœ³j·³j«³uj_}”(Œrel”j¨³Œdate”j·³ujc}”Œmb”]”j÷ )”}”(j¦j »j§]”j±Œmb”…””}”(j¶jÆjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œmb”Œrefname”jÆujÄjö j¶j”»ubasje}”jg}”ji}”j¹}”(j®»jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±ŒUnknown target name: "mb".”…””}”j¶j.Æsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j+Æubaj·}”(j¹]”j®»aj»]”j½]”jÀ]”jÂ]”j¨»aŒlevel”KŒtype”j5Œsource”jȳŒline”M»ujÄjø ubj¨»jž»ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”(jù )”}”(j¦hoj§]”j`)”}”(j¦ŒUnexpected indentation.”j§]”j±ŒUnexpected indentation.”…””}”(j¶jTÆjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jQÆubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”j5Œsource”jȳŒline”KkujÄjø j¶j™³jÇj™³hjȳjÆKjubjù )”}”(j¦hoj§]”j`)”}”(j¦Œ?Definition list ends without a blank line; unexpected unindent.”j§]”j±Œ?Definition list ends without a blank line; unexpected unindent.”…””}”(j¶joÆjÇj™³hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jlÆubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒline”MŒsource”jȳujÄjø j¶j™³jÇj™³hjȳjÆMubej†]”j+ÆajˆNj‰]”j‹NjÇj™³ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jŒÆsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j‰ÆjÇj‰Æubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j›ÆjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ"Release Notes for GAMIT/GLOBK 10.6”j§]”j±Œ"Release Notes for GAMIT/GLOBK 10.6”…””}”(j¶jªÆjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hŒ@/chandler/home/floyd/public_html/gg/docs/source/relnote/10.6.rst”jÆKj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒLast updated 12 June 2015”j§]”j±ŒLast updated 12 June 2015”…””}”(j¶j¹ÆjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKj¶j‰ÆjÇj‰Æubjس)”}”(j¦ŒF----------------------------------------------------------------------”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj׳hj¸ÆjÆKj¶j‰ÆjÇj‰Æubj`)”}”(j¦X1Release 10.6 consolidates incremental updates made since release 10.50 of July 2013. As noted in the release announcement, this release has extensive structural and format changes to accommodate GNSS SVs other than GPS. Of the files in the usual processing flow, four have changed formats: svnav.dat, dcb.dat, g-files, and c-files. The new version will read old-format g-files and dcb.dat files, but NOT svnav.dat or c-files. We will continue to update old-format svnav.dat and dcb.dat files and put them into incremental updates for another 6 to 12 months with extent 'gps' for user who do not wish to move to 10.6 immediately. There was a flaw in our old-format creation of dcb.dat from the AIUB P1C1.DCB files in the time-tagging and in not correctly accounting for different SVs with the same PRN numbers during the month. This error will degrade wide-lane ambiguity resolution in some cases. Finally, with the new code, you'll find differences in the print files for arc and model, but unless you read these with your own scripts, these changes will be seamless.”j§]”j±X7Release 10.6 consolidates incremental updates made since release 10.50 of July 2013. As noted in the release announcement, this release has extensive structural and format changes to accommodate GNSS SVs other than GPS. Of the files in the usual processing flow, four have changed formats: svnav.dat, dcb.dat, g-files, and c-files. The new version will read old-format g-files and dcb.dat files, but NOT svnav.dat or c-files. We will continue to update old-format svnav.dat and dcb.dat files and put them into incremental updates for another 6 to 12 months with extent ‘gps’ for user who do not wish to move to 10.6 immediately. There was a flaw in our old-format creation of dcb.dat from the AIUB P1C1.DCB files in the time-tagging and in not correctly accounting for different SVs with the same PRN numbers during the month. This error will degrade wide-lane ambiguity resolution in some cases. Finally, with the new code, you’ll find differences in the print files for arc and model, but unless you read these with your own scripts, these changes will be seamless.”…””}”(j¶jÑÆjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKj¶j‰ÆjÇj‰Æubj`)”}”(j¦XÊWhenever you process data beyond the date of the software release, you MUST update supporting files. For GAMIT: svnav.dat and antmod.dat for changes in PN assignments; dcb.dat for P1/C1/P2 code biases that affect wide-lane ambiguity resolution; station.info for antenna changes at reference sites; and ut1/pole files for current EOP information. Of these files, only the EOP files are automatically updated by sh_gamit. For GLOBK, you should keep current itrf08_comb.apr and itrf08_comb.eq to account for improved coordinates and antenna changes and earthquakes at reference sites. Both the GAMIT and GLOBK files are always current in incremental_updates/tables and included in any incremental_update tar-file.”j§]”j±XÊWhenever you process data beyond the date of the software release, you MUST update supporting files. For GAMIT: svnav.dat and antmod.dat for changes in PN assignments; dcb.dat for P1/C1/P2 code biases that affect wide-lane ambiguity resolution; station.info for antenna changes at reference sites; and ut1/pole files for current EOP information. Of these files, only the EOP files are automatically updated by sh_gamit. For GLOBK, you should keep current itrf08_comb.apr and itrf08_comb.eq to account for improved coordinates and antenna changes and earthquakes at reference sites. Both the GAMIT and GLOBK files are always current in incremental_updates/tables and included in any incremental_update tar-file.”…””}”(j¶jßÆjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKj¶j‰ÆjÇj‰Æubj`)”}”(j¦X4All GAMIT-GLOBK scripts that produce plots (e.g. time series and velocity maps) use Generic Mapping Tools (GMT) to do so. The release of GMT 5 in November 2013 has necessitated major alterations to the syntax of GMT commands in many scripts. The updated scripts, which use GMT 5-compatible syntax, are contained in com/ and will be the only ones maintained and developed beyond this release of GAMIT-GLOBK. We therefore recommend that all users now download and switch to using GMT 5 because the updated scripts are NOT backwards-compatible. The old scripts, which may be used with GMT 4 or prior, are now contained in the com_preGMT5/ directory. Users must prepend this directory to their path in order to continue to use GMT 4, e.g. $PATH is ...:$HOME/gg/com_preGMT5:$HOME/gg/com:$HOME/gg/gamit/bin:$HOME/gg/kf/bin:...”j§]”j±X4All GAMIT-GLOBK scripts that produce plots (e.g. time series and velocity maps) use Generic Mapping Tools (GMT) to do so. The release of GMT 5 in November 2013 has necessitated major alterations to the syntax of GMT commands in many scripts. The updated scripts, which use GMT 5-compatible syntax, are contained in com/ and will be the only ones maintained and developed beyond this release of GAMIT-GLOBK. We therefore recommend that all users now download and switch to using GMT 5 because the updated scripts are NOT backwards-compatible. The old scripts, which may be used with GMT 4 or prior, are now contained in the com_preGMT5/ directory. Users must prepend this directory to their path in order to continue to use GMT 4, e.g. $PATH is …:$HOME/gg/com_preGMT5:$HOME/gg/com:$HOME/gg/gamit/bin:$HOME/gg/kf/bin:…”…””}”(j¶jíÆjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK$j¶j‰ÆjÇj‰Æubj`)”}”(j¦XQFor plotting time series, we are transitioning from using VAL and mb files produced by ensum and multibase and used by sh_plotcrd or sh_baseline to PBO-format pos-files produced by tssum and used by sh_plot_pos. tsview can still read both mb-files and pos-files. sh_glred will accept either 'E' (for ensum/mb) or 'T' (for tssum/pos).”j§]”j±XYFor plotting time series, we are transitioning from using VAL and mb files produced by ensum and multibase and used by sh_plotcrd or sh_baseline to PBO-format pos-files produced by tssum and used by sh_plot_pos. tsview can still read both mb-files and pos-files. sh_glred will accept either ‘E’ (for ensum/mb) or ‘T’ (for tssum/pos).”…””}”(j¶jûÆjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK1j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ”sh_gamit now writes the sky plots and phase vs elevation angle plots into a /figs directory instead /gifs, and the files are no png rather than gif.”j§]”j±Œ”sh_gamit now writes the sky plots and phase vs elevation angle plots into a /figs directory instead /gifs, and the files are no png rather than gif.”…””}”(j¶j ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK7j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œwglist can now take multiple apr and eq files and accept use_site commands, so that it can fully check a globk solution.”j§]”j±Œwglist can now take multiple apr and eq files and accept use_site commands, so that it can fully check a globk solution.”…””}”(j¶jÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK;j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¡To be consistent with IGS standards, we have replaced the Bar-Sever model Kouba model for satellite yaw, removing the need for the ascii y-file generated by ARC.”j§]”j±Œ¡To be consistent with IGS standards, we have replaced the Bar-Sever model Kouba model for satellite yaw, removing the need for the ascii y-file generated by ARC.”…””}”(j¶j%ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK>j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒOther changes and comments:”j§]”j±ŒOther changes and comments:”…””}”(j¶j3ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKCj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ‹Modified memory management in globk to handle >20,000 parameters. See globk.hlp and glorg.hlp for other features added in recent versions.”j§]”j±Œ‹Modified memory management in globk to handle >20,000 parameters. See globk.hlp and glorg.hlp for other features added in recent versions.”…””}”(j¶jAÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKEj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ,Kalman filter added to tsfit (see tsfit.hlp)”•j§]”j±Œ,Kalman filter added to tsfit (see tsfit.hlp)”…””}”(j¶jOÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKHj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒÁChanged the conversion of sp3 files to g- or t-files to use the IERS2010 dirunal and semi-diurnal EOP so as to be consistent with the rotations in MODEL (differences of 2 mm in orbit position).”j§]”j±ŒÁChanged the conversion of sp3 files to g- or t-files to use the IERS2010 dirunal and semi-diurnal EOP so as to be consistent with the rotations in MODEL (differences of 2 mm in orbit position).”…””}”(j¶j]ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKJj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒŸIntroduced and made default IGRF12 for the magnetic field used to compute 2nd order ionospheric corrections. Thanks to Seiichi Shimada of NIED for this change.”j§]”j±ŒŸIntroduced and made default IGRF12 for the magnetic field used to compute 2nd order ionospheric corrections. Thanks to Seiichi Shimada of NIED for this change.”…””}”(j¶jkÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKNj¶j‰ÆjÇj‰Æubj`)”}”(j¦XÔChanges to sh_plot_pos: Switched position of north and east component plots and fixed long-standing bug with not plotting discontinuities when specifying rename- and/or eq-files and, implicitly or explicitly, using "NONE" as tsfit command file. Added additional width to time axis in figures to prevent first and/or last time series points plotting beneath y-axes, and added -w option to control fraction of time series length to add (default 0.1 = 10% on both ends).”j§]”j±XØChanges to sh_plot_pos: Switched position of north and east component plots and fixed long-standing bug with not plotting discontinuities when specifying rename- and/or eq-files and, implicitly or explicitly, using “NONE†as tsfit command file. Added additional width to time axis in figures to prevent first and/or last time series points plotting beneath y-axes, and added -w option to control fraction of time series length to add (default 0.1 = 10% on both ends).”…””}”(j¶jyÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKRj¶j‰ÆjÇj‰Æubj`)”}”(j¦X‘Changed sh_update_eop to use wget or curl rather than ftp or ncftp to download EOP files from USNO to avoid frequent ftp hang-ups. The new version supports extent 'usno' (Bulletin A finals.data from 1992, updated weekly) and 'usnd' (Bulleton A finals.daily, last 3 months only, updated daily). We no longer distribute Bulletin B since the Bulletin A value are as accurate and updated more frequently.”j§]”j±X™Changed sh_update_eop to use wget or curl rather than ftp or ncftp to download EOP files from USNO to avoid frequent ftp hang-ups. The new version supports extent ‘usno’ (Bulletin A finals.data from 1992, updated weekly) and ‘usnd’ (Bulleton A finals.daily, last 3 months only, updated daily). We no longer distribute Bulletin B since the Bulletin A value are as accurate and updated more frequently.”…””}”(j¶j‡ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKZj¶j‰ÆjÇj‰Æubj`)”}”(j¦XQReplaced hyphen ("-") with underscore ("_") for output org-file name produced by sh_glred when run in combination mode (using -ncomb) to avoid clash when being read by another GLOBK program, e.g. ensum, bcsum, etc. Output combined org-file name now of the form globk_[expt]_[YYDoY]_[YYDoY].org rather than globk_[expt]_[YYDoY]-[DoY].org.”j§]”j±XYReplaced hyphen (“-â€) with underscore (“_â€) for output org-file name produced by sh_glred when run in combination mode (using -ncomb) to avoid clash when being read by another GLOBK program, e.g. ensum, bcsum, etc. Output combined org-file name now of the form globk_[expt]_[YYDoY]_[YYDoY].org rather than globk_[expt]_[YYDoY]-[DoY].org.”…””}”(j¶j•ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKaj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒECorrect the format for reading ATMOSMAP values from a VMF1 list file.”j§]”j±ŒECorrect the format for reading ATMOSMAP values from a VMF1 list file.”…””}”(j¶j£ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKgj¶j‰ÆjÇj‰Æubj`)”}”(j¦XsFix bug in gamit/lib/read_antex.f that caused PCO and PCV values to be zero if the frequency codes are written 'G 1' and 'G 2' instead of 'G01' and 'G02". This affects the following antennas using NOAA calibrations: TPSPG_A1_6+GP, SOK_GSR2700ISX, THA800961+REC, THA800961+RTK, THA800961RECUHF, THA800961RTKUHF, NOV702_3.00, JNSCR_C146-22-1, TRM_R6, TRM_R8, JAV_TRIUMPH-1.”j§]”j±XƒFix bug in gamit/lib/read_antex.f that caused PCO and PCV values to be zero if the frequency codes are written ‘G 1’ and ‘G 2’ instead of ‘G01’ and ‘G02â€. This affects the following antennas using NOAA calibrations: TPSPG_A1_6+GP, SOK_GSR2700ISX, THA800961+REC, THA800961+RTK, THA800961RECUHF, THA800961RTKUHF, NOV702_3.00, JNSCR_C146-22-1, TRM_R6, TRM_R8, JAV_TRIUMPH-1.”…””}”(j¶j±ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKij¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒöAltered sh_makeeqdef event naming logic so that all earthquakes found in catalogs are numbered sequentially and are only given two-character IDs (e.g. see below entry) after they are selected as potentially influencing a site in the .”j§]”j±ŒöAltered sh_makeeqdef event naming logic so that all earthquakes found in catalogs are numbered sequentially and are only given two-character IDs (e.g. see below entry) after they are selected as potentially influencing a site in the .”…””}”(j¶j¿ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKpj¶j‰ÆjÇj‰Æubj`)”}”(j¦XModfified glinit so that when the make_svs command is used, the satellite antenna offsets from the latest run (run time value) are adopted as the apriori antenna offsets. Needed when merging new processing (IGS08) with early MIT global files (e.g. in IGS05).”j§]”j±XModfified glinit so that when the make_svs command is used, the satellite antenna offsets from the latest run (run time value) are adopted as the apriori antenna offsets. Needed when merging new processing (IGS08) with early MIT global files (e.g. in IGS05).”…””}”(j¶jÍÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKuj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ€Add general relativity corrections to the orbital integration, changing scale and clock slightly but little affect on positions.”j§]”j±Œ€Add general relativity corrections to the orbital integration, changing scale and clock slightly but little affect on positions.”…””}”(j¶jÛÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKzj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒFixed bugs in the mean pole used in the ocean pole tide correction and in equate decoding in glorg. Updated model output in the SINEX files.”j§]”j±ŒFixed bugs in the mean pole used in the ocean pole tide correction and in equate decoding in glorg. Updated model output in the SINEX files.”…””}”(j¶jéÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK}j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ7Fix long-standing bug causing loss of a 32nd satellite.”j§]”j±Œ7Fix long-standing bug causing loss of a 32nd satellite.”…””}”(j¶j÷ÇjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK€j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒâFixed bug in kf/glinit/read_eq_file.f that could result in the end time of rename being incorrectly set for open ended renames. Fixed bug in kf/utils/stinf_to_rename.f that could result in misssed renames after the -post date.”j§]”j±ŒâFixed bug in kf/glinit/read_eq_file.f that could result in the end time of rename being incorrectly set for open ended renames. Fixed bug in kf/utils/stinf_to_rename.f that could result in misssed renames after the -post date.”…””}”(j¶jÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK‚j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒWIncrease max_sites in /kf/utils/merge_apr.f to accommodate the current itrf08_comb.apr.”j§]”j±ŒWIncrease max_sites in /kf/utils/merge_apr.f to accommodate the current itrf08_comb.apr.”…””}”(j¶jÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK‡j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒRAdded "-H" option to "find" commands in install_software to follow symbolic links.”j§]”j±ŒZAdded “-H†option to “find†commands in install_software to follow symbolic links.”…””}”(j¶j!ÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKŠj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒCIncrease the PID in the c-file name to 6 digits for large machines.”j§]”j±ŒCIncrease the PID in the c-file name to 6 digits for large machines.”…””}”(j¶j/ÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒMNew script sh_pbor_vel to create PBO-format velocity files from GLOBK output.”j§]”j±ŒMNew script sh_pbor_vel to create PBO-format velocity files from GLOBK output.”…””}”(j¶j=ÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ:Fix bug in sh_org2vel that causes some sites to be missed.”j§]”j±Œ:Fix bug in sh_org2vel that causes some sites to be missed.”…””}”(j¶jKÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK’j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ@Replace itrf00.apr with itrf08_comb.apr as default for sh_setup.”j§]”j±Œ@Replace itrf00.apr with itrf08_comb.apr as default for sh_setup.”…””}”(j¶jYÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK”j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒtAdded new scripts sh_cats and sh_hector in com/ to analyse noise charac- teristics of time series (using pos-files).”j§]”j±ŒtAdded new scripts sh_cats and sh_hector in com/ to analyse noise charac- teristics of time series (using pos-files).”…””}”(j¶jgÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK–j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒsUpdated glorg to allow multiple site selections in equate/unequate/force commands. Fixed typo in .pos file headers.”j§]”j±ŒsUpdated glorg to allow multiple site selections in equate/unequate/force commands. Fixed typo in .pos file headers.”…””}”(j¶juÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK™j¶j‰ÆjÇj‰Æubj`)”}”(j¦XŽChanged sh_makeeqdef "-pos " option to "-f " to avoid confusion with PBO-format pos-files; changed event ID sequencing scheme from purely numeric to purely two-character (01...99, then A1...A9, B1...B9 etc. until Z1...Z9, then 1A...1Z, 2A...2Z etc. until 9A...9Z); added option to use a translation table (e.g. see ~/gg/tables/eq.transtbl) to edit automatic ID to user-friendly alternative. All automatic IDs now contain at least one numeric character, while manual IDs are recommended to be two alphabetic characters, as always. Updated USGS earthquake search URL and made minor changes to event (re) naming logic in sh_makeeqdef.”j§]”j±X–Changed sh_makeeqdef “-pos †option to “-f †to avoid confusion with PBO-format pos-files; changed event ID sequencing scheme from purely numeric to purely two-character (01…99, then A1…A9, B1…B9 etc. until Z1…Z9, then 1A…1Z, 2A…2Z etc. until 9A…9Z); added option to use a translation table (e.g. see ~/gg/tables/eq.transtbl) to edit automatic ID to user-friendly alternative. All automatic IDs now contain at least one numeric character, while manual IDs are recommended to be two alphabetic characters, as always. Updated USGS earthquake search URL and made minor changes to event (re) naming logic in sh_makeeqdef.”…””}”(j¶jƒÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKœj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ\Updated coefficents for the solid-Earth pole tide to be consistent with IERS 2010 standards.”j§]”j±Œ\Updated coefficents for the solid-Earth pole tide to be consistent with IERS 2010 standards.”…””}”(j¶j‘ÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK¦j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒAdd libration terms to UT1.”j§]”j±ŒAdd libration terms to UT1.”…””}”(j¶jŸÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK©j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒLUpdated tsfit, tscon and tsjumps to allows ~ (home directory) in file names.”j§]”j±ŒLUpdated tsfit, tscon and tsjumps to allows ~ (home directory) in file names.”…””}”(j¶j­ÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK«j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¶Add a script sh_glist2cmd to invoke existing program glist2cmd, which creates from a glist a use_site list, an input file for unify_apr, and (new) an input site list for sh_makeqdef.”j§]”j±Œ¶Add a script sh_glist2cmd to invoke existing program glist2cmd, which creates from a glist a use_site list, an input file for unify_apr, and (new) an input site list for sh_makeqdef.”…””}”(j¶j»ÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK®j¶j‰ÆjÇj‰Æubj`)”}”(j¦XAdd the EPN cumulative solution to the ITRF2008 apr and eq files. Fixed bug causing bogus entries for 73 sites when EPN or NGS steps are inconsistent with those from ITRF2008 and IGS08. See tables/renames.bad for possible errors between early 2014 and June.”j§]”j±XAdd the EPN cumulative solution to the ITRF2008 apr and eq files. Fixed bug causing bogus entries for 73 sites when EPN or NGS steps are inconsistent with those from ITRF2008 and IGS08. See tables/renames.bad for possible errors between early 2014 and June.”…””}”(j¶jÉÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK²j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒvFix problem with poorly determined average of the east component of the atmospheric load for a site close to the pole.”j§]”j±ŒvFix problem with poorly determined average of the east component of the atmospheric load for a site close to the pole.”…””}”(j¶j×ÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK·j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ_sh_org2vel: Updated longitude/latitude format to five decimal places, in keeping with org-file.”j§]”j±Œ_sh_org2vel: Updated longitude/latitude format to five decimal places, in keeping with org-file.”…””}”(j¶jåÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKºj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œaftp_info: Modified for correct igni address for IONEX files; add PANGA, EPNCB, and TrigNet sites.”j§]”j±Œaftp_info: Modified for correct igni address for IONEX files; add PANGA, EPNCB, and TrigNet sites.”…””}”(j¶jóÈjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK½j¶j‰ÆjÇj‰Æubj`)”}”(j¦X7Added additional width to time axis in figures made by sh_plot_pos to prevent first and/or last time series points plotting beneath y-axes, and added -w option to control fraction of time series length to add (default 0.1 = 10% on both ends). Corrected expected residuals file name to plot after running tsfit.”j§]”j±X7Added additional width to time axis in figures made by sh_plot_pos to prevent first and/or last time series points plotting beneath y-axes, and added -w option to control fraction of time series length to add (default 0.1 = 10% on both ends). Corrected expected residuals file name to plot after running tsfit.”…””}”(j¶jÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÀj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ´svnav.dat: Correct start date for PN06/SV49---important bug affecting data for epochs 2013 12 19 thru 2014 4 3. Fix typo in start date for PRN30/SVN49 introduced in 121220 update.”j§]”j±Œ´svnav.dat: Correct start date for PN06/SV49—important bug affecting data for epochs 2013 12 19 thru 2014 4 3. Fix typo in start date for PRN30/SVN49 introduced in 121220 update.”…””}”(j¶jÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÅj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ)Fix bug in rotation derivatives in GLOBK.”j§]”j±Œ)Fix bug in rotation derivatives in GLOBK.”…””}”(j¶jÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÉj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒFix format error in svpos.”j§]”j±ŒFix format error in svpos.”…””}”(j¶j+ÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKËj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒXMove rotation and translation estimates to be next to PMU estimates in GLOBK print file.”j§]”j±ŒXMove rotation and translation estimates to be next to PMU estimates in GLOBK print file.”…””}”(j¶j9ÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÍj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒAFix gamit/utils/merge_rinex.f to handle more than 10 observables.”j§]”j±ŒAFix gamit/utils/merge_rinex.f to handle more than 10 observables.”…””}”(j¶jGÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÐj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒbUpdated wild card use in site names in mar_neu command (needed for change in sh_gen_stats script).”j§]”j±ŒbUpdated wild card use in site names in mar_neu command (needed for change in sh_gen_stats script).”…””}”(j¶jUÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÒj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒËEdited name of temporary file in install_software to avoid accidentally overwriting any libraries/Makefile.config.new when performing (and succeeding) with automatic search for X11LIBPATH and X11INCPATH.”j§]”j±ŒËEdited name of temporary file in install_software to avoid accidentally overwriting any libraries/Makefile.config.new when performing (and succeeding) with automatic search for X11LIBPATH and X11INCPATH.”…””}”(j¶jcÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÕj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¬Fixed bug in sh_get_orbits that caused IGS orbits from the CDDIS or SOPAC archive to be operational (igsf) rather than reprocessed (igs1) prior to GPS Week 1000 (1999/3/7).”j§]”j±Œ¬Fixed bug in sh_get_orbits that caused IGS orbits from the CDDIS or SOPAC archive to be operational (igsf) rather than reprocessed (igs1) prior to GPS Week 1000 (1999/3/7).”…””}”(j¶jqÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÙj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ1Updated tscon uto handle new Measures XYZ format.”j§]”j±Œ1Updated tscon uto handle new Measures XYZ format.”…””}”(j¶jÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÝj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ)Fix problem with computing GRACE seconds.”j§]”j±Œ)Fix problem with computing GRACE seconds.”…””}”(j¶jÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKßj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒXUpdate gamit/utils/autecl.f to allow deleting post-eclipes data for Block II satellites.”j§]”j±ŒXUpdate gamit/utils/autecl.f to allow deleting post-eclipes data for Block II satellites.”…””}”(j¶j›ÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKáj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒCFix end-of-year problem with dcb.dat. Thanks to S. Shimada of NIED,”j§]”j±ŒCFix end-of-year problem with dcb.dat. Thanks to S. Shimada of NIED,”…””}”(j¶j©ÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKäj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ Fixed bug in MODEL, introduced in December 2012, which caused GPT/GPT2 values to be used for mapping functions and dry zenith delays even if VMF1 was specified.”j§]”j±Œ Fixed bug in MODEL, introduced in December 2012, which caused GPT/GPT2 values to be used for mapping functions and dry zenith delays even if VMF1 was specified.”…””}”(j¶j·ÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKæj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ-Fix version number in sh_gamit. King 130727.”j§]”j±Œ-Fix version number in sh_gamit. King 130727.”…””}”(j¶jÅÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKêj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒFFix typos is globk_comb.cmd and glorg_long.cmd templates in gg/tables.”j§]”j±ŒFFix typos is globk_comb.cmd and glorg_long.cmd templates in gg/tables.”…””}”(j¶jÓÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKìj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒFFix bugs in fitting GAMIT's model to a broadcast ephemeris (sh_bcfit).”j§]”j±ŒHFix bugs in fitting GAMIT’s model to a broadcast ephemeris (sh_bcfit).”…””}”(j¶jáÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKîj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ^New option -subdir for sh_get_rinex to speed up uncompression when there are many RINEX files.”j§]”j±Œ^New option -subdir for sh_get_rinex to speed up uncompression when there are many RINEX files.”…””}”(j¶jïÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKðj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ›Update kf/Khandler/eq_name_chng.f so that _XPS/_XCL sites can not be renamed by later renames. RESET needed to rename _X?? sites if saved to binary hfile.”j§]”j±Œ›Update kf/Khandler/eq_name_chng.f so that _XPS/_XCL sites can not be renamed by later renames. RESET needed to rename _X?? sites if saved to binary hfile.”…””}”(j¶jýÉjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKój¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒŒUpdated grdtab for modification to CoM correction to S1/S2 tidal loading and correct detection of dates out of time range of map.grid files.”j§]”j±ŒŒUpdated grdtab for modification to CoM correction to S1/S2 tidal loading and correct detection of dates out of time range of map.grid files.”…””}”(j¶j ÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆK÷j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒLAdded lunisolar tables for 2015; Updated leap.sec for June 2015 leap second.”j§]”j±ŒLAdded lunisolar tables for 2015; Updated leap.sec for June 2015 leap second.”…””}”(j¶jÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKúj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒnAllow reading of a time-of-year-dependent grid for atmospheric tidal loading (not yet recommended by the IGS).”j§]”j±ŒnAllow reading of a time-of-year-dependent grid for atmospheric tidal loading (not yet recommended by the IGS).”…””}”(j¶j'ÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKüj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒkAdd glinit/solution_inf.f, glist/glist.f, and htoglb/cresnx_file.f to /kf to fix problem with null string.”j§]”j±ŒkAdd glinit/solution_inf.f, glist/glist.f, and htoglb/cresnx_file.f to /kf to fix problem with null string.”…””}”(j¶j5ÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆKÿj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒkAdd the Earth-radiation, antenna-radiation, and 2nd-order ionospheric model nmmes to the c-file and h-file.”j§]”j±ŒkAdd the Earth-radiation, antenna-radiation, and 2nd-order ionospheric model nmmes to the c-file and h-file.”…””}”(j¶jCÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ‡Various features and updates made to the suite of globk and tsxxx programs. See help files for new features. tscomp added to suite. .”j§]”j±Œ‡Various features and updates made to the suite of globk and tsxxx programs. See help files for new features. tscomp added to suite. .”…””}”(j¶jQÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ(Increase the dimensions for IONEX files.”j§]”j±Œ(Increase the dimensions for IONEX files.”…””}”(j¶j_ÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ:Increased dimensions in kf/utils/netsel.h Herring 140718”j§]”j±Œ:Increased dimensions in kf/utils/netsel.h Herring 140718”…””}”(j¶jmÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ.Enhancements to cplotx including adding color.”j§]”j±Œ.Enhancements to cplotx including adding color.”…””}”(j¶j{ÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ“Sped up search for earthquake/rename displacements, and corrected output for field overflow in org-file and multiple/duplicate renames in sh_exglk.”j§]”j±Œ“Sped up search for earthquake/rename displacements, and corrected output for field overflow in org-file and multiple/duplicate renames in sh_exglk.”…””}”(j¶j‰ÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¬sh_upd_stnfo: corrected bugs in kf/htoglb/mstinf.f in using IGS SINEX and GIPSY sta_svec files. Add a '-nogaps' option to close gaps in erroneous entries in IGS log files.”j§]”j±Œ°sh_upd_stnfo: corrected bugs in kf/htoglb/mstinf.f in using IGS SINEX and GIPSY sta_svec files. Add a ‘-nogaps’ option to close gaps in erroneous entries in IGS log files.”…””}”(j¶j—ÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒPsh_glred: Fix remaining bugs in allowing use of PBO-style h-files (.glb extent).”j§]”j±ŒPsh_glred: Fix remaining bugs in allowing use of PBO-style h-files (.glb extent).”…””}”(j¶j¥ÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒFixed long-standing typo in format statement in gamit/makexp/makexp.f producing a compile error with gfortran 4.6ff (but not earlier compilers).”j§]”j±ŒFixed long-standing typo in format statement in gamit/makexp/makexp.f producing a compile error with gfortran 4.6ff (but not earlier compilers).”…””}”(j¶j³ÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒpTRACK: Fix minor problem with noise_tol. Fix bug in wide-lane-reference combinations (read_all_rinex.f 130730).”j§]”j±ŒpTRACK: Fix minor problem with noise_tol. Fix bug in wide-lane-reference combinations (read_all_rinex.f 130730).”…””}”(j¶jÁÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ—New Receivers: TIASAHI PENG3100-R2, JAVAD TRIUMPH_1, JAVAD TRIUMPH_1M, JAVAD TRIUMPH2,MAG111406, NOV OEM4-G2, ITT 3750300, CHX90D-OPUS, ASHTECH PM-500.”j§]”j±Œ—New Receivers: TIASAHI PENG3100-R2, JAVAD TRIUMPH_1, JAVAD TRIUMPH_1M, JAVAD TRIUMPH2,MAG111406, NOV OEM4-G2, ITT 3750300, CHX90D-OPUS, ASHTECH PM-500.”…””}”(j¶jÏÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦X7New Antennas: TIAPENG3100R2, STHCR3-G3 , JAVTRIUMPH_1M, JAVTRIUMPH_1MR, JAVTRIUMPH_LSA, Antcom ACC123CGN_XN, TRM57971.00 SCIT, LEIAX1202A, LEIAX1202A, TPSCR.G3 SCIT, MAG111406, ASH701945A NONE, TRM55970.00, TRMR6, JAV_TRIUMPH-1R, CHX90D-OPUS, JAVTRIANT_A, JAVTRIANT_B,ASH700829.3 NONE, JAVTRIANT_A, JAVTRIANT_B.”j§]”j±X7New Antennas: TIAPENG3100R2, STHCR3-G3 , JAVTRIUMPH_1M, JAVTRIUMPH_1MR, JAVTRIUMPH_LSA, Antcom ACC123CGN_XN, TRM57971.00 SCIT, LEIAX1202A, LEIAX1202A, TPSCR.G3 SCIT, MAG111406, ASH701945A NONE, TRM55970.00, TRMR6, JAV_TRIUMPH-1R, CHX90D-OPUS, JAVTRIANT_A, JAVTRIANT_B,ASH700829.3 NONE, JAVTRIANT_A, JAVTRIANT_B.”…””}”(j¶jÝÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM!j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ** 10.50 vs 10.41”j§]”j±Œ** 10.50 vs 10.41”…””}”(j¶jëÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM(j¶j‰ÆjÇj‰Æubj`)”}”(j¦X-We have provided and will keep up-to-date, ITRF2008 coordinates sites in prior releases of the ITRF as well as new sites that have been and will be added for IGS processing. The primary file, in the ITRF2008 NNR frame is itrf08_comb.apr; and there are secondary files, itrf08_comb_[plate].apr, created by rotating this file to the frames of the major plates using the Euler poles estimated by Altamimi et al. [J. Geophys. Res., 117, B07402, doi:10.1029/2011JB008930,2012]. (Note that the plate-referenced files that we created 2012-01-06 and put into incremental_updates/tables were based on preliminary vectors that changed in the final publication, so users who downloaded these should replace them by the current files.) These files should always be used in conjunc- tion with the rename file itrf08_comb.eq to assure that the 8-character site name assigned to your data matches the coordinates for the appropri- ate period. See 'apr_and_eq_files.txt' in the download documentation directory for a complete explanation of how the combined files were constructed.”j§]”j±X1We have provided and will keep up-to-date, ITRF2008 coordinates sites in prior releases of the ITRF as well as new sites that have been and will be added for IGS processing. The primary file, in the ITRF2008 NNR frame is itrf08_comb.apr; and there are secondary files, itrf08_comb_[plate].apr, created by rotating this file to the frames of the major plates using the Euler poles estimated by Altamimi et al. [J. Geophys. Res., 117, B07402, doi:10.1029/2011JB008930,2012]. (Note that the plate-referenced files that we created 2012-01-06 and put into incremental_updates/tables were based on preliminary vectors that changed in the final publication, so users who downloaded these should replace them by the current files.) These files should always be used in conjunc- tion with the rename file itrf08_comb.eq to assure that the 8-character site name assigned to your data matches the coordinates for the appropri- ate period. See ‘apr_and_eq_files.txt’ in the download documentation directory for a complete explanation of how the combined files were constructed.”…””}”(j¶jùÊjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM*j¶j‰ÆjÇj‰Æubj`)”}”(j¦X2There are improved templates in ~/gg/tables for GLOBK runs: globk_comb.cmd, glorg_comb.cmd, globk_long.cmd, glorg_long.cmd. These reflect current best practice and take advantage of the 'option' feature of the globk, glorg, and sh_glred command lines so that the same command file can be used for both repeatabilities and velocity solutions without editing the file itself. The standard southern California example has been reworked to use these file and should now be easier to execute and to use as a template for your own processing. Also, there is a new detailed recipe for processing and analyzing survey-mode (sGPS) measurements, 'sGPS_recipe.txt', to be found in the documents directory of the download site and also on the web as part of the presentations from the recent workshop held at UNAVCO (Boulder13).”j§]”j±X:There are improved templates in ~/gg/tables for GLOBK runs: globk_comb.cmd, glorg_comb.cmd, globk_long.cmd, glorg_long.cmd. These reflect current best practice and take advantage of the ‘option’ feature of the globk, glorg, and sh_glred command lines so that the same command file can be used for both repeatabilities and velocity solutions without editing the file itself. The standard southern California example has been reworked to use these file and should now be easier to execute and to use as a template for your own processing. Also, there is a new detailed recipe for processing and analyzing survey-mode (sGPS) measurements, ‘sGPS_recipe.txt’, to be found in the documents directory of the download site and also on the web as part of the presentations from the recent workshop held at UNAVCO (Boulder13).”…””}”(j¶jËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM;j¶j‰ÆjÇj‰Æubj`)”}”(j¦X½The GPT/GMF models for zenith hydrostatic delay and mapping functions have been replaced by the new GPT2 model (Lager et al., Geophys. Res. Lett., ) which is based on a more refined numerical weather model, includes semi-annual as well as annual variations, has better spatial resolution, and accounts better for height differences through a seasonally dependent lapse rate. In the new model both the ZHD and mapping funtions are derived from a table, gpt.dat, automatically linked into the experiment and day directories from ~/gg/tables. If you specify GPT or GMT in your sestbl. and have gpt.dat in ~/gg/tables, you will automatically get GPT2 (the old GPT is invoked only if gpt.dat is missing).”j§]”j±X½The GPT/GMF models for zenith hydrostatic delay and mapping functions have been replaced by the new GPT2 model (Lager et al., Geophys. Res. Lett., ) which is based on a more refined numerical weather model, includes semi-annual as well as annual variations, has better spatial resolution, and accounts better for height differences through a seasonally dependent lapse rate. In the new model both the ZHD and mapping funtions are derived from a table, gpt.dat, automatically linked into the experiment and day directories from ~/gg/tables. If you specify GPT or GMT in your sestbl. and have gpt.dat in ~/gg/tables, you will automatically get GPT2 (the old GPT is invoked only if gpt.dat is missing).”…””}”(j¶jËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMIj¶j‰ÆjÇj‰Æubj`)”}”(j¦XLGLOBK now has the ability to remove non-tidal atmospheric loading (ATML) based on the average of the day given in the h-file. Since GLOBK can not yet read an grid file to apply the ATML corrections directly, if you want to investigate their effects, the best strategy is to apply the ATML in GAMIT and then optionally retain or remove the corrections using the new command -appload_mod in the GLOBK commaand file. The preferred ATML files for GAMIT are those that have been filtered to remove sub-daily terms (atmfilt_cm.YYYY). In principle, the sub-daily thermal tides should be applied in GAMIT, but none of the current models, including a time-dependent recently developed by Ray and Ponte, has been shown to reproduce accurately the tidal loading, so the present recommendation of the IGS for the next reprocessing is to omit these terms.”j§]”j±XLGLOBK now has the ability to remove non-tidal atmospheric loading (ATML) based on the average of the day given in the h-file. Since GLOBK can not yet read an grid file to apply the ATML corrections directly, if you want to investigate their effects, the best strategy is to apply the ATML in GAMIT and then optionally retain or remove the corrections using the new command -appload_mod in the GLOBK commaand file. The preferred ATML files for GAMIT are those that have been filtered to remove sub-daily terms (atmfilt_cm.YYYY). In principle, the sub-daily thermal tides should be applied in GAMIT, but none of the current models, including a time-dependent recently developed by Ray and Ponte, has been shown to reproduce accurately the tidal loading, so the present recommendation of the IGS for the next reprocessing is to omit these terms.”…””}”(j¶j#ËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMTj¶j‰ÆjÇj‰Æubj`)”}”(j¦XALiz Petrie of the University of Newcastle has coded a model in ARC for the accelerations on the GPS satellites due to antenna radiation and Earth radiation. These models are invoked by setting 'Earth radiation model = NCELE1', now default in the sestbl. and 'fixdrv'. As part of this modification, we have reworked many of the subroutines in ARC to be more modular, added (backward-compatible) models to the ARC batch file, and coded sh_get_orbits and sh_sp3fit to read the orbital models from from a sestbl. This latter change assures that the orbital models used for creating g- and t-files from sp3 files will be consistent with the models used for the data processing. For sh_gamit processsing, the sestbl. in ../tables is automatically linked into the /igs directory. If the sestbl is absent, hard-wired models will be used.”j§]”j±XILiz Petrie of the University of Newcastle has coded a model in ARC for the accelerations on the GPS satellites due to antenna radiation and Earth radiation. These models are invoked by setting ‘Earth radiation model = NCELE1’, now default in the sestbl. and ‘fixdrv’. As part of this modification, we have reworked many of the subroutines in ARC to be more modular, added (backward-compatible) models to the ARC batch file, and coded sh_get_orbits and sh_sp3fit to read the orbital models from from a sestbl. This latter change assures that the orbital models used for creating g- and t-files from sp3 files will be consistent with the models used for the data processing. For sh_gamit processsing, the sestbl. in ../tables is automatically linked into the /igs directory. If the sestbl is absent, hard-wired models will be used.”…””}”(j¶j1ËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMbj¶j‰ÆjÇj‰Æubj`)”}”(j¦X"Three model conventions have been updated to be consistent with those used by the IGS: mean pole and short-period EOP are changed from IERS 1996 to IERS 2010, and the gravity field from EGM96 to EGM08. These changes are important for EOP estimation but have neglible effect on positioning.”j§]”j±X"Three model conventions have been updated to be consistent with those used by the IGS: mean pole and short-period EOP are changed from IERS 1996 to IERS 2010, and the gravity field from EGM96 to EGM08. These changes are important for EOP estimation but have neglible effect on positioning.”…””}”(j¶j?ËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMoj¶j‰ÆjÇj‰Æubj`)”}”(j¦XíA new script sh_plot_pos will read PBO-style pos files rather than _mb files for plotting time series. GLOBK now generates the 'PBO' lines in the print files automatically (no need to use PBOP in the print options). We have retained sh_plotcrd and the use of _mb files for this release, but they will eventually go away. The Python script ts_plot.py, introduced in Release 10.40 to read pos files will also be abandoned because it required too many non-standard Python libraries (see below).”j§]”j±XñA new script sh_plot_pos will read PBO-style pos files rather than _mb files for plotting time series. GLOBK now generates the ‘PBO’ lines in the print files automatically (no need to use PBOP in the print options). We have retained sh_plotcrd and the use of _mb files for this release, but they will eventually go away. The Python script ts_plot.py, introduced in Release 10.40 to read pos files will also be abandoned because it required too many non-standard Python libraries (see below).”…””}”(j¶jMËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMuj¶j‰ÆjÇj‰Æubj`)”}”(j¦XÕThe new script sh_plot_elmean, together with additions to the autcln summary files allow plotting of mean residuals over several days as a function of elevation angle or satellite nadir angle, providing more diagnostics for bad antenna models or tracking environments. These can be used instead of or in conjuction with the individual-day sky plots and phase vs elevation plots produced by sh_oneway from the autcln DPH files when '-pres ELEV' specified with sh_gamit.”j§]”j±XÙThe new script sh_plot_elmean, together with additions to the autcln summary files allow plotting of mean residuals over several days as a function of elevation angle or satellite nadir angle, providing more diagnostics for bad antenna models or tracking environments. These can be used instead of or in conjuction with the individual-day sky plots and phase vs elevation plots produced by sh_oneway from the autcln DPH files when ‘-pres ELEV’ specified with sh_gamit.”…””}”(j¶j[ËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM}j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ** 10.41 vs 10.40”j§]”j±Œ** 10.41 vs 10.40”…””}”(j¶jiËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM…j¶j‰ÆjÇj‰Æubj`)”}”(j¦XNew receivers: TRIMBLE NETR3, R7 GNSS, and SPS852 ; LEICA GG02PLUS, GS08PLUS, GS09, GS12, GR25, and GS25; NOV OEM6; Ashtech PF500 and PF800;, NAVCOM SF-3040 SF-3050; Topcon TPSGR5; JAVAD TR_VS; SEPT POLARX4, POLARX4TR, and POLARXS; SOK GSR2700 RSX; SOUTH S82T GNSS and S82V GNSS; STONEX S9II GNSS; IFEN NX_NTR_303_D, NX_NTR_500_D, NX_NTR_600_D, SX_NSR_RT_200, SX_NSR_RT_300, SX_NSR_RT_400, SX_NSR_RT_401, SX_NSR_RT_402, SX_NSR_RT_700, and SX_NSR_RT_800. RNG FASA+, ITT 3750300, GEOMAX Zenith10, GEOMAX Zenith20 receivrs”j§]”j±XNew receivers: TRIMBLE NETR3, R7 GNSS, and SPS852 ; LEICA GG02PLUS, GS08PLUS, GS09, GS12, GR25, and GS25; NOV OEM6; Ashtech PF500 and PF800;, NAVCOM SF-3040 SF-3050; Topcon TPSGR5; JAVAD TR_VS; SEPT POLARX4, POLARX4TR, and POLARXS; SOK GSR2700 RSX; SOUTH S82T GNSS and S82V GNSS; STONEX S9II GNSS; IFEN NX_NTR_303_D, NX_NTR_500_D, NX_NTR_600_D, SX_NSR_RT_200, SX_NSR_RT_300, SX_NSR_RT_400, SX_NSR_RT_401, SX_NSR_RT_402, SX_NSR_RT_700, and SX_NSR_RT_800. RNG FASA+, ITT 3750300, GEOMAX Zenith10, GEOMAX Zenith20 receivrs”…””}”(j¶jwËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM‡j¶j‰ÆjÇj‰Æubj`)”}”(j¦XNew antennas: TRM_R6, TRM_R8. TRM55970,TRM59900.00, TRM59900.00, and TRMAG25; NOV533 (compact), NOV702_2.02 and NOV702_3.00; ASH701023.A and ASH70123.L1; LEIGS08, LEIGS12, LEIGG02PLUS, and LEIGS08PLUS;, NavCom NAV_ANT3001BR (AT1675-20W); JAV_TRIUMPH-1, JAVTRIUMPH_VS, JNSCR_C146-22-1 and four JPSREGANT; TPSHIPER_II, TPSHIPER_II+10, TPS NET-G3A, and TPSGR5; SEPCHOKE_MC; Navxperience NAX3G+C; Stonex STHS82_7224V3.0 and STXS9SA7224V3.0; Altus APSAPS-3; Rusnavgeoset RNG80971.00; ITT3750323; GeoMax GMXZENITH10 and GMXZENITH20.”j§]”j±XNew antennas: TRM_R6, TRM_R8. TRM55970,TRM59900.00, TRM59900.00, and TRMAG25; NOV533 (compact), NOV702_2.02 and NOV702_3.00; ASH701023.A and ASH70123.L1; LEIGS08, LEIGS12, LEIGG02PLUS, and LEIGS08PLUS;, NavCom NAV_ANT3001BR (AT1675-20W); JAV_TRIUMPH-1, JAVTRIUMPH_VS, JNSCR_C146-22-1 and four JPSREGANT; TPSHIPER_II, TPSHIPER_II+10, TPS NET-G3A, and TPSGR5; SEPCHOKE_MC; Navxperience NAX3G+C; Stonex STHS82_7224V3.0 and STXS9SA7224V3.0; Altus APSAPS-3; Rusnavgeoset RNG80971.00; ITT3750323; GeoMax GMXZENITH10 and GMXZENITH20.”…””}”(j¶j…ËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒiCorrect the values in hi.dat used to convert slant height to direct height for the TPSHIPER_PLUS antenna.”j§]”j±ŒiCorrect the values in hi.dat used to convert slant height to direct height for the TPSHIPER_PLUS antenna.”…””}”(j¶j“ËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM—j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ˜Fix typos in hi.dat entries for SEN14R, SENS49R, SENS96, SENS96, SEN96R, TPS721, TRSXDS, and TRSLDR antennas; add dimensions for Leica LEIAR25 antennas.”j§]”j±Œ˜Fix typos in hi.dat entries for SEN14R, SENS49R, SENS96, SENS96, SEN96R, TPS721, TRSXDS, and TRSLDR antennas; add dimensions for Leica LEIAR25 antennas.”…””}”(j¶j¡ËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMšj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒVUpdated Makefile.config.new (to be renamed to Makefile.config) for new Linux releases.”j§]”j±ŒVUpdated Makefile.config.new (to be renamed to Makefile.config) for new Linux releases.”…””}”(j¶j¯ËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒÈCreating an earthquake file: The script sh_makeeqdef has been updated to use hypercenter locations from the EHB bulletin (via ISC) up to the end of 2008, and from the standard ISC bulleint thereafter.”j§]”j±ŒÈCreating an earthquake file: The script sh_makeeqdef has been updated to use hypercenter locations from the EHB bulletin (via ISC) up to the end of 2008, and from the standard ISC bulleint thereafter.”…””}”(j¶j½ËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ:Update sh_get_hfiles for changes in the SOPAC archive ftp.”j§]”j±Œ:Update sh_get_hfiles for changes in the SOPAC archive ftp.”…””}”(j¶jËËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM¤j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ6Fix bug in reading more than 36 SVs from a RINEX file.”j§]”j±Œ6Fix bug in reading more than 36 SVs from a RINEX file.”…””}”(j¶jÙËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM¦j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ.Fix the p-file and h-file printout for SP EOP.”j§]”j±Œ.Fix the p-file and h-file printout for SP EOP.”…””}”(j¶jçËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM¨j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒvUpdate sh_get_orbits to use repro1 orbits when down loading igsf from CDDIS. These orbits are available week 730-1459.”j§]”j±ŒvUpdate sh_get_orbits to use repro1 orbits when down loading igsf from CDDIS. These orbits are available week 730-1459.”…””}”(j¶jõËjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMªj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ=Updated grdtab to remove S1/S2 tides from non-filtered grids.”j§]”j±Œ=Updated grdtab to remove S1/S2 tides from non-filtered grids.”…””}”(j¶jÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM­j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ•Change mapping of ietide for h-files: mean-pole-tide removed is now bit 4 (8), rather than bit 5 (16). Other minor changes to 'solve'; see sversn.f.”j§]”j±Œ™Change mapping of ietide for h-files: mean-pole-tide removed is now bit 4 (8), rather than bit 5 (16). Other minor changes to ‘solve’; see sversn.f.”…””}”(j¶jÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM¯j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒÆconvertc: Updates to check reasonableness, allow more file types, fix bug in reading vel file created by velrot with longer lines, and reverse the order from lat/lon to lon/lat for GEO or GEP files.”j§]”j±ŒÆconvertc: Updates to check reasonableness, allow more file types, fix bug in reading vel file created by velrot with longer lines, and reverse the order from lat/lon to lon/lat for GEO or GEP files.”…””}”(j¶jÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM²j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ+sh_get_nav, sh_get_orbits: Add wget option.”j§]”j±Œ+sh_get_nav, sh_get_orbits: Add wget option.”…””}”(j¶j-ÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM¶j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒŸsh_PBS_gamit: changed "mailto" variable to "mail_to because" of some conflict/problem returning blank argument to -M option in qsub command, which stalls qsub.”j§]”j±Œ§sh_PBS_gamit: changed “mailto†variable to “mail_to because†of some conflict/problem returning blank argument to -M option in qsub command, which stalls qsub.”…””}”(j¶j;ÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM¸j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒFsh_eq: Removed from /com since made obsolete by eq option of sh_exglk.”j§]”j±ŒFsh_eq: Removed from /com since made obsolete by eq option of sh_exglk.”…””}”(j¶jIÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM»j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œesh_metutil/metutil: Increase dimensions for z-file entries to allow 10-second sampling over 24 hours.”j§]”j±Œesh_metutil/metutil: Increase dimensions for z-file entries to allow 10-second sampling over 24 hours.”…””}”(j¶jWÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM½j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¾sh_gamit: Add '-alpha off' and '+antalias' to ImageMagic convert to avoid transparency and pixelation in converting sky plot images from Postscript to gif; change default aprf to itrf08.apr.”j§]”j±ŒÆsh_gamit: Add ‘-alpha off’ and ‘+antalias’ to ImageMagic convert to avoid transparency and pixelation in converting sky plot images from Postscript to gif; change default aprf to itrf08.apr.”…””}”(j¶jeÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÀj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒRUpdated hfupd.f and hfupd_ut.f to find renamed sites in station.info for updating.”j§]”j±ŒRUpdated hfupd.f and hfupd_ut.f to find renamed sites in station.info for updating.”…””}”(j¶jsÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÄj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ5Updated template sestbl. to fix typo for 'Mag field'.”j§]”j±Œ9Updated template sestbl. to fix typo for ‘Mag field’.”…””}”(j¶jÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÇj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ>Updated read_pmu_inp.f to account for GPS-UTC time difference.”j§]”j±Œ>Updated read_pmu_inp.f to account for GPS-UTC time difference.”…””}”(j¶jÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÉj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ-Fixed format "errors" in tsfit.f and tssum.f.”j§]”j±Œ1Fixed format “errors†in tsfit.f and tssum.f.”…””}”(j¶jÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMËj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ9Fix bug in computng average hydrological load for h-file.”j§]”j±Œ9Fix bug in computng average hydrological load for h-file.”…””}”(j¶j«ÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÍj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ!Added displace folder to updates.”j§]”j±Œ!Added displace folder to updates.”…””}”(j¶j¹ÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÏj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒLAllow by-passing uncompress when downloading RINEX files: /com/sh_get_rinex.”j§]”j±ŒLAllow by-passing uncompress when downloading RINEX files: /com/sh_get_rinex.”…””}”(j¶jÇÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÑj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ»Fixed bug in grdtab reading OSO list files with slightly different formats; correct comments for order of tokens on the grdtab command line. Copy from gamit/grdtab: grdtab, get_otl_list.”j§]”j±Œ»Fixed bug in grdtab reading OSO list files with slightly different formats; correct comments for order of tokens on the grdtab command line. Copy from gamit/grdtab: grdtab, get_otl_list.”…””}”(j¶jÕÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÓj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ9Added "GCR APTOL" warning to email summary from sh_gamit.”j§]”j±Œ=Added “GCR APTOL†warning to email summary from sh_gamit.”…””}”(j¶jãÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM×j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ«sh_get_orbits/sh_sp3fit/ngstot: GLONASS SVS can be can be present (but are ignored); add ESA finals (ESAF) as an orbit option; fix bug with SV id is blank rather than 'G'.”j§]”j±Œ¯sh_get_orbits/sh_sp3fit/ngstot: GLONASS SVS can be can be present (but are ignored); add ESA finals (ESAF) as an orbit option; fix bug with SV id is blank rather than ‘G’.”…””}”(j¶jñÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÙj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒÔsh_glred: add options to select the command file and to input a prefix string for the globk OPTION command; add ability to search for binary files with extent 'glb') (PBO, e.g.); fix problem with 'word too long'.”j§]”j±ŒÜsh_glred: add options to select the command file and to input a prefix string for the globk OPTION command; add ability to search for binary files with extent ‘glb’) (PBO, e.g.); fix problem with ‘word too long’.”…””}”(j¶jÿÌjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÝj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¸Changes to better handle CYGWIN installations. Copy com/unimake and libraries/Makefile.config.new (and rename to Makefile.config after checking for compatibility with local settings).”j§]”j±Œ¸Changes to better handle CYGWIN installations. Copy com/unimake and libraries/Makefile.config.new (and rename to Makefile.config after checking for compatibility with local settings).”…””}”(j¶j ÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMáj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒPUpdated sh_link_rinex and sh_PBS_gamit to use -expt option for links and copies.”j§]”j±ŒPUpdated sh_link_rinex and sh_PBS_gamit to use -expt option for links and copies.”…””}”(j¶jÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMåj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒbUpdated sh_get_rinex to allow >1000 site downloads. Error with Word too long in original version.”j§]”j±ŒbUpdated sh_get_rinex to allow >1000 site downloads. Error with Word too long in original version.”…””}”(j¶j)ÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMèj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒˆUpdate globk/autcln to implement new features (see help files) and updated pole tide definitions. Makefile.generic in gen_util updated.”j§]”j±ŒˆUpdate globk/autcln to implement new features (see help files) and updated pole tide definitions. Makefile.generic in gen_util updated.”…””}”(j¶j7ÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMëj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒŒNew script to compare a list of RINEX files with one or more station.info files to check for station.info.completeness, /com/sh_stinfo_list.”j§]”j±ŒŒNew script to compare a list of RINEX files with one or more station.info files to check for station.info.completeness, /com/sh_stinfo_list.”…””}”(j¶jEÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMîj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒlChanged the USNO ftp command in gg/tables/ftp_info to use passive transfer; necessary since 1 February 2012.”j§]”j±ŒlChanged the USNO ftp command in gg/tables/ftp_info to use passive transfer; necessary since 1 February 2012.”…””}”(j¶jSÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMñj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ‡Updated kf/ctogobs/proc_phsfin.f to output mean residuals by elevation in 1-deg bins. ELMEAN lines. Bins with no data list 99.9 values.”j§]”j±Œ‡Updated kf/ctogobs/proc_phsfin.f to output mean residuals by elevation in 1-deg bins. ELMEAN lines. Bins with no data list 99.9 values.”…””}”(j¶jaÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMôj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒEUpdated frame_to_fra.f with help option and plate to use the feature.”j§]”j±ŒEUpdated frame_to_fra.f with help option and plate to use the feature.”…””}”(j¶joÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM÷j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ`Allow automatic uncompressing of bzip2 files. Copy from com: sh_crx2rnx, sh_get_rinex, sh_gamit.”j§]”j±Œ`Allow automatic uncompressing of bzip2 files. Copy from com: sh_crx2rnx, sh_get_rinex, sh_gamit.”…””}”(j¶j}ÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMùj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒIFix bug in getting the average atmospheric loading value into the h-file.”j§]”j±ŒIFix bug in getting the average atmospheric loading value into the h-file.”…””}”(j¶j‹ÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMüj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ;Update 'profile' utility to handle changed vel-file format.”j§]”j±Œ?Update ‘profile’ utility to handle changed vel-file format.”…””}”(j¶j™ÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMþj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ Corrected "find" commands in install_software with trailing slashes to follow linked directories successfully when verifying or searching for libX11 and Xlib.h.”j§]”j±Œ¤Corrected “find†commands in install_software with trailing slashes to follow linked directories successfully when verifying or searching for libX11 and Xlib.h.”…””}”(j¶j§ÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ:Allow reading of ANTEX files with 0.5-degree grid spacing.”j§]”j±Œ:Allow reading of ANTEX files with 0.5-degree grid spacing.”…””}”(j¶jµÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ5Allow processing from c-files to check model changes.”j§]”j±Œ5Allow processing from c-files to check model changes.”…””}”(j¶jÃÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ†Read met values from a RINEX met file using free-format (work-around for improperly written RINEX v2 files). gamit/model/read_metrnx.”j§]”j±Œ†Read met values from a RINEX met file using free-format (work-around for improperly written RINEX v2 files). gamit/model/read_metrnx.”…””}”(j¶jÑÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒOAdded NONE command file name feature to tsfit.f (in help but not implemented) .”j§]”j±ŒOAdded NONE command file name feature to tsfit.f (in help but not implemented) .”…””}”(j¶jßÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ\Change to model/read_metrnx.f to allow reading of mis-formatted RINEX met files from Matera.”j§]”j±Œ\Change to model/read_metrnx.f to allow reading of mis-formatted RINEX met files from Matera.”…””}”(j¶jíÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM j¶j‰ÆjÇj‰Æubj`)”}”(j¦X2TRACK: Added new relative humidity option to GPT; fixed bug in velocity apriori coordinates; updated help file; new script sh_track_to_kml; account for model differences between L1 and L2; fix bug in reading the last epoch of an IONEX file; trap better bad clocks and data; add support for C2 range data.”j§]”j±X2TRACK: Added new relative humidity option to GPT; fixed bug in velocity apriori coordinates; updated help file; new script sh_track_to_kml; account for model differences between L1 and L2; fix bug in reading the last epoch of an IONEX file; trap better bad clocks and data; add support for C2 range data.”…””}”(j¶jûÍjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒntrackRT: TRACK updates plus fixed timing problem with trackRT and BNC2.5; updated handle BNC 2.6 feed format.”j§]”j±ŒntrackRT: TRACK updates plus fixed timing problem with trackRT and BNC2.5; updated handle BNC 2.6 feed format.”…””}”(j¶j ÎjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¡Update DLAPACK routines to current versions to avoid a bug effective with gfortran 4.6 when run with optimization (now default unless -mno-align-double is sset).”j§]”j±Œ¡Update DLAPACK routines to current versions to avoid a bug effective with gfortran 4.6 when run with optimization (now default unless -mno-align-double is sset).”…””}”(j¶jÎjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ@Fix bug in kf/svpos/svdiff.f when more than 12-channels of data.”j§]”j±Œ@Fix bug in kf/svpos/svdiff.f when more than 12-channels of data.”…””}”(j¶j%ÎjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¢sh_upd_stnfo/mtinf: Fix bug with in and out station.info files with rx files; fix -rxo option; increase dimensions to work with current SOPAC station.info files.”j§]”j±Œ¢sh_upd_stnfo/mtinf: Fix bug with in and out station.info files with rx files; fix -rxo option; increase dimensions to work with current SOPAC station.info files.”…””}”(j¶j3ÎjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj e)”}”(j¦hoj§]”je)”}”(j¦Œ‘sh_setup: Change to copy in whatever is linked was station.info in ~/gg/tables, now nominally station.info.mit. Rename station.info.sopac.newfmt”j§]”(je)”}”(j¦ŒBsh_setup: Change to copy in whatever is linked was station.info in”j§]”j±ŒBsh_setup: Change to copy in whatever is linked was station.info in”…””}”(j¶jHÎjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj¸ÆjÆM!j¶jDÎubj3e)”}”(j¦hoj§]”j`)”}”(j¦ŒN~/gg/tables, now nominally station.info.mit. Rename station.info.sopac.newfmt”j§]”j±ŒN~/gg/tables, now nominally station.info.mit. Rename station.info.sopac.newfmt”…””}”(j¶jYÎjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM"j¶jVÎubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jDÎubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj¸ÆjÆM!j¶jAÎubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶j‰ÆjÇj‰Æhj¸ÆjÆNubj`)”}”(j¦Œto station.info.sopac.”j§]”j±Œto station.info.sopac.”…””}”(j¶jyÎjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM#j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œsh_makeeqdef: New script to create globk earthquake file from ”…””}”(j¶j!ÏjÇj‰ÆhNjÆNubj÷ )”}”(j¦Œhttp://neic.usgs.gov/”j§]”j±Œhttp://neic.usgs.gov/”…””}”(j¶j)ÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j+ÏujÄjö j¶j!Ïubj±Œ catalog.”…””}”(j¶j!ÏjÇj‰ÆhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM>j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒTThe command 'reset' in the eq_file will reset all of the input site extents to _GPS.”j§]”j±ŒXThe command ‘reset’ in the eq_file will reset all of the input site extents to _GPS.”…””}”(j¶jBÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMAj¶j‰ÆjÇj‰Æubj`)”}”(j¦XAdded a white-noise process to the mar_scale command so that some process noise can be applied between to h-files at the same time, useful if they were generated with differeent scales, e.g., ITRF2005 for IGS repro1 and ITRF2008 for data processed using itrf08_comb.apr.”j§]”j±XAdded a white-noise process to the mar_scale command so that some process noise can be applied between to h-files at the same time, useful if they were generated with differeent scales, e.g., ITRF2005 for IGS repro1 and ITRF2008 for data processed using itrf08_comb.apr.”…””}”(j¶jPÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMDj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ9Allow 'getrel' to work with newer GLOBK velocity formats.”j§]”j±Œ=Allow ‘getrel’ to work with newer GLOBK velocity formats.”…””}”(j¶j^ÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMIj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒuUpdated kf/utils/stinf_to_rename.f to handle current scheme of using only a 4-character ID for the initial site name.”j§]”j±ŒuUpdated kf/utils/stinf_to_rename.f to handle current scheme of using only a 4-character ID for the initial site name.”…””}”(j¶jlÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMKj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ;Fix serious bug in ARC affecting the SV yaw during eclipse.”j§]”j±Œ;Fix serious bug in ARC affecting the SV yaw during eclipse.”…””}”(j¶jzÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMNj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒžFix bug in failing to use C2 when both C2 and P2 indicated with the RINEX header but P2 zero for SVs that have C2. Copy gamit/lib/rrinex.f. Kogan/King 110420”j§]”j±ŒžFix bug in failing to use C2 when both C2 and P2 indicated with the RINEX header but P2 zero for SVs that have C2. Copy gamit/lib/rrinex.f. Kogan/King 110420”…””}”(j¶jˆÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMPj¶j‰ÆjÇj‰Æubj`)”}”(j¦XKFix bug in failure to apply center-of-mass correction (CMC) for ocean tide models when translating sp3 files to t-files; fix bug in writing MIT sp3 files. Add 'status' message for CMC corrections in both ngstot and ttongs. Copy from gamit/orbits: oversn.f, ngstot.f, rsp3hd.f, ttongs.f, wsp3hd.f, and sdtrit.f. Kogan/King 110414”j§]”j±XOFix bug in failure to apply center-of-mass correction (CMC) for ocean tide models when translating sp3 files to t-files; fix bug in writing MIT sp3 files. Add ‘status’ message for CMC corrections in both ngstot and ttongs. Copy from gamit/orbits: oversn.f, ngstot.f, rsp3hd.f, ttongs.f, wsp3hd.f, and sdtrit.f. Kogan/King 110414”…””}”(j¶j–ÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMTj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ-Fix bogus header in ANTEX file. King 110322”j§]”j±Œ-Fix bogus header in ANTEX file. King 110322”…””}”(j¶j¤ÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMZj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒûAllow use of IERS2010 model for short-period EOP (Ray model still default). Copy cversn.f, pmut1_oceans.f, and Makefile.generic from /libraries/comlib; lversn.f and srotat.f from gamit/lib; fversn.f and mdmake.f from gamit/fixdrv. Herring/King 110223”j§]”j±ŒûAllow use of IERS2010 model for short-period EOP (Ray model still default). Copy cversn.f, pmut1_oceans.f, and Makefile.generic from /libraries/comlib; lversn.f and srotat.f from gamit/lib; fversn.f and mdmake.f from gamit/fixdrv. Herring/King 110223”…””}”(j¶j²ÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM\j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒYFix htoglb bug in making ephemeris file (occurs only with Intel compiler). Herring 110202”j§]”j±ŒYFix htoglb bug in making ephemeris file (occurs only with Intel compiler). Herring 110202”…””}”(j¶jÀÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM`j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒTChange default setting in sh_plotvel to be compatible with GMT4. Ferhat/King 110119”j§]”j±ŒTChange default setting in sh_plotvel to be compatible with GMT4. Ferhat/King 110119”…””}”(j¶jÎÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMbj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒcFix problem with setting day-loop span in sh_gamit with some operating systems. Shimada/King 110117”j§]”j±ŒcFix problem with setting day-loop span in sh_gamit with some operating systems. Shimada/King 110117”…””}”(j¶jÜÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMdj¶j‰ÆjÇj‰Æubj`)”}”(j¦X°Copy into /tables itrf08.apr, IGS08_101117.apr (current IGS) (from IGS08.ssc), and IGS08_101117.eq (GLOBK rename, from soln_IGS08.snx) files. The eq fiile has names matching those in both itrf08.apr and IGS08_101117.apr; note, however, that the IGS files may have discontinuities later than those accounted for in itrf08.apr, and that the IGS08 apr file will not include coordinates for early segments used in ITRF2008. King 110106”j§]”j±X°Copy into /tables itrf08.apr, IGS08_101117.apr (current IGS) (from IGS08.ssc), and IGS08_101117.eq (GLOBK rename, from soln_IGS08.snx) files. The eq fiile has names matching those in both itrf08.apr and IGS08_101117.apr; note, however, that the IGS files may have discontinuities later than those accounted for in itrf08.apr, and that the IGS08 apr file will not include coordinates for early segments used in ITRF2008. King 110106”…””}”(j¶jêÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMfj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ_Allow sh_find_data to work over a year boundary. Copy from /com. Shimada/McClusky/King 110106”j§]”j±Œ_Allow sh_find_data to work over a year boundary. Copy from /com. Shimada/McClusky/King 110106”…””}”(j¶jøÏjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMmj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ–Add the 2011 lunisolar tables to incremental_updates/tables/. (luntab and soltab were in the 10.4 distribution, but nutabl. was missing). King 110104”j§]”j±Œ–Add the 2011 lunisolar tables to incremental_updates/tables/. (luntab and soltab were in the 10.4 distribution, but nutabl. was missing). King 110104”…””}”(j¶jÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMoj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒXRemove bogus test on t-file year > 2010. Copy gamit/fixdrv/armake.f. King 110101/110103”j§]”j±ŒXRemove bogus test on t-file year > 2010. Copy gamit/fixdrv/armake.f. King 110101/110103”…””}”(j¶jÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMrj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ/Allow more up to 20 observables in RINEX files.”j§]”j±Œ/Allow more up to 20 observables in RINEX files.”…””}”(j¶j"ÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMtj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ@Updated glist to output of sites by time all on one (long) line.”j§]”j±Œ@Updated glist to output of sites by time all on one (long) line.”…””}”(j¶j0ÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMvj¶j‰ÆjÇj‰Æubj e)”}”(j¦hoj§]”je)”}”(j¦ŒŸUpdated treatment of coordinates in renames globk (fixed problem with XCL renames with earthquakes that have been previously applied). Khandler/eq_name_chng.f ”j§]”(je)”}”(j¦ŒbUpdated treatment of coordinates in renames globk (fixed problem with XCL renames with earthquakes”j§]”j±ŒbUpdated treatment of coordinates in renames globk (fixed problem with XCL renames with earthquakes”…””}”(j¶jEÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj¸ÆjÆMyj¶jAÐubj3e)”}”(j¦hoj§]”j`)”}”(j¦Œ;that have been previously applied). Khandler/eq_name_chng.f”j§]”j±Œ;that have been previously applied). Khandler/eq_name_chng.f”…””}”(j¶jVÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMyj¶jSÐubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jAÐubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj¸ÆjÆMyj¶j>Ðubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶j‰ÆjÇj‰Æhj¸ÆjÆNubj`)”}”(j¦ŒNCorrect a bug in sh_gamit when linking IONEX files with multiple experiments.”j§]”j±ŒNCorrect a bug in sh_gamit when linking IONEX files with multiple experiments.”…””}”(j¶jvÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM{j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒJAdd slant heights for the TRM39105.00 (Zephyr w/o ground plane) to hi.dat.”j§]”j±ŒJAdd slant heights for the TRM39105.00 (Zephyr w/o ground plane) to hi.dat.”…””}”(j¶j„ÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM}j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒFCorrect the echo of the atmospheric tidal loading model in the p-file.”j§]”j±ŒFCorrect the echo of the atmospheric tidal loading model in the p-file.”…””}”(j¶j’ÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ** 10.4 vs 10.35”j§]”j±Œ** 10.4 vs 10.35”…””}”(j¶j ÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM‚j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ‘Introduction of a real-time kinematic module, trackRT. See help/trackRT.hlp for a complete description including instructions for installation.”j§]”j±Œ‘Introduction of a real-time kinematic module, trackRT. See help/trackRT.hlp for a complete description including instructions for installation.”…””}”(j¶j®ÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM„j¶j‰ÆjÇj‰Æubj`)”}”(j¦XŽChanges to the code and svnav.dat to use an appropriate radiation-pressure model and antenna offset for Block IIF satellites (only PN 25 thus far). If you need to combine new processing with MIT or SOPAC global h-files that used the old models set ' apr_svs prn_12 100 100 100 10 10 10 0R ' to unlink the radiation pressure models. Both MIT and SOPAC will rerun these days to remove the problem.”j§]”j±X’Changes to the code and svnav.dat to use an appropriate radiation-pressure model and antenna offset for Block IIF satellites (only PN 25 thus far). If you need to combine new processing with MIT or SOPAC global h-files that used the old models set ‘ apr_svs prn_12 100 100 100 10 10 10 0R ‘ to unlink the radiation pressure models. Both MIT and SOPAC will rerun these days to remove the problem.”…””}”(j¶j¼ÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM‡j¶j‰ÆjÇj‰Æubj`)”}”(j¦X˜Two new programs, tscon and tsfit, are available for prototyping GLOBK solutions. They allow you to convert PBO, REASON, and other time series to GLOBK formats and to generate in an iterative but rapid fashion appropriate models for discontinuities and earthquakes in continuous time series prior to making long globk runs. See Chapter 4 of the GLOBK Reference Manual and the help files for tscon and tsfit.”j§]”j±X˜Two new programs, tscon and tsfit, are available for prototyping GLOBK solutions. They allow you to convert PBO, REASON, and other time series to GLOBK formats and to generate in an iterative but rapid fashion appropriate models for discontinuities and earthquakes in continuous time series prior to making long globk runs. See Chapter 4 of the GLOBK Reference Manual and the help files for tscon and tsfit.”…””}”(j¶jÊÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMŽj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ’There is a new example, better designed for instruction on setting up processing with new data and incorporating a multi-year solution with GLOBK.”j§]”j±Œ’There is a new example, better designed for instruction on setting up processing with new data and incorporating a multi-year solution with GLOBK.”…””}”(j¶jØÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM”j¶j‰ÆjÇj‰Æubj`)”}”(j¦X8The c-file and h-file formats have changed. C-files from prior releases cannot be used, but the code remains compatible with older GAMIT (ascii) and GLOBK (binary) h-files. The impetus for this change was to better document models used in the processing, particularly for receiver and satellite antenna models.”j§]”j±X8The c-file and h-file formats have changed. C-files from prior releases cannot be used, but the code remains compatible with older GAMIT (ascii) and GLOBK (binary) h-files. The impetus for this change was to better document models used in the processing, particularly for receiver and satellite antenna models.”…””}”(j¶jæÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM—j¶j‰ÆjÇj‰Æubj`)”}”(j¦X Higher-order ionospheric (HOI) corrections (2nd and 3rd order, but not bending) are available in GAMIT, as described by Petrie et al. [J. Geophys. Res., 115, B03417, doi:10.1029/2009jb006677, 2010]. Using these terms requires downloading daily IONEX files containing total electron content (TEC) at 2-hr intervals from CODE into the [expt]/ionex directory and linking these into the day directory using '-ion' in the sh_gamit command file. To apply the effects in processing, set 'Ion model = GMAP' and 'Mag field = ITRF11' in the sestbl. See the new Chapter 8 of the GAMIT Reference Manual for more details. Thanks to Liz Petrie of Newcastle U (UK) for most of the work on this, and to Andrzej Araszkiewicz the Military U of Technology (Poland) for important contributions.”j§]”j±XHigher-order ionospheric (HOI) corrections (2nd and 3rd order, but not bending) are available in GAMIT, as described by Petrie et al. [J. Geophys. Res., 115, B03417, doi:10.1029/2009jb006677, 2010]. Using these terms requires downloading daily IONEX files containing total electron content (TEC) at 2-hr intervals from CODE into the [expt]/ionex directory and linking these into the day directory using ‘-ion’ in the sh_gamit command file. To apply the effects in processing, set ‘Ion model = GMAP’ and ‘Mag field = ITRF11’ in the sestbl. See the new Chapter 8 of the GAMIT Reference Manual for more details. Thanks to Liz Petrie of Newcastle U (UK) for most of the work on this, and to Andrzej Araszkiewicz the Military U of Technology (Poland) for important contributions.”…””}”(j¶jôÐjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒñThe procedure for creating and keeping an updated station.info file has been better documented and enhanced by changes to sh_upd_stnfo. See the description on p. 27 of the Introduction to GAMIT/GLOBK manual, or the README of the new example.”j§]”j±ŒñThe procedure for creating and keeping an updated station.info file has been better documented and enhanced by changes to sh_upd_stnfo. See the description on p. 27 of the Introduction to GAMIT/GLOBK manual, or the README of the new example.”…””}”(j¶jÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM©j¶j‰ÆjÇj‰Æubj`)”}”(j¦XuGLOBK will now accept multiple eq_files, allowing you to configure separate files for earthquakes, breaks, and editing (_XPS, XCL). If an eq_file entry uses the 'break' command rather than the 'rename' command, globk will assign the extent. A new RENM print option causes the full rename list to be output. glist now also allows for multiple eq_files, separated by colons.”j§]”j±X}GLOBK will now accept multiple eq_files, allowing you to configure separate files for earthquakes, breaks, and editing (_XPS, XCL). If an eq_file entry uses the ‘break’ command rather than the ‘rename’ command, globk will assign the extent. A new RENM print option causes the full rename list to be output. glist now also allows for multiple eq_files, separated by colons.”…””}”(j¶jÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM®j¶j‰ÆjÇj‰Æubj`)”}”(j¦X9We are now providing in the GRIDS directory on everest.mit.edu atmospheric loading files that have been filtered to remove the diurnal and semi-diurnal thermal tides (S1, S2) using the procedure described by Tregoning and Watson (J. Geophys. Res., 14, B09403, doi:10.1029/2009JB006344, 2009). These can be used in conjunction with atl.grid (also on everest) comprising the IERS standard S1,S2 tides (Ponte and Ray, Geophys. Res. Lett.,29, 2153, doi:10.1029/ 2002GL016340, 2002) by renaming the filtered files (atmfilt_cm.YYYY) to the standard name for unfiltered files (atmdisp_cm.YYYY) in gg/tables, and setting 'Use atl.grid = Y' and 'Tides applied = 63' in the sestbl. Based on feedback from users, we hope to eventually discontinue distribution of the unfiltered grids. Note that earlier versions of the filtered files, from either ANU or MIT, were written incorrectly; further, there was a bug in the 'model' routine that read the sub-daily ATL from the u-file, causing the north and up components to be reversed. Any use of ATL should use the new grids and Release 10.4.”j§]”j±XEWe are now providing in the GRIDS directory on everest.mit.edu atmospheric loading files that have been filtered to remove the diurnal and semi-diurnal thermal tides (S1, S2) using the procedure described by Tregoning and Watson (J. Geophys. Res., 14, B09403, doi:10.1029/2009JB006344, 2009). These can be used in conjunction with atl.grid (also on everest) comprising the IERS standard S1,S2 tides (Ponte and Ray, Geophys. Res. Lett.,29, 2153, doi:10.1029/ 2002GL016340, 2002) by renaming the filtered files (atmfilt_cm.YYYY) to the standard name for unfiltered files (atmdisp_cm.YYYY) in gg/tables, and setting ‘Use atl.grid = Y’ and ‘Tides applied = 63’ in the sestbl. Based on feedback from users, we hope to eventually discontinue distribution of the unfiltered grids. Note that earlier versions of the filtered files, from either ANU or MIT, were written incorrectly; further, there was a bug in the ‘model’ routine that read the sub-daily ATL from the u-file, causing the north and up components to be reversed. Any use of ATL should use the new grids and Release 10.4.”…””}”(j¶jÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM´j¶j‰ÆjÇj‰Æubj`)”}”(j¦XšThere is a new plotting script, ts_plot.py, that reads PBO-style time- series files (.pos), created by tscon or tssum, rather than the mb_-files created by ensum. We plan to transition to the .pos format eventually since it is more complete and flexible, but this will happen slowly and only when we're sure that users can easily install all of the libraries needed to run ts_plot.py: Python V2.7 ( http://www.python.org/download/ ); Numpy ( http://new.scipy.org/download.html ), optionally scipy; matplotlib ( http://sourceforge.net/projects/matplotlib/files/matplotlib/matplotlib-1.0/ ) and egenix-mx-base-3.1.3 ( http://www.egenix.com/products/python/mxBase/ ).”j§]”(j±Œ‡There is a new plotting script, ts_plot.py, that reads PBO-style time- series files (.pos), created by tscon or tssum, rather than the ”…””}”(j¶j,ÑjÇj‰ÆhNjÆNubj»)”}”(j¦Œmb_”j§]”j±Œmb_”…””}”j¶j4Ñsbaj·}”(j¹]”Œid2”aj»]”j½]”jÀ]”jÂ]”Œrefid”Œid1”ujÄjœ»j¶j,ÑjÇj‰ÆhNjÆNubj±X -files created by ensum. We plan to transition to the .pos format eventually since it is more complete and flexible, but this will happen slowly and only when we’re sure that users can easily install all of the libraries needed to run ts_plot.py: Python V2.7 ( ”…””}”(j¶j,ÑjÇj‰ÆhNjÆNubj÷ )”}”(j¦Œhttp://www.python.org/download/”j§]”j±Œhttp://www.python.org/download/”…””}”(j¶jIÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jKÑujÄjö j¶j,Ñubj±Œ ); Numpy ( ”…””}”(j¶j,ÑjÇj‰ÆhNjÆNubj÷ )”}”(j¦Œ"http://new.scipy.org/download.html”j§]”j±Œ"http://new.scipy.org/download.html”…””}”(j¶j\ÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j^ÑujÄjö j¶j,Ñubj±Œ# ), optionally scipy; matplotlib ( ”…””}”(j¶j,ÑjÇj‰ÆhNjÆNubj÷ )”}”(j¦ŒKhttp://sourceforge.net/projects/matplotlib/files/matplotlib/matplotlib-1.0/”j§]”j±ŒKhttp://sourceforge.net/projects/matplotlib/files/matplotlib/matplotlib-1.0/”…””}”(j¶joÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jqÑujÄjö j¶j,Ñubj±Œ ) and egenix-mx-base-3.1.3 ( ”…””}”(j¶j,ÑjÇj‰ÆhNjÆNubj÷ )”}”(j¦Œ-http://www.egenix.com/products/python/mxBase/”j§]”j±Œ-http://www.egenix.com/products/python/mxBase/”…””}”(j¶j‚ÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j„ÑujÄjö j¶j,Ñubj±Œ ).”…””}”(j¶j,ÑjÇj‰ÆhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÃj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¦Changes to tsview to enhance performance when viewing and editing large numbers of time series; recording of the reasons for edits when creating entries for eq_files.”j§]”j±Œ¦Changes to tsview to enhance performance when viewing and editing large numbers of time series; recording of the reasons for edits when creating entries for eq_files.”…””}”(j¶j›ÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÍj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒÆThere are updates to autcln and solve to better handle single-frequency data. The default in autcln now requires the user to include 'L1only' in the autcln.cmd file to process single-frequency data.”j§]”j±ŒÊThere are updates to autcln and solve to better handle single-frequency data. The default in autcln now requires the user to include ‘L1only’ in the autcln.cmd file to process single-frequency data.”…””}”(j¶j©ÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÑj¶j‰ÆjÇj‰Æubj`)”}”(j¦X÷Pseudorange resolution of wide-lane ambiguities (LC_AUTCLN) is now recommended for networks larger than 50 km and data from January 1994 (except with codeless receivers), the date from which empirically determined differential code biases (DCB) for each SV have been determined (dcb.dat) by AIUB. A new algorithm, implemented for Release 10.34, is more robust than the earlier one and gives some weight to the ionsophere-constrained phase WL. The defaults controls should work well for most networks with recent data, but you may want to test increasing the 'ion constraint' value (from the default .01 to .02) under maximum ionspheric conditions (2000-2002), or decreasing the value (to .005) for old data under minimum ionospheric conditions (1994-1998).”j§]”j±XûPseudorange resolution of wide-lane ambiguities (LC_AUTCLN) is now recommended for networks larger than 50 km and data from January 1994 (except with codeless receivers), the date from which empirically determined differential code biases (DCB) for each SV have been determined (dcb.dat) by AIUB. A new algorithm, implemented for Release 10.34, is more robust than the earlier one and gives some weight to the ionsophere-constrained phase WL. The defaults controls should work well for most networks with recent data, but you may want to test increasing the ‘ion constraint’ value (from the default .01 to .02) under maximum ionspheric conditions (2000-2002), or decreasing the value (to .005) for old data under minimum ionospheric conditions (1994-1998).”…””}”(j¶j·ÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMÕj¶j‰ÆjÇj‰Æubj`)”}”(j¦X;There are now IGS RINEX files with as many as 11 obervables, requiring an update of the code (rrxhed and rrinex in gamit/lib) and remaking the executables with MAXOBT=11 in gamit/includes/makex.h. IGS ANTEX files begining with igs05_1499.atx have more comment lines than we originally coded (50). Set MAXTXT=1000 in gamit/includes/dimpar.h. and remake gamit. Prior to an October 2008 incremental update to 10.34, failure to make this change will result in a cryptic failure in suggesting a misnamed receiver or antenna. Release 10.4 will recognize ANTEX Version 1.4.”j§]”j±X;There are now IGS RINEX files with as many as 11 obervables, requiring an update of the code (rrxhed and rrinex in gamit/lib) and remaking the executables with MAXOBT=11 in gamit/includes/makex.h. IGS ANTEX files begining with igs05_1499.atx have more comment lines than we originally coded (50). Set MAXTXT=1000 in gamit/includes/dimpar.h. and remake gamit. Prior to an October 2008 incremental update to 10.34, failure to make this change will result in a cryptic failure in suggesting a misnamed receiver or antenna. Release 10.4 will recognize ANTEX Version 1.4.”…””}”(j¶jÅÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMàj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¾Fix a bug in time argument for GPT; affects the annual signal in heights at the level of 0.2-1.0 mm. Thanks to Francois Fund (ESGT) for catching this and Paul Tregoning (ANU) for testing it.”j§]”j±Œ¾Fix a bug in time argument for GPT; affects the annual signal in heights at the level of 0.2-1.0 mm. Thanks to Francois Fund (ESGT) for catching this and Paul Tregoning (ANU) for testing it.”…””}”(j¶jÓÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMéj¶j‰ÆjÇj‰Æubj`)”}”(j¦X1Fix bugs and deficiencies in sh_upd_stnfo/mstinf to obtain a better match of entries with RINEX files and to avoid multiple entries continuous stations when not needed. Add the ability to get a station list from sites.defaults and/or the /rinex directory, and the ability to use wildcards to get multiple IGS log files. Fix bug in distinguishing between Receiver Type' and 'Receiver SN', and 'Antenna Type' and 'Antenna SN' in reading station.info files (thanks to Olivier Charade (INSU/CNRS), allow more complete updating of station.info entries mid-session.”j§]”j±X?Fix bugs and deficiencies in sh_upd_stnfo/mstinf to obtain a better match of entries with RINEX files and to avoid multiple entries continuous stations when not needed. Add the ability to get a station list from sites.defaults and/or the /rinex directory, and the ability to use wildcards to get multiple IGS log files. Fix bug in distinguishing between Receiver Type’ and ‘Receiver SN’, and ‘Antenna Type’ and ‘Antenna SN’ in reading station.info files (thanks to Olivier Charade (INSU/CNRS), allow more complete updating of station.info entries mid-session.”…””}”(j¶jáÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMíj¶j‰ÆjÇj‰Æubj`)”}”(j¦XLFix two bugs in fixdrv, both introduced in 10.35: 1) full-solution observable erroneously set when quick_pre observable = LC (allowed for backward compatibility) rather than LC_ONLY (preferred); 2) check on too-tight a priori coordinate constraints failed in sh_sigelv. Thanks to Liz Petrie (Newcastle) for catching both of these.”j§]”j±XLFix two bugs in fixdrv, both introduced in 10.35: 1) full-solution observable erroneously set when quick_pre observable = LC (allowed for backward compatibility) rather than LC_ONLY (preferred); 2) check on too-tight a priori coordinate constraints failed in sh_sigelv. Thanks to Liz Petrie (Newcastle) for catching both of these.”…””}”(j¶jïÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMöj¶j‰ÆjÇj‰Æubj`)”}”(j¦XFix bug in sh_get_nav when the day number has leading zeroes, needed for CDDIS downloads with tscsh (one line of code missed in fixes applied to most scripts for 10.35 release). Thanks to S Shimada of NIED for the catch and Mark Murray for additional cleanup.”j§]”j±XFix bug in sh_get_nav when the day number has leading zeroes, needed for CDDIS downloads with tscsh (one line of code missed in fixes applied to most scripts for 10.35 release). Thanks to S Shimada of NIED for the catch and Mark Murray for additional cleanup.”…””}”(j¶jýÑjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMüj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ™Fix bug in kf/glfor/get_max_glbd.f that resulted in wrong dimension for the partial derivative array when earthquakes logs and/or apr_rot commands used.”j§]”j±Œ™Fix bug in kf/glfor/get_max_glbd.f that resulted in wrong dimension for the partial derivative array when earthquakes logs and/or apr_rot commands used.”…””}”(j¶j ÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ:Updates to 'track' to account for millisecond range jumps.”j§]”j±Œ>Updates to ‘track’ to account for millisecond range jumps.”…””}”(j¶jÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ±Fix bug in creating station.info entries with sh_upd_stnfo when the compiler option for floating point is not real*8. Thanks to Mark Murray (New Mexico Tech) for catching this.”j§]”j±Œ±Fix bug in creating station.info entries with sh_upd_stnfo when the compiler option for floating point is not real*8. Thanks to Mark Murray (New Mexico Tech) for catching this.”…””}”(j¶j'ÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒPFix bug in utility org2stab to get a stablization list from a velocity solution.”j§]”j±ŒPFix bug in utility org2stab to get a stablization list from a velocity solution.”…””}”(j¶j5ÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ?Fix bug in sorting median process-noise values in sh_gen_stats.”j§]”j±Œ?Fix bug in sorting median process-noise values in sh_gen_stats.”…””}”(j¶jCÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒECorrect a bug in sh_update_eop after detecting an invalid EOP series.”j§]”j±ŒECorrect a bug in sh_update_eop after detecting an invalid EOP series.”…””}”(j¶jQÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ.Fix failure to link binary for utility ne2azel”j§]”j±Œ.Fix failure to link binary for utility ne2azel”…””}”(j¶j_ÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ´Add gradients to the output file of sh_metutil; trap an empty z-file from having no good observations at a site. Copy gamit/utils/metutil. Thanks to Mark Murray (New Mexico Tech).”j§]”j±Œ´Add gradients to the output file of sh_metutil; trap an empty z-file from having no good observations at a site. Copy gamit/utils/metutil. Thanks to Mark Murray (New Mexico Tech).”…””}”(j¶jmÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ•Modify sh_get_met to work with either Z or gz files, and for multiple days; update the met directories for CDDIS. Thanks to Kalev Rannat (Tallin U).”j§]”j±Œ•Modify sh_get_met to work with either Z or gz files, and for multiple days; update the met directories for CDDIS. Thanks to Kalev Rannat (Tallin U).”…””}”(j¶j{ÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦X Add ~60 receivers and ~10 antennas to rcvant.dat. Update to current IGS ANTEX file (igs05_1597.atx) and create igs05_1597_plus.atx by adding PCV models from NGS for 8 antennas not in the IGS file. Correct misspellings or official changes for 6 receivers or antennas.”j§]”j±X Add ~60 receivers and ~10 antennas to rcvant.dat. Update to current IGS ANTEX file (igs05_1597.atx) and create igs05_1597_plus.atx by adding PCV models from NGS for 8 antennas not in the IGS file. Correct misspellings or official changes for 6 receivers or antennas.”…””}”(j¶j‰ÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆMj¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ×Changes to unimake and Makefile.config to facilitate installation under CYGWIN. See the notes 'CYGWIN' under updates/documentation. Thanks to Semi Ergintav (TUBITAK) and George Vergos (AUTH) for notes and testing.”j§]”j±ŒÛChanges to unimake and Makefile.config to facilitate installation under CYGWIN. See the notes ‘CYGWIN’ under updates/documentation. Thanks to Semi Ergintav (TUBITAK) and George Vergos (AUTH) for notes and testing.”…””}”(j¶j—ÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒôAdd to sh_gamit the ability to invoke sh_metutil to get ZWD and PW (met-file) from an input z-file and o-file, and to archive, compress, or delete z- and met-files at the end of the run. Add script sh_met2pbo to concatenate multiple met-files.”j§]”j±ŒôAdd to sh_gamit the ability to invoke sh_metutil to get ZWD and PW (met-file) from an input z-file and o-file, and to archive, compress, or delete z- and met-files at the end of the run. Add script sh_met2pbo to concatenate multiple met-files.”…””}”(j¶j¥ÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM$j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ5Fix header entries and format in writing SP3-C files.”j§]”j±Œ5Fix header entries and format in writing SP3-C files.”…””}”(j¶j³ÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM)j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ¥Update Hatanaka RINEX compression routines to version 4.0.4, fixing function name conflict with getline in gcc 4.4 and cleaning handling of line-feed at end of file.”j§]”j±Œ¥Update Hatanaka RINEX compression routines to version 4.0.4, fixing function name conflict with getline in gcc 4.4 and cleaning handling of line-feed at end of file.”…””}”(j¶jÁÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM+j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ1Add output lines in Euler-pole utility conveuler.”j§]”j±Œ1Add output lines in Euler-pole utility conveuler.”…””}”(j¶jÏÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM/j¶j‰ÆjÇj‰Æubj`)”}”(j¦Œ_Modify format in utility confpol to convert N,E sigmas and correlations to confidence ellipses.”j§]”j±Œ_Modify format in utility confpol to convert N,E sigmas and correlations to confidence ellipses.”…””}”(j¶jÝÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM1j¶j‰ÆjÇj‰Æubj`)”}”(j¦ŒpNew utility check_siteid to compare 4-character IDs from glist and several external formats to detect conflicts.”j§]”j±ŒpNew utility check_siteid to compare 4-character IDs from glist and several external formats to detect conflicts.”…””}”(j¶jëÒjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¸ÆjÆM4j¶j‰ÆjÇj‰Æubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j¸Æj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj¸ÆjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j˜ÆjŒÆj§Æj›Æuj_}”(Œrel”j˜ÆŒdate”j§Æujc}”Œmb”]”j÷ )”}”(j¦j6Ñj§]”j±Œmb”…””}”(j¶j ÓjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œmb”j&Æj ÓujÄjö j¶j,Ñubasje}”jg}”ji}”j¹}”(jDÑjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±ŒUnknown target name: "mb".”…””}”j¶j!Ósbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÓubaj·}”(j¹]”jDÑaj»]”j½]”jÀ]”jÂ]”j>ÑaŒlevel”KŒtype”j5Œsource”j¸ÆŒline”MÃujÄjø ubj>Ñj4Ñujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”jù )”}”(j¦hoj§]”j`)”}”(j¦Œ?Definition list ends without a blank line; unexpected unindent.”j§]”j±Œ?Definition list ends without a blank line; unexpected unindent.”…””}”(j¶jGÓjÇj‰ÆhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jDÓubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒline”M#Œsource”j¸ÆujÄjø j¶j‰ÆjÇj‰Æhj¸ÆjÆM"ubaj†]”jÓajˆNj‰]”j‹NjÇj‰Æubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jdÓsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jaÓjÇjaÓubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jsÓjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jaÓjÇjaÓubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ10.61”j§]”j±Œ10.61”…””}”(j¶j…ÓjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j‚ÓjÇjaÓhŒA/chandler/home/floyd/public_html/gg/docs/source/relnote/10.61.rst”jÆKubj`)”}”(j¦ŒLast updated 31 March 2017”j§]”j±ŒLast updated 31 March 2017”…””}”(j¶j”ÓjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKj¶j‚ÓjÇjaÓubj`)”}”(j¦X×Release 10.61 consolidates incremental updates made since release 10.60 of June 2015 and adds a few new features. Most of the changes involve fixing bugs or improvement incrementally the GNSS enhancements of 10.60. The most important new feature for most users will be the ability to read RINEX 3 observation and navigation files in GAMIT (:program:`kf/svpos` and :program:`kf/track` are still to be updated). We have not yet modified our shell scripts to handle RINEX 3 naming conventions, however, so RINEX 3 files will need to be renamed to RINEX 2 standards (:program:`sh_rename_rinex3`). No distinction needs to be made in the file name between RINEX 2 and RINEX 3; the code will detect the version and read it correctly.”j§]”(j±XTRelease 10.61 consolidates incremental updates made since release 10.60 of June 2015 and adds a few new features. Most of the changes involve fixing bugs or improvement incrementally the GNSS enhancements of 10.60. The most important new feature for most users will be the ability to read RINEX 3 observation and navigation files in GAMIT (”…””}”(j¶j¢ÓjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`kf/svpos`”j§]”j±Œkf/svpos”…””}”(j¶jªÓjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¢Óubj±Œ and ”…””}”(j¶j¢ÓjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`kf/track`”j§]”j±Œkf/track”…””}”(j¶j¼ÓjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¢Óubj±Œ´ are still to be updated). We have not yet modified our shell scripts to handle RINEX 3 naming conventions, however, so RINEX 3 files will need to be renamed to RINEX 2 standards (”…””}”(j¶j¢ÓjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_rename_rinex3`”j§]”j±Œsh_rename_rinex3”…””}”(j¶jÎÓjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¢Óubj±Œ‰). No distinction needs to be made in the file name between RINEX 2 and RINEX 3; the code will detect the version and read it correctly.”…””}”(j¶j¢ÓjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKj¶j‚ÓjÇjaÓubj`)”}”(j¦Xy10.61 should allow users to begin exercising GAMIT with two-frequency data from any GNSS system except for Glonass, and to combine the h-files from multiple systems in GLOBK. The standard :file:`antmod.dat` file includes all systems, and we have created static versions (thru 2017.0) of :file:`svnav.dat.gnss` and :file:`dcb.dat.gnss` with entries for the other systems. (The GPS-only files, which are regularly updated have dropped the :file:`gnss` extent.) The COD empirical radiation pressure model (:content:`BERNE`) should work adequately for all systems, but we do not yet have a robust yaw model for Beidou, Galileo, or IRNSS.”j§]”(j±Œ¼10.61 should allow users to begin exercising GAMIT with two-frequency data from any GNSS system except for Glonass, and to combine the h-files from multiple systems in GLOBK. The standard ”…””}”(j¶jæÓjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`antmod.dat`”j§]”j±Œ antmod.dat”…””}”(j¶jîÓjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæÓubj±ŒQ file includes all systems, and we have created static versions (thru 2017.0) of ”…””}”(j¶jæÓjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`svnav.dat.gnss`”j§]”j±Œsvnav.dat.gnss”…””}”(j¶jÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæÓubj±Œ and ”…””}”(j¶jæÓjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`dcb.dat.gnss`”j§]”j±Œ dcb.dat.gnss”…””}”(j¶jÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæÓubj±Œg with entries for the other systems. (The GPS-only files, which are regularly updated have dropped the ”…””}”(j¶jæÓjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`gnss`”j§]”j±Œgnss”…””}”(j¶j-ÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæÓubj±Œ6 extent.) The COD empirical radiation pressure model (”…””}”(j¶jæÓjÇjaÓhNjÆNubj˜)”}”(j¦Œ:content:`BERNE`”j§]”j±ŒBERNE”…””}”(j¶jBÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jæÓubj±Œr) should work adequately for all systems, but we do not yet have a robust yaw model for Beidou, Galileo, or IRNSS.”…””}”(j¶jæÓjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKj¶j‚ÓjÇjaÓubj`)”}”(j¦X[The :file:`~/gg/tables/` directory now includes both ITRF2008 and ITRF2014 versions of IGS :file:`.apr`, :file:`.eq`, and :file:`antmod.dat` (ANTEX) files to reflect that change in IGS processing with GPS Week 1934 (29 January). Since there is a ~ 0.4 ppb step in scale (heights) between ITRF2008 and ITRF2014, and the IGS14 ANTEX files have further corrections that will cause both horizontal and vertical discontinuities up to 10 mm in height and 5 mm in vertical for about 20 antennas, we recommend that users stick with ITRF2008 files until they are ready to reprocess their entire data set. IGS orbits are now computed with ITRF2014 coordinates and SV phase-center-offsets (PCOs) but prior to Week 1934 the IGS orbits were computed with ITRF2008 and will not be recomputed until later this year. Fortunately, since GAMIT processing (unlike PPP) is relatively insensitive to the frame used for the orbits, you may continue to use ITRF2008 coordinates and PCOs with the new orbits and ITRF2014 with old ones until the IGS reprocessing is complete. See the poster ``_ and the file ``_ for details. We will provide :file:`.apr` and ANTEX files in both systems for the near future. See comments below about which orbits are download by :program:`sh_get_orbits`.”j§]”(j±ŒThe ”…””}”(j¶j[ÔjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jcÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j[Ôubj±ŒC directory now includes both ITRF2008 and ITRF2014 versions of IGS ”…””}”(j¶j[ÔjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jxÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j[Ôubj±Œ, ”…””}”(j¶j[ÔjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`.eq`”j§]”j±Œ.eq”…””}”(j¶jÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j[Ôubj±Œ, and ”…””}”(j¶j[ÔjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`antmod.dat`”j§]”j±Œ antmod.dat”…””}”(j¶j¢ÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j[Ôubj±Xž (ANTEX) files to reflect that change in IGS processing with GPS Week 1934 (29 January). Since there is a ~ 0.4 ppb step in scale (heights) between ITRF2008 and ITRF2014, and the IGS14 ANTEX files have further corrections that will cause both horizontal and vertical discontinuities up to 10 mm in height and 5 mm in vertical for about 20 antennas, we recommend that users stick with ITRF2008 files until they are ready to reprocess their entire data set. IGS orbits are now computed with ITRF2014 coordinates and SV phase-center-offsets (PCOs) but prior to Week 1934 the IGS orbits were computed with ITRF2008 and will not be recomputed until later this year. Fortunately, since GAMIT processing (unlike PPP) is relatively insensitive to the frame used for the orbits, you may continue to use ITRF2008 coordinates and PCOs with the new orbits and ITRF2014 with old ones until the IGS reprocessing is complete. See the poster ”…””}”(j¶j[ÔjÇjaÓhNjÆNubj÷ )”}”(j¦Œ7``_”j§]”j±Œ2https://mediatum.ub.tum.de/doc/1341338/1341338.pdf”…””}”(j¶j·ÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ2https://mediatum.ub.tum.de/doc/1341338/1341338.pdf”j jÆÔujÄjö j¶j[Ôubje)”}”(j¦Œ4”j§]”j·}”(j¹]”Œ0https-mediatum-ub-tum-de-doc-1341338-1341338-pdf”aj»]”j½]”Œ2https://mediatum.ub.tum.de/doc/1341338/1341338.pdf”ajÀ]”jÂ]”Œrefuri”jÆÔujÄjdj Kj¶j[Ôubj±Œ and the file ”…””}”(j¶j[ÔjÇjaÓhNjÆNubj÷ )”}”(j¦Œ=``_”j§]”j±Œ8ftp://igs-rf.ign.fr/pub/IGS14/igs08_to_igs14_offsets.txt”…””}”(j¶jØÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ8ftp://igs-rf.ign.fr/pub/IGS14/igs08_to_igs14_offsets.txt”j jçÔujÄjö j¶j[Ôubje)”}”(j¦Œ:”j§]”j·}”(j¹]”Œ6ftp-igs-rf-ign-fr-pub-igs14-igs08-to-igs14-offsets-txt”aj»]”j½]”Œ8ftp://igs-rf.ign.fr/pub/igs14/igs08_to_igs14_offsets.txt”ajÀ]”jÂ]”Œrefuri”jçÔujÄjdj Kj¶j[Ôubj±Œ for details. We will provide ”…””}”(j¶j[ÔjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jùÔjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j[Ôubj±Œl and ANTEX files in both systems for the near future. See comments below about which orbits are download by ”…””}”(j¶j[ÔjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_get_orbits`”j§]”j±Œ sh_get_orbits”…””}”(j¶jÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j[Ôubj±Œ.”…””}”(j¶j[ÔjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKj¶j‚ÓjÇjaÓubj`)”}”(j¦XÅWhenever you process data beyond the date of the software release, you *must* update supporting files. For GAMIT: :file:`svnav.dat` and :file:`antmod.dat` for changes in PN assignments; :file:`dcb.dat` for P1/C1/P2 code biases that affect wide-lane ambiguity resolution; :file:`station.info` for antenna changes at reference sites; and :file:`ut1.`/:file:`pole.` files for current EOP information. Of these files, only the EOP files are automatically updated by :program:`sh_gamit`. For GLOBK, you should keep current :file:`itrf08_comb.apr` and :file:`itrf08_comb.eq` (or their itrf14 counterparts) to account for improved coordinates and antenna changes and earthquakes at reference sites. Both the GAMIT and GLOBK files are always current in :file:`incremental_updates/tables/` and included in any :file:`incremental_updates` tar-file. As noted in the announcement of 10 December 2016, we no longer update :file:`dcb.dat` files in the format used prior to 10.60.”j§]”(j±ŒGWhenever you process data beyond the date of the software release, you ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj )”}”(j¦Œ*must*”j§]”j±Œmust”…””}”(j¶j.ÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j&Õubj±Œ% update supporting files. For GAMIT: ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`svnav.dat`”j§]”j±Œ svnav.dat”…””}”(j¶j@ÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±Œ and ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`antmod.dat`”j§]”j±Œ antmod.dat”…””}”(j¶jUÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±Œ for changes in PN assignments; ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`dcb.dat`”j§]”j±Œdcb.dat”…””}”(j¶jjÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±ŒF for P1/C1/P2 code biases that affect wide-lane ambiguity resolution; ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±Œ- for antenna changes at reference sites; and ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`ut1.`”j§]”j±Œut1.”…””}”(j¶j”ÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±Œ/”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`pole.`”j§]”j±Œpole.”…””}”(j¶j©ÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±Œd files for current EOP information. Of these files, only the EOP files are automatically updated by ”…””}”(j¶j&ÕjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j¾ÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j&Õubj±Œ%. For GLOBK, you should keep current ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`itrf08_comb.apr`”j§]”j±Œitrf08_comb.apr”…””}”(j¶jÐÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±Œ and ”…””}”j¶j&Õsbj˜)”}”(j¦Œ:file:`itrf08_comb.eq`”j§]”j±Œitrf08_comb.eq”…””}”(j¶jåÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±Œ± (or their itrf14 counterparts) to account for improved coordinates and antenna changes and earthquakes at reference sites. Both the GAMIT and GLOBK files are always current in ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ#:file:`incremental_updates/tables/`”j§]”j±Œincremental_updates/tables/”…””}”(j¶júÕjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±Œ and included in any ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`incremental_updates`”j§]”j±Œincremental_updates”…””}”(j¶jÖjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±ŒQ tar-file. As noted in the announcement of 10 December 2016, we no longer update ”…””}”(j¶j&ÕjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`dcb.dat`”j§]”j±Œdcb.dat”…””}”(j¶j$ÖjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&Õubj±Œ) files in the format used prior to 10.60.”…””}”(j¶j&ÕjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKj¶j‚ÓjÇjaÓubj`)”}”(j¦X^All GAMIT/GLOBK scripts that produce plots (e.g. time series and velocity maps) use Generic Mapping Tools (GMT) to do so. The release of GMT 5 in November 2013 has necessitated major alterations to the syntax of GMT commands in many scripts. The updated scripts, which use GMT 5-compatible syntax, are contained in :file:`com/` and will be the only ones maintained and developed beyond the 10.60 release of GAMIT/GLOBK. We therefore recommend that all users now download and switch to using GMT 5 because the updated scripts are *not* backwards-compatible. The old scripts, which may be used with GMT 4 or prior, are now contained in the :file:`com_preGMT5/` directory. Users must prepend this directory to their path in order to continue to use GMT 4, e.g. :envvar:`PATH` contains :content:`$HOME/gg/com_preGMT5:$HOME/gg/com:$HOME/gg/gamit/bin:$HOME/gg/kf/bin`.”j§]”(j±X;All GAMIT/GLOBK scripts that produce plots (e.g. time series and velocity maps) use Generic Mapping Tools (GMT) to do so. The release of GMT 5 in November 2013 has necessitated major alterations to the syntax of GMT commands in many scripts. The updated scripts, which use GMT 5-compatible syntax, are contained in ”…””}”(j¶j?ÖjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`com/`”j§]”j±Œcom/”…””}”(j¶jGÖjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?Öubj±ŒÊ and will be the only ones maintained and developed beyond the 10.60 release of GAMIT/GLOBK. We therefore recommend that all users now download and switch to using GMT 5 because the updated scripts are ”…””}”(j¶j?ÖjÇjaÓhNjÆNubj )”}”(j¦Œ*not*”j§]”j±Œnot”…””}”(j¶j\ÖjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j?Öubj±Œh backwards-compatible. The old scripts, which may be used with GMT 4 or prior, are now contained in the ”…””}”(j¶j?ÖjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`com_preGMT5/`”j§]”j±Œ com_preGMT5/”…””}”(j¶jnÖjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?Öubj±Œd directory. Users must prepend this directory to their path in order to continue to use GMT 4, e.g. ”…””}”(j¶j?ÖjÇjaÓhNjÆNubj!±)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jü]”((j,±ŒPATH”Œindex-0”hoNt”(j,±Œenvironment variable; PATH”jŽÖhoNt”eujÄh‰j¶j?Öubje)”}”(j¦hoj§]”j·}”(j¹]”jŽÖaj»]”j½]”jÀ]”jÂ]”ujÄjdj¶j?Öubj’)”}”(j¦Œ:envvar:`PATH`”j§]”j˜)”}”(j¦jÖj§]”j±ŒPATH”…””}”(j¶jŸÖjÇjaÓhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-envvar”ej½]”jÀ]”jÂ]”ujÄj—j¶j›Öubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j©ÖŒreftype”Œenvvar”Œ refexplicit”‰Œrefwarn”‰j¶jÖujÄj‘hj“ÓjÆK&j¶j?Öubj±Œ contains ”…””}”(j¶j?ÖjÇjaÓhNjÆNubj˜)”}”(j¦ŒO:content:`$HOME/gg/com_preGMT5:$HOME/gg/com:$HOME/gg/gamit/bin:$HOME/gg/kf/bin`”j§]”j±ŒD$HOME/gg/com_preGMT5:$HOME/gg/com:$HOME/gg/gamit/bin:$HOME/gg/kf/bin”…””}”(j¶j¾ÖjÇjaÓhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j?Öubj±Œ.”…””}”(j¶j?ÖjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK&j¶j‚ÓjÇjaÓubj`)”}”(j¦X}For plotting time series, we are transitioning from using :file:`VAL` and :file:`mb` files produced by :program:`ensum` and :program:`multibase` and used by :program:`sh_plotcrd` or :program:`sh_baseline` to PBO-format :file:`.pos` files produced by :program:`tssum` and used by :program:`sh_plot_pos`. :program:`tsview` can still read both :file:`mb` files and :file:`.pos` files.”j§]”(j±Œ:For plotting time series, we are transitioning from using ”…””}”(j¶j×ÖjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`VAL`”j§]”j±ŒVAL”…””}”(j¶jßÖjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Öubj±Œ and ”…””}”(j¶j×ÖjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`mb`”j§]”j±Œmb”…””}”(j¶jôÖjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Öubj±Œ files produced by ”…””}”(j¶j×ÖjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`ensum`”j§]”j±Œensum”…””}”(j¶j ×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j×Öubj±Œ and ”…””}”j¶j×Ösbjj)”}”(j¦Œ:program:`multibase`”j§]”j±Œ multibase”…””}”(j¶j×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j×Öubj±Œ and used by ”…””}”(j¶j×ÖjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_plotcrd`”j§]”j±Œ sh_plotcrd”…””}”(j¶j-×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j×Öubj±Œ or ”…””}”(j¶j×ÖjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_baseline`”j§]”j±Œ sh_baseline”…””}”(j¶j?×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j×Öubj±Œ to PBO-format ”…””}”(j¶j×ÖjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`.pos`”j§]”j±Œ.pos”…””}”(j¶jQ×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Öubj±Œ files produced by ”…””}”j¶j×Ösbjj)”}”(j¦Œ:program:`tssum`”j§]”j±Œtssum”…””}”(j¶jf×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j×Öubj±Œ and used by ”…””}”j¶j×Ösbjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶jx×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j×Öubj±Œ. ”…””}”(j¶j×ÖjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`tsview`”j§]”j±Œtsview”…””}”(j¶jŠ×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j×Öubj±Œ can still read both ”…””}”(j¶j×ÖjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`mb`”j§]”j±Œmb”…””}”(j¶jœ×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Öubj±Œ files and ”…””}”(j¶j×ÖjÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`.pos`”j§]”j±Œ.pos”…””}”(j¶j±×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×Öubj±Œ files.”…””}”(j¶j×ÖjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK-j¶j‚ÓjÇjaÓubj`)”}”(j¦ŒŸ:program:`glist` can now take multiple :file:`.apr` and :file:`.eq` files and accept :content:`use_site` commands, so that it can fully check a globk solution.”j§]”(jj)”}”(j¦Œ:program:`glist`”j§]”j±Œglist”…””}”(j¶jÐ×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÌ×ubj±Œ can now take multiple ”…””}”(j¶jÌ×jÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jâ×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÌ×ubj±Œ and ”…””}”(j¶jÌ×jÇjaÓhNjÆNubj˜)”}”(j¦Œ :file:`.eq`”j§]”j±Œ.eq”…””}”(j¶j÷×jÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÌ×ubj±Œ files and accept ”…””}”(j¶jÌ×jÇjaÓhNjÆNubj˜)”}”(j¦Œ:content:`use_site`”j§]”j±Œuse_site”…””}”(j¶j ØjÇjaÓhNjÆ•ÿNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÌ×ubj±Œ7 commands, so that it can fully check a globk solution.”…””}”(j¶jÌ×jÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK0j¶j‚ÓjÇjaÓubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒOther changes for 10.61”j§]”j±ŒOther changes for 10.61”…””}”(j¶j(ØjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j%ØjÇjaÓhj“ÓjÆK3ubj`)”}”(j¦ŒÀAdded to :file:`rcvant.dat` the following receivers: TPS NET-G5, TPS HIPER_SR, TPS MR-1, LEIGS16, LEICA GS 15, LEICA GM30, LEICA GR30, LEICA GR50, JAVAD TRE_3, JAVAD TRE_3 DELTA, SPECTRA SP80.”j§]”(j±Œ Added to ”…””}”(j¶j6ØjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`rcvant.dat`”j§]”j±Œ rcvant.dat”…””}”(j¶j>ØjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j6Øubj±Œ¥ the following receivers: TPS NET-G5, TPS HIPER_SR, TPS MR-1, LEIGS16, LEICA GS 15, LEICA GM30, LEICA GR30, LEICA GR50, JAVAD TRE_3, JAVAD TRE_3 DELTA, SPECTRA SP80.”…””}”(j¶j6ØjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK5j¶j%ØjÇjaÓubj`)”}”(j¦XÆAdded to :file:`rcvant.dat`, :file:`hi.dat` and, if needed, :file:`antmod.dat` the following antennas: SEPPOLANT_X_MF, AVGRANT_G5T, JAVGRANT_G5T+GP, JAVRINGANT_DM, JAVRINGANT_G5T, JNSCHOKERING_CM, LEICA GS16, LEIGS15.R2,TPSHIPER_SR, TWIVP6000, TPSG5_A1, TPSCR.G5, TPSPG_S1, SPP91564_1, SPP91564_2, TRMR2, 3S-02-TSADM. GMXZENITH35, GEOMAX ZENITH35, HEMA52_WB. Corrected the radius in :file:`hi.dat` for TPSCR.G3, TPSCR.G5, TPSCR.G5C and TPSCR3 antennas.”j§]”(j±Œ Added to ”…””}”(j¶jYØjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`rcvant.dat`”j§]”j±Œ rcvant.dat”…””}”(j¶jaØjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jYØubj±Œ, ”…””}”(j¶jYØjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`hi.dat`”j§]”j±Œhi.dat”…””}”(j¶jvØjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jYØubj±Œ and, if needed, ”…””}”(j¶jYØjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`antmod.dat`”j§]”j±Œ antmod.dat”…””}”(j¶j‹ØjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jYØubj±X3 the following antennas: SEPPOLANT_X_MF, AVGRANT_G5T, JAVGRANT_G5T+GP, JAVRINGANT_DM, JAVRINGANT_G5T, JNSCHOKERING_CM, LEICA GS16, LEIGS15.R2,TPSHIPER_SR, TWIVP6000, TPSG5_A1, TPSCR.G5, TPSPG_S1, SPP91564_1, SPP91564_2, TRMR2, 3S-02-TSADM. GMXZENITH35, GEOMAX ZENITH35, HEMA52_WB. Corrected the radius in ”…””}”(j¶jYØjÇjaÓhNjÆNubj˜)”}”(j¦Œ:file:`hi.dat`”j§]”j±Œhi.dat”…””}”(j¶j ØjÇjaÓhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jYØubj±Œ7 for TPSCR.G3, TPSCR.G5, TPSCR.G5C and TPSCR3 antennas.”…””}”(j¶jYØjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK8j¶j%ØjÇjaÓubj`)”}”(j¦ŒlUpdated CDDIS server to ``_ in :program:`sh_update_eop`.”j§]”(j±ŒUpdated CDDIS server to ”…””}”(j¶j»ØjÇjaÓhNjÆNubj÷ )”}”(j¦Œ7``_”j§]”j±Œ2ftp://ftp.cddis.eosdis.nasa.gov/pub/products/iers/”…””}”(j¶jÃØjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ2ftp://ftp.cddis.eosdis.nasa.gov/pub/products/iers/”j jÒØujÄjö j¶j»Øubje)”}”(j¦Œ4”j§]”j·}”(j¹]”Œ/ftp-ftp-cddis-eosdis-nasa-gov-pub-products-iers”aj»]”j½]”Œ2ftp://ftp.cddis.eosdis.nasa.gov/pub/products/iers/”ajÀ]”jÂ]”Œrefuri”jÒØujÄjdj Kj¶j»Øubj±Œ in ”…””}”(j¶j»ØjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_update_eop`”j§]”j±Œ sh_update_eop”…””}”(j¶jäØjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j»Øubj±Œ.”…””}”(j¶j»ØjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK`_ being used and added if-statements to test whether or not to include :content:`firstdifference` keyword in `Hector `_ control files, which is not valid after `Hector version 1.4 `_. Corrected allowance of :program:`tsfit` command file with no :content:`max_sigma` terms to be read.”j§]”(j±Œ Updates to ”…””}”(j¶jüØjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_hector`”j§]”j±Œ sh_hector”…””}”(j¶jÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jüØubj±Œ and ”…””}”(j¶jüØjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_cats`”j§]”j±Œsh_cats”…””}”(j¶jÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jüØubj±Œ for error analyis: Added ”…””}”(j¶jüØjÇjaÓhNjÆNubj’)”}”(j¦Œ :option:`-v`”j§]”j˜)”}”(j¦j*Ùj§]”j±Œ-v”…””}”(j¶j,ÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j(Ùubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j6ÙŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-v”ujÄj‘hj“ÓjÆK>j¶jüØubj±Œ option to define version of ”…””}”(j¶jüØjÇjaÓhNjÆNubj÷ )”}”(j¦Œ;`Hector `_”j§]”j±ŒHector”…””}”(j¶jLÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒHector”j Œ/https://segal.ubi.pt/web-services/whatishector/”ujÄjö j¶jüØubje)”}”(j¦Œ2 ”j§]”j·}”(j¹]”Œhector”aj»]”j½]”Œhector”ajÀ]”jÂ]”Œrefuri”j\ÙujÄjdj Kj¶jüØubj±ŒF being used and added if-statements to test whether or not to include ”…””}”(j¶jüØjÇjaÓhNjÆNubj˜)”}”(j¦Œ:content:`firstdifference`”j§]”j±Œfirstdifference”…””}”(j¶jnÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jüØubj±Œ keyword in ”…””}”(j¶jüØjÇjaÓhNjÆNubj÷ )”}”(j¦Œ;`Hector `_”j§]”j±ŒHector”…””}”(j¶jÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒHector”j Œ/https://segal.ubi.pt/web-services/whatishector/”ujÄjö j¶jüØubje)”}”(j¦Œ2 ”j§]”j·}”(j¹]”Œid2”aj»]”j½]”jÀ]”Œhector”ajÂ]”Œrefuri”j‘ÙujÄjdj Kj¶jüØubj±Œ) control files, which is not valid after ”…””}”(j¶jüØjÇjaÓhNjÆNubj÷ )”}”(j¦ŒY`Hector version 1.4 `_”j§]”j±ŒHector version 1.4”…””}”(j¶j£ÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒHector version 1.4”j ŒAhttps://segal.ubi.pt/web-services/whatishector/previous-versions/”ujÄjö j¶jüØubje)”}”(j¦ŒD ”j§]”j·}”(j¹]”Œhector-version-1-4”aj»]”j½]”Œhector version 1.4”ajÀ]”jÂ]”Œrefuri”j³ÙujÄjdj Kj¶jüØubj±Œ. Corrected allowance of ”…””}”(j¶jüØjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`tsfit`”j§]”j±Œtsfit”…””}”(j¶jÅÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jüØubj±Œ command file with no ”…””}”(j¶jüØjÇjaÓhNjÆNubj˜)”}”(j¦Œ:content:`max_sigma`”j§]”j±Œ max_sigma”…””}”(j¶j×ÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jüØubj±Œ terms to be read.”…””}”(j¶jüØjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK>j¶j%ØjÇjaÓubj`)”}”(j¦Œ§:program:`sh_plot_pos`, :program:`sh_hector`, :program:`sh_cats`: Added :option:`-X` option to :command:`less` to allow help contents to remain on screen upon exiting.”j§]”(jj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶jôÙjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jðÙubj±Œ, ”…””}”(j¶jðÙjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_hector`”j§]”j±Œ sh_hector”…””}”(j¶jÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jðÙubj±Œ, ”…””}”j¶jðÙsbjj)”}”(j¦Œ:program:`sh_cats`”j§]”j±Œsh_cats”…””}”(j¶jÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jðÙubj±Œ: Added ”…””}”(j¶jðÙjÇjaÓhNjÆNubj’)”}”(j¦Œ :option:`-X`”j§]”j˜)”}”(j¦j,Új§]”j±Œ-X”…””}”(j¶j.ÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j*Úubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jŒ refdomain”j8ÚŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-X”ujÄj‘hj“ÓjÆKBj¶jðÙubj±Œ option to ”…””}”(j¶jðÙjÇjaÓhNjÆNubjj)”}”(j¦Œ:command:`less`”j§]”j±Œless”…””}”(j¶jNÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jðÙubj±Œ9 to allow help contents to remain on screen upon exiting.”…””}”(j¶jðÙjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKBj¶j%ØjÇjaÓubj`)”}”(j¦Œp:program:`sh_get_rinex`/:program:`sh_cats`/:program:`sh_plot_pos`: Fix bug when accessing more than one archive.”j§]”(jj)”}”(j¦Œ:program:`sh_get_rinex`”j§]”j±Œ sh_get_rinex”…””}”(j¶jjÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jfÚubj±Œ/”…””}”(j¶jfÚjÇjaÓhNjÆNubjj)”}”(j¦Œ:program:`sh_cats`”j§]”j±Œsh_cats”…””}”(j¶j|ÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jfÚubj±Œ/”…””}”j¶jfÚsbjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶jŽÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jfÚubj±Œ/: Fix bug when accessing more than one archive.”…””}”(j¶jfÚjÇjaÓhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKEj¶j%ØjÇjaÓubj`)”}”(j¦Œµsh_plot_pos/sh_cats/sh_hector/sh_kml: Corrected parsing of options using 'echo "$@"' to 'echo "$*"' to avoid echo erroneously evaluating elements of $@ as options (e.g. "-e", "-n").”j§]”j±ŒÍsh_plot_pos/sh_cats/sh_hector/sh_kml: Corrected parsing of options using ‘echo “$@â€â€™ to ‘echo “$*â€â€™ to avoid echo erroneously evaluating elements of $@ as options (e.g. “-eâ€, “-nâ€).”…””}”(j¶j¦ÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKHj¶j%ØjÇjaÓubj`)”}”(j¦X sh_plot_pos: Change -d option to take extension that is appended to default "pos", "res" and "plots" directories, and removed velocity annotation from up component when using -u option; corrected setting of FORMAT_DATE_MAP GMT variable when using -g option for calendar dates; correct listing of pos-file(s) created by tssum from org-file(s) when "Reference frame" read from org-file(s) is not a 5-character ID. Fix a bug causing the erasure of the tsfit command file when the user specifies the -t option with no arguements.”j§]”j±Xsh_plot_pos: Change -d option to take extension that is appended to default “posâ€, “res†and “plots†directories, and removed velocity annotation from up component when using -u option; corrected setting of FORMAT_DATE_MAP GMT variable when using -g option for calendar dates; correct listing of pos-file(s) created by tssum from org-file(s) when “Reference frame†read from org-file(s) is not a 5-character ID. Fix a bug causing the erasure of the tsfit command file when the user specifies the -t option with no arguements.”…””}”(j¶j´ÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKLj¶j%ØjÇjaÓubj`)”}”(j¦Œšsh_oneway/sh_make_sky_pngs: Added if-statements to trap cases where there are no data in certain elevation-angle bins, leading to GMT/PostScript errors.”j§]”j±Œšsh_oneway/sh_make_sky_pngs: Added if-statements to trap cases where there are no data in certain elevation-angle bins, leading to GMT/PostScript errors.”…””}”(j¶jÂÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKTj¶j%ØjÇjaÓubj`)”}”(j¦Œõsh_sp3fit: Fix problem with SV selection with -t option'; fix problem reading SP3 files prior to Week 1357 (Jan 2006); reeplace the hard-wired short-period EOP in fitting SP3 files by a read ofthe sestbl; add the ability to use the Gipson model.”j§]”j±Œ÷sh_sp3fit: Fix problem with SV selection with -t option’; fix problem reading SP3 files prior to Week 1357 (Jan 2006); reeplace the hard-wired short-period EOP in fitting SP3 files by a read ofthe sestbl; add the ability to use the Gipson model.”…””}”(j¶jÐÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKXj¶j%ØjÇjaÓubj`)”}”(j¦ŒPsh_bctot: Add a maximum rms misfit tolerance to fitting the Broadcast Ephemeris.”j§]”j±ŒPsh_bctot: Add a maximum rms misfit tolerance to fitting the Broadcast Ephemeris.”…””}”(j¶jÞÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK]j¶j%ØjÇjaÓubj`)”}”(j¦ŒzUpdated glinit.f to check maximum global files not exceeded (aleady checked in glist. Added .plt files to help directory.”j§]”j±ŒzUpdated glinit.f to check maximum global files not exceeded (aleady checked in glist. Added .plt files to help directory.”…””}”(j¶jìÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK_j¶j%ØjÇjaÓubj`)”}”(j¦Œ×Added optional argument to "-h" option in sh_kml to allow constant to be added to height to account for difference between reference ellipoid (used for track "GEOD" output) and mean sea level (used by Google Earth).”j§]”j±ŒßAdded optional argument to “-h†option in sh_kml to allow constant to be added to height to account for difference between reference ellipoid (used for track “GEOD†output) and mean sea level (used by Google Earth).”…””}”(j¶júÚjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKbj¶j%ØjÇjaÓubj`)”}”(j¦ŒTUpdated deprecated "-N1" option to "-Np1" in call to GMT 5's trend1d in sh_baseline.”j§]”j±Œ^Updated deprecated “-N1†option to “-Np1†in call to GMT 5’s trend1d in sh_baseline.”…””}”(j¶jÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKfj¶j%ØjÇjaÓubj`)”}”(j¦ŒPChange default from ~/gg/tables/sittbl.short to ~/gg/tables/sittbl. in sh_setup.”j§]”j±ŒPChange default from ~/gg/tables/sittbl.short to ~/gg/tables/sittbl. in sh_setup.”…””}”(j¶jÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKhj¶j%ØjÇjaÓubj`)”}”(j¦Xnsh_glred: Ensure stripping of binary h-file extension (e.g. glx, glr, GLX, etc.) from end of base file name only and not elsewhere in the full file name, and set initial value of hfnd variable to '' (zero-length string) to fit proceeding logic. Corrected parsing of -eqf option; aded removal of temporary files after running sh_plot_pos; changed call of sh_plot_pos to accommodate new -d option syntax; added -k option to call of sh_plot_pos (previously only echo'd); changed file names written to .gdl files to "../glbf/" to avoid long absolute paths; edited sh_plot_pos's call of tsfit to use "RATE" instead of "NONE".”j§]”j±X‚sh_glred: Ensure stripping of binary h-file extension (e.g. glx, glr, GLX, etc.) from end of base file name only and not elsewhere in the full file name, and set initial value of hfnd variable to ‘’ (zero-length string) to fit proceeding logic. Corrected parsing of -eqf option; aded removal of temporary files after running sh_plot_pos; changed call of sh_plot_pos to accommodate new -d option syntax; added -k option to call of sh_plot_pos (previously only echo’d); changed file names written to .gdl files to “../glbf/†to avoid long absolute paths; edited sh_plot_pos’s call of tsfit to use “RATE†instead of “NONEâ€.”…””}”(j¶j$ÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKjj¶j%ØjÇjaÓubj`)”}”(j¦Œ[Edited GMT variables, set using gmtset, to be fully compatible with GMT 5 in sh_plot_rinex.”j§]”j±Œ[Edited GMT variables, set using gmtset, to be fully compatible with GMT 5 in sh_plot_rinex.”…””}”(j¶j2ÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKsj¶j%ØjÇjaÓubj`)”}”(j¦ŒFix to globk/glinit/glfor routines to fix bug when site has multiple log terms estimated. More output if max_glb_deriv error in encountered.”j§]”j±ŒFix to globk/glinit/glfor routines to fix bug when site has multiple log terms estimated. More output if max_glb_deriv error in encountered.”…””}”(j¶j@ÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKvj¶j%ØjÇjaÓubj`)”}”(j¦Œ‚Added use of psconvert, replacing ps2raster, for GMT versions after 5.1 in com/sh_gamit, com/sh_make_sky_pngs and com/sh_plot_pos.”j§]”j±Œ‚Added use of psconvert, replacing ps2raster, for GMT versions after 5.1 in com/sh_gamit, com/sh_make_sky_pngs and com/sh_plot_pos.”…””}”(j¶jNÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKyj¶j%ØjÇjaÓubj`)”}”(j¦Xsh_gamit: Add alternative test of disk space available using df to accommodate output format on Mac OS X; removed fall back to igni ftp if ionex file not found at cddis (avoids hang from ftp to igs.ensg.ign.fr); add product ID argument to "-ion" option to select IONEX file for download if it doesn't already exist locally (default igsg from CDDIS; see sh_get_ion); fix assignment of sp3-file name for IGS raid and ultra- rapid orbits; updated efficiency of file size checks; fixed bug when no sites are to be excluded.”j§]”j±X sh_gamit: Add alternative test of disk space available using df to accommodate output format on Mac OS X; removed fall back to igni ftp if ionex file not found at cddis (avoids hang from ftp to igs.ensg.ign.fr); add product ID argument to “-ion†option to select IONEX file for download if it doesn’t already exist locally (default igsg from CDDIS; see sh_get_ion); fix assignment of sp3-file name for IGS raid and ultra- rapid orbits; updated efficiency of file size checks; fixed bug when no sites are to be excluded.”…””}”(j¶j\ÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK|j¶j%ØjÇjaÓubj`)”}”(j¦X+MAKEX: Fix bug for mixed P2/C2 RINEX files; fix bug in makex when more than one RINEX file for a site in the session. Fix inadvertent 'fatal' reading RINEX header 'RCV CLOCK OFFS APPL'. Change the message for a bad RINEX record from a fatal to a warning. With RINEX 3, provide for a backup observable if the primary one is not available. Fix firmware warning for Trimble codelss (4.0 only, not 4.xx). Correct a long-standing misstatement in the x-file header: RADIUS, not HEIGHT. Allow geo-stationary satellites in checking for reasonable range values.”j§]”j±X3MAKEX: Fix bug for mixed P2/C2 RINEX files; fix bug in makex when more than one RINEX file for a site in the session. Fix inadvertent ‘fatal’ reading RINEX header ‘RCV CLOCK OFFS APPL’. Change the message for a bad RINEX record from a fatal to a warning. With RINEX 3, provide for a backup observable if the primary one is not available. Fix firmware warning for Trimble codelss (4.0 only, not 4.xx). Correct a long-standing misstatement in the x-file header: RADIUS, not HEIGHT. Allow geo-stationary satellites in checking for reasonable range values.”…””}”(j¶jjÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK„j¶j%ØjÇjaÓubj`)”}”(j¦Œ]MAKEX, MODEL: Add ability to use sp3 clocks rather than the navigation message in the j-file.”j§]”j±Œ]MAKEX, MODEL: Add ability to use sp3 clocks rather than the navigation message in the j-file.”…””}”(j¶jxÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKj¶j%ØjÇjaÓubj`)”}”(j¦ŒŽFIXDRV: Force the zenith delay to come from VMF1 if the mapping functions are VMF1; fix typo in name of new magfield for 2nd order ionopshere.”j§]”j±ŒŽFIXDRV: Force the zenith delay to come from VMF1 if the mapping functions are VMF1; fix typo in name of new magfield for 2nd order ionopshere.”…””}”(j¶j†ÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKj¶j%ØjÇjaÓubj`)”}”(j¦ŒDGRDTAB: Fix documentation for order and units of the ATML grid file.”j§]”j±ŒDGRDTAB: Fix documentation for order and units of the ATML grid file.”…””}”(j¶j”ÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK“j¶j%ØjÇjaÓubj`)”}”(j¦X¡ARC: Fix bugs in antenna radiation thrust for GPS Block IIR-M and IIF SVs; add write to GAMIT.status giving the antenna radiation used; clean up integration code to use SV type descriptor ('antbody') instead of GPS block number throughout; fix problem reading svnav.dat when integration extends beyond the day; fix typos in if statements resulting in "ARC/ertorb: SV body type ( ) not known" fatal.”j§]”j±X©ARC: Fix bugs in antenna radiation thrust for GPS Block IIR-M and IIF SVs; add write to GAMIT.status giving the antenna radiation used; clean up integration code to use SV type descriptor (‘antbody’) instead of GPS block number throughout; fix problem reading svnav.dat when integration extends beyond the day; fix typos in if statements resulting in “ARC/ertorb: SV body type ( ) not known†fatal.”…””}”(j¶j¢ÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK•j¶j%ØjÇjaÓubj`)”}”(j¦XÔMODEL: Fixed bug leading to blank SV body type for the translation of body type to block number for yaw; allow 1-hr IONEX files (model.h dimensions). Replace the free-format read for RINEX met files an explicit f7.1 to guard against -9999.9 values with no preceeding space. Clean up the setting of sources for P,T,H and the cho to the p-file. For the dipole component of the observable, add initialization of the integer phase (no effect with most operating systems).”j§]”j±XÔMODEL: Fixed bug leading to blank SV body type for the translation of body type to block number for yaw; allow 1-hr IONEX files (model.h dimensions). Replace the free-format read for RINEX met files an explicit f7.1 to guard against -9999.9 values with no preceeding space. Clean up the setting of sources for P,T,H and the cho to the p-file. For the dipole component of the observable, add initialization of the integer phase (no effect with most operating systems).”…””}”(j¶j°ÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKœj¶j%ØjÇjaÓubj`)”}”(j¦Œ3AUTCLN: Fix bug in normal equation initiatization.”j§]”j±Œ3AUTCLN: Fix bug in normal equation initiatization.”…””}”(j¶j¾ÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK¤j¶j%ØjÇjaÓubj`)”}”(j¦Œ"CVIEW: Fix bug in reading c-files.”j§]”j±Œ"CVIEW: Fix bug in reading c-files.”…””}”(j¶jÌÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK¦j¶j%ØjÇjaÓubj`)”}”(j¦ŒnGAMIT utilities: New program BSX2DCBTAB to translation DCBs from SINEX (bsx) to dcb.dat. Fix bugs in DCBTAB2.”j§]”j±ŒnGAMIT utilities: New program BSX2DCBTAB to translation DCBs from SINEX (bsx) to dcb.dat. Fix bugs in DCBTAB2.”…””}”(j¶jÚÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK¨j¶j%ØjÇjaÓubj`)”}”(j¦XªGLOBK: Mod to add satellite number to PRN number in satellite names i.e., PRN_01 now becomes PRN_0149 or PRN_0163 depending on when data are collected. Modified to remave NaN in pbo line when site not estimated; ensure pbo line has initial position if not estimated; mod to allow '-' in file names; Updated glfor/glb_upd_apr.f to fix bug when loads were changed to avoid error in glorg. Update glist to output satellite usage.”j§]”j±X®GLOBK: Mod to add satellite number to PRN number in satellite names i.e., PRN_01 now becomes PRN_0149 or PRN_0163 depending on when data are collected. Modified to remave NaN in pbo line when site not estimated; ensure pbo line has initial position if not estimated; mod to allow ‘-’ in file names; Updated glfor/glb_upd_apr.f to fix bug when loads were changed to avoid error in glorg. Update glist to output satellite usage.”…””}”(j¶jèÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK«j¶j%ØjÇjaÓubj`)”}”(j¦ŒgEdited "set exlst" in sh_preproc to account correctly for x-files whose site ID is four numeric digits.”j§]”j±ŒkEdited “set exlst†in sh_preproc to account correctly for x-files whose site ID is four numeric digits.”…””}”(j¶jöÛjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK²j¶j%ØjÇjaÓubj`)”}”(j¦Œ’sh_get_rinex/sh_PBS_gamit/sh_PBS_glred: Removed echo of or call to "$?" in to avoid "Newline in variable name." error on some csh implementations.”j§]”j±Œšsh_get_rinex/sh_PBS_gamit/sh_PBS_glred: Removed echo of or call to “$?†in to avoid “Newline in variable name.†error on some csh implementations.”…””}”(j¶jÜjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKµj¶j%ØjÇjaÓubj`)”}”(j¦ŒKsh_get_hfiles: Changed ftp command test string to "$ftpcmd[1]" at line 189.”j§]”j±ŒOsh_get_hfiles: Changed ftp command test string to “$ftpcmd[1]†at line 189.”…””}”(j¶jÜjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK¸j¶j%ØjÇjaÓubj`)”}”(j¦ŒFUpdated velrot to output summary statistics to output file and screen.”j§]”j±ŒFUpdated velrot to output summary statistics to output file and screen.”…””}”(j¶j ÜjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKºj¶j%ØjÇjaÓubj`)”}”(j¦Œ20,000 parameters. See globk.hlp and glorg.hlp for other features added in recent versions.”j§]”j±Œ‹Modified memory management in globk to handle >20,000 parameters. See globk.hlp and glorg.hlp for other features added in recent versions.”…””}”(j¶j4ÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKâj¶j%ØjÇjaÓubj`)”}”(j¦Œ,Kalman filter added to tsfit (see tsfit.hlp)”j§]”j±Œ,Kalman filter added to tsfit (see tsfit.hlp)”…””}”(j¶jBÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKåj¶j%ØjÇjaÓubj`)”}”(j¦ŒÁChanged the conversion of sp3 files to g- or t-files to use the IERS2010 dirunal and semi-diurnal EOP so as to be consistent with the rotations in MODEL (differences of 2 mm in orbit position).”j§]”j±ŒÁChanged the conversion of sp3 files to g- or t-files to use the IERS2010 dirunal and semi-diurnal EOP so as to be consistent with the rotations in MODEL (differences of 2 mm in orbit position).”…””}”(j¶jPÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKçj¶j%ØjÇjaÓubj`)”}”(j¦ŒŸIntroduced and made default IGRF12 for the magnetic field used to compute 2nd order ionospheric corrections. Thanks to Seiichi Shimada of NIED for this change.”j§]”j±ŒŸIntroduced and made default IGRF12 for the magnetic field used to compute 2nd order ionospheric corrections. Thanks to Seiichi Shimada of NIED for this change.”…””}”(j¶j^ÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKëj¶j%ØjÇjaÓubj`)”}”(j¦XÔChanges to sh_plot_pos: Switched position of north and east component plots and fixed long-standing bug with not plotting discontinuities when specifying rename- and/or eq-files and, implicitly or explicitly, using "NONE" as tsfit command file. Added additional width to time axis in figures to prevent first and/or last time series points plotting beneath y-axes, and added -w option to control fraction of time series length to add (default 0.1 = 10% on both ends).”j§]”j±XØChanges to sh_plot_pos: Switched position of north and east component plots and fixed long-standing bug with not plotting discontinuities when specifying rename- and/or eq-files and, implicitly or explicitly, using “NONE†as tsfit command file. Added additional width to time axis in figures to prevent first and/or last time series points plotting beneath y-axes, and added -w option to control fraction of time series length to add (default 0.1 = 10% on both ends).”…””}”(j¶jlÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKïj¶j%ØjÇjaÓubj`)”}”(j¦ŒÑChanged sh_get_orbits so that IGS final orbits downloaded from CDDIS are repro2 rather than repro1 for GPS weeks 658 to 1831. IGS final orbits down- oaded from SOPAC are still repro1 (for GPS weeks 730-1459).”j§]”j±ŒÑChanged sh_get_orbits so that IGS final orbits downloaded from CDDIS are repro2 rather than repro1 for GPS weeks 658 to 1831. IGS final orbits down- oaded from SOPAC are still repro1 (for GPS weeks 730-1459).”…””}”(j¶jzÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆK÷j¶j%ØjÇjaÓubj`)”}”(j¦X‘Changed sh_update_eop to use wget or curl rather than ftp or ncftp to download EOP files from USNO to avoid frequent ftp hang-ups. The new version supports extent 'usno' (Bulletin A finals.data from 1992, updated weekly) and 'usnd' (Bulleton A finals.daily, last 3 months only, updated daily). We no longer distribute Bulletin B since the Bulletin A value are as accurate and updated more frequently.”j§]”j±X™Changed sh_update_eop to use wget or curl rather than ftp or ncftp to download EOP files from USNO to avoid frequent ftp hang-ups. The new version supports extent ‘usno’ (Bulletin A finals.data from 1992, updated weekly) and ‘usnd’ (Bulleton A finals.daily, last 3 months only, updated daily). We no longer distribute Bulletin B since the Bulletin A value are as accurate and updated more frequently.”…””}”(j¶jˆÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆKûj¶j%ØjÇjaÓubj`)”}”(j¦XQReplaced hyphen ("-") with underscore ("_") for output org-file name produced by sh_glred when run in combination mode (using -ncomb) to avoid clash when being read by another GLOBK program, e.g. ensum, bcsum, etc. Output combined org-file name now of the form globk_[expt]_[YYDoY]_[YYDoY].org rather than globk_[expt]_[YYDoY]-[DoY].org.”j§]”j±XYReplaced hyphen (“-â€) with underscore (“_â€) for output org-file name produced by sh_glred when run in combination mode (using -ncomb) to avoid clash when being read by another GLOBK program, e.g. ensum, bcsum, etc. Output combined org-file name now of the form globk_[expt]_[YYDoY]_[YYDoY].org rather than globk_[expt]_[YYDoY]-[DoY].org.”…””}”(j¶j–ÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦ŒECorrect the format for reading ATMOSMAP values from a VMF1 list file.”j§]”j±ŒECorrect the format for reading ATMOSMAP values from a VMF1 list file.”…””}”(j¶j¤ÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦XsFix bug in gamit/lib/read_antex.f that caused PCO and PCV values to be zero if the frequency codes are written 'G 1' and 'G 2' instead of 'G01' and 'G02". This affects the following antennas using NOAA calibrations: TPSPG_A1_6+GP, SOK_GSR2700ISX, THA800961+REC, THA800961+RTK, THA800961RECUHF, THA800961RTKUHF, NOV702_3.00, JNSCR_C146-22-1, TRM_R6, TRM_R8, JAV_TRIUMPH-1.”j§]”j±XƒFix bug in gamit/lib/read_antex.f that caused PCO and PCV values to be zero if the frequency codes are written ‘G 1’ and ‘G 2’ instead of ‘G01’ and ‘G02â€. This affects the following antennas using NOAA calibrations: TPSPG_A1_6+GP, SOK_GSR2700ISX, THA800961+REC, THA800961+RTK, THA800961RECUHF, THA800961RTKUHF, NOV702_3.00, JNSCR_C146-22-1, TRM_R6, TRM_R8, JAV_TRIUMPH-1.”…””}”(j¶j²ÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM j¶j%ØjÇjaÓubj`)”}”(j¦ŒöAltered sh_makeeqdef event naming logic so that all earthquakes found in catalogs are numbered sequentially and are only given two-character IDs (e.g. see below entry) after they are selected as potentially influencing a site in the .”j§]”j±ŒöAltered sh_makeeqdef event naming logic so that all earthquakes found in catalogs are numbered sequentially and are only given two-character IDs (e.g. see below entry) after they are selected as potentially influencing a site in the .”…””}”(j¶jÀÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦XModfified glinit so that when the make_svs command is used, the satellite antenna offsets from the latest run (run time value) are adopted as the apriori antenna offsets. Needed when merging new processing (IGS08) with early MIT global files (e.g. in IGS05).”j§]”j±XModfified glinit so that when the make_svs command is used, the satellite antenna offsets from the latest run (run time value) are adopted as the apriori antenna offsets. Needed when merging new processing (IGS08) with early MIT global files (e.g. in IGS05).”…””}”(j¶jÎÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦Œ€Add general relativity corrections to the orbital integration, changing scale and clock slightly but little affect on positions.”j§]”j±Œ€Add general relativity corrections to the orbital integration, changing scale and clock slightly but little affect on positions.”…””}”(j¶jÜÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦ŒFixed bugs in the mean pole used in the ocean pole tide correction and in equate decoding in glorg. Updated model output in the SINEX files.”j§]”j±ŒFixed bugs in the mean pole used in the ocean pole tide correction and in equate decoding in glorg. Updated model output in the SINEX files.”…””}”(j¶jêÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦Œ7Fix long-standing bug causing loss of a 32nd satellite.”j§]”j±Œ7Fix long-standing bug causing loss of a 32nd satellite.”…””}”(j¶jøÝjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM!j¶j%ØjÇjaÓubj`)”}”(j¦ŒâFixed bug in kf/glinit/read_eq_file.f that could result in the end time of rename being incorrectly set for open ended renames. Fixed bug in kf/utils/stinf_to_rename.f that could result in misssed renames after the -post date.”j§]”j±ŒâFixed bug in kf/glinit/read_eq_file.f that could result in the end time of rename being incorrectly set for open ended renames. Fixed bug in kf/utils/stinf_to_rename.f that could result in misssed renames after the -post date.”…””}”(j¶jÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM#j¶j%ØjÇjaÓubj`)”}”(j¦ŒWIncrease max_sites in /kf/utils/merge_apr.f to accommodate the current itrf08_comb.apr.”j§]”j±ŒWIncrease max_sites in /kf/utils/merge_apr.f to accommodate the current itrf08_comb.apr.”…””}”(j¶jÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM(j¶j%ØjÇjaÓubj`)”}”(j¦ŒRAdded "-H" option to "find" commands in install_software to follow symbolic links.”j§]”j±ŒZAdded “-H†option to “find†commands in install_software to follow symbolic links.”…””}”(j¶j"ÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM+j¶j%ØjÇjaÓubj`)”}”(j¦ŒCIncrease the PID in the c-file name to 6 digits for large machines.”j§]”j±ŒCIncrease the PID in the c-file name to 6 digits for large machines.”…””}”(j¶j0ÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM.j¶j%ØjÇjaÓubj`)”}”(j¦ŒMNew script sh_pbor_vel to create PBO-format velocity files from GLOBK output.”j§]”j±ŒMNew script sh_pbor_vel to create PBO-format velocity files from GLOBK output.”…””}”(j¶j>ÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM0j¶j%ØjÇjaÓubj`)”}”(j¦Œ:Fix bug in sh_org2vel that causes some sites to be missed.”j§]”j±Œ:Fix bug in sh_org2vel that causes some sites to be missed.”…””}”(j¶jLÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM3j¶j%ØjÇjaÓubj`)”}”(j¦Œ@Replace itrf00.apr with itrf08_comb.apr as default for sh_setup.”j§]”j±Œ@Replace itrf00.apr with itrf08_comb.apr as default for sh_setup.”…””}”(j¶jZÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM5j¶j%ØjÇjaÓubj`)”}”(j¦ŒtAdded new scripts sh_cats and sh_hector in com/ to analyse noise charac- teristics of time series (using pos-files).”j§]”j±ŒtAdded new scripts sh_cats and sh_hector in com/ to analyse noise charac- teristics of time series (using pos-files).”…””}”(j¶jhÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM7j¶j%ØjÇjaÓubj`)”}”(j¦ŒsUpdated glorg to allow multiple site selections in equate/unequate/force commands. Fixed typo in .pos file headers.”j§]”j±ŒsUpdated glorg to allow multiple site selections in equate/unequate/force commands. Fixed typo in .pos file headers.”…””}”(j¶jvÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM:j¶j%ØjÇjaÓubj`)”}”(j¦XŽChanged sh_makeeqdef "-pos " option to "-f " to avoid confusion with PBO-format pos-files; changed event ID sequencing scheme from purely numeric to purely two-character (01...99, then A1...A9, B1...B9 etc. until Z1...Z9, then 1A...1Z, 2A...2Z etc. until 9A...9Z); added option to use a translation table (e.g. see ~/gg/tables/eq.transtbl) to edit automatic ID to user-friendly alternative. All automatic IDs now contain at least one numeric character, while manual IDs are recommended to be two alphabetic characters, as always. Updated USGS earthquake search URL and made minor changes to event (re) naming logic in sh_makeeqdef.”j§]”j±X–Changed sh_makeeqdef “-pos †option to “-f †to avoid confusion with PBO-format pos-files; changed event ID sequencing scheme from purely numeric to purely two-character (01…99, then A1…A9, B1…B9 etc. until Z1…Z9, then 1A…1Z, 2A…2Z etc. until 9A…9Z); added option to use a translation table (e.g. see ~/gg/tables/eq.transtbl) to edit automatic ID to user-friendly alternative. All automatic IDs now contain at least one numeric character, while manual IDs are recommended to be two alphabetic characters, as always. Updated USGS earthquake search URL and made minor changes to event (re) naming logic in sh_makeeqdef.”…””}”(j¶j„ÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM=j¶j%ØjÇjaÓubj`)”}”(j¦Œ\Updated coefficents for the solid-Earth pole tide to be consistent with IERS 2010 standards.”j§]”j±Œ\Updated coefficents for the solid-Earth pole tide to be consistent with IERS 2010 standards.”…””}”(j¶j’ÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMGj¶j%ØjÇjaÓubj`)”}”(j¦ŒAdd libration terms to UT1.”j§]”j±ŒAdd libration terms to UT1.”…””}”(j¶j ÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMJj¶j%ØjÇjaÓubj`)”}”(j¦ŒLUpdated tsfit, tscon and tsjumps to allows ~ (home directory) in file names.”j§]”j±ŒLUpdated tsfit, tscon and tsjumps to allows ~ (home directory) in file names.”…””}”(j¶j®ÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMLj¶j%ØjÇjaÓubj`)”}”(j¦Œ¶Add a script sh_glist2cmd to invoke existing program glist2cmd, which creates from a glist a use_site list, an input file for unify_apr, and (new) an input site list for sh_makeqdef.”j§]”j±Œ¶Add a script sh_glist2cmd to invoke existing program glist2cmd, which creates from a glist a use_site list, an input file for unify_apr, and (new) an input site list for sh_makeqdef.”…””}”(j¶j¼ÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMOj¶j%ØjÇjaÓubj`)”}”(j¦XAdd the EPN cumulative solution to the ITRF2008 apr and eq files. Fixed bug causing bogus entries for 73 sites when EPN or NGS steps are inconsistent with those from ITRF2008 and IGS08. See tables/renames.bad for possible errors between early 2014 and June.”j§]”j±XAdd the EPN cumulative solution to the ITRF2008 apr and eq files. Fixed bug causing bogus entries for 73 sites when EPN or NGS steps are inconsistent with those from ITRF2008 and IGS08. See tables/renames.bad for possible errors between early 2014 and June.”…””}”(j¶jÊÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMSj¶j%ØjÇjaÓubj`)”}”(j¦ŒvFix problem with poorly determined average of the east component of the atmospheric load for a site close to the pole.”j§]”j±ŒvFix problem with poorly determined average of the east component of the atmospheric load for a site close to the pole.”…””}”(j¶jØÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMXj¶j%ØjÇjaÓubj`)”}”(j¦Œ_sh_org2vel: Updated longitude/latitude format to five decimal places, in keeping with org-file.”j§]”j±Œ_sh_org2vel: Updated longitude/latitude format to five decimal places, in keeping with org-file.”…””}”(j¶jæÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM[j¶j%ØjÇjaÓubj`)”}”(j¦Œaftp_info: Modified for correct igni address for IONEX files; add PANGA, EPNCB, and TrigNet sites.”j§]”j±Œaftp_info: Modified for correct igni address for IONEX files; add PANGA, EPNCB, and TrigNet sites.”…””}”(j¶jôÞjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM^j¶j%ØjÇjaÓubj`)”}”(j¦X7Added additional width to time axis in figures made by sh_plot_pos to prevent first and/or last time series points plotting beneath y-axes, and added -w option to control fraction of time series length to add (default 0.1 = 10% on both ends). Corrected expected residuals file name to plot after running tsfit.”j§]”j±X7Added additional width to time axis in figures made by sh_plot_pos to prevent first and/or last time series points plotting beneath y-axes, and added -w option to control fraction of time series length to add (default 0.1 = 10% on both ends). Corrected expected residuals file name to plot after running tsfit.”…””}”(j¶jßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMaj¶j%ØjÇjaÓubj`)”}”(j¦Œ´svnav.dat: Correct start date for PN06/SV49---important bug affecting data for epochs 2013 12 19 thru 2014 4 3. Fix typo in start date for PRN30/SVN49 introduced in 121220 update.”j§]”j±Œ´svnav.dat: Correct start date for PN06/SV49—important bug affecting data for epochs 2013 12 19 thru 2014 4 3. Fix typo in start date for PRN30/SVN49 introduced in 121220 update.”…””}”(j¶jßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMfj¶j%ØjÇjaÓubj`)”}”(j¦Œ)Fix bug in rotation derivatives in GLOBK.”j§]”j±Œ)Fix bug in rotation derivatives in GLOBK.”…””}”(j¶jßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMjj¶j%ØjÇjaÓubj`)”}”(j¦ŒFix format error in svpos.”j§]”j±ŒFix format error in svpos.”…””}”(j¶j,ßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMlj¶j%ØjÇjaÓubj`)”}”(j¦ŒXMove rotation and translation estimates to be next to PMU estimates in GLOBK print file.”j§]”j±ŒXMove rotation and translation estimates to be next to PMU estimates in GLOBK print file.”…””}”(j¶j:ßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMnj¶j%ØjÇjaÓubj`)”}”(j¦ŒAFix gamit/utils/merge_rinex.f to handle more than 10 observables.”j§]”j±ŒAFix gamit/utils/merge_rinex.f to handle more than 10 observables.”…””}”(j¶jHßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMqj¶j%ØjÇjaÓubj`)”}”(j¦ŒbUpdated wild card use in site names in mar_neu command (needed for change in sh_gen_stats script).”j§]”j±ŒbUpdated wild card use in site names in mar_neu command (needed for change in sh_gen_stats script).”…””}”(j¶jVßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMsj¶j%ØjÇjaÓubj`)”}”(j¦ŒËEdited name of temporary file in install_software to avoid accidentally overwriting any libraries/Makefile.config.new when performing (and succeeding) with automatic search for X11LIBPATH and X11INCPATH.”j§]”j±ŒËEdited name of temporary file in install_software to avoid accidentally overwriting any libraries/Makefile.config.new when performing (and succeeding) with automatic search for X11LIBPATH and X11INCPATH.”…””}”(j¶jdßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMvj¶j%ØjÇjaÓubj`)”}”(j¦Œ1Updated tscon uto handle new Measures XYZ format.”j§]”j±Œ1Updated tscon uto handle new Measures XYZ format.”…””}”(j¶jrßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMzj¶j%ØjÇjaÓubj`)”}”(j¦Œ)Fix problem with computing GRACE seconds.”j§]”j±Œ)Fix problem with computing GRACE seconds.”…””}”(j¶j€ßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM|j¶j%ØjÇjaÓubj`)”}”(j¦ŒXUpdate gamit/utils/autecl.f to allow deleting post-eclipes data for Block II satellites.”j§]”j±ŒXUpdate gamit/utils/autecl.f to allow deleting post-eclipes data for Block II satellites.”…””}”(j¶jŽßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM~j¶j%ØjÇjaÓubj`)”}”(j¦ŒCFix end-of-year problem with dcb.dat. Thanks to S. Shimada of NIED,”j§]”j±ŒCFix end-of-year problem with dcb.dat. Thanks to S. Shimada of NIED,”…””}”(j¶jœßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦Œ Fixed bug in MODEL, introduced in December 2012, which caused GPT/GPT2 values to be used for mapping functions and dry zenith delays even if VMF1 was specified.”j§]”j±Œ Fixed bug in MODEL, introduced in December 2012, which caused GPT/GPT2 values to be used for mapping functions and dry zenith delays even if VMF1 was specified.”…””}”(j¶jªßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMƒj¶j%ØjÇjaÓubj`)”}”(j¦Œ-Fix version number in sh_gamit. King 130727.”j§]”j±Œ-Fix version number in sh_gamit. King 130727.”…””}”(j¶j¸ßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM‡j¶j%ØjÇjaÓubj`)”}”(j¦ŒFFix typos is globk_comb.cmd and glorg_long.cmd templates in gg/tables.”j§]”j±ŒFFix typos is globk_comb.cmd and glorg_long.cmd templates in gg/tables.”…””}”(j¶jÆßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM‰j¶j%ØjÇjaÓubj`)”}”(j¦ŒFFix bugs in fitting GAMIT's model to a broadcast ephemeris (sh_bcfit).”j§]”j±ŒHFix bugs in fitting GAMIT’s model to a broadcast ephemeris (sh_bcfit).”…””}”(j¶jÔßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM‹j¶j%ØjÇjaÓubj`)”}”(j¦Œ^New option -subdir for sh_get_rinex to speed up uncompression when there are many RINEX files.”j§]”j±Œ^New option -subdir for sh_get_rinex to speed up uncompression when there are many RINEX files.”…””}”(j¶jâßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦Œ›Update kf/Khandler/eq_name_chng.f so that _XPS/_XCL sites can not be renamed by later renames. RESET needed to rename _X?? sites if saved to binary hfile.”j§]”j±Œ›Update kf/Khandler/eq_name_chng.f so that _XPS/_XCL sites can not be renamed by later renames. RESET needed to rename _X?? sites if saved to binary hfile.”…””}”(j¶jðßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦ŒŒUpdated grdtab for modification to CoM correction to S1/S2 tidal loading and correct detection of dates out of time range of map.grid files.”j§]”j±ŒŒUpdated grdtab for modification to CoM correction to S1/S2 tidal loading and correct detection of dates out of time range of map.grid files.”…””}”(j¶jþßjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM”j¶j%ØjÇjaÓubj`)”}”(j¦ŒLAdded lunisolar tables for 2015; Updated leap.sec for June 2015 leap second.”j§]”j±ŒLAdded lunisolar tables for 2015; Updated leap.sec for June 2015 leap second.”…””}”(j¶j àjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM—j¶j%ØjÇjaÓubj`)”}”(j¦ŒnAllow reading of a time-of-year-dependent grid for atmospheric tidal loading (not yet recommended by the IGS).”j§]”j±ŒnAllow reading of a time-of-year-dependent grid for atmospheric tidal loading (not yet recommended by the IGS).”…””}”(j¶jàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM™j¶j%ØjÇjaÓubj`)”}”(j¦ŒkAdd glinit/solution_inf.f, glist/glist.f, and htoglb/cresnx_file.f to /kf to fix problem with null string.”j§]”j±ŒkAdd glinit/solution_inf.f, glist/glist.f, and htoglb/cresnx_file.f to /kf to fix problem with null string.”…””}”(j¶j(àjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMœj¶j%ØjÇjaÓubj`)”}”(j¦ŒkAdd the Earth-radiation, antenna-radiation, and 2nd-order ionospheric model nmmes to the c-file and h-file.”j§]”j±ŒkAdd the Earth-radiation, antenna-radiation, and 2nd-order ionospheric model nmmes to the c-file and h-file.”…””}”(j¶j6àjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMŸj¶j%ØjÇjaÓubj`)”}”(j¦Œ‡Various features and updates made to the suite of globk and tsxxx programs. See help files for new features. tscomp added to suite. .”j§]”j±Œ‡Various features and updates made to the suite of globk and tsxxx programs. See help files for new features. tscomp added to suite. .”…””}”(j¶jDàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM¢j¶j%ØjÇjaÓubj`)”}”(j¦Œ(Increase the dimensions for IONEX files.”j§]”j±Œ(Increase the dimensions for IONEX files.”…””}”(j¶jRàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM¥j¶j%ØjÇjaÓubj`)”}”(j¦Œ:Increased dimensions in kf/utils/netsel.h Herring 140718”j§]”j±Œ:Increased dimensions in kf/utils/netsel.h Herring 140718”…””}”(j¶j`àjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM§j¶j%ØjÇjaÓubj`)”}”(j¦Œ.Enhancements to cplotx including adding color.”j§]”j±Œ.Enhancements to cplotx including adding color.”…””}”(j¶jnàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM©j¶j%ØjÇjaÓubj`)”}”(j¦Œ“Sped up search for earthquake/rename displacements, and corrected output for field overflow in org-file and multiple/duplicate renames in sh_exglk.”j§]”j±Œ“Sped up search for earthquake/rename displacements, and corrected output for field overflow in org-file and multiple/duplicate renames in sh_exglk.”…””}”(j¶j|àjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM«j¶j%ØjÇjaÓubj`)”}”(j¦Œ¬sh_upd_stnfo: corrected bugs in kf/htoglb/mstinf.f in using IGS SINEX and GIPSY sta_svec files. Add a '-nogaps' option to close gaps in erroneous entries in IGS log files.”j§]”j±Œ°sh_upd_stnfo: corrected bugs in kf/htoglb/mstinf.f in using IGS SINEX and GIPSY sta_svec files. Add a ‘-nogaps’ option to close gaps in erroneous entries in IGS log files.”…””}”(j¶jŠàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM®j¶j%ØjÇjaÓubj`)”}”(j¦ŒPsh_glred: Fix remaining bugs in allowing use of PBO-style h-files (.glb extent).”j§]”j±ŒPsh_glred: Fix remaining bugs in allowing use of PBO-style h-files (.glb extent).”…””}”(j¶j˜àjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM²j¶j%ØjÇjaÓubj`)”}”(j¦ŒFixed long-standing typo in format statement in gamit/makexp/makexp.f producing a compile error with gfortran 4.6ff (but not earlier compilers).”j§]”j±ŒFixed long-standing typo in format statement in gamit/makexp/makexp.f producing a compile error with gfortran 4.6ff (but not earlier compilers).”…””}”(j¶j¦àjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM´j¶j%ØjÇjaÓubj`)”}”(j¦ŒpTRACK: Fix minor problem with noise_tol. Fix bug in wide-lane-reference combinations (read_all_rinex.f 130730).”j§]”j±ŒpTRACK: Fix minor problem with noise_tol. Fix bug in wide-lane-reference combinations (read_all_rinex.f 130730).”…””}”(j¶j´àjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM·j¶j%ØjÇjaÓubj`)”}”(j¦Œ—New Receivers: TIASAHI PENG3100-R2, JAVAD TRIUMPH_1, JAVAD TRIUMPH_1M, JAVAD TRIUMPH2,MAG111406, NOV OEM4-G2, ITT 3750300, CHX90D-OPUS, ASHTECH PM-500.”j§]”j±Œ—New Receivers: TIASAHI PENG3100-R2, JAVAD TRIUMPH_1, JAVAD TRIUMPH_1M, JAVAD TRIUMPH2,MAG111406, NOV OEM4-G2, ITT 3750300, CHX90D-OPUS, ASHTECH PM-500.”…””}”(j¶jÂàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMºj¶j%ØjÇjaÓubj`)”}”(j¦X7New Antennas: TIAPENG3100R2, STHCR3-G3 , JAVTRIUMPH_1M, JAVTRIUMPH_1MR, JAVTRIUMPH_LSA, Antcom ACC123CGN_XN, TRM57971.00 SCIT, LEIAX1202A, LEIAX1202A, TPSCR.G3 SCIT, MAG111406, ASH701945A NONE, TRM55970.00, TRMR6, JAV_TRIUMPH-1R, CHX90D-OPUS, JAVTRIANT_A, JAVTRIANT_B,ASH700829.3 NONE, JAVTRIANT_A, JAVTRIANT_B.”j§]”j±X7New Antennas: TIAPENG3100R2, STHCR3-G3 , JAVTRIUMPH_1M, JAVTRIUMPH_1MR, JAVTRIUMPH_LSA, Antcom ACC123CGN_XN, TRM57971.00 SCIT, LEIAX1202A, LEIAX1202A, TPSCR.G3 SCIT, MAG111406, ASH701945A NONE, TRM55970.00, TRMR6, JAV_TRIUMPH-1R, CHX90D-OPUS, JAVTRIANT_A, JAVTRIANT_B,ASH700829.3 NONE, JAVTRIANT_A, JAVTRIANT_B.”…””}”(j¶jÐàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM¾j¶j%ØjÇjaÓubj`)”}”(j¦Œ** 10.50 vs 10.41”j§]”j±Œ** 10.50 vs 10.41”…””}”(j¶jÞàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMÅj¶j%ØjÇjaÓubj`)”}”(j¦X-We have provided and will keep up-to-date, ITRF2008 coordinates sites in prior releases of the ITRF as well as new sites that have been and will be added for IGS processing. The primary file, in the ITRF2008 NNR frame is itrf08_comb.apr; and there are secondary files, itrf08_comb_[plate].apr, created by rotating this file to the frames of the major plates using the Euler poles estimated by Altamimi et al. [J. Geophys. Res., 117, B07402, doi:10.1029/2011JB008930,2012]. (Note that the plate-referenced files that we created 2012-01-06 and put into incremental_updates/tables were based on preliminary vectors that changed in the final publication, so users who downloaded these should replace them by the current files.) These files should always be used in conjunc- tion with the rename file itrf08_comb.eq to assure that the 8-character site name assigned to your data matches the coordinates for the appropri- ate period. See 'apr_and_eq_files.txt' in the download documentation directory for a complete explanation of how the combined files were constructed.”j§]”j±X1We have provided and will keep up-to-date, ITRF2008 coordinates sites in prior releases of the ITRF as well as new sites that have been and will be added for IGS processing. The primary file, in the ITRF2008 NNR frame is itrf08_comb.apr; and there are secondary files, itrf08_comb_[plate].apr, created by rotating this file to the frames of the major plates using the Euler poles estimated by Altamimi et al. [J. Geophys. Res., 117, B07402, doi:10.1029/2011JB008930,2012]. (Note that the plate-referenced files that we created 2012-01-06 and put into incremental_updates/tables were based on preliminary vectors that changed in the final publication, so users who downloaded these should replace them by the current files.) These files should always be used in conjunc- tion with the rename file itrf08_comb.eq to assure that the 8-character site name assigned to your data matches the coordinates for the appropri- ate period. See ‘apr_and_eq_files.txt’ in the download documentation directory for a complete explanation of how the combined files were constructed.”…””•}”(j¶jìàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMÇj¶j%ØjÇjaÓubj`)”}”(j¦X2There are improved templates in ~/gg/tables for GLOBK runs: globk_comb.cmd, glorg_comb.cmd, globk_long.cmd, glorg_long.cmd. These reflect current best practice and take advantage of the 'option' feature of the globk, glorg, and sh_glred command lines so that the same command file can be used for both repeatabilities and velocity solutions without editing the file itself. The standard southern California example has been reworked to use these file and should now be easier to execute and to use as a template for your own processing. Also, there is a new detailed recipe for processing and analyzing survey-mode (sGPS) measurements, 'sGPS_recipe.txt', to be found in the documents directory of the download site and also on the web as part of the presentations from the recent workshop held at UNAVCO (Boulder13).”j§]”j±X:There are improved templates in ~/gg/tables for GLOBK runs: globk_comb.cmd, glorg_comb.cmd, globk_long.cmd, glorg_long.cmd. These reflect current best practice and take advantage of the ‘option’ feature of the globk, glorg, and sh_glred command lines so that the same command file can be used for both repeatabilities and velocity solutions without editing the file itself. The standard southern California example has been reworked to use these file and should now be easier to execute and to use as a template for your own processing. Also, there is a new detailed recipe for processing and analyzing survey-mode (sGPS) measurements, ‘sGPS_recipe.txt’, to be found in the documents directory of the download site and also on the web as part of the presentations from the recent workshop held at UNAVCO (Boulder13).”…””}”(j¶júàjÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMØj¶j%ØjÇjaÓubj`)”}”(j¦X½The GPT/GMF models for zenith hydrostatic delay and mapping functions have been replaced by the new GPT2 model (Lager et al., Geophys. Res. Lett., ) which is based on a more refined numerical weather model, includes semi-annual as well as annual variations, has better spatial resolution, and accounts better for height differences through a seasonally dependent lapse rate. In the new model both the ZHD and mapping funtions are derived from a table, gpt.dat, automatically linked into the experiment and day directories from ~/gg/tables. If you specify GPT or GMT in your sestbl. and have gpt.dat in ~/gg/tables, you will automatically get GPT2 (the old GPT is invoked only if gpt.dat is missing).”j§]”j±X½The GPT/GMF models for zenith hydrostatic delay and mapping functions have been replaced by the new GPT2 model (Lager et al., Geophys. Res. Lett., ) which is based on a more refined numerical weather model, includes semi-annual as well as annual variations, has better spatial resolution, and accounts better for height differences through a seasonally dependent lapse rate. In the new model both the ZHD and mapping funtions are derived from a table, gpt.dat, automatically linked into the experiment and day directories from ~/gg/tables. If you specify GPT or GMT in your sestbl. and have gpt.dat in ~/gg/tables, you will automatically get GPT2 (the old GPT is invoked only if gpt.dat is missing).”…””}”(j¶jájÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMæj¶j%ØjÇjaÓubj`)”}”(j¦XLGLOBK now has the ability to remove non-tidal atmospheric loading (ATML) based on the average of the day given in the h-file. Since GLOBK can not yet read an grid file to apply the ATML corrections directly, if you want to investigate their effects, the best strategy is to apply the ATML in GAMIT and then optionally retain or remove the corrections using the new command -appload_mod in the GLOBK commaand file. The preferred ATML files for GAMIT are those that have been filtered to remove sub-daily terms (atmfilt_cm.YYYY). In principle, the sub-daily thermal tides should be applied in GAMIT, but none of the current models, including a time-dependent recently developed by Ray and Ponte, has been shown to reproduce accurately the tidal loading, so the present recommendation of the IGS for the next reprocessing is to omit these terms.”j§]”j±XLGLOBK now has the ability to remove non-tidal atmospheric loading (ATML) based on the average of the day given in the h-file. Since GLOBK can not yet read an grid file to apply the ATML corrections directly, if you want to investigate their effects, the best strategy is to apply the ATML in GAMIT and then optionally retain or remove the corrections using the new command -appload_mod in the GLOBK commaand file. The preferred ATML files for GAMIT are those that have been filtered to remove sub-daily terms (atmfilt_cm.YYYY). In principle, the sub-daily thermal tides should be applied in GAMIT, but none of the current models, including a time-dependent recently developed by Ray and Ponte, has been shown to reproduce accurately the tidal loading, so the present recommendation of the IGS for the next reprocessing is to omit these terms.”…””}”(j¶jájÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMñj¶j%ØjÇjaÓubj`)”}”(j¦XALiz Petrie of the University of Newcastle has coded a model in ARC for the accelerations on the GPS satellites due to antenna radiation and Earth radiation. These models are invoked by setting 'Earth radiation model = NCELE1', now default in the sestbl. and 'fixdrv'. As part of this modification, we have reworked many of the subroutines in ARC to be more modular, added (backward-compatible) models to the ARC batch file, and coded sh_get_orbits and sh_sp3fit to read the orbital models from from a sestbl. This latter change assures that the orbital models used for creating g- and t-files from sp3 files will be consistent with the models used for the data processing. For sh_gamit processsing, the sestbl. in ../tables is automatically linked into the /igs directory. If the sestbl is absent, hard-wired models will be used.”j§]”j±XILiz Petrie of the University of Newcastle has coded a model in ARC for the accelerations on the GPS satellites due to antenna radiation and Earth radiation. These models are invoked by setting ‘Earth radiation model = NCELE1’, now default in the sestbl. and ‘fixdrv’. As part of this modification, we have reworked many of the subroutines in ARC to be more modular, added (backward-compatible) models to the ARC batch file, and coded sh_get_orbits and sh_sp3fit to read the orbital models from from a sestbl. This latter change assures that the orbital models used for creating g- and t-files from sp3 files will be consistent with the models used for the data processing. For sh_gamit processsing, the sestbl. in ../tables is automatically linked into the /igs directory. If the sestbl is absent, hard-wired models will be used.”…””}”(j¶j$ájÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMÿj¶j%ØjÇjaÓubj`)”}”(j¦X"Three model conventions have been updated to be consistent with those used by the IGS: mean pole and short-period EOP are changed from IERS 1996 to IERS 2010, and the gravity field from EGM96 to EGM08. These changes are important for EOP estimation but have neglible effect on positioning.”j§]”j±X"Three model conventions have been updated to be consistent with those used by the IGS: mean pole and short-period EOP are changed from IERS 1996 to IERS 2010, and the gravity field from EGM96 to EGM08. These changes are important for EOP estimation but have neglible effect on positioning.”…””}”(j¶j2ájÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆM j¶j%ØjÇjaÓubj`)”}”(j¦XíA new script sh_plot_pos will read PBO-style pos files rather than _mb files for plotting time series. GLOBK now generates the 'PBO' lines in the print files automatically (no need to use PBOP in the print options). We have retained sh_plotcrd and the use of _mb files for this release, but they will eventually go away. The Python script ts_plot.py, introduced in Release 10.40 to read pos files will also be abandoned because it required too many non-standard Python libraries (see below).”j§]”j±XñA new script sh_plot_pos will read PBO-style pos files rather than _mb files for plotting time series. GLOBK now generates the ‘PBO’ lines in the print files automatically (no need to use PBOP in the print options). We have retained sh_plotcrd and the use of _mb files for this release, but they will eventually go away. The Python script ts_plot.py, introduced in Release 10.40 to read pos files will also be abandoned because it required too many non-standard Python libraries (see below).”…””}”(j¶j@ájÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubj`)”}”(j¦XÕThe new script sh_plot_elmean, together with additions to the autcln summary files allow plotting of mean residuals over several days as a function of elevation angle or satellite nadir angle, providing more diagnostics for bad antenna models or tracking environments. These can be used instead of or in conjuction with the individual-day sky plots and phase vs elevation plots produced by sh_oneway from the autcln DPH files when '-pres ELEV' specified with sh_gamit.”j§]”j±XÙThe new script sh_plot_elmean, together with additions to the autcln summary files allow plotting of mean residuals over several days as a function of elevation angle or satellite nadir angle, providing more diagnostics for bad antenna models or tracking environments. These can be used instead of or in conjuction with the individual-day sky plots and phase vs elevation plots produced by sh_oneway from the autcln DPH files when ‘-pres ELEV’ specified with sh_gamit.”…””}”(j¶jNájÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“ÓjÆMj¶j%ØjÇjaÓubej·}”(j¹]”Œother-changes-for-10-61”aj»]”j½]”Œother changes for 10.61”ajÀ]”jÂ]”ujÄh_j¶j‚ÓjÇjaÓhj“ÓjÆK3ubej·}”(j¹]”Œid1”aj»]”j½]”Œ10.61”ajÀ]”jÂ]”ujÄh_j¶jaÓjÇjaÓhj“ÓjÆKubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j“Ój}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj“ÓjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jpÓjdÓjÓjsÓuj_}”(Œrel”jpÓŒdate”jÓujc}”je}”jg}”(jiájfájÐÔjÍÔjñÔjîÔjaáj^ájÜØjÙØjfÙjcÙj½ÙjºÙuji}”(jiá‰jÐÔˆjñÔˆjaá‰jÜ؈jfÙˆj½Ùˆuj¹}”(jfáj‚ÓjÍÔjÇÔjîÔjèÔjŽÖj’Öj^áj%ØjÙØjÓØjcÙj]Ùj˜Ùj’ÙjºÙj´Ùujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”jù )”}”(j¦hoj§]”j`)”}”(j¦Œ)Duplicate explicit target name: "hector".”j§]”j±Œ-Duplicate explicit target name: “hectorâ€.”…””}”(j¶jájÇjaÓhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jŒáubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j˜ÙaŒlevel”KŒtype”jŒsource”j“ÓŒline”KujÄjø j¶j%ØjÇjaÓhj“ÓjÆK@ubaj†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ-Hyperlink target "index-0" is not referenced.”…””}”j¶j«ásbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j¨áubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j“ÓŒline”K&ujÄjø ubajˆNj‰]”j‹NjÇjaÓubjøj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jÆásbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÃájÇjÃáubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jÕájÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÃájÇjÃáubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ10.7”j§]”j±Œ10.7”…””}”(j¶jçájÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jäájÇjÃáhŒA/chandler/home/floyd/public_html/gg/docs/source/relnote/10.70.rst”jÆKubj`)”}”(j¦ŒLast updated 13 June 2018”j§]”j±ŒLast updated 13 June 2018”…””}”(j¶jöájÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKj¶jäájÇjÃáubj`)”}”(j¦ŒÈRelease 10.7 consolidates incremental updates made since release 10.61 of April 2017 and completes the modifications to GAMIT allowing for separate processing of GPS, Beidou, Galileo, and now Glonass.”j§]”j±ŒÈRelease 10.7 consolidates incremental updates made since release 10.61 of April 2017 and completes the modifications to GAMIT allowing for separate processing of GPS, Beidou, Galileo, and now Glonass.”…””}”(j¶jâjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKj¶jäájÇjÃáubj`)”}”(j¦X:program:`sh_get_rinex` will download RINEX 3 files from CDDIS or UNAVCO, renaming them to RINEX 2 conventions. The orbit specification in :program:`sh_gamit` and :program:`sh_get_orbits` is now a 4-character code (e.g. :option:`igsf`, :option:`comf`, ...) rather than using the separate :option:`-center` and :option:`-pre` inputs (though these will still work). See the help for :program:`sh_gamit` or :program:`sh_get_orbits` for the list of supported codes. Navigation files for dates after GPS Week 1624 will always those from MGEX :file:`brdm[DDD]0.[yy]p` (identical to brdc for GPS), then renamed to :file:`brdm[DDD]0.[YY]n`. If a system other than GPS is requested, the SP3 files are downloaded from the CDDIS MGEX directory and renamed if necessary to the conventional short form :file:`[orb][WWWWD].sp3`. For the g-files, :program:`sh_gamit` replaces the orbit-precision 5th character by the lower-case GNSS code so that multiple g-files can exist in the :file:`gfiles/` directory. If :option:`-gnss` is specified in the :program:`sh_gamit` command line the day directories will automatically use a letter extent (:file:`G`, file:`R`, :file:`C`, :file:`E`); otherwise GPS is assumed and the day directory will be the usual 3-digit number unless :option:`-netext` is specified in the command line. To combine for each day the h-files from each GNSS, run :program:`sh_glred` with, e.g., :option:`-netext G R C E`.”j§]”(jj)”}”(j¦Œ:program:`sh_get_rinex`”j§]”j±Œ sh_get_rinex”…””}”(j¶jâjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jâubj±Œt will download RINEX 3 files from CDDIS or UNAVCO, renaming them to RINEX 2 conventions. The orbit specification in ”…””}”(j¶jâjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j(âjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jâubj±Œ and ”…””}”(j¶jâjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_get_orbits`”j§]”j±Œ sh_get_orbits”…””}”(j¶j:âjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jâubj±Œ! is now a 4-character code (e.g. ”…””}”(j¶jâjÇjÃáhNjÆNubj’)”}”(j¦Œ:option:`igsf`”j§]”j˜)”}”(j¦jNâj§]”j±Œigsf”…””}”(j¶jPâjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jLâubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”jZâŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œigsf”ujÄj‘hjõájÆK j¶jâubj±Œ, ”…””}”(j¶jâjÇjÃáhNjÆNubj’)”}”(j¦Œ:option:`comf`”j§]”j˜)”}”(j¦jrâj§]”j±Œcomf”…””}”(j¶jtâjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jpâubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”j~âŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œcomf”ujÄj‘hjõájÆK j¶jâubj±Œ&, …) rather than using the separate ”…””}”(j¶jâjÇjÃáhNjÆNubj’)”}”(j¦Œ:option:`-center`”j§]”j˜)”}”(j¦j–âj§]”j±Œ-center”…””}”(j¶j˜âjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j”âubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”j¢âŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-center”ujÄj‘hjõájÆK j¶jâubj±Œ and ”…””}”j¶jâsbj’)”}”(j¦Œ:option:`-pre`”j§]”j˜)”}”(j¦jºâj§]”j±Œ-pre”…””}”(j¶j¼âjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j¸âubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”jÆâŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-pre”ujÄj‘hjõájÆK j¶jâubj±Œ9 inputs (though these will still work). See the help for ”…””}”(j¶jâjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jÜâjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jâubj±Œ or ”…””}”(j¶jâjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_get_orbits`”j§]”j±Œ sh_get_orbits”…””}”(j¶jîâjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jâubj±Œm for the list of supported codes. Navigation files for dates after GPS Week 1624 will always those from MGEX ”…””}”(j¶jâjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`brdm[DDD]0.[yy]p`”j§]”j±Œbrdm[DDD]0.[yy]p”…””}”(j¶jãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jâubj±Œ. (identical to brdc for GPS), then renamed to ”…””}”(j¶jâjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`brdm[DDD]0.[YY]n`”j§]”j±Œbrdm[DDD]0.[YY]n”…””}”(j¶jãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jâubj±Œž. If a system other than GPS is requested, the SP3 files are downloaded from the CDDIS MGEX directory and renamed if necessary to the conventional short form ”…””}”(j¶jâjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`[orb][WWWWD].sp3`”j§]”j±Œ[orb][WWWWD].sp3”…””}”(j¶j*ãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jâubj±Œ. For the g-files, ”…””}”(j¶jâjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j?ãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jâubj±Œr replaces the orbit-precision 5th character by the lower-case GNSS code so that multiple g-files can exist in the ”…””}”(j¶jâjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`gfiles/`”j§]”j±Œgfiles/”…””}”(j¶jQãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jâubj±Œ directory. If ”…””}”(j¶jâjÇjÃáhNjÆNubj’)”}”(j¦Œ:option:`-gnss`”j§]”j˜)”}”(j¦jhãj§]”j±Œ-gnss”…””}”(j¶jjãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jfãubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”jtãŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-gnss”ujÄj‘hjõájÆK j¶jâubj±Œ is specified in the ”…””}”(j¶jâjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jŠãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jâubj±ŒJ command line the day directories will automatically use a letter extent (”…””}”(j¶jâjÇjÃáhNjÆNubj˜)”}”(j¦Œ :file:`G`”j§]”j±ŒG”…””}”(j¶jœãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jâubj±Œ, file:”…””}”(j¶jâjÇjÃáhNjÆNubj©Œtitle_reference”“”)”}”(j¦Œ`R`”j§]”j±ŒR”…””}”(j¶j³ãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj±ãj¶jâubj±Œ, ”…””}”j¶jâsbj˜)”}”(j¦Œ :file:`C`”j§]”j±ŒC”…””}”(j¶jÅãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jâubj±Œ, ”…””}”j¶jâsbj˜)”}”(j¦Œ :file:`E`”j§]”j±ŒE”…””}”(j¶jÚãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jâubj±ŒZ); otherwise GPS is assumed and the day directory will be the usual 3-digit number unless ”…””}”(j¶jâjÇjÃáhNjÆNubj’)”}”(j¦Œ:option:`-netext`”j§]”j˜)”}”(j¦jñãj§]”j±Œ-netext”…””}”(j¶jóãjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jïãubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”jýãŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-netext”ujÄj‘hjõájÆK j¶jâubj±Œ[ is specified in the command line. To combine for each day the h-files from each GNSS, run ”…””}”(j¶jâjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jäjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jâubj±Œ with, e.g., ”…””}”(j¶jâjÇjÃáhNjÆNubj’)”}”(j¦Œ:option:`-netext G R C E`”j§]”j˜)”}”(j¦j'äj§]”j±Œ-netext G R C E”…””}”(j¶j)äjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j%äubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”j3äŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-netext G R C E”ujÄj‘hjõájÆK j¶jâubj±Œ.”…””}”(j¶jâjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK j¶jäájÇjÃáubj`)”}”(j¦ŒêSince ftp is increasingly unavailable on new operating systems, we're migrating to a download scheme that uses curl for MacOS and wget for other operating systems. We need to know if users require the use of the programs ftp or ncftp.”j§]”j±ŒìSince ftp is increasingly unavailable on new operating systems, we’re migrating to a download scheme that uses curl for MacOS and wget for other operating systems. We need to know if users require the use of the programs ftp or ncftp.”…””}”(j¶jOäjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKj¶jäájÇjÃáubj`)”}”(j¦ŒæThe first line in the d-file and the :program:`model` batch file is changed, replacing the obsolete session number and static/kinematic code with the GNSS code. These files will not be compatible between 10.7 and earlier versions.”j§]”(j±Œ%The first line in the d-file and the ”…””}”(j¶j]äjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶jeäjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j]äubj±Œ± batch file is changed, replacing the obsolete session number and static/kinematic code with the GNSS code. These files will not be compatible between 10.7 and earlier versions.”…””}”(j¶j]äjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKj¶jäájÇjÃáubj`)”}”(j¦Xr:program:`arc` and :program:`model` can now read a multi-year planetary ephemeris file and use a subroutine to get nutations, so the use of the single-year :file:`soltab.`, :file:`luntab.`, and :file:`nutabl.` files is no longer necessary. For now they will still be linked but the new scheme will be automatically used if the :file:`nbody` file is present. It is always linked into the :file:`[expt]/tables/` and day directories, so you control this by linking either :file:`nbody740.2020.asc` or :file:`JPL.DE200` to :file:`nbody` in :file:`~/gg/tables/`. Our tests have shown that with :file:`nbody740.2020` (the original source for :file:`soltab.` and :file:`luntab.`) the processing results are virtually identical to using the yearly files. We have thus far found no improvement (or degradation) when using DE200. Beginning in 2019, we will no longer provide the yearly files.”j§]”(jj)”}”(j¦Œ:program:`arc`”j§]”j±Œarc”…””}”(j¶jäjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j}äubj±Œ and ”…””}”(j¶j}äjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶j“äjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j}äubj±Œy can now read a multi-year planetary ephemeris file and use a subroutine to get nutations, so the use of the single-year ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`soltab.`”j§]”j±Œsoltab.”…””}”(j¶j¥äjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ, ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`luntab.`”j§]”j±Œluntab.”…””}”(j¶jºäjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ, and ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`nutabl.`”j§]”j±Œnutabl.”…””}”(j¶jÏäjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œv files is no longer necessary. For now they will still be linked but the new scheme will be automatically used if the ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ :file:`nbody`”j§]”j±Œnbody”…””}”(j¶jääjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ/ file is present. It is always linked into the ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`[expt]/tables/`”j§]”j±Œ[expt]/tables/”…””}”(j¶jùäjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ< and day directories, so you control this by linking either ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`nbody740.2020.asc`”j§]”j±Œnbody740.2020.asc”…””}”(j¶jåjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ or ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`JPL.DE200`”j§]”j±Œ JPL.DE200”…””}”(j¶j#åjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ to ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ :file:`nbody`”j§]”j±Œnbody”…””}”(j¶j8åjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ in ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jMåjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ!. Our tests have shown that with ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`nbody740.2020`”j§]”j±Œ nbody740.2020”…””}”(j¶jbåjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ (the original source for ”…””}”(j¶j}äjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`soltab.`”j§]”j±Œsoltab.”…””}”(j¶jwåjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±Œ and ”…””}”j¶j}äsbj˜)”}”(j¦Œ:file:`luntab.`”j§]”j±Œluntab.”…””}”(j¶jŒåjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}äubj±ŒÓ) the processing results are virtually identical to using the yearly files. We have thus far found no improvement (or degradation) when using DE200. Beginning in 2019, we will no longer provide the yearly files.”…””}”(j¶j}äjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKj¶jäájÇjÃáubj`)”}”(j¦X˜The code in :program:`arc` is significantly changed to allow for 3rd and 4th degree solid-Earth tides, ocean tides, perturbations by Venus and Jupiter, a newer value for C20, and time-variable C30 and C40, but thus far these changes seem to offer no improvement, at least for single-day processing. There are new entries in the :file:`sestbl.` to set the highest degree harmonics for static gravity, solid-Earth tides, and ocean tides, currently set to :content:`12 2 0`, the effective values for previous releases. The area-to-mass ratios for Glonass, Beidou, and Galileo have been changed so that the estimated coefficient for the direct force is close to unity.”j§]”(j±Œ The code in ”…””}”(j¶j§åjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`arc`”j§]”j±Œarc”…””}”(j¶j¯åjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j§åubj±X. is significantly changed to allow for 3rd and 4th degree solid-Earth tides, ocean tides, perturbations by Venus and Jupiter, a newer value for C20, and time-variable C30 and C40, but thus far these changes seem to offer no improvement, at least for single-day processing. There are new entries in the ”…””}”(j¶j§åjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jÁåjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j§åubj±Œn to set the highest degree harmonics for static gravity, solid-Earth tides, and ocean tides, currently set to ”…””}”(j¶j§åjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`12 2 0`”j§]”j±Œ12 2 0”…””}”(j¶jÖåjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j§åubj±ŒÂ, the effective values for previous releases. The area-to-mass ratios for Glonass, Beidou, and Galileo have been changed so that the estimated coefficient for the direct force is close to unity.”…””}”(j¶j§åjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK j¶jäájÇjÃáubj`)”}”(j¦Œr:program:`yawtab` is now coded for all GNSS but not thoroughly tested for for a broad range of eclipse conditions.”j§]”(jj)”}”(j¦Œ:program:`yawtab`”j§]”j±Œyawtab”…””}”(j¶jóåjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jïåubj±Œa is now coded for all GNSS but not thoroughly tested for for a broad range of eclipse conditions.”…””}”(j¶jïåjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK$j¶jäájÇjÃáubj`)”}”(j¦X™The GLOBK suite is updated to support GNSS with a new satellite naming scheme. For GPS the default is to retain the :content:`PRN_` form where :content:`` is 2-digit PRN, :content:`` is 2-digit satellite vehicle number. The new scheme is :content:`_` where :content:`sys` is :content:`G`--GPS, :content:`R`-Glonass, :content:`E`-Galileo, :content:`C`-Beidou and the SV number has 3-digits. The :content:`use_prnn N` command will invoke using the new scheme for all satellites. GNSS h-files are automatically detected and no special changes to command files are needed. :program:`htoglb` generates binary H-files with new naming scheme.”j§]”(j±ŒtThe GLOBK suite is updated to support GNSS with a new satellite naming scheme. For GPS the default is to retain the ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`PRN_`”j§]”j±Œ PRN_”…””}”(j¶jæjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œ form where ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ”…””}”(j¶j&æjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œ is 2-digit PRN, ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ”…””}”(j¶j9æjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œ8 is 2-digit satellite vehicle number. The new scheme is ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`_`”j§]”j±Œ_”…””}”(j¶jLæjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œ where ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`sys`”j§]”j±Œsys”…””}”(j¶j_æjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œ is ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ :content:`G`”j§]”j±ŒG”…””}”(j¶jræjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œ–GPS, ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ :content:`R`”j§]”j±ŒR”…””}”(j¶j…æjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œ -Glonass, ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ :content:`E`”j§]”j±ŒE”…””}”(j¶j˜æjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œ -Galileo, ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ :content:`C`”j§]”j±ŒC”…””}”(j¶j«æjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œ,-Beidou and the SV number has 3-digits. The ”…””}”(j¶j æjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`use_prnn N`”j§]”j±Œ use_prnn N”…””}”(j¶j¾æjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j æubj±Œš command will invoke using the new scheme for all satellites. GNSS h-files are automatically detected and no special changes to command files are needed. ”…””}”(j¶j æjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`htoglb`”j§]”j±Œhtoglb”…””}”(j¶jÑæjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j æubj±Œ1 generates binary H-files with new naming scheme.”…””}”(j¶j æjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK&j¶jäájÇjÃáubj`)”}”(j¦X GLOBK suite has had various dimensions increased for GNSS and network sizes. The :program:`tssum`/:program:`tscon`/:program:`tsfit` programs take 7 Gb of memory to run UNR stations. Change content:`max_ent` in :file:`kf/blsum/tssum.h` to go back to the earlier size.”j§]”(j±ŒQGLOBK suite has had various dimensions increased for GNSS and network sizes. The ”…””}”(j¶jéæjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`tssum`”j§]”j±Œtssum”…””}”(j¶jñæjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jéæubj±Œ/”…””}”(j¶jéæjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`tscon`”j§]”j±Œtscon”…””}”(j¶jçjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jéæubj±Œ/”…””}”j¶jéæsbjj)”}”(j¦Œ:program:`tsfit`”j§]”j±Œtsfit”…””}”(j¶jçjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jéæubj±ŒB programs take 7 Gb of memory to run UNR stations. Change content:”…””}”(j¶jéæjÇjÃáhNjÆNubj²ã)”}”(j¦Œ `max_ent`”j§]”j±Œmax_ent”…””}”(j¶j'çjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj±ãj¶jéæubj±Œ in ”…””}”(j¶jéæjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`kf/blsum/tssum.h`”j§]”j±Œkf/blsum/tssum.h”…””}”(j¶j9çjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jéæubj±Œ to go back to the earlier size.”…””}”(j¶jéæjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK-j¶jäájÇjÃáubj`)”}”(j¦X:program:`track` is updated for GNSS processing. There is a new command :content:`tr_gnss ` to select which GNSS and combination of GNSS to process. The :content:`RM_CSLIP` algorithm and modified and has meaning of some of the arguments changed (see the help file). In this version, ambiguity resolution for GLONASS can be problematic and not recommended. Use the :content:`FLOAT_TYPE` command to set the sigma limits to zero. This version of track can only process up to RINEX version 2.11. RINEX 3 capability will be added soon.”j§]”(jj)”}”(j¦Œ:program:`track`”j§]”j±Œtrack”…””}”(j¶jXçjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jTçubj±Œ8 is updated for GNSS processing. There is a new command ”…””}”(j¶jTçjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`tr_gnss `”j§]”j±Œtr_gnss ”…””}”(j¶jjçjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jTçubj±Œ> to select which GNSS and combination of GNSS to process. The ”…””}”(j¶jTçjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`RM_CSLIP`”j§]”j±ŒRM_CSLIP”…””}”(j¶j}çjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jTçubj±ŒÀ algorithm and modified and has meaning of some of the arguments changed (see the help file). In this version, ambiguity resolution for GLONASS can be problematic and not recommended. Use the ”…””}”(j¶jTçjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`FLOAT_TYPE`”j§]”j±Œ FLOAT_TYPE”…””}”(j¶jçjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jTçubj±Œ‘ command to set the sigma limits to zero. This version of track can only process up to RINEX version 2.11. RINEX 3 capability will be added soon.”…””}”(j¶jTçjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK1j¶jäájÇjÃáubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒOther changes for 10.7”j§]”j±ŒOther changes for 10.7”…””}”(j¶j¬çjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j©çjÇjÃáhjõájÆK:ubj`)”}”(j¦ŒNew utility program :program:`stnfo_cont` to enforce continuity in :file:`station.info` entries when made from sparse individual RINEX headers.”j§]”(j±ŒNew utility program ”…””}”(j¶jºçjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`stnfo_cont`”j§]”j±Œ stnfo_cont”…””}”(j¶jÂçjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jºçubj±Œ to enforce continuity in ”…””}”(j¶jºçjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jÔçjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jºçubj±Œ8 entries when made from sparse individual RINEX headers.”…””}”(j¶jºçjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKj¶j©çjÇjÃáubj`)”}”(j¦ŒuFix the labeling and # parameters for the :content:`ECOM2` (:content:`BERN2`) radiation pressure model in the c-file.”j§]”(j±Œ*Fix the labeling and # parameters for the ”…””}”(j¶jèjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`ECOM2`”j§]”j±ŒECOM2”…””}”(j¶j%èjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jèubj±Œ (”…””}”(j¶jèjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`BERN2`”j§]”j±ŒBERN2”…””}”(j¶j8èjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jèubj±Œ)) radiation pressure model in the c-file.”…””}”(j¶jèjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK@j¶j©çjÇjÃáubj`)”}”(j¦Œ8Add the tide wave names to the model line of the p-file.”j§]”j±Œ8Add the tide wave names to the model line of the p-file.”…””}”(j¶jQèjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKBj¶j©çjÇjÃáubj`)”}”(j¦Œ\Allow more tham 99 zenith delays per site (total number fo all sites still limited to 2500).”j§]”j±Œ\Allow more tham 99 zenith delays per site (total number fo all sites still limited to 2500).”…””}”(j¶j_èjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKDj¶j©çjÇjÃáubj`)”}”(j¦Œ~Use the h-file rather than the q-file names as the basis of the tmp files in :program:`solve` to avoid ambiguity across years.”j§]”(j±ŒMUse the h-file rather than the q-file names as the basis of the tmp files in ”…””}”(j¶jmèjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`solve`”j§]”j±Œsolve”…””}”(j¶juèjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jmèubj±Œ! to avoid ambiguity across years.”…””}”(j¶jmèjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKFj¶j©çjÇjÃáubj`)”}”(j¦ŒMIn :program:`model`, add the tidal wave names to the OTL model in the p-file.”j§]”(j±ŒIn ”…””}”(j¶jèjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`model`”j§]”j±Œmodel”…””}”(j¶j•èjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jèubj±Œ:, add the tidal wave names to the OTL model in the p-file.”…””}”(j¶jèjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKHj¶j©çjÇjÃáubj`)”}”(j¦Œ·Add the SP3 file name to the calling arguments for :program:`sh_makexp` in order to get this into the :program:`makex` command file; fix mltiple bugs in makex for Glonass and Galileo.”j§]”(j±Œ3Add the SP3 file name to the calling arguments for ”…””}”(j¶j­èjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_makexp`”j§]”j±Œ sh_makexp”…””}”(j¶jµèjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j­èubj±Œ in order to get this into the ”…””}”(j¶j­èjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`makex`”j§]”j±Œmakex”…””}”(j¶jÇèjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j­èubj±ŒA command file; fix mltiple bugs in makex for Glonass and Galileo.”…””}”(j¶j­èjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKJj¶j©çjÇjÃáubj`)”}”(j¦Œí:program:`sh_eq_model`: Script to model (using :program:`simplexfd`) single fault earthquakes using coseismic offsets in :file:`.vel` format. Needs a simplex base file (see help). Uses programs in new :file:`~/gg/kf/displace/` directory.”j§]”(jj)”}”(j¦Œ:program:`sh_eq_model`”j§]”j±Œ sh_eq_model”…””}”(j¶jãèjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jßèubj±Œ: Script to model (using ”…””}”(j¶jßèjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`simplexfd`”j§]”j±Œ simplexfd”…””}”(j¶jõèjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jßèubj±Œ6) single fault earthquakes using coseismic offsets in ”…””}”(j¶jßèjÇjÃáhNjÆNubj˜)”}”(j¦Œ :file:`.vel`”j§]”j±Œ.vel”…””}”(j¶jéjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jßèubj±ŒD format. Needs a simplex base file (see help). Uses programs in new ”…””}”(j¶jßèjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/kf/displace/`”j§]”j±Œ~/gg/kf/displace/”…””}”(j¶jéjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jßèubj±Œ directory.”…””}”(j¶jßèjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKMj¶j©çjÇjÃáubj`)”}”(j¦Œø:program:`sh_makeeqdef`: Rewritten in bash and updated to allow different schemes for calculating radius of influence of earthquakes (new :option:`-r` option). Default radius and all other options are backwards compatible with the original version.”j§]”(jj)”}”(j¦Œ:program:`sh_makeeqdef`”j§]”j±Œ sh_makeeqdef”…””}”(j¶j;éjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j7éubj±Œs: Rewritten in bash and updated to allow different schemes for calculating radius of influence of earthquakes (new ”…””}”(j¶j7éjÇjÃáhNjÆNubj’)”}”(j¦Œ :option:`-r`”j§]”j˜)”}”(j¦jOéj§]”j±Œ-r”…””}”(j¶jQéjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jMéubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”j[éŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-r”ujÄj‘hjõájÆKQj¶j7éubj±Œb option). Default radius and all other options are backwards compatible with the original version.”…””}”(j¶j7éjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKQj¶j©çjÇjÃáubj`)”}”(j¦ŒË:program:`unimake`: Updated to handle C main programs and include file " " strings; Added stripping of parentheses to :content:`osver` variable to account for more recent changes to Cygwin OS release ID.”j§]”(jj)”}”(j¦Œ:program:`unimake`”j§]”j±Œunimake”…””}”(j¶j{éjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jwéubj±Œh: Updated to handle C main programs and include file “ “ strings; Added stripping of parentheses to ”…””}”(j¶jwéjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`osver`”j§]”j±Œosver”…””}”(j¶jéjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jwéubj±ŒE variable to account for more recent changes to Cygwin OS release ID.”…””}”(j¶jwéjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKTj¶j©çjÇjÃáubj`)”}”(j¦ŒL:program:`sh_network_sel`: Added additional documentation about file 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ID.”j§]”(jj)”}”(j¦Œ:program:`sh_rename_rinex3`”j§]”j±Œsh_rename_rinex3”…””}”(j¶j|ìjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jxìubj±Œg: Corrected definition of RINEX 2 conventional file name not to translate directory name, only site ID.”…””}”(j¶jxìjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKoj¶j©çjÇjÃáubj`)”}”(j¦Xb:program:`sh_get_hfiles`/:program:`sh_get_ion`/:program:`sh_get_met`/:program:`sh_get_orbits`/:program:`sh_get_rinex`/:program:`sh_get_stinfo`: Added trap to use :program:`ncftp` when :program:`ftp` client is actually :program:`gftp`, which interacts with the server differently to legacy :program:`ftp` and is tricky to use for non-interactive sessions.”j§]”(jj)”}”(j¦Œ:program:`sh_get_hfiles`”j§]”j±Œ sh_get_hfiles”…””}”(j¶j˜ìjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ/”…””}”(j¶j”ìjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_get_ion`”j§]”j±Œ sh_get_ion”…””}”(j¶jªìjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ/”…””}”j¶j”ìsbjj)”}”(j¦Œ:program:`sh_get_met`”j§]”j±Œ sh_get_met”…””}”(j¶j¼ìjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ/”…””}”j¶j”ìsbjj)”}”(j¦Œ:program:`sh_get_orbits`”j§]”j±Œ sh_get_orbits”…””}”(j¶jÎìjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ/”…””}”j¶j”ìsbjj)”}”(j¦Œ:program:`sh_get_rinex`”j§]”j±Œ sh_get_rinex”…””}”(j¶jàìjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ/”…””}”j¶j”ìsbjj)”}”(j¦Œ:program:`sh_get_stinfo`”j§]”j±Œ sh_get_stinfo”…””}”(j¶jòìjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ: Added trap to use ”…””}”(j¶j”ìjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`ncftp`”j§]”j±Œncftp”…””}”(j¶jíjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ when ”…””}”(j¶j”ìjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`ftp`”j§]”j±Œftp”…””}”(j¶jíjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ client is actually ”…””}”(j¶j”ìjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`gftp`”j§]”j±Œgftp”…””}”(j¶j(íjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ8, which interacts with the server differently to legacy ”…””}”(j¶j”ìjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`ftp`”j§]”j±Œftp”…””}”(j¶j:íjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j”ìubj±Œ3 and is tricky to use for non-interactive sessions.”…””}”(j¶j”ìjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKqj¶j©çjÇjÃáubj`)”}”(j¦ŒŒ:program:`sh_cats`, :program:`sh_hector`: Added an output rename file (:file:`.xcl`) to exclude points that fail any maximum sigma criteria.”j§]”(jj)”}”(j¦Œ:program:`sh_cats`”j§]”j±Œsh_cats”…””}”(j¶jVíjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jRíubj±Œ, ”…””}”(j¶jRíjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_hector`”j§]”j±Œ sh_hector”…””}”(j¶jhíjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jRíubj±Œ: Added an output rename file (”…””}”(j¶jRíjÇjÃáhNjÆNubj˜)”}”(j¦Œ :file:`.xcl`”j§]”j±Œ.xcl”…””}”(j¶jzíjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jRíubj±Œ9) to exclude points that fail any maximum sigma criteria.”…””}”(j¶jRíjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKsj¶j©çjÇjÃáubj`)”}”(j¦Œ›:program:`sh_sigelv`: Added explicit format (ISO 8601) to :content:`$rdate` variable to avoid complications arising from locales with non-Latin characters.”j§]”(jj)”}”(j¦Œ:program:`sh_sigelv`”j§]”j±Œ sh_sigelv”…””}”(j¶j™íjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j•íubj±Œ&: Added explicit format (ISO 8601) to ”…””}”(j¶j•íjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`$rdate`”j§]”j±Œ$rdate”…””}”(j¶j«íjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j•íubj±ŒP variable to avoid complications arising from locales with non-Latin characters.”…””}”(j¶j•íjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKuj¶j©çjÇjÃáubj`)”}”(j¦Œ’:program:`sh_plot`: Updated the :option:`-B` option so that multiple values can be used to be consistent with GMT 5 multiple :option:`-B` options.”j§]”(jj)”}”(j¦Œ:program:`sh_plot`”j§]”j±Œsh_plot”…””}”(j¶jÈíjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÄíubj±Œ: Updated the ”…””}”(j¶jÄíjÇjÃáhNjÆNubj’)”}”(j¦Œ :option:`-B`”j§]”j˜)”}”(j¦jÜíj§]”j±Œ-B”…””}”(j¶jÞíjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jÚíubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”jèíŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-B”ujÄj‘hjõájÆKwj¶jÄíubj±ŒQ option so that multiple values can be used to be consistent with GMT 5 multiple ”…””}”(j¶jÄíjÇjÃáhNjÆNubj’)”}”(j¦Œ :option:`-B`”j§]”j˜)”}”(j¦•jîj§]”j±Œ-B”…””}”(j¶jîjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jþíubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”j îŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-B”ujÄj‘hjõájÆKwj¶jÄíubj±Œ options.”…””}”(j¶jÄíjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKwj¶j©çjÇjÃáubj`)”}”(j¦Œ%:program:`sh_strain`: Mods for GMT 5.”j§]”(jj)”}”(j¦Œ:program:`sh_strain`”j§]”j±Œ sh_strain”…””}”(j¶j,îjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j(îubj±Œ: Mods for GMT 5.”…””}”(j¶j(îjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKyj¶j©çjÇjÃáubj`)”}”(j¦X¥:program:`sh_apr2otl`: New script which converts a GAMIT/GLOBK :file:`.apr` file to the format necessary for input to the ocean tide loading service at ``_, whose output is in the format of the GAMIT :file:`otl.list` file. Our recommendation is to select "Yes" to the question "Do you want to correct your loading values for the motion?" when using this web service.”j§]”(jj)”}”(j¦Œ:program:`sh_apr2otl`”j§]”j±Œ sh_apr2otl”…””}”(j¶jHîjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jDîubj±Œ*: New script which converts a GAMIT/GLOBK ”…””}”(j¶jDîjÇjÃáhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jZîjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jDîubj±ŒM file to the format necessary for input to the ocean tide loading service at ”…””}”(j¶jDîjÇjÃáhNjÆNubj÷ )”}”(j¦Œ:``_”j§]”j±Œ5http://holt.oso.chalmers.se/loading/index.html#select”…””}”(j¶joîjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ5http://holt.oso.chalmers.se/loading/index.html#select”j j~îujÄjö j¶jDîubje)”}”(j¦Œ7”j§]”j·}”(j¹]”Œ3http-holt-oso-chalmers-se-loading-index-html-select”aj»]”j½]”Œ5http://holt.oso.chalmers.se/loading/index.html#select”ajÀ]”jÂ]”Œrefuri”j~îujÄjdj Kj¶jDîubj±Œ-, whose output is in the format of the GAMIT ”…””}”(j¶jDîjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`otl.list`”j§]”j±Œotl.list”…””}”(j¶jîjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jDîubj±Œž file. Our recommendation is to select “Yes†to the question “Do you want to correct your loading values for the motion?†when using this web service.”…””}”(j¶jDîjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK{j¶j©çjÇjÃáubj`)”}”(j¦XM:program:`sh_crx2rnx`: Fixed erroneous addition of :option:`-c` (standard output) option to :command:`gzip` when not piping file to subsequent command, and added :command:`gzip`, :command:`bzip2` and :command:`xz` decompression commands for non-Hatanaka-compressed files; corrected RINEX o-file extent for which to use :command:`xz`.”j§]”(jj)”}”(j¦Œ:program:`sh_crx2rnx`”j§]”j±Œ sh_crx2rnx”…””}”(j¶j¯îjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j«îubj±Œ: Fixed erroneous addition of ”…””}”(j¶j«îjÇjÃáhNjÆNubj’)”}”(j¦Œ :option:`-c`”j§]”j˜)”}”(j¦jÃîj§]”j±Œ-c”…””}”(j¶jÅîjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jÁîubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”jÏîŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-c”ujÄj‘hjõájÆK~j¶j«îubj±Œ (standard output) option to ”…””}”(j¶j«îjÇjÃáhNjÆNubjj)”}”(j¦Œ:command:`gzip`”j§]”j±Œgzip”…””}”(j¶jåîjÇjÃáhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶j«îubj±Œ7 when not piping file to subsequent command, and added ”…””}”(j¶j«îjÇjÃáhNjÆNubjj)”}”(j¦Œ:command:`gzip`”j§]”j±Œgzip”…””}”(j¶j÷îjÇjÃáhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶j«îubj±Œ, ”…””}”(j¶j«îjÇjÃáhNjÆNubjj)”}”(j¦Œ:command:`bzip2`”j§]”j±Œbzip2”…””}”(j¶j ïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶j«îubj±Œ and ”…””}”(j¶j«îjÇjÃáhNjÆNubjj)”}”(j¦Œ :command:`xz`”j§]”j±Œxz”…””}”(j¶jïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶j«îubj±Œj decompression commands for non-Hatanaka-compressed files; corrected RINEX o-file extent for which to use ”…””}”(j¶j«îjÇjÃáhNjÆNubjj)”}”(j¦Œ :command:`xz`”j§]”j±Œxz”…””}”(j¶j-ïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶j«îubj±Œ.”…””}”(j¶j«îjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK~j¶j©çjÇjÃáubj`)”}”(j¦ŒÕ:program:`sh_get_x-files`: New script that downloads GIPSY x-files and extracts the scale change estimates so that they can be re-applied when :program:`tscon` converts UNR and JPL time-series files to PBO format.”j§]”(jj)”}”(j¦Œ:program:`sh_get_x-files`”j§]”j±Œsh_get_x-files”…””}”(j¶jIïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jEïubj±Œv: New script that downloads GIPSY x-files and extracts the scale change estimates so that they can be re-applied when ”…””}”(j¶jEïjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`tscon`”j§]”j±Œtscon”…””}”(j¶j[ïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jEïubj±Œ6 converts UNR and JPL time-series files to PBO format.”…””}”(j¶jEïjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKj¶j©çjÇjÃáubj`)”}”(j¦ŒQ:program:`sh_get_ion`: Changed :command:`uncompress` to :program:`sh_uncompress`.”j§]”(jj)”}”(j¦Œ:program:`sh_get_ion`”j§]”j±Œ sh_get_ion”…””}”(j¶jwïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jsïubj±Œ : Changed ”…””}”(j¶jsïjÇjÃáhNjÆNubjj)”}”(j¦Œ:command:`uncompress`”j§]”j±Œ uncompress”…””}”(j¶j‰ïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jsïubj±Œ to ”…””}”(j¶jsïjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`sh_uncompress`”j§]”j±Œ sh_uncompress”…””}”(j¶j›ïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jsïubj±Œ.”…””}”(j¶jsïjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKƒj¶j©çjÇjÃáubj`)”}”(j¦Œš:program:`sh_get_rinex`: Changed :content:`*` to :content:`[0-9]` to avoid getting hourly :content:`[a-z]` files; add download of 30S or 15S Rinex3 files.”j§]”(jj)”}”(j¦Œ:program:`sh_get_rinex`”j§]”j±Œ sh_get_rinex”…””}”(j¶j·ïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j³ïubj±Œ : Changed ”…””}”(j¶j³ïjÇjÃáhNjÆNubj˜)”}”(j¦Œ :content:`*`”j§]”j±Œ*”…””}”(j¶jÉïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j³ïubj±Œ to ”…””}”(j¶j³ïjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`[0-9]`”j§]”j±Œ[0-9]”…””}”(j¶jÜïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j³ïubj±Œ to avoid getting hourly ”…””}”(j¶j³ïjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`[a-z]`”j§]”j±Œ[a-z]”…””}”(j¶jïïjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j³ïubj±Œ0 files; add download of 30S or 15S Rinex3 files.”…””}”(j¶j³ïjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆK…j¶j©çjÇjÃáubj`)”}”(j¦ŒU:program:`make_globk`: Check status of :program:`track` make and terminate if failed.”j§]”(jj)”}”(j¦Œ:program:`make_globk`”j§]”j±Œ make_globk”…””}”(j¶j ðjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jðubj±Œ: Check status of ”…””}”(j¶jðjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`track`”j§]”j±Œtrack”…””}”(j¶jðjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jðubj±Œ make and terminate if failed.”…””}”(j¶jðjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKˆj¶j©çjÇjÃáubj`)”}”(j¦Œ¯:program:`sh_plot_pos`: Corrected typo in if-statement on line 604 that parses :option:`-n` option and missing :content:`$tmp/` for :file:`temp.excl.[enu]` files on line 1615.”j§]”(jj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶j:ðjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j6ðubj±Œ9: Corrected typo in if-statement on line 604 that parses ”…””}”(j¶j6ðjÇjÃáhNjÆNubj’)”}”(j¦Œ :option:`-n`”j§]”j˜)”}”(j¦jNðj§]”j±Œ-n”…””}”(j¶jPðjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jLðubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jøŒ refdomain”jZðŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-n”ujÄj‘hjõájÆKŠj¶j6ðubj±Œ option and missing ”…””}”(j¶j6ðjÇjÃáhNjÆNubj˜)”}”(j¦Œ:content:`$tmp/`”j§]”j±Œ$tmp/”…””}”(j¶jpðjÇjÃáhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j6ðubj±Œ for ”…””}”(j¶j6ðjÇjÃáhNjÆNubj˜)”}”(j¦Œ:file:`temp.excl.[enu]`”j§]”j±Œtemp.excl.[enu]”…””}”(j¶jƒðjÇjÃáhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j6ðubj±Œ files on line 1615.”…””}”(j¶j6ðjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKŠj¶j©çjÇjÃáubj`)”}”(j¦ŒÑ:program:`svsp3` updated for GNSS processing with new command line options. This program will replace :program:`svdiff` and :program:`svpos` in the future. Currently rinex 2.11 but will be upgraded to rinex 3.”j§]”(jj)”}”(j¦Œ:program:`svsp3`”j§]”j±Œsvsp3”…””}”(j¶j¢ðjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jžðubj±ŒV updated for GNSS processing with new command line options. This program will replace ”…””}”(j¶jžðjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`svdiff`”j§]”j±Œsvdiff”…””}”(j¶j´ðjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jžðubj±Œ and ”…””}”(j¶jžðjÇjÃáhNjÆNubjj)”}”(j¦Œ:program:`svpos`”j§]”j±Œsvpos”…””}”(j¶jÆðjÇjÃáhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jžðubj±ŒE in the future. Currently rinex 2.11 but will be upgraded to rinex 3.”…””}”(j¶jžðjÇjÃáhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjõájÆKŒj¶j©çjÇjÃáubej·}”(j¹]”Œother-changes-for-10-7”aj»]”j½]”Œother changes for 10.7”ajÀ]”jÂ]”ujÄh_j¶jäájÇjÃáhjõájÆK:ubej·}”(j¹]”Œid1”aj»]”j½]”Œ10.7”ajÀ]”jÂ]”ujÄh_j¶jÃájÇjÃáhjõájÆKubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jõáj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjõájNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jÒájÆájáájÕáuj_}”(Œrel”jÒáŒdate”jááujc}”je}”jg}”(jëðjèðjãðjàðjˆîj…îuji}”(jëð‰jãð‰jˆîˆuj¹}”(jèðjäájàðj©çj¸êj¼êj…îjîujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”jiKs…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ-Hyperlink target "index-0" is not referenced.”…””}”j¶jñsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jñubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jõáŒline”K`ujÄjø ubajˆNj‰]”j‹NjÇjÃáubjñj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j-ñsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j*ñjÇj*ñubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j<ñjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j*ñjÇj*ñubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ10.71”j§]”j±Œ10.71”…””}”(j¶jNñjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jKñjÇj*ñhŒA/chandler/home/floyd/public_html/gg/docs/source/relnote/10.71.rst”jÆKubj`)”}”(j¦XRelease 10.71 consolidates incremental updates made since release 10.70 of June 2018 and completes modifications to GAMIT following recommendations for the `IGS's repro3 `_. Significant changes of which most users should be aware are:”j§]”(j±ŒœRelease 10.71 consolidates incremental updates made since release 10.70 of June 2018 and completes modifications to GAMIT following recommendations for the ”…””}”(j¶j]ñjÇj*ñhNjÆNubj÷ )”}”(j¦Œ7`IGS's repro3 `_”j§]”j±ŒIGS’s repro3”…””}”(j¶jeñjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ IGS's repro3”j Œ%http://acc.igs.org/repro3/repro3.html”ujÄjö j¶j]ñubje)”}”(j¦Œ( ”j§]”j·}”(j¹]”Œ igs-s-repro3”aj»]”j½]”Œ igs's repro3”ajÀ]”jÂ]”Œrefuri”juñujÄjdj Kj¶j]ñubj±Œ>. Significant changes of which most users should be aware are:”…””}”(j¶j]ñjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKj¶jKñjÇj*ñubj“)”}”(j¦hoj§]”(j˜)”}”(j¦XThe radiation pressure model is expanded from 9 to 13 parameters, adding two twice-per-revolution (2/rev) and two 4/rev terms. GAMIT will carry all 13 parameters, designated :content:`ECOMC` (for Empirical CODE Models 1 and 2 combined) in :file:`tables/sestbl.` In generating fits to the IGS orbits, we recommend using :content:`ECOMC` (the default). Note that if you estimate orbits in GAMIT (:content:`RELAX.` in :file:`tables/sestbl.`) you cannot mix in GLOBK the 10.71 processing with pre-10.71 processing that uses the 9-parameter (BERNE or ECOM1) models. When combining regional processing with MIT or SIO global h-files, you should always run GAMIT without orbit estimation (:content:`BASELINE` in :file:`tables/sestbl.`), as we have long recommended. Even with the same version, different choices of orbit modeling parameters are likely to make the MIT combined binary-files incompatible with recently processed. If :content:`BASELINE` model is used in the GAMIT processing, the incompatibilities will be minor but in :content:`RELAX` mode they can be severe (high :math:`\chi^2` increments). Removing all :content:`apr_svs`, :content:`mar_svs`, :content:`apr_rad` and :content:`mar_rad` options in the GLOBK command file should minimize the effects of incompatibilities. ”j§]”j`)”}”(j¦XÿThe radiation pressure model is expanded from 9 to 13 parameters, adding two twice-per-revolution (2/rev) and two 4/rev terms. GAMIT will carry all 13 parameters, designated :content:`ECOMC` (for Empirical CODE Models 1 and 2 combined) in :file:`tables/sestbl.` In generating fits to the IGS orbits, we recommend using :content:`ECOMC` (the default). Note that if you estimate orbits in GAMIT (:content:`RELAX.` in :file:`tables/sestbl.`) you cannot mix in GLOBK the 10.71 processing with pre-10.71 processing that uses the 9-parameter (BERNE or ECOM1) models. When combining regional processing with MIT or SIO global h-files, you should always run GAMIT without orbit estimation (:content:`BASELINE` in :file:`tables/sestbl.`), as we have long recommended. Even with the same version, different choices of orbit modeling parameters are likely to make the MIT combined binary-files incompatible with recently processed. If :content:`BASELINE` model is used in the GAMIT processing, the incompatibilities will be minor but in :content:`RELAX` mode they can be severe (high :math:`\chi^2` increments). Removing all :content:`apr_svs`, :content:`mar_svs`, :content:`apr_rad` and :content:`mar_rad` options in the GLOBK command file should minimize the effects of incompatibilities.”j§]”(j±Œ®The radiation pressure model is expanded from 9 to 13 parameters, adding two twice-per-revolution (2/rev) and two 4/rev terms. GAMIT will carry all 13 parameters, designated ”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`ECOMC`”j§]”j±ŒECOMC”…””}”(j¶jœñjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±Œ1 (for Empirical CODE Models 1 and 2 combined) in ”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/sestbl.`”j§]”j±Œtables/sestbl.”…””}”(j¶j¯ñjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j”ñubj±Œ: In generating fits to the IGS orbits, we recommend using ”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`ECOMC`”j§]”j±ŒECOMC”…””}”(j¶jÄñjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±Œ; (the default). Note that if you estimate orbits in GAMIT (”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`RELAX.`”j§]”j±ŒRELAX.”…””}”(j¶j×ñjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±Œ in ”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/sestbl.`”j§]”j±Œtables/sestbl.”…””}”(j¶jêñjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j”ñubj±Œõ) you cannot mix in GLOBK the 10.71 processing with pre-10.71 processing that uses the 9-parameter (BERNE or ECOM1) models. When combining regional processing with MIT or SIO global h-files, you should always run GAMIT without orbit estimation (”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`BASELINE`”j§]”j±ŒBASELINE”…””}”(j¶jÿñjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±Œ in ”…””}”j¶j”ñsbj˜)”}”(j¦Œ:file:`tables/sestbl.`”j§]”j±Œtables/sestbl.”…””}”(j¶jòjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j”ñubj±ŒÅ), as we have long recommended. Even with the same version, different choices of orbit modeling parameters are likely to make the MIT combined binary-files incompatible with recently processed. If ”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`BASELINE`”j§]”j±ŒBASELINE”…””}”(j¶j'òjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±ŒS model is used in the GAMIT processing, the incompatibilities will be minor but in ”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`RELAX`”j§]”j±ŒRELAX”…””}”(j¶j:òjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±Œ mode they can be severe (high ”…””}”(j¶j”ñjÇj*ñhNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶jMòjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶j”ñubj±Œ increments). Removing all ”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`apr_svs`”j§]”j±Œapr_svs”…””}”(j¶j_òjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±Œ, ”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`mar_svs`”j§]”j±Œmar_svs”…””}”(j¶jròjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±Œ, ”…””}”j¶j”ñsbj˜)”}”(j¦Œ:content:`apr_rad`”j§]”j±Œapr_rad”…””}”(j¶j…òjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±Œ and ”…””}”(j¶j”ñjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`mar_rad`”j§]”j±Œmar_rad”…””}”(j¶j˜òjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j”ñubj±ŒT options in the GLOBK command file should minimize the effects of incompatibilities.”…””}”(j¶j”ñjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKj¶jñubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦XBeidou processing now uses L6/C6 (B3 at 1268.53 MHz) rather than L7/C7 (B2b at 1207.140 MHz) as the lower-frequency observable to accommodate the tracking configuration of most of the current GNSS receivers providing public data. Based on a sampling of 230 RINEX files from the archives, about 50% include only L6/C6 compared with about 5% that include only L7/C7. The higher-frequency observable will remain L2/C2 (B1-2 at 1561.098 MHz) since very few of the public RINEX files contain L1/C1 from the B1 at 1575.42 MHz transmitted by BDS-3 satellites. If L7/C7 is the only observable present (i.e., no L6/C6), GAMIT will try to process the data along with L7/C7 receivers but there may be ambiguity resolution issues. Users should assess data files and process together only those sites with the same frequency data. There are still some issues with clock estimates for Beidou data and pre-fit editing in :program:`autcln`. ”j§]”j`)”}”(j¦XœBeidou processing now uses L6/C6 (B3 at 1268.53 MHz) rather than L7/C7 (B2b at 1207.140 MHz) as the lower-frequency observable to accommodate the tracking configuration of most of the current GNSS receivers providing public data. Based on a sampling of 230 RINEX files from the archives, about 50% include only L6/C6 compared with about 5% that include only L7/C7. The higher-frequency observable will remain L2/C2 (B1-2 at 1561.098 MHz) since very few of the public RINEX files contain L1/C1 from the B1 at 1575.42 MHz transmitted by BDS-3 satellites. If L7/C7 is the only observable present (i.e., no L6/C6), GAMIT will try to process the data along with L7/C7 receivers but there may be ambiguity resolution issues. Users should assess data files and process together only those sites with the same frequency data. There are still some issues with clock estimates for Beidou data and pre-fit editing in :program:`autcln`.”j§]”(j±XŠBeidou processing now uses L6/C6 (B3 at 1268.53 MHz) rather than L7/C7 (B2b at 1207.140 MHz) as the lower-frequency observable to accommodate the tracking configuration of most of the current GNSS receivers providing public data. Based on a sampling of 230 RINEX files from the archives, about 50% include only L6/C6 compared with about 5% that include only L7/C7. The higher-frequency observable will remain L2/C2 (B1-2 at 1561.098 MHz) since very few of the public RINEX files contain L1/C1 from the B1 at 1575.42 MHz transmitted by BDS-3 satellites. If L7/C7 is the only observable present (i.e., no L6/C6), GAMIT will try to process the data along with L7/C7 receivers but there may be ambiguity resolution issues. Users should assess data files and process together only those sites with the same frequency data. There are still some issues with clock estimates for Beidou data and pre-fit editing in ”…””}”(j¶j»òjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`autcln`”j§]”j±Œautcln”…””}”(j¶jÃòjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j»òubj±Œ.”…””}”(j¶j»òjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKj¶j·òubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦XkThe default :file:`tables/sestbl.` now has the 2nd-order ionosphere model turned on. The IGSG IONEX files will be used by default. If processing near-real time, the :option:`-ion igrg` option should be used with :program:`sh_gamit`. We also recommend always including the :content:`Inertial Reference System` option (current default :content:`IAU0A`) explicitly. ”j§]”j`)”}”(j¦XjThe default :file:`tables/sestbl.` now has the 2nd-order ionosphere model turned on. The IGSG IONEX files will be used by default. If processing near-real time, the :option:`-ion igrg` option should be used with :program:`sh_gamit`. We also recommend always including the :content:`Inertial Reference System` option (current default :content:`IAU0A`) explicitly.”j§]”(j±Œ The default ”…””}”(j¶jåòjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/sestbl.`”j§]”j±Œtables/sestbl.”…””}”(j¶jíòjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jåòubj±Œƒ now has the 2nd-order ionosphere model turned on. The IGSG IONEX files will be used by default. If processing near-real time, the ”…””}”(j¶jåòjÇj*ñhNjÆNubj’)”}”(j¦Œ:option:`-ion igrg`”j§]”j˜)”}”(j¦jój§]”j±Œ -ion igrg”…””}”(j¶jójÇj*ñhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jóubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jñŒ refdomain”jóŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -ion igrg”ujÄj‘hj\ñjÆKj¶jåòubj±Œ option should be used with ”…””}”(j¶jåòjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j&ójÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jåòubj±Œ). We also recommend always including the ”…””}”(j¶jåòjÇj*ñhNjÆNubj˜)”}”(j¦Œ$:content:`Inertial Reference System`”j§]”j±ŒInertial Reference System”…””}”(j¶j8ójÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jåòubj±Œ option (current default ”…””}”(j¶jåòjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`IAU0A`”j§]”j±ŒIAU0A”…””}”(j¶jKójÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jåòubj±Œ ) explicitly.”…””}”(j¶jåòjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKj¶jáòubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦X:file:`tables/svnav.dat` is now linked to the IGS satellite metadata SINEX file (:file:`igs_metadata.snx`). Release 10.70 and earlier versions of GAMIT cannot read this file format and :file:`svnav.dat` needs to be linked to :file:`svanv.dat.allgnss`, which will be maintained for the foreseeable future. Several changes to files in the :file:`tables/` directory may be incompatible with early versions of GAMIT. ”j§]”j`)”}”(j¦Xœ:file:`tables/svnav.dat` is now linked to the IGS satellite metadata SINEX file (:file:`igs_metadata.snx`). Release 10.70 and earlier versions of GAMIT cannot read this file format and :file:`svnav.dat` needs to be linked to :file:`svanv.dat.allgnss`, which will be maintained for the foreseeable future. Several changes to files in the :file:`tables/` directory may be incompatible with early versions of GAMIT.”j§]”(j˜)”}”(j¦Œ:file:`tables/svnav.dat`”j§]”j±Œtables/svnav.dat”…””}”(j¶jrójÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jnóubj±Œ9 is now linked to the IGS satellite metadata SINEX file (”…””}”(j¶jnójÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`igs_metadata.snx`”j§]”j±Œigs_metadata.snx”…””}”(j¶j‡ójÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jnóubj±ŒP). Release 10.70 and earlier versions of GAMIT cannot read this file format and ”…””}”(j¶jnójÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`svnav.dat`”j§]”j±Œ svnav.dat”…””}”(j¶jœójÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jnóubj±Œ needs to be linked to ”…””}”(j¶jnójÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`svanv.dat.allgnss`”j§]”j±Œsvanv.dat.allgnss”…””}”(j¶j±ójÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jnóubj±ŒW, which will be maintained for the foreseeable future. Several changes to files in the ”…””}”(j¶jnójÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jÆójÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jnóubj±Œ< directory may be incompatible with early versions of GAMIT.”…””}”(j¶jnójÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKj¶jjóubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦X—The :file:`tables/station.info` file now accommodates another optional column (:content:`AntDAZ` in the header line) to specify the azimuth (clockwise from true north) of the antenna. Conventionally antennas are aligned with true north but some (and likely many others that we don't know about yet) are recorded as set to another azimuth. The :content:`AntDAZ` azimuth is read to rotate the phase center offsets (PCOs) and phase center variations (PCVs) from the ANTEX file (:file:`tables/antmod.dat`) to correct for the azimuth of the antenna. :program:`sh_upd_stnfo` can extract this information from IGS log files if the :content:`AntDAZ` header is included (users should ensure that there are no non-numeric values in the columns below :content:`AntDAZ`; white space in OK). The IGS will not implement this feature until ITRF2020 is released (that is, it will be part of repro3 but not the operational processing). ”j§]”j`)”}”(j¦X–The :file:`tables/station.info` file now accommodates another optional column (:content:`AntDAZ` in the header line) to specify the azimuth (clockwise from true north) of the antenna. Conventionally antennas are aligned with true north but some (and likely many others that we don't know about yet) are recorded as set to another azimuth. The :content:`AntDAZ` azimuth is read to rotate the phase center offsets (PCOs) and phase center variations (PCVs) from the ANTEX file (:file:`tables/antmod.dat`) to correct for the azimuth of the antenna. :program:`sh_upd_stnfo` can extract this information from IGS log files if the :content:`AntDAZ` header is included (users should ensure that there are no non-numeric values in the columns below :content:`AntDAZ`; white space in OK). The IGS will not implement this feature until ITRF2020 is released (that is, it will be part of repro3 but not the operational processing).”j§]”(j±ŒThe ”…””}”(j¶jëójÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/station.info`”j§]”j±Œtables/station.info”…””}”(j¶jóójÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jëóubj±Œ0 file now accommodates another optional column (”…””}”(j¶jëójÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`AntDAZ`”j§]”j±ŒAntDAZ”…””}”(j¶jôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëóubj±Œù in the header line) to specify the azimuth (clockwise from true north) of the antenna. Conventionally antennas are aligned with true north but some (and likely many others that we don’t know about yet) are recorded as set to another azimuth. The ”…””}”(j¶jëójÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`AntDAZ`”j§]”j±ŒAntDAZ”…””}”(j¶jôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëóubj±Œs azimuth is read to rotate the phase center offsets (PCOs) and phase center variations (PCVs) from the ANTEX file (”…””}”(j¶jëójÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/antmod.dat`”j§]”j±Œtables/antmod.dat”…””}”(j¶j.ôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jëóubj±Œ-) to correct for the azimuth of the antenna. ”…””}”(j¶jëójÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_upd_stnfo`”j§]”j±Œ sh_upd_stnfo”…””}”(j¶jCôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jëóubj±Œ8 can extract this information from IGS log files if the ”…””}”(j¶jëójÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`AntDAZ`”j§]”j±ŒAntDAZ”…””}”(j¶jUôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëóubj±Œc header is included (users should ensure that there are no non-numeric values in the columns below ”…””}”(j¶jëójÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`AntDAZ`”j§]”j±ŒAntDAZ”…””}”(j¶jhôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëóubj±Œ¡; white space in OK). The IGS will not implement this feature until ITRF2020 is released (that is, it will be part of repro3 but not the operational processing).”…””}”(j¶jëójÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK!j¶jçóubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦XWe have changed many symbolic links in :file:`tables/` to be relative, rather than absolute, which assume that users install a local :file:`GRIDS/` directory at the same level as the source code (e.g. :file:`gamit/`, :file:`libraries/`, :file:`kf/`, :file:`maps/`, :file:`tables/`, etc.), where grids downloaded from ftp://everest.mit.edu/pub/GRIDS/ should be stored. Creation of specific symbolic links, e.g. :file:`atml.grid`, :file:`map.grid`, :file:`met.grid`, by the user to the corresponding grid files is then no longer necessary. ”j§]”j`)”}”(j¦XWe have changed many symbolic links in :file:`tables/` to be relative, rather than absolute, which assume that users install a local :file:`GRIDS/` directory at the same level as the source code (e.g. :file:`gamit/`, :file:`libraries/`, :file:`kf/`, :file:`maps/`, :file:`tables/`, etc.), where grids downloaded from ftp://everest.mit.edu/pub/GRIDS/ should be stored. Creation of specific symbolic links, e.g. :file:`atml.grid`, :file:`map.grid`, :file:`met.grid`, by the user to the corresponding grid files is then no longer necessary.”j§]”(j±Œ'We have changed many symbolic links in ”…””}”(j¶j‹ôjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶j“ôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±ŒO to be relative, rather than absolute, which assume that users install a local ”…””}”(j¶j‹ôjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`GRIDS/`”j§]”j±ŒGRIDS/”…””}”(j¶j¨ôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±Œ6 directory at the same level as the source code (e.g. ”…””}”(j¶j‹ôjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`gamit/`”j§]”j±Œgamit/”…””}”(j¶j½ôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±Œ, ”…””}”(j¶j‹ôjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`libraries/`”j§]”j±Œ libraries/”…””}”(j¶jÒôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±Œ, ”…””}”j¶j‹ôsbj˜)”}”(j¦Œ :file:`kf/`”j§]”j±Œkf/”…””}”(j¶jçôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±Œ, ”…””}”j¶j‹ôsbj˜)”}”(j¦Œ :file:`maps/`”j§]”j±Œmaps/”…””}”(j¶jüôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±Œ, ”…””}”j¶j‹ôsbj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jõjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±Œ%, etc.), where grids downloaded from ”…””}”(j¶j‹ôjÇj*ñhNjÆNubj÷ )”}”(j¦Œ ftp://everest.mit.edu/pub/GRIDS/”j§]”j±Œ ftp://everest.mit.edu/pub/GRIDS/”…””}”(j¶j&õjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j(õujÄjö j¶j‹ôubj±Œ= should be stored. Creation of specific symbolic links, e.g. ”…””}”(j¶j‹ôjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`atml.grid`”j§]”j±Œ atml.grid”…””}”(j¶j9õjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±Œ, ”…””}”j¶j‹ôsbj˜)”}”(j¦Œ:file:`map.grid`”j§]”j±Œmap.grid”…””}”(j¶jNõjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±Œ, ”…””}”j¶j‹ôsbj˜)”}”(j¦Œ:file:`met.grid`”j§]”j±Œmet.grid”…””}”(j¶jcõjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j‹ôubj±ŒJ, by the user to the corresponding grid files is then no longer necessary.”…””}”(j¶j‹ôjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK(j¶j‡ôubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦Xú:program:`sh_gamit` now will remake g-files from SP3 files each time it is run to ensure that the orbit models in :file:`tables/sestbl.` are consistent with the :program:`sh_sp3fit` models (these models are now read from :file:`sestbl.` provided a copy can be found in the standard processing directories). For sub-network processing, g-files should be made once before proceeding to process each sub-network (assumed to be in parallel) using the :option:`-remakeg N` option used with :program:`sh_gamit`. ”j§]”j`)”}”(j¦Xù:program:`sh_gamit` now will remake g-files from SP3 files each time it is run to ensure that the orbit models in :file:`tables/sestbl.` are consistent with the :program:`sh_sp3fit` models (these models are now read from :file:`sestbl.` provided a copy can be found in the standard processing directories). For sub-network processing, g-files should be made once before proceeding to process each sub-network (assumed to be in parallel) using the :option:`-remakeg N` option used with :program:`sh_gamit`.”j§]”(jj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jŒõjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jˆõubj±Œ_ now will remake g-files from SP3 files each time it is run to ensure that the orbit models in ”…””}”(j¶jˆõjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/sestbl.`”j§]”j±Œtables/sestbl.”…””}”(j¶jžõjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jˆõubj±Œ are consistent with the ”…””}”(j¶jˆõjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_sp3fit`”j§]”j±Œ sh_sp3fit”…””}”(j¶j³õjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jˆõubj±Œ( models (these models are now read from ”…””}”(j¶jˆõjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jÅõjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jˆõubj±ŒÓ provided a copy can be found in the standard processing directories). For sub-network processing, g-files should be made once before proceeding to process each sub-network (assumed to be in parallel) using the ”…””}”(j¶jˆõjÇj*ñhNjÆNubj’)”}”(j¦Œ:option:`-remakeg N`”j§]”j˜)”}”(j¦jÜõj§]”j±Œ -remakeg N”…””}”(j¶jÞõjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jÚõubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jñŒ refdomain”jèõŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -remakeg N”ujÄj‘hj\ñjÆK+j¶jˆõubj±Œ option used with ”…””}”(j¶jˆõjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jþõjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jˆõubj±Œ.”…””}”(j¶jˆõjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK+j¶j„õubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦Œ¿We remind users that when processing GLONASS data the ambiguity free (:file:`.glr`) binary h-files should be used in GLOBK. Also remember that a multi-GNSS orbit file should be used as well. ”j§]”j`)”}”(j¦Œ¾We remind users that when processing GLONASS data the ambiguity free (:file:`.glr`) binary h-files should be used in GLOBK. Also remember that a multi-GNSS orbit file should be used as well.”j§]”(j±ŒFWe remind users that when processing GLONASS data the ambiguity free (”…””}”(j¶j öjÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`.glr`”j§]”j±Œ.glr”…””}”(j¶j(öjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j öubj±Œl) binary h-files should be used in GLOBK. Also remember that a multi-GNSS orbit file should be used as well.”…””}”(j¶j öjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK.j¶jöubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦XÏThe format for the :content:`apr_svs` and :content:`mar_svs` radiation parameters specification in the GLOBK command file has changed, with the unused :content:`zrad` and :content:`xrad` entries removed (see Pre 5.32 and Post 5.32 discussion in :file:`~/gg/help/globk.hlp`). The options using the :content:`R` format remains unchanged. Older :program:`globk` commands with explicit radiation parameter constraints and process noise may need to be updated. ”j§]”j`)”}”(j¦XÎThe format for the :content:`apr_svs` and :content:`mar_svs` radiation parameters specification in the GLOBK command file has changed, with the unused :content:`zrad` and :content:`xrad` entries removed (see Pre 5.32 and Post 5.32 discussion in :file:`~/gg/help/globk.hlp`). The options using the :content:`R` format remains unchanged. Older :program:`globk` commands with explicit radiation parameter constraints and process noise may need to be updated.”j§]”(j±ŒThe format for the ”…””}”(j¶jMöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`apr_svs`”j§]”j±Œapr_svs”…””}”(j¶jUöjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jMöubj±Œ and ”…””}”(j¶jMöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`mar_svs`”j§]”j±Œmar_svs”…””}”(j¶jhöjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jMöubj±Œ[ radiation parameters specification in the GLOBK command file has changed, with the unused ”…””}”(j¶jMöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`zrad`”j§]”j±Œzrad”…””}”(j¶j{öjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jMöubj±Œ and ”…””}”j¶jMösbj˜)”}”(j¦Œ:content:`xrad`”j§]”j±Œxrad”…””}”(j¶jŽöjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jMöubj±Œ; entries removed (see Pre 5.32 and Post 5.32 discussion in ”…””}”(j¶jMöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/help/globk.hlp`”j§]”j±Œ~/gg/help/globk.hlp”…””}”(j¶j¡öjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jMöubj±Œ). The options using the ”…””}”(j¶jMöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`R`”j§]”j±ŒR”…””}”(j¶j¶öjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jMöubj±Œ! format remains unchanged. Older ”…””}”(j¶jMöjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jÉöjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jMöubj±Œa commands with explicit radiation parameter constraints and process noise may need to be updated.”…””}”(j¶jMöjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK1j¶jIöubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦XGLOBK has moved to using :content:`_` syntax for satellite identifiers in output files (e.g. the :file:`.org` file), where :content:`` is :content:`G`, :content:`R`, :content:`E` or :content:`C`, and :content:`` and :content:`` are Satellite Vehicle Number and Pseudo-Random Noise code, respectively. For GPS, the default is still :content:`PRN_`. The new format for GPS can be invoked with the :content:`use_prn n` command near the top of the command file. (See :file:`~/gg/help/globk.hlp`.) ”j§]”j`)”}”(j¦XGLOBK has moved to using :content:`_` syntax for satellite identifiers in output files (e.g. the :file:`.org` file), where :content:`` is :content:`G`, :content:`R`, :content:`E` or :content:`C`, and :content:`` and :content:`` are Satellite Vehicle Number and Pseudo-Random Noise code, respectively. For GPS, the default is still :content:`PRN_`. The new format for GPS can be invoked with the :content:`use_prn n` command near the top of the command file. (See :file:`~/gg/help/globk.hlp`.)”j§]”(j±ŒGLOBK has moved to using ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`_`”j§]”j±Œ_”…””}”(j¶jóöjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œ< syntax for satellite identifiers in output files (e.g. the ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶j÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jëöubj±Œ file), where ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ”…””}”(j¶j÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œ is ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ :content:`G`”j§]”j±ŒG”…””}”(j¶j.÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œ, ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ :content:`R`”j§]”j±ŒR”…””}”(j¶jA÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œ, ”…””}”j¶jëösbj˜)”}”(j¦Œ :content:`E`”j§]”j±ŒE”…””}”(j¶jT÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œ or ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ :content:`C`”j§]”j±ŒC”…””}”(j¶jg÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œ, and ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ”…””}”(j¶jz÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œ and ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:``”j§]”j±Œ”…””}”(j¶j÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œh are Satellite Vehicle Number and Pseudo-Random Noise code, respectively. For GPS, the default is still ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`PRN_`”j§]”j±ŒPRN_”…””}”(j¶j ÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œ1. The new format for GPS can be invoked with the ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`use_prn n`”j§]”j±Œ use_prn n”…””}”(j¶j³÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jëöubj±Œ0 command near the top of the command file. (See ”…””}”(j¶jëöjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/help/globk.hlp`”j§]”j±Œ~/gg/help/globk.hlp”…””}”(j¶jÆ÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jëöubj±Œ.)”…””}”(j¶jëöjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK5j¶jçöubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦Œ¸New wild card features in file names now allow dates and times to be used based on the date and time of the h-file being processed. (See 5.32 features in :file:`~/gg/help/globk.hlp`.) ”j§]”j`)”}”(j¦Œ·New wild card features in file names now allow dates and times to be used based on the date and time of the h-file being processed. (See 5.32 features in :file:`~/gg/help/globk.hlp`.)”j§]”(j±ŒšNew wild card features in file names now allow dates and times to be used based on the date and time of the h-file being processed. (See 5.32 features in ”…””}”(j¶jë÷jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/help/globk.hlp`”j§]”j±Œ~/gg/help/globk.hlp”…””}”(j¶jó÷jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jë÷ubj±Œ.)”…””}”(j¶jë÷jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK:j¶jç÷ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦ŒÄGLOBK can now do reference frame realization in back solutions. This will happen automatically if :program:`glorg` is invoked in a GLOBK command file with the :content:`bak_file` option included. ”j§]”j`)”}”(j¦ŒÃGLOBK can now do reference frame realization in back solutions. This will happen automatically if :program:`glorg` is invoked in a GLOBK command file with the :content:`bak_file` option included.”j§]”(j±ŒbGLOBK can now do reference frame realization in back solutions. This will happen automatically if ”…””}”(j¶jøjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j øjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jøubj±Œ- is invoked in a GLOBK command file with the ”…””}”(j¶jøjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`bak_file`”j§]”j±Œbak_file”…””}”(j¶j2øjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jøubj±Œ option included.”…””}”(j¶jøjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK=j¶jøubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦X|We will no longer provide `GMT `_ :file:`.grd` files in the :file:`maps/` directory to reduce the size of the archive (:file:`.tar`) files. Instead we now provide a new script, :program:`sh_dem`, which will download and create a local copy of a chosen digital elevation model (DEM) over a geographic region, both selected using the script options. The script is now called by :program:`sh_plotvel` if the :option:`-topo`, :option:`-topo_file` and/or :option:`-illu_file` options are used; if the latter is given without an argument, :program:`sh_plotvel` will create a :file:`.grd` file of the gradient for plotting shaded-relief (illumination) from the topographic :file:`.grd` file named or created with the :option:`-topo_file` option. Both :program:`sh_dem` and :program:`sh_plotvel` require `GMT `_ to run. ”j§]”j`)”}”(j¦X{We will no longer provide `GMT `_ :file:`.grd` files in the :file:`maps/` directory to reduce the size of the archive (:file:`.tar`) files. Instead we now provide a new script, :program:`sh_dem`, which will download and create a local copy of a chosen digital elevation model (DEM) over a geographic region, both selected using the script options. The script is now called by :program:`sh_plotvel` if the :option:`-topo`, :option:`-topo_file` and/or :option:`-illu_file` options are used; if the latter is given without an argument, :program:`sh_plotvel` will create a :file:`.grd` file of the gradient for plotting shaded-relief (illumination) from the topographic :file:`.grd` file named or created with the :option:`-topo_file` option. Both :program:`sh_dem` and :program:`sh_plotvel` require `GMT `_ to run.”j§]”(j±ŒWe will no longer provide ”…””}”(j¶jUøjÇj*ñhNjÆNubj÷ )”}”(j¦Œ/`GMT `_”j§]”j±ŒGMT”…””}”(j¶j]øjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGMT”j Œ&https://www.generic-mapping-tools.org/”ujÄjö j¶jUøubje)”}”(j¦Œ) ”j§]”j·}”(j¹]”Œgmt”aj»]”j½]”Œgmt”ajÀ]”jÂ]”Œrefuri”jmøujÄjdj Kj¶jUøubj±Œ ”…””}”(j¶jUøjÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`.grd`”j§]”j±Œ.grd”…””}”(j¶jøjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jUøubj±Œ files in the ”…””}”(j¶jUøjÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`maps/`”j§]”j±Œmaps/”…””}”(j¶j”øjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jUøubj±Œ. directory to reduce the size of the archive (”…””}”(j¶jUøjÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`.tar`”j§]”j±Œ.tar”…””}”(j¶j©øjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jUøubj±Œ.) files. Instead we now provide a new script, ”…””}”(j¶jUøjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_dem`”j§]”j±Œsh_dem”…””}”(j¶j¾øjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jUøubj±Œ¶, which will download and create a local copy of a chosen digital elevation model (DEM) over a geographic region, both selected using the script options. The script is now called by ”…””}”(j¶jUøjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_plotvel`”j§]”j±Œ sh_plotvel”…””}”(j¶jÐøjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jUøubj±Œ if the ”…””}”(j¶jUøjÇj*ñhNjÆNubj’)”}”(j¦Œ:option:`-topo`”j§]”j˜)”}”(j¦jäøj§]”j±Œ-topo”…””}”(j¶jæøjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jâøubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jñŒ refdomain”jðøŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-topo”ujÄj‘hj\ñjÆK@j¶jUøubj±Œ, ”…””}”(j¶jUøjÇj*ñhNjÆNubj’)”}”(j¦Œ:option:`-topo_file`”j§]”j˜)”}”(j¦jùj§]”j±Œ -topo_file”…””}”(j¶j ùjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jùubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jñŒ refdomain”jùŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -topo_file”ujÄj‘hj\ñjÆK@j¶jUøubj±Œ and/or ”…””}”(j¶jUøjÇj*ñhNjÆNubj’)”}”(j¦Œ:option:`-illu_file`”j§]”j˜)”}”(j¦j,ùj§]”j±Œ -illu_file”…””}”(j¶j.ùjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j*ùubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jñŒ refdomain”j8ùŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -illu_file”ujÄj‘hj\ñjÆK@j¶jUøubj±Œ? options are used; if the latter is given without an argument, ”…””}”(j¶jUøjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_plotvel`”j§]”j±Œ sh_plotvel”…””}”(j¶jNùjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jUøubj±Œ will create a ”…””}”(j¶jUøjÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`.grd`”j§]”j±Œ.grd”…””}”(j¶j`ùjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jUøubj±ŒU file of the gradient for plotting shaded-relief (illumination) from the topographic ”…””}”(j¶jUøjÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`.grd`”j§]”j±Œ.grd”…””}”(j¶juùjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jUøubj±Œ file named or created with the ”…””}”(j¶jUøjÇj*ñhNjÆNubj’)”}”(j¦Œ:option:`-topo_file`”j§]”j˜)”}”(j¦jŒùj§]”j±Œ -topo_file”…””}”(j¶jŽùjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jŠùubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jñŒ refdomain”j˜ùŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -topo_file”ujÄj‘hj\ñjÆK@j¶jUøubj±Œ option. Both ”…””}”(j¶jUøjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_dem`”j§]”j±Œsh_dem”…””}”(j¶j®ùjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jUøubj±Œ and ”…””}”(j¶jUøjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_plotvel`”j§]”j±Œ sh_plotvel”…””}”(j¶jÀùjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jUøubj±Œ require ”…””}”(j¶jUøjÇj*ñhNjÆNubj÷ )”}”(j¦Œ/`GMT `_”j§]”j±ŒGMT”…””}”(j¶jÒùjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒGMT”j Œ&https://www.generic-mapping-tools.org/”ujÄjö j¶jUøubje)”}”(j¦Œ) ”j§]”j·}”(j¹]”Œid2”aj»]”j½]”jÀ]”Œgmt”ajÂ]”Œrefuri”jâùujÄjdj Kj¶jUøubj±Œ to run.”…””}”(j¶jUøjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK@j¶jQøubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦X™GMT version 6.0.0 was released in November 2019. Scripts in :file:`com/` that use GMT to produce plots were updated for GAMIT/GLOBK 10.6 to accommodate major changes in the syntax of GMT version 5 commands (see relnote.10.6); the old scripts, using GMT 4 syntax, are still available in :file:`com_preGMT5/` but are no longer maintained. Although we have not done extensive testing yet, we understand that `GMT 6 is fully backwards compatible with GMT 5 `_ and should work seamlessly with our scripts currently in :file:`com/`, which explicitly call :program:`gmt` (now the sole GMT executable) throughout. ”j§]”j`)”}”(j¦X˜GMT version 6.0.0 was released in November 2019. Scripts in :file:`com/` that use GMT to produce plots were updated for GAMIT/GLOBK 10.6 to accommodate major changes in the syntax of GMT version 5 commands (see relnote.10.6); the old scripts, using GMT 4 syntax, are still available in :file:`com_preGMT5/` but are no longer maintained. Although we have not done extensive testing yet, we understand that `GMT 6 is fully backwards compatible with GMT 5 `_ and should work seamlessly with our scripts currently in :file:`com/`, which explicitly call :program:`gmt` (now the sole GMT executable) throughout.”j§]”(j±Œ`_”j§]”j±Œ.GMT 6 is fully backwards compatible with GMT 5”…””}”(j¶j6újÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ.GMT 6 is fully backwards compatible with GMT 5”j Œ9https://docs.generic-mapping-tools.org/6.0/migrating.html”ujÄjö j¶júubje)”}”(j¦Œ< ”j§]”j·}”(j¹]”Œ.gmt-6-is-fully-backwards-compatible-with-gmt-5”aj»]”j½]”Œ.gmt 6 is fully backwards compatible with gmt 5”ajÀ]”jÂ]”Œrefuri”jFúujÄjdj Kj¶júubj±Œ: and should work seamlessly with our scripts currently in ”…””}”(j¶jújÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`com/`”j§]”j±Œcom/”…””}”(j¶jXújÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶júubj±Œ, which explicitly call ”…””}”(j¶jújÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`gmt`”j§]”j±Œgmt”…””}”(j¶jmújÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶júubj±Œ* (now the sole GMT executable) throughout.”…””}”(j¶jújÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKFj¶júubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦XÀWe have become aware that the GMT installation available via the software repository for Ubuntu 16.04 LTS does not include the supplemental programs, most significantly :program:`psvelo` for GAMIT/GLOBK. We recommend upgrading your Ubuntu operating system or building GMT from source. See https://gmt.soest.hawaii.edu/projects/gmt/wiki/Installing#Linux and our `"Known Issues" web page `_ for more information. ”•j§]”j`)”}”(j¦X¿We have become aware that the GMT installation available via the software repository for Ubuntu 16.04 LTS does not include the supplemental programs, most significantly :program:`psvelo` for GAMIT/GLOBK. We recommend upgrading your Ubuntu operating system or building GMT from source. See https://gmt.soest.hawaii.edu/projects/gmt/wiki/Installing#Linux and our `"Known Issues" web page `_ for more information.”j§]”(j±Œ©We have become aware that the GMT installation available via the software repository for Ubuntu 16.04 LTS does not include the supplemental programs, most significantly ”…””}”(j¶jújÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`psvelo`”j§]”j±Œpsvelo”…””}”(j¶j—újÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶júubj±Œg for GAMIT/GLOBK. We recommend upgrading your Ubuntu operating system or building GMT from source. See ”…””}”(j¶jújÇj*ñhNjÆNubj÷ )”}”(j¦Œ?https://gmt.soest.hawaii.edu/projects/gmt/wiki/Installing#Linux”j§]”j±Œ?https://gmt.soest.hawaii.edu/projects/gmt/wiki/Installing#Linux”…””}”(j¶j©újÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j«úujÄjö j¶júubj±Œ and our ”…””}”(j¶jújÇj*ñhNjÆNubj÷ )”}”(j¦Œ@`"Known Issues" web page `_”j§]”j±Œ“Known Issues†web page”…””}”(j¶j¼újÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ"Known Issues" web page”j Œ#http://geoweb.mit.edu/gg/issues.php”ujÄjö j¶júubje)”}”(j¦Œ& ”j§]”j·}”(j¹]”Œknown-issues-web-page”aj»]”j½]”Œ"known issues" web page”ajÀ]”jÂ]”Œrefuri”jÌúujÄjdj Kj¶júubj±Œ for more information.”…””}”(j¶jújÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKKj¶j‹úubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubj˜)”}”(j¦XWe have also become aware that there seems to be an issue with the implementation of gfortran version 7 on at least Ubuntu 18.04 LTS and openSUSE Leap 15.1 operating systems, resulting in failed compilation with segmentation fault error messages, including :content:`See for instructions.` We recommend upgrading to another version of gcc/gfortan, or downgrading to gcc/gfortran version 6. See our `"Known Issues" web page `_ for more information. ”j§]”j`)”}”(j¦XWe have also become aware that there seems to be an issue with the implementation of gfortran version 7 on at least Ubuntu 18.04 LTS and openSUSE Leap 15.1 operating systems, resulting in failed compilation with segmentation fault error messages, including :content:`See for instructions.` We recommend upgrading to another version of gcc/gfortan, or downgrading to gcc/gfortran version 6. See our `"Known Issues" web page `_ for more information.”j§]”(j±XWe have also become aware that there seems to be an issue with the implementation of gfortran version 7 on at least Ubuntu 18.04 LTS and openSUSE Leap 15.1 operating systems, resulting in failed compilation with segmentation fault error messages, including ”…””}”(j¶jîújÇj*ñhNjÆNubj˜)”}”(j¦ŒJ:content:`See for instructions.`”j§]”j±Œ?See for instructions.”…””}”(j¶jöújÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jîúubj±Œm We recommend upgrading to another version of gcc/gfortan, or downgrading to gcc/gfortran version 6. See our ”…””}”(j¶jîújÇj*ñhNjÆNubj÷ )”}”(j¦Œ@`"Known Issues" web page `_”j§]”j±Œ“Known Issues†web page”…””}”(j¶j ûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”Œ"Known Issues" web page”j Œ#http://geoweb.mit.edu/gg/issues.php”ujÄjö j¶jîúubje)”}”(j¦Œ& ”j§]”j·}”(j¹]”Œid3”aj»]”j½]”jÀ]”Œ"known issues" web page”ajÂ]”Œrefuri”jûujÄjdj Kj¶jîúubj±Œ for more information.”…””}”(j¶jîújÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKNj¶jêúubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jñjÇj*ñhj\ñjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKj¶jKñjÇj*ñubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ*Summary of specific changes (by directory)”j§]”j±Œ*Summary of specific changes (by directory)”…””}”(j¶j@ûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j=ûjÇj*ñhj\ñjÆKRubj`)”}”(j¦Œ :file:`com/`”j§]”j˜)”}”(j¦jPûj§]”j±Œcom/”…””}”(j¶jRûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jNûubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKTj¶j=ûjÇj*ñubjFš)”}”(j¦XÛ :program:`links.arc`, :program:`links.com`, :program:`links.day` * Updated to link :file:`otides.dat` and to avoid linking the old ephemeris files (:file:`soltab.`, :file:`luntab.`, :file:`nutabl.`) if :file:`~/gg/tables/nbody` exists. * Fixed typos. :program:`sh_cleanup` * Added missing closing curly bracket in test to remove n-files on lines 386 and 387. Floyd/Pickle 190507 :program:`sh_gamit` * Revert to using GPS-only RINEX 2 instead of MGEX RINEX 3 nav files when processing GPS data since :program:`sh_rx2apr` (:program:`svpos`/:program:`svdiff`) doesn't yet recognize RINEX 3. * Fix bug in naming files for :option:`-jclock sp3` option. * Fixed a typo in call to :program:`sh_setup` causing the :file:`lfile.` not to be updated from the :file:`.apr` file. * Correct version number - now :content:`10.70 2019/8/14`. :program:`sh_get_orbits` * Placed :content:`$noclean` variable in quotes in if-test at end to ensure a string match rather than interpretation as a test, which causes an error. :program:`sh_glred` * Removed debug statement that forced archiving of the binary h-files. :program:`sh_hector` * Minor edits to some :command:`awk` commands. :program:`sh_makex` * Initialize the :content:`$sp3file` variable to avoid a problem when running stand-alone. :program:`sh_otlcmc` * New script to create :file:`tables/otlcmc.dat` file from :file:`.cmc` files at http://holt.oso.chalmers.se/loading/CMC/. :program:`sh_plot_elmean` * Updated color scheme to work with GMT 5. Small changes to line widths. :program:`sh_rx2apr` * Updated :command:`grep` commands to select only records that begin with a space before the site ID, ignoring any :content:`EXTENDED` records that may be in the :file:`.apr` file. :program:`sh_sp3fit` * Fix bug in writing model names for the :program:`arc` input file. :program:`sh_tshist` * Updated script to fully implement :content:`pos_res` type. Original only partially updated from :file:`com_pre5GMT/` version. :program:`sh_upd_stnfo` (and :file:`kf/htoglb/mstinf.[fh]`) * Added :option:`-debug` option to help diagnose problems with bad year in IGS logfiles and fixed a bug associated with first antenna starting after the first receiver entry. :program:`sh_update_dcb` * Added explicit internal test for presence of :file:`tables/svnav.dat`, needed for :program:`gamit/utils/dcbtab2`. :program:`sh_update_eop` * Updated to circumvent the shutdown of maia.usno.navy.mil and toshi.nofs.navy.mil from 2019-10-24 to 2020-04-30. ”j§]”j e)”}”(j¦hoj§]”(je)”}”(j¦Œû:program:`links.arc`, :program:`links.com`, :program:`links.day` * Updated to link :file:`otides.dat` and to avoid linking the old ephemeris files (:file:`soltab.`, :file:`luntab.`, :file:`nutabl.`) if :file:`~/gg/tables/nbody` exists. * Fixed typos. ”j§]”(je)”}”(j¦Œ@:program:`links.arc`, :program:`links.com`, :program:`links.day`”j§]”(jj)”}”(j¦Œ:program:`links.arc`”j§]”j±Œ links.arc”…””}”(j¶jwûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jsûubj±Œ, ”…””}”(j¶jsûjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`links.com`”j§]”j±Œ links.com”…””}”(j¶j‰ûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jsûubj±Œ, ”…””}”j¶jsûsbjj)”}”(j¦Œ:program:`links.day`”j§]”j±Œ links.day”…””}”(j¶j›ûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jsûubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKXj¶joûubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”(j˜)”}”(j¦Œ¨Updated to link :file:`otides.dat` and to avoid linking the old ephemeris files (:file:`soltab.`, :file:`luntab.`, :file:`nutabl.`) if :file:`~/gg/tables/nbody` exists.”j§]”j`)”}”(j¦j·ûj§]”(j±ŒUpdated to link ”…””}”(j¶j¹ûjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`otides.dat`”j§]”j±Œ otides.dat”…””}”(j¶jÀûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¹ûubj±Œ/ and to avoid linking the old ephemeris files (”…””}”(j¶j¹ûjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`soltab.`”j§]”j±Œsoltab.”…””}”(j¶jÕûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¹ûubj±Œ, ”…””}”(j¶j¹ûjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`luntab.`”j§]”j±Œluntab.”…””}”(j¶jêûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¹ûubj±Œ, ”…””}”j¶j¹ûsbj˜)”}”(j¦Œ:file:`nutabl.`”j§]”j±Œnutabl.”…””}”(j¶jÿûjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¹ûubj±Œ) if ”…””}”(j¶j¹ûjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/nbody`”j§]”j±Œ~/gg/tables/nbody”…””}”(j¶jüjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¹ûubj±Œ exists.”…””}”(j¶j¹ûjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKWj¶jµûubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j²ûubj˜)”}”(j¦Œ Fixed typos. ”j§]”j`)”}”(j¦Œ Fixed typos.”j§]”j±Œ Fixed typos.”…””}”(j¶j9üjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKXj¶j5üubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j²ûubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKWj¶j¯ûubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶joûubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKXj¶jlûubje)”}”(j¦Œ€:program:`sh_cleanup` * Added missing closing curly bracket in test to remove n-files on lines 386 and 387. Floyd/Pickle 190507 ”j§]”(je)”}”(j¦Œ:program:`sh_cleanup`”j§]”jj)”}”(j¦jeüj§]”j±Œ sh_cleanup”…””}”(j¶jgüjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jcüubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK[j¶j_üubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒhAdded missing closing curly bracket in test to remove n-files on lines 386 and 387. Floyd/Pickle 190507 ”j§]”j`)”}”(j¦ŒgAdded missing closing curly bracket in test to remove n-files on lines 386 and 387. Floyd/Pickle 190507”j§]”j±ŒgAdded missing closing curly bracket in test to remove n-files on lines 386 and 387. Floyd/Pickle 190507”…””}”(j¶j„üjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK[j¶j€üubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j}üubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK[j¶jzüubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j_üubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK[j¶jlûubje)”}”(j¦X¿:program:`sh_gamit` * Revert to using GPS-only RINEX 2 instead of MGEX RINEX 3 nav files when processing GPS data since :program:`sh_rx2apr` (:program:`svpos`/:program:`svdiff`) doesn't yet recognize RINEX 3. * Fix bug in naming files for :option:`-jclock sp3` option. * Fixed a typo in call to :program:`sh_setup` causing the :file:`lfile.` not to be updated from the :file:`.apr` file. * Correct version number - now :content:`10.70 2019/8/14`. ”j§]”(je)”}”(j¦Œ:program:`sh_gamit`”j§]”jj)”}”(j¦j°üj§]”j±Œsh_gamit”…””}”(j¶j²üjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j®üubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKaj¶jªüubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”(j˜)”}”(j¦ŒºRevert to using GPS-only RINEX 2 instead of MGEX RINEX 3 nav files when processing GPS data since :program:`sh_rx2apr` (:program:`svpos`/:program:`svdiff`) doesn't yet recognize RINEX 3.”j§]”j`)”}”(j¦jÍüj§]”(j±ŒbRevert to using GPS-only RINEX 2 instead of MGEX RINEX 3 nav files when processing GPS data since ”…””}”(j¶jÏüjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_rx2apr`”j§]”j±Œ sh_rx2apr”…””}”(j¶jÖüjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÏüubj±Œ (”…””}”(j¶jÏüjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`svpos`”j§]”j±Œsvpos”…””}”(j¶jèüjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÏüubj±Œ/”…””}”(j¶jÏüjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`svdiff`”j§]”j±Œsvdiff”…””}”(j¶júüjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÏüubj±Œ") doesn’t yet recognize RINEX 3.”…””}”(j¶jÏüjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK^j¶jËüubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÈüubj˜)”}”(j¦Œ9Fix bug in naming files for :option:`-jclock sp3` option.”j§]”j`)”}”(j¦jýj§]”(j±ŒFix bug in naming files for ”…””}”(j¶jýjÇj*ñhNjÆNubj’)”}”(j¦Œ:option:`-jclock sp3`”j§]”j˜)”}”(j¦j%ýj§]”j±Œ -jclock sp3”…””}”(j¶j'ýjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j#ýubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jñŒ refdomain”j1ýŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ -jclock sp3”ujÄj‘hj\ñjÆK_j¶jýubj±Œ option.”…””}”(j¶jýjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK_j¶jýubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÈüubj˜)”}”(j¦ŒtFixed a typo in call to :program:`sh_setup` causing the :file:`lfile.` not to be updated from the :file:`.apr` file.”j§]”j`)”}”(j¦jUýj§]”(j±ŒFixed a typo in call to ”…””}”(j¶jWýjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`sh_setup`”j§]”j±Œsh_setup”…””}”(j¶j^ýjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jWýubj±Œ causing the ”…””}”(j¶jWýjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`lfile.`”j§]”j±Œlfile.”…””}”(j¶jpýjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jWýubj±Œ not to be updated from the ”…””}”(j¶jWýjÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶j…ýjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jWýubj±Œ file.”…””}”(j¶jWýjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK`j¶jSýubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÈüubj˜)”}”(j¦Œ9Correct version number - now :content:`10.70 2019/8/14`. ”j§]”j`)”}”(j¦Œ8Correct version number - now :content:`10.70 2019/8/14`.”j§]”(j±ŒCorrect version number - now ”…””}”(j¶jªýjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`10.70 2019/8/14`”j§]”j±Œ10.70 2019/8/14”…””}”(j¶j²ýjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jªýubj±Œ.”…””}”(j¶jªýjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKaj¶j¦ýubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÈüubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK^j¶jÅüubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jªüubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKaj¶jlûubje)”}”(j¦Œ±:program:`sh_get_orbits` * Placed :content:`$noclean` variable in quotes in if-test at end to ensure a string match rather than interpretation as a test, which causes an error. ”j§]”(je)”}”(j¦Œ:program:`sh_get_orbits`”j§]”jj)”}”(j¦jéýj§]”j±Œ sh_get_orbits”…””}”(j¶jëýjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jçýubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKdj¶jãýubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ–Placed :content:`$noclean` variable in quotes in if-test at end to ensure a string match rather than interpretation as a test, which causes an error. ”j§]”j`)”}”(j¦Œ•Placed :content:`$noclean` variable in quotes in if-test at end to ensure a string match rather than interpretation as a test, which causes an error.”j§]”(j±ŒPlaced ”…””}”(j¶jþjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`$noclean`”j§]”j±Œ$noclean”…””}”(j¶jþjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jþubj±Œ{ variable in quotes in if-test at end to ensure a string match rather than interpretation as a test, which causes an error.”…””}”(j¶jþjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKdj¶jþubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jþubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKdj¶jþýubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jãýubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKdj¶jlûubje)”}”(j¦Œ[:program:`sh_glred` * Removed debug statement that forced archiving of the binary h-files. ”j§]”(je)”}”(j¦Œ:program:`sh_glred`”j§]”jj)”}”(j¦jGþj§]”j±Œsh_glred”…””}”(j¶jIþjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jEþubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKgj¶jAþubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒERemoved debug statement that forced archiving of the binary h-files. ”j§]”j`)”}”(j¦ŒDRemoved debug statement that forced archiving of the binary h-files.”j§]”j±ŒDRemoved debug statement that forced archiving of the binary h-files.”…””}”(j¶jfþjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKgj¶jbþubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j_þubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKgj¶j\þubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jAþubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKgj¶jlûubje)”}”(j¦ŒD:program:`sh_hector` * Minor edits to some :command:`awk` commands. ”j§]”(je)”}”(j¦Œ:program:`sh_hector`”j§]”jj)”}”(j¦j’þj§]”j±Œ sh_hector”…””}”(j¶j”þjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jþubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKjj¶jŒþubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ-Minor edits to some :command:`awk` commands. ”j§]”j`)”}”(j¦Œ,Minor edits to some :command:`awk` commands.”j§]”(j±ŒMinor edits to some ”…””}”(j¶j±þjÇj*ñhNjÆNubjj)”}”(j¦Œ:command:`awk`”j§]”j±Œawk”…””}”(j¶j¹þjÇj*ñhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶j±þubj±Œ commands.”…””}”(j¶j±þjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKjj¶j­þubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jªþubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKjj¶j§þubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jŒþubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKjj¶jlûubje)”}”(j¦Œo:program:`sh_makex` * Initialize the :content:`$sp3file` variable to avoid a problem when running stand-alone. ”j§]”(je)”}”(j¦Œ:program:`sh_makex`”j§]”jj)”}”(j¦jïþj§]”j±Œsh_makex”…””}”(j¶jñþjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jíþubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKmj¶jéþubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒYInitialize the :content:`$sp3file` variable to avoid a problem when running stand-alone. ”j§]”j`)”}”(j¦ŒXInitialize the :content:`$sp3file` variable to avoid a problem when running stand-alone.”j§]”(j±ŒInitialize the ”…””}”(j¶jÿjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`$sp3file`”j§]”j±Œ$sp3file”…””}”(j¶jÿjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÿubj±Œ6 variable to avoid a problem when running stand-alone.”…””}”(j¶jÿjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKmj¶j ÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKmj¶jÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jéþubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKmj¶jlûubje)”}”(j¦Œ:program:`sh_otlcmc` * New script to create :file:`tables/otlcmc.dat` file from :file:`.cmc` files at http://holt.oso.chalmers.se/loading/CMC/. ”j§]”(je)”}”(j¦Œ:program:`sh_otlcmc`”j§]”jj)”}”(j¦jMÿj§]”j±Œ sh_otlcmc”…””}”(j¶jOÿjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jKÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKpj¶jGÿubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒyNew script to create :file:`tables/otlcmc.dat` file from :file:`.cmc` files at http://holt.oso.chalmers.se/loading/CMC/. ”j§]”j`)”}”(j¦ŒxNew script to create :file:`tables/otlcmc.dat` file from :file:`.cmc` files at http://holt.oso.chalmers.se/loading/CMC/.”j§]”(j±ŒNew script to create ”…””}”(j¶jlÿjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/otlcmc.dat`”j§]”j±Œtables/otlcmc.dat”…””}”(j¶jtÿjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jlÿubj±Œ file from ”…””}”(j¶jlÿjÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`.cmc`”j§]”j±Œ.cmc”…””}”(j¶j‰ÿjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jlÿubj±Œ files at ”…””}”(j¶jlÿjÇj*ñhNjÆNubj÷ )”}”(j¦Œ(http://holt.oso.chalmers.se/loading/CMC/”j§]”j±Œ(http://holt.oso.chalmers.se/loading/CMC/”…””}”(j¶jžÿjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j ÿujÄjö j¶jlÿubj±Œ.”…””}”(j¶jlÿjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKpj¶jhÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jeÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKpj¶jbÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jGÿubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKpj¶jlûubje)”}”(j¦Œc:program:`sh_plot_elmean` * Updated color scheme to work with GMT 5. Small changes to line widths. ”j§]”(je)”}”(j¦Œ:program:`sh_plot_elmean`”j§]”jj)”}”(j¦jÕÿj§]”j±Œsh_plot_elmean”…””}”(j¶j×ÿjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKsj¶jÏÿubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒGUpdated color scheme to work with GMT 5. Small changes to line widths. ”j§]”j`)”}”(j¦ŒFUpdated color scheme to work with GMT 5. Small changes to line widths.”j§]”j±ŒFUpdated color scheme to work with GMT 5. Small changes to line widths.”…””}”(j¶jôÿjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKsj¶jðÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jíÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKsj¶jêÿubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jÏÿubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKsj¶jlûubje)”}”(j¦ŒÊ:program:`sh_rx2apr` * Updated :command:`grep` commands to select only records that begin with a space before the site ID, ignoring any :content:`EXTENDED` records that may be in the :file:`.apr` file. ”j§]”(je)”}”(j¦Œ:program:`sh_rx2apr`”j§]”jj)”}”(j¦j j§]”j±Œ sh_rx2apr”…””}”(j¶j"jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKvj¶jubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ³Updated :command:`grep` commands to select only records that begin with a space before the site ID, ignoring any :content:`EXTENDED` records that may be in the :file:`.apr` file. ”j§]”j`)”}”(j¦Œ²Updated :command:`grep` commands to select only records that begin with a space before the site ID, ignoring any :content:`EXTENDED` records that may be in the :file:`.apr` file.”j§]”(j±ŒUpdated ”…””}”(j¶j?jÇj*ñhNjÆNubjj)”}”(j¦Œ:command:`grep`”j§]”j±Œgrep”…””}”(j¶jGjÇj*ñhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶j?ubj±ŒZ commands to select only records that begin with a space before the site ID, ignoring any ”…””}”(j¶j?jÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`EXTENDED`”j§]”j±ŒEXTENDED”…””}”(j¶jYjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j?ubj±Œ records that may be in the ”…””}”(j¶j?jÇj*ñhNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶jljÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j?ubj±Œ file.”…””}”(j¶j?jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKvj¶j;ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j8ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKvj¶j5ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKvj¶jlûubje)”}”(j¦ŒY:program:`sh_sp3fit` * Fix bug in writing model names for the :program:`arc` input file. ”j§]”(je)”}”(j¦Œ:program:`sh_sp3fit`”j§]”jj)”}”(j¦j¥j§]”j±Œ sh_sp3fit”…””}”(j¶j§jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j£ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKyj¶jŸubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒBFix bug in writing model names for the :program:`arc` input file. ”j§]”j`)”}”(j¦ŒAFix bug in writing model names for the :program:`arc` input file.”j§]”(j±Œ'Fix bug in writing model names for the ”…””}”(j¶jÄjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`arc`”j§]”j±Œarc”…””}”(j¶jÌjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÄubj±Œ input file.”…””}”(j¶jÄjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKyj¶jÀubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j½ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKyj¶jºubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jŸubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKyj¶jlûubje)”}”(j¦Œ•:program:`sh_tshist` * Updated script to fully implement :content:`pos_res` type. Original only partially updated from :file:`com_pre5GMT/` version. ”j§]”(je)”}”(j¦Œ:program:`sh_tshist`”j§]”jj)”}”(j¦jj§]”j±Œ sh_tshist”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK|j¶jüubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ~Updated script to fully implement :content:`pos_res` type. Original only partially updated from :file:`com_pre5GMT/` version. ”j§]”j`)”}”(j¦Œ}Updated script to fully implement :content:`pos_res` type. Original only partially updated from :file:`com_pre5GMT/` version.”j§]”(j±Œ"Updated script to fully implement ”…””}”(j¶j!jÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`pos_res`”j§]”j±Œpos_res”…””}”(j¶j)jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j!ubj±Œ, type. Original only partially updated from ”…””}”(j¶j!jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`com_pre5GMT/`”j§]”j±Œ com_pre5GMT/”…””}”(j¶j<jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j!ubj±Œ version.”…””}”(j¶j!jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK|j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK|j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jüubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK|j¶jlûubje)”}”(j¦Œë:program:`sh_upd_stnfo` (and :file:`kf/htoglb/mstinf.[fh]`) * Added :option:`-debug` option to help diagnose problems with bad year in IGS logfiles and fixed a bug associated with first antenna starting after the first receiver entry. ”j§]”(je)”}”(j¦Œ;:program:`sh_upd_stnfo` (and :file:`kf/htoglb/mstinf.[fh]`)”j§]”(jj)”}”(j¦Œ:program:`sh_upd_stnfo`”j§]”j±Œ sh_upd_stnfo”…””}”(j¶jwjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jsubj±Œ (and ”…””}”(j¶jsjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`kf/htoglb/mstinf.[fh]`”j§]”j±Œkf/htoglb/mstinf.[fh]”…””}”(j¶j‰jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œ)”…””}”(j¶jsjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKj¶joubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ­Added :option:`-debug` option to help diagnose problems with bad year in IGS logfiles and fixed a bug associated with first antenna starting after the first receiver entry. ”j§]”j`)”}”(j¦Œ¬Added :option:`-debug` option to help diagnose problems with bad year in IGS logfiles and fixed a bug associated with first antenna starting after the first receiver entry.”j§]”(j±ŒAdded ”…””}”(j¶j®jÇj*ñhNjÆNubj’)”}”(j¦Œ:option:`-debug`”j§]”j˜)”}”(j¦j¸j§]”j±Œ-debug”…””}”(j¶jºjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶j¶ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jñŒ refdomain”jÄŒreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-debug”ujÄj‘hj\ñjÆKj¶j®ubj±Œ– option to help diagnose problems with bad year in IGS logfiles and fixed a bug associated with first antenna starting after the first receiver entry.”…””}”(j¶j®jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKj¶jªubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j§ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKj¶j¤ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶joubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKj¶jlûubje)”}”(j¦Œ:program:`sh_update_dcb` * Added explicit internal test for presence of :file:`tables/svnav.dat`, needed for :program:`gamit/utils/dcbtab2`. ”j§]”(je)”}”(j¦Œ:program:`sh_update_dcb`”j§]”jj)”}”(j¦jþj§]”j±Œ sh_update_dcb”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jüubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK‚j¶jøubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒrAdded explicit internal test for presence of :file:`tables/svnav.dat`, needed for :program:`gamit/utils/dcbtab2`. ”j§]”j`)”}”(j¦ŒqAdded explicit internal test for presence of :file:`tables/svnav.dat`, needed for :program:`gamit/utils/dcbtab2`.”j§]”(j±Œ-Added explicit internal test for presence of ”…””}”(j¶jjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/svnav.dat`”j§]”j±Œtables/svnav.dat”…””}”(j¶j%jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ , needed for ”…””}”(j¶jjÇj*ñhNjÆNubjj)”}”(j¦Œ:program:`gamit/utils/dcbtab2`”j§]”j±Œgamit/utils/dcbtab2”…””}”(j¶j:jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jubj±Œ.”…””}”(j¶jjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK‚j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK‚j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jøubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK‚j¶jlûubje)”}”(j¦Œ‹:program:`sh_update_eop` * Updated to circumvent the shutdown of maia.usno.navy.mil and toshi.nofs.navy.mil from 2019-10-24 to 2020-04-30. ”j§]”(je)”}”(j¦Œ:program:`sh_update_eop`”j§]”jj)”}”(j¦jpj§]”j±Œ sh_update_eop”…””}”(j¶jrjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jnubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK…j¶jjubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒpUpdated to circumvent the shutdown of maia.usno.navy.mil and toshi.nofs.navy.mil from 2019-10-24 to 2020-04-30. ”j§]”j`)”}”(j¦ŒoUpdated to circumvent the shutdown of maia.usno.navy.mil and toshi.nofs.navy.mil from 2019-10-24 to 2020-04-30.”j§]”j±ŒoUpdated to circumvent the shutdown of maia.usno.navy.mil and toshi.nofs.navy.mil from 2019-10-24 to 2020-04-30.”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK…j¶j‹ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jˆubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK…j¶j…ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jjubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK…j¶jlûubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶jhûubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjEšhj\ñjÆKVj¶j=ûjÇj*ñubj`)”}”(j¦Œ:file:`gamit/`”j§]”j˜)”}”(j¦jÃj§]”j±Œgamit/”…””}”(j¶jÅjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÁubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK‡j¶j=ûjÇj*ñubjFš)”}”(j¦X :file:`orbits/kouba_gps.f`, :file:`orbits/oversn.f`; :file:`arc/ertorb.f`, :file:`arc/earthradTUM.f`, :file:`arc/aversn.f`; :file:`lib/gpsblock.f`, :file:`lib/lversn.f` * Updated for Block IIIA SV. WARNING: Will recongize GPS Block IIIA but use IIF values for Earth radiation pressure and yaw. :file:`arc/satprop.f`, :file:`arc/earthradTUM.f` * Updated for Block III SV. * Temporarily use IIF Earth radiation model for Block IIIA for :content:`NCLE1` (set for TUM1) and remove debug print from :file:`earthradTUM.f`. :program:`arc/sbfn` * Fix bug in effect of General Relativity on satellite (~ 8 mm over 24 hrs). :file:`includes/makex.h`, :file:`lib/rrinex.f` * Increase maximum line length to 1024, and associated maximum observables allowed in :file:`rrinex.f` and :content:`MAXOBT` in :file:`makex.h` to 63, to accommodate long records in RINEX 3 files. :program:`lib/clkera` * Erroneous extra read of :content:`clkoff`, apparently a problem with Intel compiler but not gfortran. :file:`lib/linear.f`, :file:`model/get_antinfo.f`, :file:`model/get_antpcv.f`, :file:`model/get_svantpcv.f` * Fix problem with interpolation of elevation-only PCVs. :file:`lib/rrxhed.f` * Skipped reading of SV-dependent wavelength factors in a RINEX header since this feature is not yet supported. :file:`lib/sel_obtyp.f` * Fix problem with omitted Beidou observable. * Remove debug print statements. :file:`makex/get_navclk.f` * Fix bug in not recognizing GNSS code "I" on the nav file. :file:`makex/getsp3.f` * Added test for sp3d format. :file:`makex/rbatch.f` * Add trap for :content:`numsit` > :content:`maxsit` in new-format case. * Correct fix of trap for :content:`numsit`. :file:`makex/mversn.f`, :file:`model/j_from_sp3.f`, :file:`model/getnav.f` * Allow reading sp3 "d" and fix getting the program name for warning/fatal messages. :program:`makexp` * Assign the SP3 file name when running manually. * Revoked Zou/King 180912 update and reverted to version 9.86. * Added correct handling of SP3 file name when running manually. :file:`model/call_mag.f`, :file:`model/iondel.f`, :file:`model/mag13.f`, :file:`model/setup.f`; :file:`fixdrv/bmake.f`; :file:`tables/sestbl.` * Added IGRF13 magnetic field model and changed default from IGRF12 to IGRF13. :file:`model/setup.f` * Fix frequency check so that it works for L1-only. :program:`model/update_coords` * Add missing "debug" in call to :content:`get_antinfo`. :program:`utils/metutil` * Change linear interpolation routine to be scalar rather than vector. ”j§]”j e)”}”(j¦hoj§]”(je)”}”(j¦X&:file:`orbits/kouba_gps.f`, :file:`orbits/oversn.f`; :file:`arc/ertorb.f`, :file:`arc/earthradTUM.f`, :file:`arc/aversn.f`; :file:`lib/gpsblock.f`, :file:`lib/lversn.f` * Updated for Block IIIA SV. WARNING: Will recongize GPS Block IIIA but use IIF values for Earth radiation pressure and yaw. ”j§]”(je)”}”(j¦Œ¨:file:`orbits/kouba_gps.f`, :file:`orbits/oversn.f`; :file:`arc/ertorb.f`, :file:`arc/earthradTUM.f`, :file:`arc/aversn.f`; :file:`lib/gpsblock.f`, :file:`lib/lversn.f`”j§]”(j˜)”}”(j¦Œ:file:`orbits/kouba_gps.f`”j§]”j±Œorbits/kouba_gps.f”…””}”(j¶jêjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæubj±Œ, ”…””}”(j¶jæjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`orbits/oversn.f`”j§]”j±Œorbits/oversn.f”…””}”(j¶jÿjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæubj±Œ; ”…””}”(j¶jæjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`arc/ertorb.f`”j§]”j±Œ arc/ertorb.f”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæubj±Œ, ”…””}”j¶jæsbj˜)”}”(j¦Œ:file:`arc/earthradTUM.f`”j§]”j±Œarc/earthradTUM.f”…””}”(j¶j)jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæubj±Œ, ”…””}”j¶jæsbj˜)”}”(j¦Œ:file:`arc/aversn.f`”j§]”j±Œ arc/aversn.f”…””}”(j¶j>jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæubj±Œ; ”…””}”j¶jæsbj˜)”}”(j¦Œ:file:`lib/gpsblock.f`”j§]”j±Œlib/gpsblock.f”…””}”(j¶jSjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæubj±Œ, ”…””}”j¶jæsbj˜)”}”(j¦Œ:file:`lib/lversn.f`”j§]”j±Œ lib/lversn.f”…””}”(j¶jhjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jæubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKŠj¶jâubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ{Updated for Block IIIA SV. WARNING: Will recongize GPS Block IIIA but use IIF values for Earth radiation pressure and yaw. ”j§]”j`)”}”(j¦ŒzUpdated for Block IIIA SV. WARNING: Will recongize GPS Block IIIA but use IIF values for Earth radiation pressure and yaw.”j§]”j±ŒzUpdated for Block IIIA SV. WARNING: Will recongize GPS Block IIIA but use IIF values for Earth radiation pressure and yaw.”…””}”(j¶j‰jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKŠj¶j…ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j‚ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKŠj¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jâubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKŠj¶jßubje)”}”(j¦Œß:file:`arc/satprop.f`, :file:`arc/earthradTUM.f` * Updated for Block III SV. * Temporarily use IIF Earth radiation model for Block IIIA for :content:`NCLE1` (set for TUM1) and remove debug print from :file:`earthradTUM.f`. ”j§]”(je)”}”(j¦Œ0:file:`arc/satprop.f`, :file:`arc/earthradTUM.f`”j§]”(j˜)”}”(j¦Œ:file:`arc/satprop.f`”j§]”j±Œ arc/satprop.f”…””}”(j¶j·jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j³ubj±Œ, ”…””}”(j¶j³jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`arc/earthradTUM.f`”j§]”j±Œarc/earthradTUM.f”…””}”(j¶jÌjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j³ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKŽj¶j¯ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”(j˜)”}”(j¦ŒUpdated for Block III SV.”j§]”j`)”}”(j¦jëj§]”j±ŒUpdated for Block III SV.”…””}”(j¶jíjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKj¶jéubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jæubj˜)”}”(j¦ŒTemporarily use IIF Earth radiation model for Block IIIA for :content:`NCLE1` (set for TUM1) and remove debug print from :file:`earthradTUM.f`. ”j§]”j`)”}”(j¦ŒTemporarily use IIF Earth radiation model for Block IIIA for :content:`NCLE1` (set for TUM1) and remove debug print from :file:`earthradTUM.f`.”j§]”(j±Œ=Temporarily use IIF Earth radiation model for Block IIIA for ”…””}”(j¶jjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`NCLE1`”j§]”j±ŒNCLE1”…””}”(j¶j jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jubj±Œ, (set for TUM1) and remove debug print from ”…””}”(j¶jjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`earthradTUM.f`”j§]”j±Œ earthradTUM.f”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ.”…””}”(j¶jjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKŽj¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jæubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKj¶jãubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j¯ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKŽj¶jßubje)”}”(j¦Œa:program:`arc/sbfn` * Fix bug in effect of General Relativity on satellite (~ 8 mm over 24 hrs). ”j§]”(je)”}”(j¦Œ:program:`arc/sbfn`”j§]”jj)”}”(j¦jXj§]”j±Œarc/sbfn”…””}”(j¶jZjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jVubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK‘j¶jRubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒKFix bug in effect of General Relativity on satellite (~ 8 mm over 24 hrs). ”j§]”j`)”}”(j¦ŒJFix bug in effect of General Relativity on satellite (~ 8 mm over 24 hrs).”j§]”j±ŒJFix bug in effect of General Relativity on satellite (~ 8 mm over 24 hrs).”…””}”(j¶jwjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK‘j¶jsubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jpubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK‘j¶jmubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jRubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK‘j¶jßubje)”}”(j¦Œô:file:`includes/makex.h`, :file:`lib/rrinex.f` * Increase maximum line length to 1024, and associated maximum observables allowed in :file:`rrinex.f` and :content:`MAXOBT` in :file:`makex.h` to 63, to accommodate long records in RINEX 3 files. ”j§]”(je)”}”(j¦Œ.:file:`includes/makex.h`, :file:`lib/rrinex.f`”j§]”(j˜)”}”(j¦Œ:file:`includes/makex.h`”j§]”j±Œincludes/makex.h”…””}”(j¶j¥jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¡ubj±Œ, ”…””}”(j¶j¡jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`lib/rrinex.f`”j§]”j±Œ lib/rrinex.f”…””}”(j¶jºjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¡ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK”j¶jubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒÃIncrease maximum line length to 1024, and associated maximum observables allowed in :file:`rrinex.f` and :content:`MAXOBT` in :file:`makex.h` to 63, to accommodate long records in RINEX 3 files. ”j§]”j`)”}”(j¦ŒÂIncrease maximum line length to 1024, and associated maximum observables allowed in :file:`rrinex.f` and :content:`MAXOBT` in :file:`makex.h` to 63, to accommodate long records in RINEX 3 files.”j§]”(j±ŒTIncrease maximum line length to 1024, and associated maximum observables allowed in ”…””}”(j¶jÛjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`rrinex.f`”j§]”j±Œrrinex.f”…””}”(j¶jãjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÛubj±Œ and ”…””}”(j¶jÛjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`MAXOBT`”j§]”j±ŒMAXOBT”…””}”(j¶jøjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jÛubj±Œ in ”…””}”(j¶jÛjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`makex.h`”j§]”j±Œmakex.h”…””}”(j¶j jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÛubj±Œ5 to 63, to accommodate long records in RINEX 3 files.”…””}”(j¶jÛjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK”j¶j×ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÔubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK”j¶jÑubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK”j¶jßubje)”}”(j¦Œ~:program:`lib/clkera` * Erroneous extra read of :content:`clkoff`, apparently a problem with Intel compiler but not gfortran. ”j§]”(je)”}”(j¦Œ:program:`lib/clkera`”j§]”jj)”}”(j¦jDj§]”j±Œ lib/clkera”…””}”(j¶jFjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jBubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK—j¶j>ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒfErroneous extra read of :content:`clkoff`, apparently a problem with Intel compiler but not gfortran. ”j§]”j`)”}”(j¦ŒeErroneous extra read of :content:`clkoff`, apparently a problem with Intel compiler but not gfortran.”j§]”(j±ŒErroneous extra read of ”…””}”(j¶jcjÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`clkoff`”j§]”j±Œclkoff”…””}”(j¶jkjÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jcubj±Œ<, apparently a problem with Intel compiler but not gfortran.”…””}”(j¶jcjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK—j¶j_ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j\ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK—j¶jYubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j>ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK—j¶jßubje)”}”(j¦Œ¥:file:`lib/linear.f`, :file:`model/get_antinfo.f`, :file:`model/get_antpcv.f`, :file:`model/get_svantpcv.f` * Fix problem with interpolation of elevation-only PCVs. ”j§]”(je)”}”(j¦Œk:file:`lib/linear.f`, :file:`model/get_antinfo.f`, :file:`model/get_antpcv.f`, :file:`model/get_svantpcv.f`”j§]”(j˜)”}”(j¦Œ:file:`lib/linear.f`”j§]”j±Œ lib/linear.f”…””}”(j¶j¤jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubj±Œ, ”…””}”(j¶j jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`model/get_antinfo.f`”j§]”j±Œmodel/get_antinfo.f”…””}”(j¶j¹jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubj±Œ, ”…””}”j¶j sbj˜)”}”(j¦Œ:file:`model/get_antpcv.f`”j§]”j±Œmodel/get_antpcv.f”…””}”(j¶jÎjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubj±Œ, ”…””}”j¶j sbj˜)”}”(j¦Œ:file:`model/get_svantpcv.f`”j§]”j±Œmodel/get_svantpcv.f”…””}”(j¶jãjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKšj¶jœubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ7Fix problem with interpolation of elevation-only PCVs. ”j§]”j`)”}”(j¦Œ6Fix problem with interpolation of elevation-only PCVs.”j§]”j±Œ6Fix problem with interpolation of elevation-only PCVs.”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKšj¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jýubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKšj¶júubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jœubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKšj¶jßubje)”}”(j¦Œ…:file:`lib/rrxhed.f` * Skipped reading of SV-dependent wavelength factors in a RINEX header since this feature is not yet supported. ”j§]”(je)”}”(j¦Œ:file:`lib/rrxhed.f`”j§]”j˜)”}”(j¦j0j§]”j±Œ lib/rrxhed.f”…””}”(j¶j2jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j.ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKj¶j*ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒnSkipped reading of SV-dependent wavelength factors in a RINEX header since this feature is not yet supported. ”j§]”j`)”}”(j¦ŒmSkipped reading of SV-dependent wavelength factors in a RINEX header since this feature is not yet supported.”j§]”j±ŒmSkipped reading of SV-dependent wavelength factors in a RINEX header since this feature is not yet supported.”…””}”(j¶jRjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKj¶jNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jKubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKj¶jHubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j*ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKj¶jßubje)”}”(j¦Œg:file:`lib/sel_obtyp.f` * Fix problem with omitted Beidou observable. * Remove debug print statements. ”j§]”(je)”}”(j¦Œ:file:`lib/sel_obtyp.f`”j§]”j˜)”}”(j¦j~j§]”j±Œlib/sel_obtyp.f”…””}”(j¶j€jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j|ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK¡j¶jxubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”(j˜)”}”(j¦Œ+Fix problem with omitted Beidou observable.”j§]”j`)”}”(j¦jžj§]”j±Œ+Fix problem with omitted Beidou observable.”…””}”(j¶j jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK j¶jœubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j™ubj˜)”}”(j¦ŒRemove debug print statements. ”j§]”j`)”}”(j¦ŒRemove debug print statements.”j§]”j±ŒRemove debug print statements.”…””}”(j¶j·jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK¡j¶j³ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j™ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK j¶j–ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jxubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK¡j¶jßubje)”}”(j¦ŒW:file:`makex/get_navclk.f` * Fix bug in not recognizing GNSS code "I" on the nav file. ”j§]”(je)”}”(j¦Œ:file:`makex/get_navclk.f`”j§]”j˜)”}”(j¦jãj§]”j±Œmakex/get_navclk.f”…””}”(j¶jåjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jáubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK¤j¶jÝubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ:Fix bug in not recognizing GNSS code "I" on the nav file. ”j§]”j`)”}”(j¦Œ9Fix bug in not recognizing GNSS code "I" on the nav file.”j§]”j±Œ=Fix bug in not recognizing GNSS code “I†on the nav file.”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK¤j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jþubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK¤j¶jûubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jÝubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK¤j¶jßubje)”}”(j¦Œ5:file:`makex/getsp3.f` * Added test for sp3d format. ”j§]”(je)”}”(j¦Œ:file:`makex/getsp3.f`”j§]”j˜)”}”(j¦j1j§]”j±Œmakex/getsp3.f”…””}”(j¶j3jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j/ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK§j¶j+ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒAdded test for sp3d format. ”j§]”j`)”}”(j¦ŒAdded test for sp3d format.”j§]”j±ŒAdded test for sp3d format.”…””}”(j¶jSjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK§j¶jOubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jLubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK§j¶jIubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j+ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK§j¶jßubje)”}”(j¦Œ:file:`makex/rbatch.f` * Add trap for :content:`numsit` > :content:`maxsit` in new-format case. * Correct fix of trap for :content:`numsit`. ”j§]”(je)”}”(j¦Œ:file:`makex/rbatch.f`”j§]”j˜)”}”(j¦jj§]”j±Œmakex/rbatch.f”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j}ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK«j¶jyubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”(j˜)”}”(j¦ŒFAdd trap for :content:`numsit` > :content:`maxsit` in new-format case.”j§]”j`)”}”(j¦jŸj§]”(j±Œ Add trap for ”…””}”(j¶j¡jÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`numsit`”j§]”j±Œnumsit”…””}”(j¶j¨jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¡ubj±Œ > ”…””}”(j¶j¡jÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`maxsit`”j§]”j±Œmaxsit”…””}”(j¶j»jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¡ubj±Œ in new-format case.”…””}”(j¶j¡jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKªj¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jšubj˜)”}”(j¦Œ+Correct fix of trap for :content:`numsit`. ”j§]”j`)”}”(j¦Œ*Correct fix of trap for :content:`numsit`.”j§]”(j±ŒCorrect fix of trap for 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sbj˜)”}”(j¦Œ:file:`tables/sestbl.`”j§]”j±Œtables/sestbl.”…””}”(j¶jz jÇj*ñhNjÆNubaj·}”(j¹•]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK¶j¶j ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒMAdded IGRF13 magnetic field model and changed default from IGRF12 to IGRF13. ”j§]”j`)”}”(j¦ŒLAdded IGRF13 magnetic field model and changed default from IGRF12 to IGRF13.”j§]”j±ŒLAdded IGRF13 magnetic field model and changed default from IGRF12 to IGRF13.”…””}”(j¶j› jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK¶j¶j— ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j” ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK¶j¶j‘ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK¶j¶jßubje)”}”(j¦ŒJ:file:`model/setup.f` * Fix frequency check so that it works for L1-only. ”j§]”(je)”}”(j¦Œ:file:`model/setup.f`”j§]”j˜)”}”(j¦jÇ j§]”j±Œ model/setup.f”…””}”(j¶jÉ jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÅ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK¹j¶jÁ ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ2Fix frequency check so that it works for L1-only. ”j§]”j`)”}”(j¦Œ1Fix frequency check so that it works for L1-only.”j§]”j±Œ1Fix frequency check so that it works for L1-only.”…””}”(j¶jé jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆK¹j¶jå ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jâ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆK¹j¶jß ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jÁ ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK¹j¶jßubje)”}”(j¦ŒX:program:`model/update_coords` * Add missing "debug" in call to :content:`get_antinfo`. ”j§]”(je)”}”(j¦Œ:program:`model/update_coords`”j§]”jj)”}”(j¦j j§]”j±Œmodel/update_coords”…””}”(j¶j jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆK¼j¶j ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ7Add missing "debug" in call to :content:`get_antinfo`. ”j§]”j`)”}”(j¦Œ6Add missing "debug" in call to :content:`get_antinfo`.”j§]”(j±Œ#Add missing “debug†in 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jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKÄj¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKÄj¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jå ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÄj¶jâ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶jÞ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjEšhj\ñjÆKÃj¶j=ûjÇj*ñubj`)”}”(j¦Œ :file:`kf/`”j§]”j˜)”}”(j¦jA j§]”j±Œkf/”…””}”(j¶jC jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j? ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKÆj¶j=ûjÇj*ñubjFš)”}”(j¦X,:file:`blsum/tscon.f` * Added assumption that UNR/NGL :file:`.txyz2` files without a reference frame explicitly in the file name are the latest IGS14 version. :program:`displace` * Updated Makefile, grid calculations and added tensile component to calculations. :file:`gen_util/name_to_block.f` * Changes BLOCK III to BLOCK IIIA so that correct satellite number is assigned to the new PRN03. :file:`gen_util/real_stats.f` * Updated dimensioning and bounds checking. Very long time series could cause segmentation violations. :file:`gen_util/sp3_lib.f`, :file:`includes/sp3_def.h` * Updated maximum number of nadir angles values and added a dimensioning test. :file:`gen_util/sp3_lib.f` * Fixed bug in :content:`report_stat` call that is invoked in updated :file:`sp3_def.h` is not used. * Increased max nadir values to 41 for Galileo chamber calibrations. :file:`globk/read_glb_mar.f` * Critical update needed to make the :content:`SOURCE` command work. :file:`glout/write_iers.f` * Updated formats to allow more than 99 reference frame sites. :file:`htoglb/mstinf.[fh]` (and :program:`com/sh_upd_stnfo`) * Added :option:`-debug` option to help diagnose problems with bad year in IGS logfiles and fixed a bug associated with first antenna starting after the first receiver entry. :program:`track`, :file:`gen_util/sp3_lib.f` * Updated for Beidou B7 phase and range measurements. :program:`utils/corcom` * Updated output formats to allow for fast ice velocities. :file:`utils/glbtog.[fh]` * Fixed bugs with writing G-files for non-GPS systems. ”j§]”j e)”}”(j¦hoj§]”(je)”}”(j¦ŒŸ:file:`blsum/tscon.f` * Added assumption that UNR/NGL :file:`.txyz2` files without a reference frame explicitly in the file name are the latest IGS14 version. ”j§]”(je)”}”(j¦Œ:file:`blsum/tscon.f`”j§]”j˜)”}”(j¦jf j§]”j±Œ blsum/tscon.f”…””}”(j¶jh jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jd ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÉj¶j` ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ‡Added assumption that UNR/NGL :file:`.txyz2` files without a reference frame explicitly in the file name are the latest IGS14 version. ”j§]”j`)”}”(j¦Œ†Added assumption that UNR/NGL :file:`.txyz2` files without a reference frame explicitly in the file name are the latest IGS14 version.”j§]”(j±ŒAdded assumption that UNR/NGL ”…””}”(j¶jˆ jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`.txyz2`”j§]”j±Œ.txyz2”…””}”(j¶j jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jˆ ubj±ŒZ files without a reference frame explicitly in the file name are the latest IGS14 version.”…””}”(j¶jˆ jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKÉj¶j„ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKÉj¶j~ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j` ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÉj¶j] ubje)”}”(j¦Œg:program:`displace` * Updated Makefile, grid calculations and added tensile component to calculations. ”j§]”(je)”}”(j¦Œ:program:`displace`”j§]”jj)”}”(j¦jÉ j§]”j±Œdisplace”…””}”(j¶jË jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÇ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÌj¶jà ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒQUpdated Makefile, grid calculations and added tensile component to calculations. ”j§]”j`)”}”(j¦ŒPUpdated Makefile, grid calculations and added tensile component to calculations.”j§]”j±ŒPUpdated Makefile, grid calculations and added tensile component to calculations.”…””}”(j¶jè jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKÌj¶jä ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶já ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKÌj¶jÞ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jà ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÌj¶j] ubje)”}”(j¦Œ‚:file:`gen_util/name_to_block.f` * Changes BLOCK III to BLOCK IIIA so that correct satellite number is assigned to the new PRN03. ”j§]”(je)”}”(j¦Œ :file:`gen_util/name_to_block.f`”j§]”j˜)”}”(j¦j j§]”j±Œgen_util/name_to_block.f”…””}”(j¶j jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÏj¶j ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ_Changes BLOCK III to BLOCK IIIA so that correct satellite number is assigned to the new PRN03. ”j§]”j`)”}”(j¦Œ^Changes BLOCK III to BLOCK IIIA so that correct satellite number is assigned to the new PRN03.”j§]”j±Œ^Changes BLOCK III to BLOCK IIIA so that correct satellite number is assigned to the new PRN03.”…””}”(j¶j6 jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKÏj¶j2 ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j/ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKÏj¶j, ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÏj¶j] ubje)”}”(j¦Œ…:file:`gen_util/real_stats.f` * Updated dimensioning and bounds checking. Very long time series could cause segmentation violations. ”j§]”(je)”}”(j¦Œ:file:`gen_util/real_stats.f`”j§]”j˜)”}”(j¦jb j§]”j±Œgen_util/real_stats.f”…””}”(j¶jd jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j` ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÒj¶j\ ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒeUpdated dimensioning and bounds checking. Very long time series could cause segmentation violations. ”j§]”j`)”}”(j¦ŒdUpdated dimensioning and bounds checking. Very long time series could cause segmentation violations.”j§]”j±ŒdUpdated dimensioning and bounds checking. Very long time series could cause segmentation violations.”…””}”(j¶j„ jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKÒj¶j€ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j} ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKÒj¶jz ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j\ ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÒj¶j] ubje)”}”(j¦Œ†:file:`gen_util/sp3_lib.f`, :file:`includes/sp3_def.h` * Updated maximum number of nadir angles values and added a dimensioning test. ”j§]”(je)”}”(j¦Œ6:file:`gen_util/sp3_lib.f`, :file:`includes/sp3_def.h`”j§]”(j˜)”}”(j¦Œ:file:`gen_util/sp3_lib.f`”j§]”j±Œgen_util/sp3_lib.f”…””}”(j¶j² jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j® ubj±Œ, ”…””}”(j¶j® jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`includes/sp3_def.h`”j§]”j±Œincludes/sp3_def.h”…””}”(j¶jÇ jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j® ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÕj¶jª ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒMUpdated maximum number of nadir angles values and added a dimensioning test. ”j§]”j`)”}”(j¦ŒLUpdated maximum number of nadir angles values and added a dimensioning test.”j§]”j±ŒLUpdated maximum number of nadir angles values and added a dimensioning test.”…””}”(j¶jè jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKÕj¶jä ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶já ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKÕj¶jÞ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jª ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÕj¶j] ubje)”}”(j¦ŒÅ:file:`gen_util/sp3_lib.f` * Fixed bug in :content:`report_stat` call that is invoked in updated :file:`sp3_def.h` is not used. * Increased max nadir values to 41 for Galileo chamber calibrations. ”j§]”(je)”}”(j¦Œ:file:`gen_util/sp3_lib.f`”j§]”j˜)”}”(j¦j j§]”j±Œgen_util/sp3_lib.f”…””}”(j¶j jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÙj¶j ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”(j˜)”}”(j¦ŒbFixed bug in :content:`report_stat` call that is invoked in updated :file:`sp3_def.h` is not used.”j§]”j`)”}”(j¦j4 j§]”(j±Œ Fixed bug in ”…””}”(j¶j6 jÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`report_stat`”j§]”j±Œ report_stat”…””}”(j¶j= jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j6 ubj±Œ! call that is invoked in updated ”…””}”(j¶j6 jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`sp3_def.h`”j§]”j±Œ sp3_def.h”…””}”(j¶jP jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j6 ubj±Œ is not used.”…””}”(j¶j6 jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKØj¶j2 ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j/ ubj˜)”}”(j¦ŒCIncreased max nadir values to 41 for Galileo chamber calibrations. ”j§]”j`)”}”(j¦ŒBIncreased max nadir values to 41 for Galileo chamber calibrations.”j§]”j±ŒBIncreased max nadir values to 41 for Galileo chamber calibrations.”…””}”(j¶ju jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKÙj¶jq ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j/ ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKØj¶j, ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÙj¶j] ubje)”}”(j¦Œb:file:`globk/read_glb_mar.f` * Critical update needed to make the :content:`SOURCE` command work. ”j§]”(je)”}”(j¦Œ:file:`globk/read_glb_mar.f`”j§]”j˜)”}”(j¦j¡ j§]”j±Œglobk/read_glb_mar.f”…””}”(j¶j£ jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŸ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÜj¶j› ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒCCritical update needed to make the :content:`SOURCE` command work. ”j§]”j`)”}”(j¦ŒBCritical update needed to make the :content:`SOURCE` command work.”j§]”(j±Œ#Critical update needed to make the ”…””}”(j¶jà jÇj*ñhNjÆNubj˜)”}”(j¦Œ:content:`SOURCE`”j§]”j±ŒSOURCE”…””}”(j¶jË jÇj*ñhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jà ubj±Œ command work.”…””}”(j¶jà jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKÜj¶j¿ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j¼ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKÜj¶j¹ ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j› ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKÜj¶j] ubje)”}”(j¦ŒZ:file:`glout/write_iers.f` * Updated formats to allow more than 99 reference frame sites. ”j§]”(je)”}”(j¦Œ:file:`glout/write_iers.f`”j§]”j˜)”}”(j¦jj§]”j±Œglout/write_iers.f”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKßj¶jü ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ=Updated formats to allow more than 99 reference frame sites. ”j§]”j`)”}”(j¦Œ`_. :file:`hi.dat` * Added TRM159800.00 antenna. :file:`igs_metadata.snx` * Added from http://mgex.igs.org/ (currently :file:`igs_metadata_2091.snx`, as of the date of this release) and augmented with a bespoke block for the yaw of each satellite, currently read from :file:`tables/svnav.dat` with some assumptions for some satellites and systems. :file:`rcvant.dat` * Fully updated to match IGS codes for all receivers and antennas, following ftp://igs.org/pub/station/general/rcvr_ant.tab. * Records of other known antennas, from the old :file:`rcvant.dat` and those in the NGS ANTEX file (see description of :file:`antmod.dat`, above), are added. * The 14th character, indicating support for the receiver or antenna in GAMIT, is updated to identify the source of antenna calibration. See header for more information. :file:`svnav.dat` * Metadata for GLONASS (R), Galileo (E), Beidou (C), IRNSS (I) and QZSS (J) fully updated to match :file:`tables/igs_metadata.snx` (from http://mgex.igs.org/), which will ultimately supercede :file:`tables/svnav.dat`; metadata for GPS assumed to be good (will be verified ultimately). :file:`otlcmc.dat` * Replaced the provisional center-of-mass corrections for FES2012 with new official ones from H. G. Scherneck. The differences are less than 0.05 mm. ”j§]”j e)”}”(j¦hoj§]”(je)”}”(j¦Œ}:file:`luntab.2020.J2000`, :file:`soltab.2020.J2000`, :file:`nutabl.2020` * Added luni-solar tables for 2020 from JPL DE200. ”j§]”(je)”}”(j¦ŒI:file:`luntab.2020.J2000`, :file:`soltab.2020.J2000`, :file:`nutabl.2020`”j§]”(j˜)”}”(j¦Œ:file:`luntab.2020.J2000`”j§]”j±Œluntab.2020.J2000”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŒubj±Œ, ”…””}”(j¶jŒjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`soltab.2020.J2000`”j§]”j±Œsoltab.2020.J2000”…””}”(j¶j¥jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŒubj±Œ, ”…””}”j¶jŒsbj˜)”}”(j¦Œ:file:`nutabl.2020`”j§]”j±Œ nutabl.2020”…””}”(j¶jºjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŒubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKõj¶jˆubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ1Added luni-solar tables for 2020 from JPL DE200. ”j§]”j`)”}”(j¦Œ0Added luni-solar tables for 2020 from JPL DE200.”j§]”j±Œ0Added luni-solar tables for 2020 from JPL DE200.”…””}”(j¶jÛjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKõj¶j×ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÔubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆKõj¶jÑubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jˆubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKõj¶j…ubje)”}”(j¦XÑ:file:`antmod.dat` * Now linked to an IGS14 rather than IGS08 ANTEX file, which is no longer updated by the IGS for new launches. As noted in relnote.10.61, this will create a 2--3 mm discontinuity in height for all antennas and 5--10 mm discontinuities in horizontal and height for about 20 antennas. * Updated regularly to the latest IGS14 ANTEX file (currently :file:`igs14_2091.atx`, as of the date of this release). * Linked from 2019-10-10 (GPS week 2074) onwards to the IGS14 ANTEX file supplemented with calibrations provided by the National Geodetic Survey (NGS) (currently :file:`ngs14_2091.atx`), plus some additional entries copied from similar records to accommodate antennas without any official calibrations. :file:`tables/antmod.dat` is linked to :file:`tables/ngs14_2091_plus.atx`, at the time of this release. * Updated GLONASS SVs R801, R802, R855, R856, R858 and R859 to match extended IGS designations (K1A, K1B and M+) in :file:`tables/igs_metadata.snx`. ”j§]”(je)”}”(j¦Œ:file:`antmod.dat`”j§]”j˜)”}”(j¦jj§]”j±Œ antmod.dat”…””}”(j¶j jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆKûj¶jubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”(j˜)”}”(j¦XNow linked to an IGS14 rather than IGS08 ANTEX file, which is no longer updated by the IGS for new launches. As noted in relnote.10.61, this will create a 2--3 mm discontinuity in height for all antennas and 5--10 mm discontinuities in horizontal and height for about 20 antennas.”j§]”j`)”}”(j¦j'j§]”j±XNow linked to an IGS14 rather than IGS08 ANTEX file, which is no longer updated by the IGS for new launches. As noted in relnote.10.61, this will create a 2–3 mm discontinuity in height for all antennas and 5–10 mm discontinuities in horizontal and height for about 20 antennas.”…””}”(j¶j)jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆKøj¶j%ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j"ubj˜)”}”(j¦ŒtUpdated regularly to the latest IGS14 ANTEX file (currently :file:`igs14_2091.atx`, as of the date of this release).”j§]”j`)”}”(j¦j>j§]”(j±Œ`_. ”j§]”(je)”}”(j¦Œ:file:`leap.sec`”j§]”j˜)”}”(j¦j j§]”j±Œleap.sec”…””}”(j¶j¢jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jžubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆM j¶jšubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ§Extended limit of table to 31 December 2020 with no additional leap seconds, following to `IERS Bulletin C 59 `_. ”j§]”j`)”}”(j¦Œ¦Extended limit of table to 31 December 2020 with no additional leap seconds, following to `IERS Bulletin C 59 `_.”j§]”(j±ŒZExtended limit of table to 31 December 2020 with no additional leap seconds, following to ”…””}”(j¶jÂjÇj*ñhNjÆNubj÷ )”}”(j¦ŒK`IERS Bulletin C 59 `_”j§]”j±ŒIERS Bulletin C 59”…””}”(j¶jÊjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒIERS Bulletin C 59”j Œ3https://hpiers.obspm.fr/eoppc/bul/bulc/bulletinc.59”ujÄjö j¶jÂubje)”}”(j¦Œ6 ”j§]”j·}”(j¹]”Œiers-bulletin-c-59”aj»]”j½]”Œiers bulletin c 59”ajÀ]”jÂ]”Œrefuri”jÚujÄjdj Kj¶jÂubj±Œ.”…””}”(j¶jÂjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆM j¶j¾ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j»ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆM j¶j¸ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jšubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆM j¶j…ubje)”}”(j¦Œ-:file:`hi.dat` * Added TRM159800.00 antenna. ”j§]”(je)”}”(j¦Œ:file:`hi.dat`”j§]”j˜)”}”(j¦jj§]”j±Œhi.dat”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆM j¶j ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦ŒAdded TRM159800.00 antenna. ”j§]”j`)”}”(j¦ŒAdded TRM159800.00 antenna.”j§]”j±ŒAdded TRM159800.00 antenna.”…””}”(j¶j2jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆM j¶j.ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j+ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆM j¶j(ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆM j¶j…ubje)”}”(j¦X+:file:`igs_metadata.snx` * Added from http://mgex.igs.org/ (currently :file:`igs_metadata_2091.snx`, as of the date of this release) and augmented with a bespoke block for the yaw of each satellite, currently read from :file:`tables/svnav.dat` with some assumptions for some satellites and systems. ”j§]”(je)”}”(j¦Œ:file:`igs_metadata.snx`”j§]”j˜)”}”(j¦j^j§]”j±Œigs_metadata.snx”…””}”(j¶j`jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j\ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆMj¶jXubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦XAdded from http://mgex.igs.org/ (currently :file:`igs_metadata_2091.snx`, as of the date of this release) and augmented with a bespoke block for the yaw of each satellite, currently read from :file:`tables/svnav.dat` with some assumptions for some satellites and systems. ”j§]”j`)”}”(j¦XAdded from http://mgex.igs.org/ (currently :file:`igs_metadata_2091.snx`, as of the date of this release) and augmented with a bespoke block for the yaw of each satellite, currently read from :file:`tables/svnav.dat` with some assumptions for some satellites and systems.”j§]”(j±Œ Added from ”…””}”(j¶j€jÇj*ñhNjÆNubj÷ )”}”(j¦Œhttp://mgex.igs.org/”j§]”j±Œhttp://mgex.igs.org/”…””}”(j¶jˆjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jŠujÄjö j¶j€ubj±Œ (currently ”…””}”(j¶j€jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`igs_metadata_2091.snx`”j§]”j±Œigs_metadata_2091.snx”…””}”(j¶j›jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j€ubj±Œx, as of the date of this release) and augmented with a bespoke block for the yaw of each satellite, currently read from ”…””}”(j¶j€jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/svnav.dat`”j§]”j±Œtables/svnav.dat”…””}”(j¶j°jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j€ubj±Œ7 with some assumptions for some satellites and systems.”…””}”(j¶j€jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆMj¶j|ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jyubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆMj¶jvubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jXubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆMj¶j…ubje)”}”(j¦XØ:file:`rcvant.dat` * Fully updated to match IGS codes for all receivers and antennas, following ftp://igs.org/pub/station/general/rcvr_ant.tab. * Records of other known antennas, from the old :file:`rcvant.dat` and those in the NGS ANTEX file (see description of :file:`antmod.dat`, above), are added. * The 14th character, indicating support for the receiver or antenna in GAMIT, is updated to identify the source of antenna calibration. See header for more information. ”j§]”(je)”}”(j¦Œ:file:`rcvant.dat`”j§]”j˜)”}”(j¦jéj§]”j±Œ rcvant.dat”…””}”(j¶jëjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jçubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆMj¶jãubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”(j˜)”}”(j¦ŒzFully updated to match IGS codes for all receivers and antennas, following ftp://igs.org/pub/station/general/rcvr_ant.tab.”j§]”j`)”}”(j¦j j§]”(j±ŒKFully updated to match IGS codes for all receivers and antennas, following ”…””}”(j¶j jÇj*ñhNjÆNubj÷ )”}”(j¦Œ.ftp://igs.org/pub/station/general/rcvr_ant.tab”j§]”j±Œ.ftp://igs.org/pub/station/general/rcvr_ant.tab”…””}”(j¶jjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jujÄjö j¶j ubj±Œ.”…””}”(j¶j jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆMj¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jubj˜)”}”(j¦Œ›Records of other known antennas, from the old :file:`rcvant.dat` and those in the NGS ANTEX file (see description of :file:`antmod.dat`, above), are added.”j§]”j`)”}”(j¦j3j§]”(j±Œ.Records of other known antennas, from the old ”…””}”(j¶j5jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`rcvant.dat`”j§]”j±Œ rcvant.dat”…””}”(j¶j<jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j5ubj±Œ5 and those in the NGS ANTEX file (see description of ”…””}”(j¶j5jÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`antmod.dat`”j§]”j±Œ antmod.dat”…””}”(j¶jQjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j5ubj±Œ, above), are added.”…””}”(j¶j5jÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆMj¶j1ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jubj˜)”}”(j¦Œ¨The 14th character, indicating support for the receiver or antenna in GAMIT, is updated to identify the source of antenna calibration. See header for more information. ”j§]”j`)”}”(j¦Œ§The 14th character, indicating support for the receiver or antenna in GAMIT, is updated to identify the source of antenna calibration. See header for more information.”j§]”j±Œ§The 14th character, indicating support for the receiver or antenna in GAMIT, is updated to identify the source of antenna calibration. See header for more information.”…””}”(j¶jvjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆMj¶jrubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆMj¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jãubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆMj¶j…ubje)”}”(j¦X/:file:`svnav.dat` * Metadata for GLONASS (R), Galileo (E), Beidou (C), IRNSS (I) and QZSS (J) fully updated to match :file:`tables/igs_metadata.snx` (from http://mgex.igs.org/), which will ultimately supercede :file:`tables/svnav.dat`; metadata for GPS assumed to be good (will be verified ultimately). ”j§]”(je)”}”(j¦Œ:file:`svnav.dat`”j§]”j˜)”}”(j¦j¢j§]”j±Œ svnav.dat”…””}”(j¶j¤jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆMj¶jœubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦XMetadata for GLONASS (R), Galileo (E), Beidou (C), IRNSS (I) and QZSS (J) fully updated to match :file:`tables/igs_metadata.snx` (from http://mgex.igs.org/), which will ultimately supercede :file:`tables/svnav.dat`; metadata for GPS assumed to be good (will be verified ultimately). ”j§]”j`)”}”(j¦XMetadata for GLONASS (R), Galileo (E), Beidou (C), IRNSS (I) and QZSS (J) fully updated to match :file:`tables/igs_metadata.snx` (from http://mgex.igs.org/), which will ultimately supercede :file:`tables/svnav.dat`; metadata for GPS assumed to be good (will be verified ultimately).”j§]”(j±ŒaMetadata for GLONASS (R), Galileo (E), Beidou (C), IRNSS (I) and QZSS (J) fully updated to match ”…””}”(j¶jÄjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/igs_metadata.snx`”j§]”j±Œtables/igs_metadata.snx”…””}”(j¶jÌjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÄubj±Œ (from ”…””}”(j¶jÄjÇj*ñhNjÆNubj÷ )”}”(j¦Œhttp://mgex.igs.org/”j§]”j±Œhttp://mgex.igs.org/”…””}”(j¶jájÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”jãujÄjö j¶jÄubj±Œ#), which will ultimately supercede ”…””}”(j¶jÄjÇj*ñhNjÆNubj˜)”}”(j¦Œ:file:`tables/svnav.dat`”j§]”j±Œtables/svnav.dat”…””}”(j¶jôjÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÄubj±ŒD; metadata for GPS assumed to be good (will be verified ultimately).”…””}”(j¶jÄjÇj*ñhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆMj¶jÀubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j½ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆMj¶jºubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶jœubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆMj¶j…ubje)”}”(j¦Œ©:file:`otlcmc.dat` * Replaced the provisional center-of-mass corrections for FES2012 with new official ones from H. G. Scherneck. The differences are less than 0.05 mm. ”j§]”(je)”}”(j¦Œ:file:`otlcmc.dat`”j§]”j˜)”}”(j¦j-j§]”j±Œ otlcmc.dat”…””}”(j¶j/jÇj*ñhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j+ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆMj¶j'ubj3e)”}”(j¦hoj§]”j“)”}”(j¦hoj§]”j˜)”}”(j¦Œ”Replaced the provisional center-of-mass corrections for FES2012 with new official ones from H. G. Scherneck. The differences are less than 0.05 mm. ”j§]”j`)”}”(j¦Œ“Replaced the provisional center-of-mass corrections for FES2012 with new official ones from H. G. Scherneck. The differences are less than 0.05 mm.”j§]”j±Œ“Replaced the provisional center-of-mass corrections for FES2012 with new official ones from H. G. Scherneck. The differences are less than 0.05 mm.”…””}”(j¶jOjÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj\ñjÆMj¶jKubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jHubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jåjæujÄj’hj\ñjÆMj¶jEubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj2ej¶j'ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjehj\ñjÆMj¶j…ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj ej¶jubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjEšhj\ñjÆKôj¶j=ûjÇj*ñubje)”}”(j¦Œ.. _relnote.10.71_refs:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒrelnote-10-71-refs”ujÄjdjÆM j¶j=ûjÇj*ñhj\ñubej·}”(j¹]”Œ(summary-of-specific-changes-by-directory”aj»]”j½]”Œ*summary of specific changes (by directory)”ajÀ]”jÂ]”ujÄh_j¶jKñjÇj*ñhj\ñjÆKRubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ References”j§]”j±Œ References”…””}”(j¶j—jÇj*ñhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j”jÇj*ñhj\ñjÆMubj}‹)”}”(j¦hoj§]”j·}”(j¹]”Œid5”aj»]”j½]”jÀ]”jÂ]”Œdocname”jñujÄj|‹j¶j”jÇj*ñhj\ñjÆM"ubej·}”(j¹]”(Œ references”j‹ej»]”j½]”(Œ references”Œrelnote.10.71_refs”ejÀ]”jÂ]”ujÄh_j¶jKñjÇj*ñhj\ñjÆMjÒ }”j¶jsjÔ 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136”…””}”(j¶jæjÇjÔhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jÔjÇjÔubje)”}”(j¦Œ.. _test_gamit2014:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒtest-gamit2014”ujÄjdjÆKj¶jÔjÇjÔhŒJ/chandler/home/floyd/public_html/gg/docs/source/test_install/gamit2014.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(•j¦ŒRepeat Steps 1 and 2 for 2014”j§]”j±ŒRepeat Steps 1 and 2 for 2014”…””}”(j¶jjÇjÔhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jjÇjÔhjjÆKubj`)”}”(j¦Œ%From the :file:`2014/` directory, run”j§]”(j±Œ From the ”…””}”(j¶jjÇjÔhNjÆNubj˜)”}”(j¦Œ :file:`2014/`”j§]”j±Œ2014/”…””}”(j¶jjÇjÔhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ directory, run”…””}”(j¶jjÇjÔhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆKj¶jjÇjÔubj)”}”(j¦Œ$ sh_setup -yr 2014”j§]”j±Œ$ sh_setup -yr 2014”…””}”j¶j5sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjjÆKj¶jjÇjÔubj`)”}”(j¦ŒoIn the :file:`2014/tables/` directory, edit :file:`process.defaults` for the :content:`mailto` variable and run”j§]”(j±ŒIn the ”…””}”(j¶jEjÇjÔhNjÆNubj˜)”}”(j¦Œ:file:`2014/tables/`”j§]”j±Œ 2014/tables/”…””}”(j¶jMjÇjÔhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jEubj±Œ directory, edit ”…””}”(j¶jEjÇjÔhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶jbjÇjÔhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jEubj±Œ for the ”…””}”(j¶jEjÇjÔhNjÆNubj˜)”}”(j¦Œ:content:`mailto`”j§]”j±Œmailto”…””}”(j¶jwjÇjÔhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jEubj±Œ variable and run”…””}”(j¶jEjÇjÔhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆK j¶jjÇjÔubj)”}”(j¦Œ7$ sh_upd_stnfo -l sd $ mv station.info.new station.info”j§]”j±Œ7$ sh_upd_stnfo -l sd $ mv station.info.new station.info”…””}”j¶jsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjjÆKj¶jjÇjÔubj`)”}”(j¦ŒhFrom the :file:`2014/` directory, run GAMIT for two days (days-of-year 113 and 114) for GPS and GLONASS:”j§]”(j±Œ From the ”…””}”(j¶j jÇjÔhNjÆNubj˜)”}”(j¦Œ :file:`2014/`”j§]”j±Œ2014/”…””}”(j¶j¨jÇjÔhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j ubj±ŒR directory, run GAMIT for two days (days-of-year 113 and 114) for GPS and GLONASS:”…””}”(j¶j jÇjÔhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆKj¶jjÇjÔubj)”}”(j¦Œñ$ sh_gamit -expt eura -gnss G -s 2014 113 114 -pres ELEV -orbit igsf -copt x k p -dopts c ao >& sh_gamit_2014G.log $ sh_gamit -expt eura -gnss R -s 2014 113 114 -jclock sp3 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2014R.log”j§]”j±Œñ$ sh_gamit -expt eura -gnss G -s 2014 113 114 -pres ELEV -orbit igsf -copt x k p -dopts c ao >& sh_gamit_2014G.log $ sh_gamit -expt eura -gnss R -s 2014 113 114 -jclock sp3 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2014R.log”…””}”j¶jÃsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjjÆKj¶jjÇjÔubj`)”}”(j¦ŒaThen copy (and optionally edit) the :program:`globk` and :program:`glorg` command file templates:”j§]”(j±Œ$Then copy (and optionally edit) the ”…””}”(j¶jÓjÇjÔhNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jÛjÇjÔhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓubj±Œ and ”…””}”(j¶jÓjÇjÔhNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jíjÇjÔhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jÓubj±Œ command file templates:”…””}”(j¶jÓjÇjÔhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆKj¶jjÇjÔubj)”}”(j¦Œ$ sh_glred -cmd”j§]”j±Œ$ sh_glred -cmd”…””}”j¶jsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjjÆKj¶jjÇjÔubj`)”}”(j¦Œ*Finally run GLOBK to generate time series:”j§]”j±Œ*Finally run GLOBK to generate time series:”…””}”(j¶jjÇjÔhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆK j¶jjÇjÔubj)”}”(j¦ŒV$ sh_glred -s 2014 113 2014 114 -expt eura -netext G R -opt H G T >& sh_glred_2014.log”j§]”j±ŒV$ sh_glred -s 2014 113 2014 114 -expt eura -netext G R -opt H G T >& sh_glred_2014.log”…””}”j¶j#sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjjÆK"j¶jjÇjÔubj`)”}”(j¦Œ8and a combined binary h-file for the two processed days:”j§]”j±Œ8and a combined binary h-file for the two processed days:”…””}”(j¶j3jÇjÔhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆK&j¶jjÇjÔubj)”}”(j¦Œr$ sh_glred -s 2014 113 2014 114 -expt eura -netext G R -ncomb 2 -globk_cmd_prefix COMB -opt G >& sh_glred_comb.log”j§]”j±Œr$ sh_glred -s 2014 113 2014 114 -expt eura -netext G R -ncomb 2 -globk_cmd_prefix COMB -opt G >& sh_glred_comb.log”…””}”j¶jAsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjjÆK(j¶jjÇjÔubj`)”}”(j¦ŒÚWe've specified only 2 days in 2014 to save run time for the test. We included only GPS and GLONASS for 2014 since there were too few Beidou and Galileo satellites available at that time to obtain an accurate solution.”j§]”j±ŒÜWe’ve specified only 2 days in 2014 to save run time for the test. We included only GPS and GLONASS for 2014 since there were too few Beidou and Galileo satellites available at that time to obtain an accurate solution.”…””}”(j¶jQjÇjÔhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjjÆK,j¶jjÇjÔubej·}”(j¹]”(Œrepeat-steps-1-and-2-for-2014”jÿej»]”j½]”(Œrepeat steps 1 and 2 for 2014”Œtest_gamit2014”ejÀ]”jÂ]”ujÄh_j¶jÔjÇjÔhjjÆKjÒ }”jejõsjÔ }”jÿjõsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jãj×jòjæuj_}”(Œrel”jãŒdate”jòujc}”je}”jÿ]”jõasjg}”(jejÿjdjauji}”(jeˆjd‰uj¹}”(jÿjjajujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ4Hyperlink target "test-gamit2014" is not referenced.”…””}”j¶jsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jŒubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jŒline”KujÄjø ubajˆNj‰]”j‹NjÇjÔubjój£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jªsbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j§jÇj§ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j¹jÇj§hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j§jÇj§ubje)”}”(j¦Œ.. _test_gamit2016:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒtest-gamit2016”ujÄjdjÆKj¶j§jÇj§hŒJ/chandler/home/floyd/public_html/gg/docs/source/test_install/gamit2016.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒRepeat Steps 1 and 2 for 2016”j§]”j±ŒRepeat Steps 1 and 2 for 2016”…””}”(j¶j×jÇj§hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶jÔjÇj§hjÓjÆKubj`)”}”(j¦Œ%From the :file:`2016/` directory, run”j§]”(j±Œ From the ”…””}”(j¶jåjÇj§hNjÆNubj˜)”}”(j¦Œ :file:`2016/`”j§]”j±Œ2016/”…””}”(j¶jíjÇj§hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jåubj±Œ directory, run”…””}”(j¶jåjÇj§hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÓjÆKj¶jÔjÇj§ubj)”}”(j¦Œ$ sh_setup -yr 2016”j§]”j±Œ$ sh_setup -yr 2016”…””}”j¶jsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÓjÆKj¶jÔjÇj§ubj`)”}”(j¦ŒoIn the :file:`2016/tables/` directory, edit :file:`process.defaults` for the :content:`mailto` variable and run”j§]”(j±ŒIn the ”…””}”(j¶jjÇj§hNjÆNubj˜)”}”(j¦Œ:file:`2016/tables/`”j§]”j±Œ 2016/tables/”…””}”(j¶j jÇj§hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ directory, edit ”…””}”(j¶jjÇj§hNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶j5jÇj§hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ for the ”…””}”(j¶jjÇj§hNjÆNubj˜)”}”(j¦Œ:content:`mailto`”j§]”j±Œmailto”…””}”(j¶jJjÇj§hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jubj±Œ variable and run”…””}”(j¶jjÇj§hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÓjÆK j¶jÔjÇj§ubj)”}”(j¦Œ7$ sh_upd_stnfo -l sd $ mv station.info.new station.info”j§]”j±Œ7$ sh_upd_stnfo -l sd $ mv station.info.new station.info”…””}”j¶jcsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÓjÆKj¶jÔjÇj§ubj`)”}”(j¦ŒyFrom the :file:`2016/` directory, run GAMIT for two days (days-of-year 101 and 102) for GPS, GLONASS, Galileo and BeiDou:”j§]”(j±Œ From the ”…””}”(j¶jsjÇj§hNjÆNubj˜)”}”(j¦Œ :file:`2016/`”j§]”j±Œ2016/”…””}”(j¶j{jÇj§hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jsubj±Œc directory, run GAMIT for two days (days-of-year 101 and 102) for GPS, GLONASS, Galileo and BeiDou:”…””}”(j¶jsjÇj§hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÓjÆKj¶jÔjÇj§ubj)”}”(j¦Xà$ sh_gamit -expt eura -gnss G -s 2016 101 102 -pres ELEV -orbit igsf -copt x k p -dopts c ao >& sh_gamit_2016G.log $ sh_gamit -expt eura -gnss R -s 2016 101 102 -jclock sp3 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2016R.log $ sh_gamit -expt eura -gnss E -s 2016 101 102 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2016E.log $ sh_gamit -expt eura -gnss C -lfreq 7 -s 2016 101 102 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2016C.log”j§]”j±Xà$ sh_gamit -expt eura -gnss G -s 2016 101 102 -pres ELEV -orbit igsf -copt x k p -dopts c ao >& sh_gamit_2016G.log $ sh_gamit -expt eura -gnss R -s 2016 101 102 -jclock sp3 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2016R.log $ sh_gamit -expt eura -gnss E -s 2016 101 102 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2016E.log $ sh_gamit -expt eura -gnss C -lfreq 7 -s 2016 101 102 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2016C.log”…””}”j¶j–sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÓjÆKj¶jÔjÇj§ubj`)”}”(j¦ŒaThen copy (and optionally edit) the :program:`globk` and :program:`glorg` command file templates:”j§]”(j±Œ$Then copy (and optionally edit) the ”…””}”(j¶j¦jÇj§hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j®jÇj§hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¦ubj±Œ and ”…””}”(j¶j¦jÇj§hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jÀjÇj§hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¦ubj±Œ command file templates:”…””}”(j¶j¦jÇj§hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÓjÆKj¶jÔjÇj§ubj)”}”(j¦Œ$ sh_glred -cmd”j§]”j±Œ$ sh_glred -cmd”…””}”j¶jØsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÓjÆKj¶jÔjÇj§ubj`)”}”(j¦Œ*Finally run GLOBK to generate time series:”j§]”j±Œ*Finally run GLOBK to generate time series:”…””}”(j¶jèjÇj§hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÓjÆK"j¶jÔjÇj§ubj)”}”(j¦ŒZ$ sh_glred -s 2016 101 2016 102 -expt eura -netext G R E C -opt H G T >& sh_glred_2016.log”j§]”j±ŒZ$ sh_glred -s 2016 101 2016 102 -expt eura -netext G R E C -opt H G T >& sh_glred_2016.log”…””}”j¶jösbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÓjÆK$j¶jÔjÇj§ubj`)”}”(j¦Œ8and a combined binary h-file for the two processed days:”j§]”j±Œ8and a combined binary h-file for the two processed days:”…””}”(j¶jjÇj§hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÓjÆK(j¶jÔjÇj§ubj)”}”(j¦Œv$ sh_glred -s 2016 101 2016 102 -expt eura -netext G R E C -ncomb 2 -globk_cmd_prefix COMB -opt G >& sh_glred_comb.log”j§]”j±Œv$ sh_glred -s 2016 101 2016 102 -expt eura -netext G R E C -ncomb 2 -globk_cmd_prefix COMB -opt G >& sh_glred_comb.log”…””}”j¶jsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhjÓjÆK*j¶jÔjÇj§ubj`)”}”(j¦ŒBWe've specified only 2 days in 2016 to save run time for the test.”j§]”j±ŒDWe’ve specified only 2 days in 2016 to save run time for the test.”…””}”(j¶j$jÇj§hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hjÓjÆK.j¶jÔjÇj§ubej·}”(j¹]”(Œrepeat-steps-1-and-2-for-2016”jÒej»]”j½]”(Œrepeat steps 1 and 2 for 2016”Œtest_gamit2016”ejÀ]”jÂ]”ujÄh_j¶j§jÇj§hjÓjÆKjÒ }”j8jÈsjÔ }”jÒjÈsubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”jÓj}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMjÓjNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j¶jªjÅj¹uj_}”(Œrel”j¶Œdate”jÅujc}”je}”jÒ]”jÈasjg}”(j8jÒj7j4uji}”(j8ˆj7‰uj¹}”(jÒjÔj4jÔujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ4Hyperlink target "test-gamit2016" is not referenced.”…””}”j¶jbsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j_ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”jÓŒline”KujÄjø ubajˆNj‰]”j‹NjÇj§ubjíj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j}sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jzjÇjzubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jŒjÇjzhNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jzjÇjzubje)”}”(j¦Œ.. _test_gamit2018:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒtest-gamit2018”ujÄjdjÆKj¶jzjÇjzhŒJ/chandler/home/floyd/public_html/gg/docs/source/test_install/gamit2018.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ Run GAMIT for three days in 2018”j§]”j±Œ Run GAMIT for three days in 2018”…””}”(j¶jªjÇjzhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j§jÇjzhj¦jÆKubj`)”}”(j¦Œ0In the :file:`test_install/2018/` directory type”j§]”(j±ŒIn the ”…””}”(j¶j¸jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`test_install/2018/`”j§]”j±Œtest_install/2018/”…””}”(j¶jÀjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¸ubj±Œ directory type”…””}”(j¶j¸jÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆKj¶j§jÇjzubj)”}”(j¦Œ$ sh_setup -yr 2018”j§]”j±Œ$ sh_setup -yr 2018”…””}”j¶jÛsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj¦jÆKj¶j§jÇjzubj©Œ container”“”)”}”(j¦hoj§]”(j©Œrubric”“”)”}”(j¦ŒWhat did this command do?”j§]”j±ŒWhat did this command do?”…””}”(j¶jòjÇjzhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjðj¶jíhj¦jÆKubj`)”}”(j¦XhYou should notice that a :file:`tables/` sub-directory was created, which contains copies of several critical files, most generic but some specific to the year, from the main :file:`~/gg/tables/` directory. You may wish to edit some of these files to suit your needs to process your experiment. Take a look at what was generated, e.g. :console:`ls -l tables/`.”j§]”(j±ŒYou should notice that a ”…””}”(j¶jjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ‡ sub-directory was created, which contains copies of several critical files, most generic but some specific to the year, from the main ”…””}”(j¶jjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±ŒŒ directory. You may wish to edit some of these files to suit your needs to process your experiment. Take a look at what was generated, e.g. ”…””}”(j¶jjÇjzhNjÆNubj˜)”}”(j¦Œ:console:`ls -l tables/`”j§]”j±Œ ls -l tables/”…””}”(j¶j2jÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶jubj±Œ.”…””}”(j¶jjÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆKj¶jíubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œis_div”ˆŒdesign_component”Œdropdown”Œopened”‰Œtype”jSŒ has_title”ˆŒicon”Œquestion”Œcontainer_classes”]”Œsd-mb-3”aŒ title_classes”]”(Œ sd-bg-warning”Œsd-bg-text-warning”eŒ body_classes”]”ujÄjëhj¦jÆK j¶j§jÇjzubj`)”}”(j¦X·The :file:`2018/tables/` directory will now contain links to most standard files in :file:`~/gg/tables/` and copies of these files for :file:`process.defaults`, :file:`sestbl.`, :file:`station.info` (complete MIT version), and :file:`autcln.cmd`. The :file:`sites.defaults` file was written for this test (ordinarily one would construct this station list) and already in the directory, and therefore not overwritten by :program:`sh_setup`.”j§]”(j±ŒThe ”…””}”(j¶jbjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`2018/tables/`”j§]”j±Œ 2018/tables/”…””}”(j¶jjjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jbubj±Œ< directory will now contain links to most standard files in ”…””}”(j¶jbjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jbubj±Œ and copies of these files for ”…””}”(j¶jbjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`process.defaults`”j§]”j±Œprocess.defaults”…””}”(j¶j”jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jbubj±Œ, ”…””}”(j¶jbjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶j©jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jbubj±Œ, ”…””}”j¶jbsbj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j¾jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jbubj±Œ (complete MIT version), and ”…””}”(j¶jbjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`autcln.cmd`”j§]”j±Œ autcln.cmd”…””}”(j¶jÓjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jbubj±Œ. The ”…””}”(j¶jbjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jèjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jbubj±Œ’ file was written for this test (ordinarily one would construct this station list) and already in the directory, and therefore not overwritten by ”…””}”(j¶jbjÇjzhNjÆNubjj)”}”(j¦Œ:program:`sh_setup`”j§]”j±Œsh_setup”…””}”(j¶jýjÇjzhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jbubj±Œ.”…””}”(j¶jbjÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆKj¶j§jÇjzubj`)”}”(j¦XêExamine :file:`tables/sites.defaults` to note that it has been set up to download from a remote archive (CDDIS by default) RINEX files for ten IGS stations and :content:`xstinfo` is set to avoid any automatic update of :file:`station.info` during processing. Note also that the :file:`sittbl.` copied from :file:`~/gg/tables/` is set up to impose moderate constraints on IGS core stations to support ambiguity resolution in GAMIT; the four included in test_install are more than sufficient.”j§]”(j±ŒExamine ”…””}”(j¶jjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`tables/sites.defaults`”j§]”j±Œtables/sites.defaults”…””}”(j¶jjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ{ to note that it has been set up to download from a remote archive (CDDIS by default) RINEX files for ten IGS stations and ”…””}”(j¶jjÇjzhNjÆNubj˜)”}”(j¦Œ:content:`xstinfo`”j§]”j±Œxstinfo”…””}”(j¶j2jÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jubj±Œ) is set to avoid any automatic update of ”…””}”(j¶jjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jEjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ' during processing. Note also that the ”…””}”(j¶jjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`sittbl.`”j§]”j±Œsittbl.”…””}”(j¶jZjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ copied from ”…””}”(j¶jjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶jojÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jubj±Œ¤ is set up to impose moderate constraints on IGS core stations to support ambiguity resolution in GAMIT; the four included in test_install are more than sufficient.”…””}”(j¶jjÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆKj¶j§jÇjzubj`)”}”(j¦X£Edit :file:`tables/process.defaults` to change the :content:`mailto` to your own email address to receive the :program:`sh_gamit` summary file. (If left null, it reverts to :command:`whoami`, so this change may not be needed.) Note that :content:`aprf`, used to initialize the :file:`lfile.` for GAMIT points to :file:`igb14_comb.apr`, which has been copied by :program:`sh_setup` to the :file:`2018/tables/` directory.”j§]”(j±ŒEdit ”…””}”(j¶jŠjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`tables/process.defaults`”j§]”j±Œtables/process.defaults”…””}”(j¶j’jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŠubj±Œ to change the ”…””}”(j¶jŠjÇjzhNjÆNubj˜)”}”(j¦Œ:content:`mailto`”j§]”j±Œmailto”…””}”(j¶j§jÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jŠubj±Œ* to your own email address to receive the ”…””}”(j¶jŠjÇjzhNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶jºjÇjzhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jŠubj±Œ, summary file. (If left null, it reverts to ”…””}”(j¶jŠjÇjzhNjÆNubjj)”}”(j¦Œ:command:`whoami`”j§]”j±Œwhoami”…””}”(j¶jÌjÇjzhNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶jŠubj±Œ/, so this change may not be needed.) Note that ”…””}”(j¶jŠjÇjzhNjÆNubj˜)”}”(j¦Œ:content:`aprf`”j§]”j±Œaprf”…””}”(j¶jÞjÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jŠubj±Œ, used to initialize the ”…””}”(j¶jŠjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`lfile.`”j§]”j±Œlfile.”…””}”(j¶jñjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŠubj±Œ for GAMIT points to ”…””}”(j¶jŠjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`igb14_comb.apr`”j§]”j±Œigb14_comb.apr”…””}”(j¶jjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŠubj±Œ, which has been copied by ”…””}”(j¶jŠjÇjzhNjÆNubjj)”}”(j¦Œ:program:`sh_setup`”j§]”j±Œsh_setup”…””}”(j¶jjÇjzhNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jŠubj±Œ to the ”…””}”(j¶jŠjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`2018/tables/`”j§]”j±Œ 2018/tables/”…””}”(j¶j-jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jŠubj±Œ directory.”…””}”(j¶jŠjÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆKj¶j§jÇjzubj`)”}”(j¦ŒéIf you have not downloaded or copied from an earlier distribution the (large) grid file for ocean tidal loading and do not wish to use it, change :content:`Tides applied` in :file:`tables/sestbl.` from :content:`31` to :content:`23`.”j§]”(j±Œ’If you have not downloaded or copied from an earlier distribution the (large) grid file for ocean tidal loading and do not wish to use it, change ”…””}”(j¶jHjÇjzhNjÆNubj˜)”}”(j¦Œ:content:`Tides applied`”j§]”j±Œ Tides applied”…””}”(j¶jPjÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jHubj±Œ in ”…””}”(j¶jHjÇjzhNjÆNubj˜)”}”(j¦Œ:file:`tables/sestbl.`”j§]”j±Œtables/sestbl.”…””}”(j¶jcjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jHubj±Œ from ”…””}”(j¶jHjÇjzhNjÆNubj˜)”}”(j¦Œ :content:`31`”j§]”j±Œ31”…””}”(j¶jxjÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jHubj±Œ to ”…””}”(j¶jHjÇjzhNjÆNubj˜)”}”(j¦Œ :content:`23`”j§]”j±Œ23”…””}”(j¶j‹jÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jHubj±Œ.”…””}”(j¶jHjÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆKj¶j§jÇjzubj`)”}”(j¦Œ€Construct a small, experiment-specific station.info file by using the following procedure in the :file:`2018/tables/` directory:”j§]”(j±ŒaConstruct a small, experiment-specific station.info file by using the following procedure in the ”…””}”(j¶j¤jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`2018/tables/`”j§]”j±Œ 2018/tables/”…””}”(j¶j¬jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¤ubj±Œ directory:”…””}”(j¶j¤jÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆKj¶j§jÇjzubj)”}”(j¦Œ$ sh_upd_stnfo -l sd”j§]”j±Œ$ sh_upd_stnfo -l sd”…””}”j¶jÇsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj¦jÆK!j¶j§jÇjzubj`)”}”(j¦Xîwill create :file:`station.info.new`, using from the MIT station.info only the sites listed in :file:`sites.defaults`. (This step will take a while since the MIT global :file:`station.info` file is so long.) After checking, rename it to :file:`station.info` (overwriting the no-longer-useful MIT :file:`station.info`). (In your own processing, if you have stations that are not in the MIT :file:`station.info` file, you can add their entries from the RINEX headers by running in :file:`tables/`”j§]”(j±Œ will create ”…””}”(j¶j×jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`station.info.new`”j§]”j±Œstation.info.new”…””}”(j¶jßjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×ubj±Œ;, using from the MIT station.info only the sites listed in ”…””}”(j¶j×jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jôjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×ubj±Œ4. (This step will take a while since the MIT global ”…””}”(j¶j×jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×ubj±Œ0 file is so long.) After checking, rename it to ”…””}”(j¶j×jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×ubj±Œ' (overwriting the no-longer-useful MIT ”…””}”(j¶j×jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶j3jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×ubj±ŒI). (In your own processing, if you have stations that are not in the MIT ”…””}”(j¶j×jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`station.info`”j§]”j±Œ station.info”…””}”(j¶jHjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×ubj±ŒF file, you can add their entries from the RINEX headers by running in ”…””}”(j¶j×jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶j]jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j×ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆK%j¶j§jÇjzubj)”}”(j¦Œ$$ sh_upd_stnfo -files ../rinex/*.18o”j§]”j±Œ$$ sh_upd_stnfo -files ../rinex/*.18o”…””}”j¶jtsbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj¦jÆK*j¶j§jÇjzubj`)”}”(j¦Œv(See :numref:`intro_proc_example` of :doc:`/intro/index` for what to do if the RINEX header entries are non-standard.)”j§]”(j±Œ(See ”…””}”(j¶j„jÇjzhNjÆNubj’)”}”(j¦Œ:numref:`intro_proc_example`”j§]”j˜)”}”(j¦jŽj§]”j±Œintro_proc_example”…””}”(j¶jjÇjzhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-numref”ej½]”jÀ]”jÂ]”ujÄj—j¶jŒubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jíŒ refdomain”jšŒreftype”Œnumref”Œ refexplicit”‰Œrefwarn”ˆj¶Œintro_proc_example”ujÄj‘hj¦jÆK.j¶j„ubj±Œ of ”…””}”(j¶j„jÇjzhNjÆNubj’)”}”(j¦Œ:doc:`/intro/index`”j§]”j)”}”(j¦j²j§]”j±Œ /intro/index”…””}”(j¶j´jÇjzhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-doc”ej½]”jÀ]”jÂ]”ujÄj*j¶j°ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jíŒ refdomain”j¾Œreftype”Œdoc”Œ refexplicit”‰Œrefwarn”ˆj¶Œ /intro/index”ujÄj‘hj¦jÆK.j¶j„ubj±Œ> for what to do if the RINEX header entries are non-standard.)”…””}”(j¶j„jÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆK.j¶j§jÇjzubj`)”}”(j¦X%GAMIT currently supports processing of each GNSS separately, with the day directories for each created with a single-letter added to designate the system, e.g. :file:`095G/`, :file:`095R/`, :file:`095E/`, :file:`095C/`. If you wish to test full GNSS capability, type at the :file:`2018/` level”j§]”(j±Œ GAMIT currently supports processing of each GNSS separately, with the day directories for each created with a single-letter added to designate the system, e.g. ”…””}”(j¶jÚjÇjzhNjÆNubj˜)”}”(j¦Œ :file:`095G/`”j§]”j±Œ095G/”…””}”(j¶jâjÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÚubj±Œ, ”…””}”(j¶jÚjÇjzhNjÆNubj˜)”}”(j¦Œ :file:`095R/`”j§]”j±Œ095R/”…””}”(j¶j÷jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÚubj±Œ, ”…””}”j¶jÚsbj˜)”}”(j¦Œ :file:`095E/`”j§]”j±Œ095E/”…””}”(j¶j jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÚubj±Œ, ”…””}”j¶jÚsbj˜)”}”(j¦Œ :file:`095C/`”j§]”j±Œ095C/”…””}”(j¶j! jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÚubj±Œ8. If you wish to test full GNSS capability, type at the ”…””}”(j¶jÚjÇjzhNjÆNubj˜)”}”(j¦Œ :file:`2018/`”j§]”j±Œ2018/”…””}”(j¶j6 jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jÚubj±Œ level”…””}”(j¶jÚjÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆK0j¶j§jÇjzubj)”}”(j¦XÚ$ sh_gamit -expt eura -gnss G -s 2018 095 097 -pres ELEV -orbit igsf -copt x k p -dopts c ao >& sh_gamit_2018G.log sh_gamit -expt eura -gnss R -s 2018 095 097 -jclock sp3 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2018R.log sh_gamit -expt eura -gnss E -s 2018 095 097 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2018E.log sh_gamit -expt eura -gnss C -lfreq 7 -s 2018 095 097 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2018C.log”j§]”j±XÚ$ sh_gamit -expt eura -gnss G -s 2018 095 097 -pres ELEV -orbit igsf -copt x k p -dopts c ao >& sh_gamit_2018G.log sh_gamit -expt eura -gnss R -s 2018 095 097 -jclock sp3 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2018R.log sh_gamit -expt eura -gnss E -s 2018 095 097 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2018E.log sh_gamit -expt eura -gnss C -lfreq 7 -s 2018 095 097 -pres ELEV -orbit codm -copt x k p -dopts c ao >& sh_gamit_2018C.log”…””}”j¶jQ sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj¦jÆK3j¶j§jÇjzubj`)”}”(j¦Œ‡For GPS-only, execute only the first command and omit the :option:`-gnss` so that the day directory names will be the day-of-year only.”j§]”(j±Œ:For GPS-only, execute only the first command and omit the ”…””}”(j¶ja jÇjzhNjÆNubj’)”}”(j¦Œ:option:`-gnss`”j§]”j˜)”}”(j¦jk j§]”j±Œ-gnss”…””}”(j¶jm jÇjzhNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶ji ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jíŒ refdomain”jw Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶Œ-gnss”ujÄj‘hj¦jÆK:j¶ja ubj±Œ> so that the day directory names will be the day-of-year only.”…””}”(j¶ja jÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆK:j¶j§jÇjzubj`)”}”(j¦XkA summary file should be emailed to you as each day completes execution. Check these files for number of stations (6), postfit RMS (3–15 mm, none 0), postfit NRMS (~ 0.2), ambiguity resolution and coordinate adjustments (< 30 cm). For this large network, the 2018 ambiguity resolution is 80–90% for GPS and Galileo, 40–50% for Beidou, but near zero for GLONASS due to poor orbits), a condition also reflected in the sky plots in the :file:`figs/` directory. Allowing the GLONASS orbits to adjust (:content:`RELAX` mode in the :file:`sestbl.`) will improve the fit signficantly. To view the result of the fit of GAMIT's orbit model to the input orbit, see the RMS files in :file:`igs/`. To view the complete editing statistics see :file:`autcln.prefit.sum` and :file:`autcln.post.sum` in the day directories; for the least-squares adjustment, see :file:`qeuraa.{}`.”j§]”(j±X·A summary file should be emailed to you as each day completes execution. Check these files for number of stations (6), postfit RMS (3–15 mm, none 0), postfit NRMS (~ 0.2), ambiguity resolution and coordinate adjustments (< 30 cm). For this large network, the 2018 ambiguity resolution is 80–90% for GPS and Galileo, 40–50% for Beidou, but near zero for GLONASS due to poor orbits), a condition also reflected in the sky plots in the ”…””}”(j¶j“ jÇjzhNjÆNubj˜)”}”(j¦Œ :file:`figs/`”j§]”j±Œfigs/”…””}”(j¶j› jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j“ ubj±Œ3 directory. Allowing the GLONASS orbits to adjust (”…””}”(j¶j“ jÇjzhNjÆNubj˜)”}”(j¦Œ:content:`RELAX`”j§]”j±ŒRELAX”…””}”(j¶j° jÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j“ ubj±Œ mode in the ”…””}”(j¶j“ jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jà jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j“ ubj±Œ…) will improve the fit signficantly. To view the result of the fit of GAMIT’s orbit model to the input orbit, see the RMS files in ”…””}”(j¶j“ jÇjzhNjÆNubj˜)”}”(j¦Œ :file:`igs/`”j§]”j±Œigs/”…””}”(j¶jØ jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j“ ubj±Œ.. To view the complete editing statistics see ”…””}”(j¶j“ jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`autcln.prefit.sum`”j§]”j±Œautcln.prefit.sum”…””}”(j¶jí jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j“ ubj±Œ and ”…””}”(j¶j“ jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`autcln.post.sum`”j§]”j±Œautcln.post.sum”…””}”(j¶j!jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j“ ubj±Œ? in the day directories; for the least-squares adjustment, see ”…””}”(j¶j“ jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`qeuraa.{}`”j§]”(j±Œqeuraa.”…””}”(j¶j!jÇjzhNjÆNubj )”}”(j¦Œ”j§]”j±Œ”…””}”(j¶j!jÇjzhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j!ubej·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j“ ubj±Œ.”…””}”(j¶j“ jÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆK` (730 Mb). You may, however, substitute the smaller (45 Mb) :download:`otl_CSR4.grid `, or you may turn off ocean tidal loading by setting :content:`Tides applied = 23` and :content:`Use otl.grid = N` in the :file:`sestbl.` (Note that the links to the other grid and list files (:file:`met.grid`, :file:`met.list`, :file:`map.grid`, etc.) can remain empty for running the example and for most processing.”j§]”j`)”}”(j¦X\The example is set up to use ocean tidal loading (:content:`Use otl.grid = Y` in the :file:`sestbl.`), which requires you to have previously downloaded into :file:`~/gg/GRIDS/` an OTL file from ftp://everest.mit.edu/pub/GRIDS/ and to have verify this file is linked to :file:`~/gg/tables/otl.grid`. The IERS/IGS standard model is :download:`otl_FES2004.grid ` (730 Mb). You may, however, substitute the smaller (45 Mb) :download:`otl_CSR4.grid `, or you may turn off ocean tidal loading by setting :content:`Tides applied = 23` and :content:`Use otl.grid = N` in the :file:`sestbl.` (Note that the links to the other grid and list files (:file:`met.grid`, :file:`met.list`, :file:`map.grid`, etc.) can remain empty for running the example and for most processing.”j§]”(j±Œ2The example is set up to use ocean tidal loading (”…””}”(j¶jp"jÇjzhNjÆNubj˜)”}”(j¦Œ:content:`Use otl.grid = Y`”j§]”j±ŒUse otl.grid = Y”…””}”(j¶jx"jÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jp"ubj±Œ in the ”…””}”(j¶jp"jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶j‹"jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jp"ubj±Œ9), which requires you to have previously downloaded into ”…””}”(j¶jp"jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/GRIDS/`”j§]”j±Œ ~/gg/GRIDS/”…””}”(j¶j "jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jp"ubj±Œ an OTL file from ”…””}”(j¶jp"jÇjzhNjÆNubj÷ )”}”(j¦Œ ftp://everest.mit.edu/pub/GRIDS/”j§]”j±Œ ftp://everest.mit.edu/pub/GRIDS/”…””}”(j¶jµ"jÇjzhNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefuri”j·"ujÄjö j¶jp"ubj±Œ+ and to have verify this file is linked to ”…””}”(j¶jp"jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/otl.grid`”j§]”j±Œ~/gg/tables/otl.grid”…””}”(j¶jÈ"jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jp"ubj±Œ!. The IERS/IGS standard model is ”…””}”(j¶jp"jÇjzhNjÆNubj^®)”}”(j¦ŒO:download:`otl_FES2004.grid `”j§]”j˜)”}”(j¦jß"j§]”j±Œotl_FES2004.grid”…””}”(j¶já"jÇjzhNjÆNubaj·}”(j¹]”j»]”(j£Œdownload”ej½]”jÀ]”jÂ]”ujÄj—j¶jÝ"ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jíŒ refdomain”hoŒreftype”jë"Œ refexplicit”ˆŒrefwarn”‰j¶Œ0ftp://everest.mit.edu/pub/GRIDS/otl_FES2004.grid”j jú"ujÄj]®hj¦jÆKSj¶jp"ubj±Œ< (730 Mb). You may, however, substitute the smaller (45 Mb) ”…””}”(j¶jp"jÇjzhNjÆNubj^®)”}”(j¦ŒI:download:`otl_CSR4.grid `”j§]”j˜)”}”(j¦j#j§]”j±Œ otl_CSR4.grid”…””}”(j¶j#jÇjzhNjÆNubaj·}”(j¹]”j»]”(j£Œdownload”ej½]”jÀ]”jÂ]”ujÄj—j¶jÿ"ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jíŒ refdomain”hoŒreftype”j #Œ refexplicit”ˆŒrefwarn”‰j¶Œ-ftp://everest.mit.edu/pub/GRIDS/otl_CSR4.grid”j j#ujÄj]®hj¦jÆKSj¶jp"ubj±Œ5, or you may turn off ocean tidal loading by setting ”…””}”(j¶jp"jÇjzhNjÆNubj˜)”}”(j¦Œ:content:`Tides applied = 23`”j§]”j±ŒTides applied = 23”…””}”(j¶j!#jÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jp"ubj±Œ and ”…””}”(j¶jp"jÇjzhNjÆNubj˜)”}”(j¦Œ:content:`Use otl.grid = N`”j§]”j±ŒUse otl.grid = N”…””}”(j¶j4#jÇjzhNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jp"ubj±Œ in the ”…””}”j¶jp"sbj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jG#jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jp"ubj±Œ8 (Note that the links to the other grid and list files (”…””}”(j¶jp"jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`met.grid`”j§]”j±Œmet.grid”…””}”(j¶j\#jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jp"ubj±Œ, ”…””}”(j¶jp"jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`met.list`”j§]”j±Œmet.list”…””}”(j¶jq#jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jp"ubj±Œ, ”…””}”j¶jp"sbj˜)”}”(j¦Œ:file:`map.grid`”j§]”j±Œmap.grid”…””}”(j¶j†#jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jp"ubj±ŒI, etc.) can remain empty for running the example and for most processing.”…””}”(j¶jp"jÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆKSj¶jl"ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jz!jÇjzhj¦jÆNubj˜)”}”(j¦ŒáIf you want or need to run the example without having internet access while running, you can pre-load the RINEX, navigation, and orbit files into the :file:`rinex/`, :file:`brdc/`, and :file:`igs/` directories, respectively. ”j§]”j`)”}”(j¦ŒàIf you want or need to run the example without having internet access while running, you can pre-load the RINEX, navigation, and orbit files into the :file:`rinex/`, :file:`brdc/`, and :file:`igs/` directories, respectively.”j§]”(j±Œ–If you want or need to run the example without having internet access while running, you can pre-load the RINEX, navigation, and orbit files into the ”…””}”(j¶j«#jÇjzhNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶j³#jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j«#ubj±Œ, ”…””}”(j¶j«#jÇjzhNjÆNubj˜)”}”(j¦Œ :file:`brdc/`”j§]”j±Œbrdc/”…””}”(j¶jÈ#jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j«#ubj±Œ, and ”…””}”(j¶j«#jÇjzhNjÆNubj˜)”}”(j¦Œ :file:`igs/`”j§]”j±Œigs/”…””}”(j¶jÝ#jÇjzhNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j«#ubj±Œ directories, respectively.”…””}”(j¶j«#jÇjzhNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj¦jÆKWj¶j§#ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jz!jÇjzhj¦jÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j“>j”>j•>hoj–>j—>ujÄjW9j¶j§jÇjzhj¦jÆKNubej·}”(j¹]”(Œ run-gamit-for-three-days-in-2018”j¥ej»]”j½]”(Œ run gamit for three days in 2018”Œtest_gamit2018”ejÀ]”jÂ]”ujÄh_j¶jzjÇjzhj¦jÆKjÒ }”j $j›sjÔ }”j¥j›subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j¦j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj¦jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j‰j}j˜jŒuj_}”(Œrel”j‰Œdate”j˜ujc}”je}”(j¥]”j›ajh!]”j^!aujg}”(j $j¥j $j$ju!jh!uji}”(j $ˆj $‰ju!ˆuj¹}”(j¥j§j$j§jh!ji!ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”(jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ4Hyperlink target "test-gamit2018" is not referenced.”…””}”j¶j5$sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j2$ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j¦Œline”KujÄjø ubjù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ:Hyperlink target "test-gamit2018-notes" is not referenced.”…””}”j¶jO$sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jL$ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j¦Œline”KNujÄjø ubejˆNj‰]”j‹NjÇjzubjèj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jj$sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jg$jÇjg$ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jy$jÇjg$hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jg$jÇjg$ubje)”}”(j¦Œ.. _test_globk2018:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒtest-globk2018”ujÄjdjÆKj¶jg$jÇjg$hŒJ/chandler/home/floyd/public_html/gg/docs/source/test_install/globk2018.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒCRun GLOBK to get repeatabilities and a combined H-file for the span”j§]”j±ŒCRun GLOBK to get repeatabilities and a combined H-file for the span”…””}”(j¶j—$jÇjg$hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j”$jÇjg$hj“$jÆKubj`)”}”(j¦Œ!From the :file:`2018/` directory:”j§]”(j±Œ From the ”…””}”(j¶j¥$jÇjg$hNjÆNubj˜)”}”(j¦Œ :file:`2018/`”j§]”j±Œ2018/”…””}”(j¶j­$jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¥$ubj±Œ directory:”…””}”(j¶j¥$jÇjg$hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“$jÆKj¶j”$jÇjg$ubj)”}”(j¦Œ$ sh_glred -cmd”j§]”j±Œ$ sh_glred -cmd”…””}”j¶jÈ$sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj“$jÆKj¶j”$jÇjg$ubj`)”}”(j¦Œvto get the :file:`globk.cmd` and :file:`glorg.cmd` files copied from :file:`~/gg/tables/` to :file:`2018/gsoln/`, then”j§]”(j±Œ to get the ”…””}”(j¶jØ$jÇjg$hNjÆNubj˜)”}”(j¦Œ:file:`globk.cmd`”j§]”j±Œ globk.cmd”…””}”(j¶jà$jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jØ$ubj±Œ and ”…””}”(j¶jØ$jÇjg$hNjÆNubj˜)”}”(j¦Œ:file:`glorg.cmd`”j§]”j±Œ glorg.cmd”…””}”(j¶jõ$jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jØ$ubj±Œ files copied from ”…””}”(j¶jØ$jÇjg$hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶j %jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jØ$ubj±Œ to ”…””}”(j¶jØ$jÇjg$hNjÆNubj˜)”}”(j¦Œ:file:`2018/gsoln/`”j§]”j±Œ 2018/gsoln/”…””}”(j¶j%jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jØ$ubj±Œ, then”…””}”(j¶jØ$jÇjg$hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“$jÆK j¶j”$jÇjg$ubj)”}”(j¦ŒW$ sh_glred -s 2018 095 2018 097 -expt eura -netext G R E C -opt R H G T >& sh_glred.log”j§]”j±ŒW$ sh_glred -s 2018 095 2018 097 -expt eura -netext G R E C -opt R H G T >& sh_glred.log”…””}”j¶j:%sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj“$jÆKj¶j”$jÇjg$ubj`)”}”(j¦XäThe script as commanded will translate the GAMIT plain text h-files in each day directory to GLOBK binary h-files (:file:`.glx`) and put them into the :file:`glbf/` directory (:console:`H` option); create a :file:`.gdl` file for each day listing the h-file, run GLOBK for each day (:console:`G` option) using :file:`globk.cmd` and :file:`glorg.cmd`; and generate time series plots (:console:`T` option using :console:`.pos` files, program :program:`tssum` and :program:`sh_plot_pos`).”j§]”(j±ŒsThe script as commanded will translate the GAMIT plain text h-files in each day directory to GLOBK binary h-files (”…””}”(j¶jJ%jÇjg$hNjÆNubj˜)”}”(j¦Œ :file:`.glx`”j§]”j±Œ.glx”…””}”(j¶jR%jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jJ%ubj±Œ) and put them into the ”…””}”(j¶jJ%jÇjg$hNjÆNubj˜)”}”(j¦Œ :file:`glbf/`”j§]”j±Œglbf/”…””}”(j¶jg%jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jJ%ubj±Œ directory (”…””}”(j¶jJ%jÇjg$hNjÆNubj˜)”}”(j¦Œ :console:`H`”j§]”j±ŒH”…””}”(j¶j|%jÇjg$hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶jJ%ubj±Œ option); create a ”…””}”(j¶jJ%jÇjg$hNjÆNubj˜)”}”(j¦Œ :file:`.gdl`”j§]”j±Œ.gdl”…””}”(j¶j%jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jJ%ubj±Œ? file for each day listing the h-file, run GLOBK for each day (”…””}”(j¶jJ%jÇjg$hNjÆNubj˜)”}”(j¦Œ :console:`G`”j§]”j±ŒG”…””}”(j¶j¤%jÇjg$hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶jJ%ubj±Œ option) using ”…””}”(j¶jJ%jÇjg$hNjÆNubj˜)”}”(j¦Œ:file:`globk.cmd`”j§]”j±Œ globk.cmd”…””}”(j¶j·%jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jJ%ubj±Œ and ”…””}”(j¶jJ%jÇjg$hNjÆNubj˜)”}”(j¦Œ:file:`glorg.cmd`”j§]”j±Œ glorg.cmd”…””}”(j¶jÌ%jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jJ%ubj±Œ"; and generate time series plots (”…””}”(j¶jJ%jÇjg$hNjÆNubj˜)”}”(j¦Œ :console:`T`”j§]”j±ŒT”…””}”(j¶já%jÇjg$hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶jJ%ubj±Œ option using ”…””}”(j¶jJ%jÇjg$hNjÆNubj˜)”}”(j¦Œ:console:`.pos`”j§]”j±Œ.pos”…””}”(j¶jô%jÇjg$hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶jJ%ubj±Œ files, program ”…””}”(j¶jJ%jÇjg$hNjÆNubjj)”}”(j¦Œ:program:`tssum`”j§]”j±Œtssum”…””}”(j¶j&jÇjg$hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jJ%ubj±Œ and ”…””}”j¶jJ%sbjj)”}”(j¦Œ:program:`sh_plot_pos`”j§]”j±Œ sh_plot_pos”…””}”(j¶j&jÇjg$hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jJ%ubj±Œ).”…””}”(j¶jJ%jÇjg$hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“$jÆKj¶j”$jÇjg$ubj`)”}”(j¦X…For this test the :program:`globk`/:program:`glred` and :program:`glorg` command files created in :file:`gsoln/` by :console:`sh_glred -cmd` will work without editing; however, in general there are changes you may need to make, for example, to define the reference frame with translation-only rather than tranlsation and rotation, and to change the list of reference (stabilization) sites.”j§]”(j±ŒFor this test the ”…””}”(j¶j1&jÇjg$hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j9&jÇjg$hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j1&ubj±Œ/”…””}”(j¶j1&jÇjg$hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jK&jÇjg$hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j1&ubj±Œ and ”…””}”(j¶j1&jÇjg$hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶j]&jÇjg$hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j1&ubj±Œ command files created in ”…””•}”(j¶j1&jÇjg$hNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶jo&jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j1&ubj±Œ by ”…””}”(j¶j1&jÇjg$hNjÆNubj˜)”}”(j¦Œ:console:`sh_glred -cmd`”j§]”j±Œ sh_glred -cmd”…””}”(j¶j„&jÇjg$hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j1&ubj±Œù will work without editing; however, in general there are changes you may need to make, for example, to define the reference frame with translation-only rather than tranlsation and rotation, and to change the list of reference (stabilization) sites.”…””}”(j¶j1&jÇjg$hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“$jÆKj¶j”$jÇjg$ubj`)”}”(j¦XNThe daily plots combining the GNSS measurements for each day, may be found in :file:`gsoln/plots_2018_095-2018_097/`. You can view the :file:`.org` files to see what :program:`globk` did, paying attention to the stabilization iteration (what sites were removed), the :math:`\chi^2` increments in the :console:`EXPERIMENT LIST`, and the statitics of the stabilization (:console:`POS STATISTICS`). In your own runs processing many days, it is convenient to get a quick summary by :command:`grep`'ing on :file:`.org` with :console:`USED` (from the :math:`\chi^2` list) and :console:`POS STAT`.”j§]”(j±ŒNThe daily plots combining the GNSS measurements for each day, may be found in ”…””}”(j¶j&jÇjg$hNjÆNubj˜)”}”(j¦Œ&:file:`gsoln/plots_2018_095-2018_097/`”j§]”j±Œgsoln/plots_2018_095-2018_097/”…””}”(j¶j¥&jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&ubj±Œ. You can view the ”…””}”(j¶j&jÇjg$hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶jº&jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&ubj±Œ files to see what ”…””}”(j¶j&jÇjg$hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jÏ&jÇjg$hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j&ubj±ŒU did, paying attention to the stabilization iteration (what sites were removed), the ”…””}”(j¶j&jÇjg$hNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶já&jÇjg$hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶j&ubj±Œ increments in the ”…””}”(j¶j&jÇjg$hNjÆNubj˜)”}”(j¦Œ:console:`EXPERIMENT LIST`”j§]”j±ŒEXPERIMENT LIST”…””}”(j¶jó&jÇjg$hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j&ubj±Œ*, and the statitics of the stabilization (”…””}”(j¶j&jÇjg$hNjÆNubj˜)”}”(j¦Œ:console:`POS STATISTICS`”j§]”j±ŒPOS STATISTICS”…””}”(j¶j'jÇjg$hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j&ubj±ŒU). In your own runs processing many days, it is convenient to get a quick summary by ”…””}”(j¶j&jÇjg$hNjÆNubjj)”}”(j¦Œ:command:`grep`”j§]”j±Œgrep”…””}”(j¶j'jÇjg$hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶j&ubj±Œ ’ing on ”…””}”(j¶j&jÇjg$hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶j+'jÇjg$hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j&ubj±Œ with ”…””}”(j¶j&jÇjg$hNjÆNubj˜)”}”(j¦Œ:console:`USED`”j§]”j±ŒUSED”…””}”(j¶j@'jÇjg$hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j&ubj±Œ (from the ”…””}”(j¶j&jÇjg$hNjÆNubjO )”}”(j¦Œ:math:`\chi^2`”j§]”j±Œ\chi^2”…””}”(j¶jS'jÇjg$hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjN j¶j&ubj±Œ list) and ”…””}”(j¶j&jÇjg$hNjÆNubj˜)”}”(j¦Œ:console:`POS STAT`”j§]”j±ŒPOS STAT”…””}”(j¶je'jÇjg$hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j&ubj±Œ.”…””}”(j¶j&jÇjg$hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“$jÆKj¶j”$jÇjg$ubj`)”}”(j¦Œ‡Next combine the days to get a single H-file for the 3-day span to use for the multi-year repeatabilities (time series) and velocities.”j§]”j±Œ‡Next combine the days to get a single H-file for the 3-day span to use for the multi-year repeatabilities (time series) and velocities.”…””}”(j¶j~'jÇjg$hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj“$jÆKj¶j”$jÇjg$ubj)”}”(j¦Œv$ sh_glred -s 2018 095 2018 097 -expt eura -netext G R E C -ncomb 3 -globk_cmd_prefix COMB -opt G >& sh_glred_comb.log”j§]”j±Œv$ sh_glred -s 2018 095 2018 097 -expt eura -netext G R E C -ncomb 3 -globk_cmd_prefix COMB -opt G >& sh_glred_comb.log”…””}”j¶jŒ'sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj“$jÆKj¶j”$jÇjg$ubej·}”(j¹]”(ŒCrun-globk-to-get-repeatabilities-and-a-combined-h-file-for-the-span”j’$ej»]”j½]”(ŒCrun globk to get repeatabilities and a combined h-file for the span”Œtest_globk2018”ejÀ]”jÂ]”ujÄh_j¶jg$jÇjg$hj“$jÆKjÒ }”j¢'jˆ$sjÔ }”j’$jˆ$subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j“$j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj“$jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jv$jj$j…$jy$uj_}”(Œrel”jv$Œdate”j…$ujc}”je}”j’$]”jˆ$asjg}”(j¢'j’$j¡'jž'uji}”(j¢'ˆj¡'‰uj¹}”(j’$j”$jž'j”$ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ4Hyperlink target "test-globk2018" is not referenced.”…””}”j¶jÌ'sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÉ'ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j“$Œline”KujÄjø ubajˆNj‰]”j‹NjÇjg$ubjôj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jç'sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jä'jÇjä'ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jö'jÇjä'hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jä'jÇjä'ubje)”}”(j¦Œ.. _test_globk_vels:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒtest-globk-vels”ujÄjdjÆKj¶jä'jÇjä'hŒK/chandler/home/floyd/public_html/gg/docs/source/test_install/globk_vels.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ*Run GLOBK to get 3-epoch (4-yr) velocities”j§]”j±Œ*Run GLOBK to get 3-epoch (4-yr) velocities”…””}”(j¶j(jÇjä'hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j(jÇjä'hj(jÆKubj`)”}”(j¦Œ$Get velocities from the 4-year span:”j§]”j±Œ$Get velocities from the 4-year span:”…””}”(j¶j"(jÇjä'hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj(jÆKj¶j(jÇjä'ubj)”}”(j¦Œj$ rm globk_vel.org globk_vel.log $ globk 6 globk_vel.prt globk_vel.log eura.gdl globk.cmd VEL >& globk.out”j§]”j±Œj$ rm globk_vel.org globk_vel.log $ globk 6 globk_vel.prt globk_vel.log eura.gdl globk.cmd VEL >& globk.out”…””}”j¶j0(sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj(jÆKj¶j(jÇjä'ubj`)”}”(j¦Œ‹where the :option:`VEL` token at the end tells :program:`globk` to uncomment the lines in :file:`globk.cmd` that begin with :content:`VEL`.”j§]”(j±Œ where the ”…””}”(j¶j@(jÇjä'hNjÆNubj’)”}”(j¦Œ :option:`VEL`”j§]”j˜)”}”(j¦jJ(j§]”j±ŒVEL”…””}”(j¶jL(jÇjä'hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œ std-option”ej½]”jÀ]”jÂ]”ujÄj—j¶jH(ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jôŒ refdomain”jV(Œreftype”Œoption”Œ refexplicit”‰Œrefwarn”ˆjµNj¶ŒVEL”ujÄj‘hj(jÆK j¶j@(ubj±Œ token at the end tells ”…””}”(j¶j@(jÇjä'hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶jl(jÇjä'hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j@(ubj±Œ to uncomment the lines in ”…””}”(j¶j@(jÇjä'hNjÆNubj˜)”}”(j¦Œ:file:`globk.cmd`”j§]”j±Œ globk.cmd”…””}”(j¶j~(jÇjä'hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j@(ubj±Œ that begin with ”…””}”(j¶j@(jÇjä'hNjÆNubj˜)”}”(j¦Œ:content:`VEL`”j§]”j±ŒVEL”…””}”(j¶j“(jÇjä'hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j@(ubj±Œ.”…””}”(j¶j@(jÇjä'hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj(jÆK j¶j(jÇjä'ubj`)”}”(j¦XÈCheck the :file:`globk_vel.org` file under :content:`EXPERIMENT LIST` for the chi2 increments (< 1.0) in stacking the 3 H-files and the stabilization statistics in the :content:`VEL STATISTICS` and :content:`POS STATISTICS` lines. For this network and the IGS14 (ITRF2014) :file:`.apr` file, the 9 stabilization stations fit the reference frame in velocity at the level of ~ 1 mm/yr horizontal and 5 mm/yr vertical with uncertainties about half of the rms.”j§]”(j±Œ Check the ”…””}”(j¶j¬(jÇjä'hNjÆNubj˜)”}”(j¦Œ:file:`globk_vel.org`”j§]”j±Œ globk_vel.org”…””}”(j¶j´(jÇjä'hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¬(ubj±Œ file under ”…””}”(j¶j¬(jÇjä'hNjÆNubj˜)”}”(j¦Œ:content:`EXPERIMENT LIST`”j§]”j±ŒEXPERIMENT LIST”…””}”(j¶jÉ(jÇjä'hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¬(ubj±Œc for the chi2 increments (< 1.0) in stacking the 3 H-files and the stabilization statistics in the ”…””}”(j¶j¬(jÇjä'hNjÆNubj˜)”}”(j¦Œ:content:`VEL STATISTICS`”j§]”j±ŒVEL STATISTICS”…””}”(j¶jÜ(jÇjä'hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¬(ubj±Œ and ”…””}”(j¶j¬(jÇjä'hNjÆNubj˜)”}”(j¦Œ:content:`POS STATISTICS`”j§]”j±ŒPOS STATISTICS”…””}”(j¶jï(jÇjä'hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j¬(ubj±Œ2 lines. For this network and the IGS14 (ITRF2014) ”…””}”(j¶j¬(jÇjä'hNjÆNubj˜)”}”(j¦Œ :file:`.apr`”j§]”j±Œ.apr”…””}”(j¶j)jÇjä'hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j¬(ubj±Œ« file, the 9 stabilization stations fit the reference frame in velocity at the level of ~ 1 mm/yr horizontal and 5 mm/yr vertical with uncertainties about half of the rms.”…””}”(j¶j¬(jÇjä'hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj(jÆKj¶j(jÇjä'ubej·}”(j¹]”(Œ(run-globk-to-get-3-epoch-4-yr-velocities”j(ej»]”j½]”(Œ*run globk to get 3-epoch (4-yr) velocities”Œtest_globk_vels”ejÀ]”jÂ]”ujÄh_j¶jä'jÇjä'hj(jÆKjÒ }”j#)j(sjÔ }”j(j(subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j(j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj(jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jó'jç'j(jö'uj_}”(Œrel”jó'Œdate”j(ujc}”je}”j(]”j(asjg}”(j#)j(j")j)uji}”(j#)ˆj")‰uj¹}”(j(j(j)j(ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ5Hyperlink target "test-globk-vels" is not referenced.”…””}”j¶jM)sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jJ)ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j(Œline”KujÄjø ubajˆNj‰]”j‹NjÇjä'ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jh)sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶je)jÇje)ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶jw)jÇje)hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶je)jÇje)ubje)”}”(j¦Œ.. _test_glred_ts:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ test-glred-ts”ujÄjdjÆKj¶je)jÇje)hŒI/chandler/home/floyd/public_html/gg/docs/source/test_install/glred_ts.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦Œ+Run GLOBK to get 3-epoch (4-yr) time series”j§]”j±Œ+Run GLOBK to get 3-epoch (4-yr) time series”…””}”(j¶j•)jÇje)hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j’)jÇje)hj‘)jÆKubj`)”}”(j¦X%The key user-specific controls for this step (also incorporated in the :program:`sh_glred` runs within each year) are the list of sites to be used in defining the reference frame, and the *a priori* coordinates for these sites. Here we use the same sites and coordinate file (:file:`igb14_comb.apr`) as in the single-year solutions, but this may not always be the case. For the multi-year repeatabilities, we will use the combined H-files (:file:`.GLX`) created in the year :file:`gsoln/` directories. So create a solution directory at the top level”j§]”(j±ŒGThe key user-specific controls for this step (also incorporated in the ”…””}”(j¶j£)jÇje)hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j«)jÇje)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j£)ubj±Œb runs within each year) are the list of sites to be used in defining the reference frame, and the ”…””}”(j¶j£)jÇje)hNjÆNubj )”}”(j¦Œ *a priori*”j§]”j±Œa priori”…””}”(j¶j½)jÇje)hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj j¶j£)ubj±ŒN coordinates for these sites. Here we use the same sites and coordinate file (”…””}”(j¶j£)jÇje)hNjÆNubj˜)”}”(j¦Œ:file:`igb14_comb.apr`”j§]”j±Œigb14_comb.apr”…””}”(j¶jÏ)jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£)ubj±ŒŽ) as in the single-year solutions, but this may not always be the case. For the multi-year repeatabilities, we will use the combined H-files (”…””}”(j¶j£)jÇje)hNjÆNubj˜)”}”(j¦Œ :file:`.GLX`”j§]”j±Œ.GLX”…””}”(j¶jä)jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£)ubj±Œ) created in the year ”…””}”(j¶j£)jÇje)hNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶jù)jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j£)ubj±Œ= directories. So create a solution directory at the top level”…””}”(j¶j£)jÇje)hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‘)jÆKj¶j’)jÇje)ubj)”}”(j¦Œ $ mkdir vsoln”j§]”j±Œ $ mkdir vsoln”…””}”j¶j*sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj‘)jÆK j¶j’)jÇje)ubj`)”}”(j¦Œ\then change to the new directory and create a list of combined h-files for :program:`globk`:”j§]”(j±ŒKthen change to the new directory and create a list of combined h-files for ”…””}”(j¶j$*jÇje)hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j,*jÇje)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j$*ubj±Œ:”…””}”(j¶j$*jÇje)hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‘)jÆKj¶j’)jÇje)ubj)”}”(j¦Œ.$ cd vsoln $ ls ../????/gsoln/H*GLX > eura.gdl”j§]”j±Œ.$ cd vsoln $ ls ../????/gsoln/H*GLX > eura.gdl”…””}”j¶jD*sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj‘)jÆKj¶j’)jÇje)ubj`)”}”(j¦X=Also copy the default template :file:`globk.cmd` and :file:`glorg.cmd` files to this directory, either using the same :console:`sh_glred -cmd`, as before, or directly from :file:`~/gg/tables/`. For large or complex data sets, it's helpful at this point to run :program:`glist` which will check for blunders and give you a list of all the sites used and their spans. Program :program:`glist2cmd` can then be helpful in establishing a :content:`use_site` list. It may also be desirable to aggregate the data within each year, both to save time in the multi-year combination and to provide more representative long-term statistics. The procedure for doing this is given in the file `sGPS_recipe.txt `_ in the documentation directory on the web site.”j§]”(j±ŒAlso copy the default template ”…””}”(j¶jT*jÇje)hNjÆNubj˜)”}”(j¦Œ:file:`globk.cmd`”j§]”j±Œ globk.cmd”…””}”(j¶j\*jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jT*ubj±Œ and ”…””}”(j¶jT*jÇje)hNjÆNubj˜)”}”(j¦Œ:file:`glorg.cmd`”j§]”j±Œ glorg.cmd”…””}”(j¶jq*jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jT*ubj±Œ0 files to this directory, either using the same ”…””}”(j¶jT*jÇje)hNjÆNubj˜)”}”(j¦Œ:console:`sh_glred -cmd`”j§]”j±Œ sh_glred -cmd”…””}”(j¶j†*jÇje)hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶jT*ubj±Œ, as before, or directly from ”…””}”(j¶jT*jÇje)hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶j™*jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jT*ubj±ŒF. For large or complex data sets, it’s helpful at this point to run ”…””}”(j¶jT*jÇje)hNjÆNubjj)”}”(j¦Œ:program:`glist`”j§]”j±Œglist”…””}”(j¶j®*jÇje)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jT*ubj±Œb which will check for blunders and give you a list of all the sites used and their spans. Program ”…””}”(j¶jT*jÇje)hNjÆNubjj)”}”(j¦Œ:program:`glist2cmd`”j§]”j±Œ glist2cmd”…””}”(j¶jÀ*jÇje)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jT*ubj±Œ' can then be helpful in establishing a ”…””}”(j¶jT*jÇje)hNjÆNubj˜)”}”(j¦Œ:content:`use_site`”j§]”j±Œuse_site”…””}”(j¶jÒ*jÇje)hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶jT*ubj±Œã list. It may also be desirable to aggregate the data within each year, both to save time in the multi-year combination and to provide more representative long-term statistics. The procedure for doing this is given in the file ”…””}”(j¶jT*jÇje)hNjÆNubj÷ )”}”(j¦Œf`sGPS_recipe.txt `_”j§]”j±ŒsGPS_recipe.txt”…””}”(j¶jå*jÇje)hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œname”ŒsGPS_recipe.txt”j ŒQhttp://geoweb.mit.edu/gg/courses/202303_GAGE-SAGE/examples/survey/sGPS_recipe.txt”ujÄjö j¶jT*ubje)”}”(j¦ŒT ”j§]”j·}”(j¹]”Œsgps-recipe-txt”aj»]”j½]”Œsgps_recipe.txt”ajÀ]”jÂ]”Œrefuri”jõ*ujÄjdj Kj¶jT*ubj±Œ0 in the documentation directory on the web site.”…””}”(j¶jT*jÇje)hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‘)jÆKj¶j’)jÇje)ubj)”}”(j¦Œv$ rm globk_replong.org globk_replong.log $ glred 6 globk_replong.prt globk_replong.log eura.gdl globk.cmd >& glred.out”j§]”j±Œv$ rm globk_replong.org globk_replong.log $ glred 6 globk_replong.prt globk_replong.log eura.gdl globk.cmd >& glred.out”…””}”j¶j +sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj‘)jÆKj¶j’)jÇje)ubj`)”}”(j¦X;Unlike in :program:`sh_glred`, the :command:`rm` command may be needed here since :program:`glred` will concatenate the new :file:`.log` and :file:`.org` files with any previous files of the same name. The :file:`globk_replong.prt` will not be created since we have set :content:`prt_opt NOPR` in :file:`globk.cmd`.”j§]”(j±Œ Unlike in ”…””}”(j¶j+jÇje)hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶j%+jÇje)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j+ubj±Œ, the ”…””}”(j¶j+jÇje)hNjÆNubjj)”}”(j¦Œ :command:`rm`”j§]”j±Œrm”…””}”(j¶j7+jÇje)hNjÆNubaj·}”(j¹]”j»]”jvaj½]”jÀ]”jÂ]”ujÄjij¶j+ubj±Œ" command may be needed here since ”…””}”(j¶j+jÇje)hNjÆNubjj)”}”(j¦Œ:program:`glred`”j§]”j±Œglred”…””}”(j¶jI+jÇje)hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j+ubj±Œ will concatenate the new ”…””}”(j¶j+jÇje)hNjÆNubj˜)”}”(j¦Œ :file:`.log`”j§]”j±Œ.log”…””}”(j¶j[+jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j+ubj±Œ and ”…””}”(j¶j+jÇje)hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶jp+jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j+ubj±Œ5 files with any previous files of the same name. The ”…””}”(j¶j+jÇje)hNjÆNubj˜)”}”(j¦Œ:file:`globk_replong.prt`”j§]”j±Œglobk_replong.prt”…””}”(j¶j…+jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j+ubj±Œ' will not be created since we have set ”…””}”(j¶j+jÇje)hNjÆNubj˜)”}”(j¦Œ:content:`prt_opt NOPR`”j§]”j±Œ prt_opt NOPR”…””}”(j¶jš+jÇje)hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjÉjÊej½]”jÀ]”jÂ]”Œlanguage”jÊujÄj—j¶j+ubj±Œ in ”…””}”(j¶j+jÇje)hNjÆNubj˜)”}”(j¦Œ:file:`globk.cmd`”j§]”j±Œ globk.cmd”…””}”(j¶j­+jÇje)hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j+ubj±Œ.”…””}”(j¶j+jÇje)hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj‘)jÆK!j¶j’)jÇje)ubej·}”(j¹]”(Œ)run-globk-to-get-3-epoch-4-yr-time-series”j)ej»]”j½]”(Œ+run globk to get 3-epoch (4-yr) time series”Œ test_glred_ts”ejÀ]”jÂ]”ujÄh_j¶je)jÇje)hj‘)jÆKjÒ }”jÎ+j†)sjÔ }”j)j†)subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j‘)j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj‘)jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(jt)jh)jƒ)jw)uj_}”(Œrel”jt)Œdate”jƒ)ujc}”je}”j)]”j†)asjg}”(jÎ+j)jÍ+jÊ+jÿ*jü*uji}”(jÎ+ˆjÍ+‰jÿ*ˆuj¹}”(j)j’)jÊ+j’)jü*jö*ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ3Hyperlink target "test-glred-ts" is not referenced.”…””}”j¶jø+sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jõ+ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j‘)Œline”KujÄjø ubajˆNj‰]”j‹NjÇje)ubjêj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j,sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j,jÇj,ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j",jÇj,hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j,jÇj,ubje)”}”(j¦Œ.. _test_install:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ test-install”ujÄjdjÆKj¶j,jÇj,hŒF/chandler/home/floyd/public_html/gg/docs/source/test_install/index.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒInstallation Test”j§]”j±ŒInstallation Test”…””}”(j¶j@,jÇj,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j=,jÇj,hj<,jÆKubjí)”}”(j¦hoj§]”jò)”}”(j¦hoj§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j¶jêjü]”(NŒtest_install/gamit2018”†”NŒtest_install/globk2018”†”NŒtest_install/gamit2016”†”NŒtest_install/gamit2014”†”NŒtest_install/glred_ts”†”NŒtest_install/globk_vels”†”NŒtest_install/plots”†”NŒtest_install/review”†”ejþ]”(j[,j],j_,ja,jc,je,jg,ji,ejJÿÿÿÿjNj‰jˆj‰jKj‰j]”ujÄjñhj<,jÆKj¶jN,ubaj·}”(j¹]”j»]”j aj½]”jÀ]”jÂ]”ujÄjìj¶j=,jÇj,hj<,jÆNubj`)”}”(j¦X+This example serves the dual purpose of testing your installation and guiding a new user through the basic steps to get time series and velocities from GAMIT/GLOBK processing. In the latter sense, it replaces the Southern California example from earlier releases in order to add GNSS other than GPS.”j§]”j±X+This example serves the dual purpose of testing your installation and guiding a new user through the basic steps to get time series and velocities from GAMIT/GLOBK processing. In the latter sense, it replaces the Southern California example from earlier releases in order to add GNSS other than GPS.”…””}”(j¶js,jÇj,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆKj¶j=,jÇj,ubj`)”}”(j¦ŒüIf you are an experienced user, you may want to simply execute the batch file :file:`runtest` to complete all steps without intervention in about 90 minutes. In fact, running just one day or one GNSS for 2018 will likely confirm a correct installation.”j§]”(j±ŒNIf you are an experienced user, you may want to simply execute the batch file ”…””}”(j¶j,jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`runtest`”j§]”j±Œruntest”…””}”(j¶j‰,jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j,ubj±ŒŸ to complete all steps without intervention in about 90 minutes. In fact, running just one day or one GNSS for 2018 will likely confirm a correct installation.”…””}”(j¶j,jÇj,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆKj¶j=,jÇj,ubj`)”}”(j¦ŒÊIf you are a novice, however, we strongly recommend that you read this tutorial thoroughly, execute each of the commands manually and peruse the results until you understand what that step accomplished.”j§]”j±ŒÊIf you are a novice, however, we strongly recommend that you read this tutorial thoroughly, execute each of the commands manually and peruse the results until you understand what that step accomplished.”…””}”(j¶j¤,jÇj,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆKj¶j=,jÇj,ubj`)”}”(j¦XAs noted in the installation README, you will need to download :download:`otl_FES2004.grid ` to a :file:`~/gg/GRIDS/` directory at the same level as your main installation or edit the :file:`sestbl.` to omit ocean tidal loading.”j§]”(j±Œ?As noted in the installation README, you will need to download ”…””}”(j¶j²,jÇj,hNjÆNubj^®)”}”(j¦ŒO:download:`otl_FES2004.grid `”j§]”j˜)”}”(j¦j¼,j§]”j±Œotl_FES2004.grid”…””}”(j¶j¾,jÇj,hNjÆNubaj·}”(j¹]”j»]”(j£Œdownload”ej½]”jÀ]”jÂ]”ujÄj—j¶jº,ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jêŒ refdomain”hoŒreftype”jÈ,Œ refexplicit”ˆŒrefwarn”‰j¶Œ0ftp://everest.mit.edu/pub/GRIDS/otl_FES2004.grid”j j×,ujÄj]®hj<,jÆKj¶j²,ubj±Œ to a ”…””}”(j¶j²,jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/GRIDS/`”j§]”j±Œ ~/gg/GRIDS/”…””}”(j¶jÜ,jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j²,ubj±ŒC directory at the same level as your main installation or edit the ”…””}”(j¶j²,jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`sestbl.`”j§]”j±Œsestbl.”…””}”(j¶jñ,jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j²,ubj±Œ to omit ocean tidal loading.”…””}”(j¶j²,jÇj,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆKj¶j=,jÇj,ubj`)”}”(j¦ŒThe example is set up to:”j§]”j±ŒThe example is set up to:”…””}”(j¶j -jÇj,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆKj¶j=,jÇj,ubjX9)”}”(j¦hoj§]”(j˜)”}”(j¦ŒüDownload RINEX 3 files from CDDIS for ten continuous stations in Europe and environs for three days in 2014, 2016 and 2018 (note that if long names were used for the RINEX 3 files, they will be renamed to the older short-names as part of the download);”j§]”j`)”}”(j¦j-j§]”j±ŒüDownload RINEX 3 files from CDDIS for ten continuous stations in Europe and environs for three days in 2014, 2016 and 2018 (note that if long names were used for the RINEX 3 files, they will be renamed to the older short-names as part of the download);”…””}”(j¶j!-jÇj,hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆKj¶j-ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j-jÇj,hj<,jÆNubj˜)”}”(j¦Œ`Conduct phase processing (:program:`sh_gamit`) for GPS-only or GPS, GLONASS, Galileo and Beidou;”j§]”j`)”}”(j¦j6-j§]”(j±ŒConduct phase processing (”…””}”(j¶j8-jÇj,hNjÆNubjj)”}”(j¦Œ:program:`sh_gamit`”j§]”j±Œsh_gamit”…””}”(j¶j?-jÇj,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j8-ubj±Œ3) for GPS-only or GPS, GLONASS, Galileo and Beidou;”…””}”(j¶j8-jÇj,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆK j¶j4-ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j-jÇj,hj<,jÆNubj˜)”}”(j¦Œ®Compute and plot daily repeatabilities (:program:`sh_glred`) for each year and combine the daily h-files (:file:`.glx`) into a single H-file for each year (:file:`.GLX`); and”j§]”j`)”}”(j¦j_-j§]”(j±Œ(Compute and plot daily repeatabilities (”…””}”(j¶ja-jÇj,hNjÆNubjj)”}”(j¦Œ:program:`sh_glred`”j§]”j±Œsh_glred”…””}”(j¶jh-jÇj,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶ja-ubj±Œ/) for each year and combine the daily h-files (”…””}”(j¶ja-jÇj,hNjÆNubj˜)”}”(j¦Œ :file:`.glx`”j§]”j±Œ.glx”…””}”(j¶jz-jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶ja-ubj±Œ&) into a single H-file for each year (”…””}”(j¶ja-jÇj,hNjÆNubj˜)”}”(j¦Œ :file:`.GLX`”j§]”j±Œ.GLX”…””}”(j¶j-jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶ja-ubj±Œ); and”…””}”(j¶ja-jÇj,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆK!j¶j]-ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j-jÇj,hj<,jÆNubj˜)”}”(j¦ŒiCompute repeatabilities and velocities for the three years together (:program:`globk`/:program:`glorg`). ”j§]”j`)”}”(j¦ŒhCompute repeatabilities and velocities for the three years together (:program:`globk`/:program:`glorg`).”j§]”(j±ŒECompute repeatabilities and velocities for the three years together (”…””}”(j¶j´-jÇj,hNjÆNubjj)”}”(j¦Œ:program:`globk`”j§]”j±Œglobk”…””}”(j¶j¼-jÇj,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j´-ubj±Œ/”…””}”(j¶j´-jÇj,hNjÆNubjj)”}”(j¦Œ:program:`glorg`”j§]”j±Œglorg”…””}”(j¶jÎ-jÇj,hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j´-ubj±Œ).”…””}”(j¶j´-jÇj,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆK"j¶j°-ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j-jÇj,hj<,jÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j“>j”>j•>hoj–>j—>ujÄjW9j¶j=,jÇj,hj<,jÆKubj`)”}”(j¦ŒãThe only input file provided in the example is :file:`sites.defaults`, which is always specific to the network one is processing. All of the others are copied or linked from :file:`~/gg/tables/` and will work for most networks.”j§]”(j±Œ/The only input file provided in the example is ”…””}”(j¶jò-jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`sites.defaults`”j§]”j±Œsites.defaults”…””}”(j¶jú-jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jò-ubj±Œi, which is always specific to the network one is processing. All of the others are copied or linked from ”…””}”(j¶jò-jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/tables/`”j§]”j±Œ ~/gg/tables/”…””}”(j¶j.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶jò-ubj±Œ! and will work for most networks.”…””}”(j¶jò-jÇj,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆK$j¶j=,jÇj,ubj`)”}”(j¦XãThe structure established by this test of the installation has three GAMIT processing directories, named (arbitrarily) by year (:file:`2014/`, :file:`2016/`, :file:`2018/`), each of which has below it a :file:`rinex/`, :file:`tables/` and :file:`gsoln/` directory specific to that year. At the top level there is a processing directory (:file:`vsoln/`) and a :file:`tables/` directory for the multi-year GLOBK solution. The steps described assume that you have downloaded ocean tidal loading grid (e.g. :download:`otl_FES2004.grid `) to a :file:`~/gg/GRIDS/` directory (:console:`mkdir ~/gg/GRIDS` if it doesn't exist already) and have internet access while processing; if you do not have these, see :ref:`Notes 3 and 4 `. In directory :file:`check_files/` are saved copies of the q-files and :file:`.org` files for each day, and the :file:`.org` files and PostScript files for the multi-year repeatablities and velocities.”j§]”(j±Œ€The structure established by this test of the installation has three GAMIT processing directories, named (arbitrarily) by year (”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ :file:`2014/`”j§]”j±Œ2014/”…””}”(j¶j2.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ, ”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ :file:`2016/`”j§]”j±Œ2016/”…””}”(j¶jG.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ, ”…””}”j¶j*.sbj˜)”}”(j¦Œ :file:`2018/`”j§]”j±Œ2018/”…””}”(j¶j\.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ ), each of which has below it a ”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`rinex/`”j§]”j±Œrinex/”…””}”(j¶jq.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ, ”…””}”j¶j*.sbj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶j†.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ and ”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`gsoln/`”j§]”j±Œgsoln/”…””}”(j¶j›.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±ŒT directory specific to that year. At the top level there is a processing directory (”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`vsoln/`”j§]”j±Œvsoln/”…””}”(j¶j°.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ) and a ”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`tables/`”j§]”j±Œtables/”…””}”(j¶jÅ.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ directory for the multi-year GLOBK solution. The steps described assume that you have downloaded ocean tidal loading grid (e.g. ”…””}”(j¶j*.jÇj,hNjÆNubj^®)”}”(j¦ŒO:download:`otl_FES2004.grid `”j§]”j˜)”}”(j¦jÜ.j§]”j±Œotl_FES2004.grid”…””}”(j¶jÞ.jÇj,hNjÆNubaj·}”(j¹]”j»]”(j£Œdownload”ej½]”jÀ]”jÂ]”ujÄj—j¶jÚ.ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jêŒ refdomain”hoŒreftype”jè.Œ refexplicit”ˆŒrefwarn”‰j¶Œ0ftp://everest.mit.edu/pub/GRIDS/otl_FES2004.grid”j j÷.ujÄj]®hj<,jÆK'j¶j*.ubj±Œ) to a ”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`~/gg/GRIDS/`”j§]”j±Œ ~/gg/GRIDS/”…””}”(j¶jü.jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ directory (”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ:console:`mkdir ~/gg/GRIDS`”j§]”j±Œmkdir ~/gg/GRIDS”…””}”(j¶j/jÇj,hNjÆNubaj·}”(j¹]”j»]”(jÇjÈjóej½]”jÀ]”jÂ]”Œlanguage”jøujÄj—j¶j*.ubj±Œi if it doesn’t exist already) and have internet access while processing; if you do not have these, see ”…””}”(j¶j*.jÇj,hNjÆNubj’)”}”(j¦Œ+:ref:`Notes 3 and 4 `”j§]”j)”}”(j¦j&/j§]”j±Œ Notes 3 and 4”…””}”(j¶j(/jÇj,hNjÆNubaj·}”(j¹]”j»]”(j£Œstd”Œstd-ref”ej½]”jÀ]”jÂ]”ujÄj*j¶j$/ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œrefdoc”jêŒ refdomain”j2/Œreftype”Œref”Œ refexplicit”ˆŒrefwarn”ˆj¶Œtest_gamit2018_notes”ujÄj‘hj<,jÆK'j¶j*.ubj±Œ. In directory ”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ:file:`check_files/`”j§]”j±Œ check_files/”…””}”(j¶jH/jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ% are saved copies of the q-files and ”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶j]/jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±Œ files for each day, and the ”…””}”(j¶j*.jÇj,hNjÆNubj˜)”}”(j¦Œ :file:`.org`”j§]”j±Œ.org”…””}”(j¶jr/jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j*.ubj±ŒM files and PostScript files for the multi-year repeatablities and velocities.”…””}”(j¶j*.jÇj,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆK'j¶j=,jÇj,ubj`)”}”(j¦ŒþBefore you start, make sure that you have constructed the paths and aliases described in the installation README. The example may be run from any directory on your system, preferably the place you intend to process your own data, not under :file:`~/gg/`.”j§]”(j±ŒðBefore you start, make sure that you have constructed the paths and aliases described in the installation README. The example may be run from any directory on your system, preferably the place you intend to process your own data, not under ”…””}”(j¶j/jÇj,hNjÆNubj˜)”}”(j¦Œ :file:`~/gg/`”j§]”j±Œ~/gg/”…””}”(j¶j•/jÇj,hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j/ubj±Œ.”…””}”(j¶j/jÇj,hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj<,jÆK-j¶j=,jÇj,ubej·}”(j¹]”(Œinstallation-test”j;,ej»]”j½]”(Œinstallation test”Œ test_install”ejÀ]”jÂ]”ujÄh_j¶j,jÇj,hj<,jÆKjÒ }”j¶/j1,sjÔ }”j;,j1,subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j<,j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj<,jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j,j,j.,j",uj_}”(Œrel”j,Œdate”j.,ujc}”je}”j;,]”j1,asjg}”(j¶/j;,jµ/j²/uji}”(j¶/ˆjµ/‰uj¹}”(j;,j=,j²/j=,ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ2Hyperlink target "test-install" is not referenced.”…””}”j¶jà/sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jÝ/ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j<,Œline”KujÄjø ubajˆNj‰]”j‹NjÇj,ubjj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶jû/sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jø/jÇjø/ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j 0jÇjø/hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶jø/jÇjø/ubje)”}”(j¦Œ.. _test_plots:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ test-plots”ujÄjdjÆKj¶jø/jÇjø/hŒF/chandler/home/floyd/public_html/gg/docs/source/test_install/plots.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒPlot time series and velocities”j§]”j±ŒPlot time series and velocities”…””}”(j¶j(0jÇjø/hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j%0jÇjø/hj$0jÆKubj`)”}”(j¦Œ9Create the :file:`.pos` (time series) files for plotting:”j§]”(j±Œ Create the ”…””}”(j¶j60jÇjø/hNjÆNubj˜)”}”(j¦Œ :file:`.pos`”j§]”j±Œ.pos”…””}”(j¶j>0jÇjø/hNjÆNubaj·}”(j¹]”j»]”Œfile”aj½]”jÀ]”jÂ]”Œrole”Œfile”ujÄj—j¶j60ubj±Œ" (time series) files for plotting:”…””}”(j¶j60jÇjø/hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj$0jÆKj¶j%0jÇjø/ubj)”}”(j¦Œ.$ tssum . mit.final.igs14 -R globk_replong.org”j§]”j±Œ.$ tssum . mit.final.igs14 -R globk_replong.org”…””}”j¶jY0sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj$0jÆKj¶j%0jÇjø/ubj`)”}”(j¦Œ(Create the multi-year time series plots:”j§]”j±Œ(Create the multi-year time series plots:”…””}”(j¶ji0jÇjø/hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj$0jÆK j¶j%0jÇjø/ubj)”}”(j¦Œ@$ sh_plot_pos -f *.pos -r -t NONE -u -t1 2014-001T -t2 2018-180T”j§]”j±Œ@$ sh_plot_pos -f *.pos -r -t NONE -u -t1 2014-001T -t2 2018-180T”…””}”j¶jw0sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj$0jÆKj¶j%0jÇjø/ubj`)”}”(j¦ŒPlot the velocities:”j§]”j±ŒPlot the velocities:”…””}”(j¶j‡0jÇjø/hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj$0jÆKj¶j%0jÇjø/ubj)”}”(j¦Œ]$ sh_plotvel -ps euratest -f globk_vel.org -R-60/50/-5/55 -factor 0.5 -arrow_value 10 -page L”j§]”j±Œ]$ sh_plotvel -ps euratest -f globk_vel.org -R-60/50/-5/55 -factor 0.5 -arrow_value 10 -page L”…””}”j¶j•0sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”j/j0j&‰hyŒconsole”j(}”ujÄjhj$0jÆKj¶j%0jÇjø/ubj`)”}”(j¦Œs(Type :program:`sh_plotvel` without arguments to see the full range of options for producing more attractive maps.)”j§]”(j±Œ(Type ”…””}”(j¶j¥0jÇjø/hNjÆNubjj)”}”(j¦Œ:program:`sh_plotvel`”j§]”j±Œ sh_plotvel”…””}”(j¶j­0jÇjø/hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶j¥0ubj±ŒX without arguments to see the full range of options for producing more attractive maps.)”…””}”(j¶j¥0jÇjø/hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj$0jÆKj¶j%0jÇjø/ubej·}”(j¹]”(Œplot-time-series-and-velocities”j#0ej»]”j½]”(Œplot time series and velocities”Œ test_plots”ejÀ]”jÂ]”ujÄh_j¶jø/jÇjø/hj$0jÆKjÒ }”jË0j0sjÔ }”j#0j0subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j$0j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj$0jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j0jû/j0j 0uj_}”(Œrel”j0Œdate”j0ujc}”je}”j#0]”j0asjg}”(jË0j#0jÊ0jÇ0uji}”(jË0ˆjÊ0‰uj¹}”(j#0j%0jÇ0j%0ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ0Hyperlink target "test-plots" is not referenced.”…””}”j¶jõ0sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶jò0ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j$0Œline”KujÄjø ubajˆNj‰]”j‹NjÇjø/ubjìj£)”}”(j¦hoj§]”(j«)”}”(j¦Œ.. |rel| replace:: 10.71”j§]”j±Œ10.71”…””}”j¶j1sbaj·}”(j¹]”j»]”j½]”Œrel”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j 1jÇj 1ubj«)”}”(j¦Œ.. |date| replace:: |today| ”j§]”j±Œ2024 136”…””}”(j¶j1jÇj 1hNjÆNubaj·}”(j¹]”j»]”j½]”Œdate”ajÀ]”jÂ]”ujÄjªhjÅjÆKj¶j 1jÇj 1ubje)”}”(j¦Œ.. _test_review:”j§]”j·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jpŒ test-review”ujÄjdjÆKj¶j 1jÇj 1hŒG/chandler/home/floyd/public_html/gg/docs/source/test_install/review.rst”ubj×)”}”(j¦hoj§]”(jÜ)”}”(j¦ŒReview”j§]”j±ŒReview”…””}”(j¶j=1jÇj 1hNjÆNubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄjÛj¶j:1jÇj 1hj91jÆKubj`)”}”(j¦ŒºTo start over from scratch, run :program:`sh_clean_test`, once for each year and once for the velocity solution. (Type the name of the script without arguments to see the documentation.)”j§]”(j±Œ To start over from scratch, run ”…””}”(j¶jK1jÇj 1hNjÆNubjj)”}”(j¦Œ:program:`sh_clean_test`”j§]”j±Œ sh_clean_test”…””}”(j¶jS1jÇj 1hNjÆNubaj·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÄjij¶jK1ubj±Œ‚, once for each year and once for the velocity solution. (Type the name of the script without arguments to see the documentation.)”…””}”(j¶jK1jÇj 1hNjÆNubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_hj91jÆKj¶j:1jÇj 1ubej·}”(j¹]”(Œreview”j81ej»]”j½]”(Œreview”Œ test_review”ejÀ]”jÂ]”ujÄh_j¶j 1jÇj 1hj91jÆKjÒ }”jq1j.1sjÔ }”j81j.1subej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œsource”j91j}”(j!Kj"KuujÄj¢j#Nj$Njfj')”}”(j*NjÛNj+Nj,Nj-Nj.Nj/j0j1Kj2Kj3Nj4Nj5Nj6KjxKj7Kj8Nj9Nj:ˆjth“j;j<j=j>j?j<j@jAjBjCj|hzjDNhNjEhojhjijFNjGNjHNjINjJNjKNjLNjMj91jNNjOjPjyˆjQKjRM'jpNjnjojSjTjsNjqjrjUKh¥‰jVjWj}ˆjzj{jX‰ju‰jYKjv‰jjjkjl‰jmˆjw‰hkNubjZNj[]”j]}”(j1j1j+1j1uj_}”(Œrel”j1Œdate”j+1ujc}”je}”j81]”j.1asjg}”(jq1j81jp1jm1uji}”(jq1ˆjp1‰uj¹}”(j81j:1jm1j:1ujl}”jn}”jp]”jr]”jt]”jv]”jx]”jz]”j|Kj}Kj~j€}”…”R”j„]”j†]”jù )”}”(j¦hoj§]”j`)”}”(j¦hoj§]”j±Œ1Hyperlink target "test-review" is not referenced.”…””}”j¶j›1sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj_j¶j˜1ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œlevel”KŒtype”jŒsource”j91Œline”KujÄjø ubajˆNj‰]”j‹NjÇj 1ubuŒmetadata”jƒj„Œdict”“”…”R”Œtitles”}”(jëjÜ)”}”(j¦hoj§]”j±ŒGAMIT Reference 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jÜ)”}”(j¦hoj§]”j±ŒPreface”…””}”j¶j52sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jî1]”KaujÄjÛubjjÜ)”}”(j¦hoj§]”j˜)”}”(j§]”j±Œ autcln.cmd”…””}”j¶jF2sbaj¦jjÄj—j·}”(j¹]”j»]”jaj½]”jÀ]”jÂ]”jjujÆNhNj¶jC2ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jî1]”(KKKeujÄjÛubjýjÜ)”}”(j¦hoj§]”j˜)”}”(j§]”j±Œ globk.cmd”…””}”j¶j]2sbaj¦jjÄj—j·}”(j¹]”j»]”j aj½]”jÀ]”jÂ]”jjujÆNhNj¶jZ2ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jî1]”(KKKeujÄjÛubjéjÜ)”}”(j¦hoj§]”j˜)”}”(j§]”j±Œ glorg.cmd”…””}”j¶jt2sbaj¦j¤&jÄj—j·}”(j¹]”j»]”j°&aj½]”jÀ]”jÂ]”j´&jµ&ujÆNhNj¶jq2ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”jî1]”(KKKeujÄjÛubjjÜ)”}”(j¦hoj§]”j±ŒEditing the Control 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5j¶j©8ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j¦8ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’ubjÿj“)”}”(j¦hoj§]”j˜)”}”(j¦hoj§]”j 5)”}”(j¦hoj§]”j÷ )”}”(j¦hoj§]”(j±ŒUsing ”…””}”j¶jã8sbjj)”}”(j§]”j±Œsh_gamit”…””}”j¶jê8sbaj¦j 8jÄjij·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÆNhNj¶jã8ubj±Œ and ”…””}”j¶jã8sbjj)”}”(j§]”j±Œsh_glred”…””}”j¶jû8sbaj¦j8jÄjij·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÆNhNj¶jã8ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œinternal”ˆŒrefuri”jÿŒ anchorname”hojî1j3ujÄjö j¶jà8ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj 5j¶jÝ8ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÚ8ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’ubj j“)”}”(j¦hoj§]”j˜)”}”(j¦hoj§]”j 5)”}”(j¦hoj§]”j÷ )”}”(j¦hoj§]”j±ŒSummary of Program Flow”…””}”j¶j,9sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œinternal”ˆŒrefuri”j Œ anchorname”hojî1j+3ujÄjö j¶j)9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj 5j¶j&9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j#9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’ubjj“)”}”(j¦hoj§]”j˜)”}”(j¦hoj§]”(j 5)”}”(j¦hoj§]”j÷ )”}”(j¦hoj§]”j±Œ)Automatic Processing with GAMIT and 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anchorname”hojî1j^3ujÄjö j¶jÎ9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj 5j¶jË9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jÈ9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’ubjj“)”}”(j¦hoj§]”j˜)”}”(j¦hoj§]”j 5)”}”(j¦hoj§]”j÷ )”}”(j¦hoj§]”jj)”}”(j§]”j±Œsh_glred”…””}”j¶j:sbaj¦j™njÄjij·}”(j¹]”j»]”j‰aj½]”jÀ]”jÂ]”ujÆNhNj¶j:ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œinternal”ˆŒrefuri”jŒ anchorname”hojî1ju3ujÄjö j¶j:ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj 5j¶jÿ9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jü9ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’ubjj“)”}”(j¦hoj§]”j˜)”}”(j¦hoj§]”j 5)”}”(j¦hoj§]”j÷ )”}”(j¦hoj§]”j±ŒCombining h-files”…””}”j¶j9:sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œinternal”ˆŒrefuri”jŒ anchorname”hojî1jƒ3ujÄjö j¶j6:ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj 5j¶j3:ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j0:ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’ubj j“)”}”(j¦hoj§]”j˜)”}”(j¦hoj§]”j 5)”}”(j¦hoj§]”j÷ )”}”(j¦hoj§]”j±Œ Data Editing”…””}”j¶jd:sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œinternal”ˆŒrefuri”j Œ anchorname”hojî1j‘3ujÄjö j¶ja:ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj 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anchorname”Œ#other-changes-for-10-61”ujÄjö j¶jD>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj 5j¶jA>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j>>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’j¶j">ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’ubjøj“)”}”(j¦hoj§]”j˜)”}”(j¦hoj§]”(j 5)”}”(j¦hoj§]”j÷ )”}”(j¦hoj§]”j±Œ10.7”…””}”j¶j>sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œinternal”ˆŒrefuri”jøŒ anchorname”houjÄjö j¶j|>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj 5j¶jy>ubj“)”}”(j¦hoj§]”j˜)”}”(j¦hoj§]”j 5)”}”(j¦hoj§]”j÷ )”}”(j¦hoj§]”j±ŒOther changes for 10.7”…””}”j¶jž>sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œinternal”ˆŒrefuri”jøŒ anchorname”Œ#other-changes-for-10-7”ujÄjö j¶j›>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj 5j¶j˜>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶j•>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’j¶jy>ubej·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj—j¶jv>ubaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”ujÄj’ubjñj“)”}”(j¦hoj§]”j˜)”}”(j¦hoj§]”(j 5)”}”(j¦hoj§]”j÷ )”}”(j¦hoj§]”j±Œ10.71”…””}”j¶jÖ>sbaj·}”(j¹]”j»]”j½]”jÀ]”jÂ]”Œinternal”ˆŒrefuri”jñŒ anchorname”houjÄjö 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Kouba_2009”NŒLagler_et_al_2013”NŒMao_et_al_1999”NŒMcCaffrey_et_al_2007”NŒMcClusky_et_al_2000”NŒMontenbruck_et_al_2015”NŒPetrie_et_al_2010”NŒSchaffrin_and_Bock_1988”NŒSchmid_et_al_2007”NŒ Williams_2003”NŒZiebart_et_al_2002”Nu†””ŒC/chandler/home/floyd/public_html/gg/docs/source/relnote/relnote.bib”jüBGAÙËíz}”ŒKreemer_et_al_2018”Ns†””uŒpybtex.database”ŒBibliographyData”“”)”}”(jüŒ pybtex.utils”ŒOrderedCaseInsensitiveDict”“”)”}”(Œ_dict”}”(Œaltamimi_et_al_2012”j#CŒEntry”“”)”}”(Œtype”Œarticle”Œ original_type”Œarticle”Œfields”j*C)”}”(j-C}”(Œtitle”Œ{ITRF}2008 plate motion model”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ117”Œnumber”ŒB7”Œpages”hoŒkeywords”Œplate motion, reference frames”Œdoi”Œ10.1029/2011JB008930”Œ//url”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2011JB008930”Œ//eprint”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2011JB008930”Œabstract”XˆThe ITRF2008 velocity field is demonstrated to be of higher quality and more precise than past ITRF solutions. We estimated an absolute tectonic plate motion model made up of 14 major plates, using velocities of 206 sites of high geodetic quality (far from plate boundaries, deformation zones and Glacial Isostatic Adjustment (GIA) regions), derived from and consistent with ITRF2008. The precision of the estimated model is evaluated to be at the level of 0.3 mm/a WRMS. No GIA corrections were applied to site velocities prior to estimating plate rotation poles, as our selected sites are outside the Fennoscandia regions where the GIA models we tested are performing reasonably well, and far from GIA areas where the models would degrade the fit (Antarctica and North America). Our selected velocity field has small origin rate bias components following the three axis (X, Y, Z), respectively 0.41 ± 0.54, 0.22 ± 0.64 and 0.41 ± 0.60 (95 per cent confidence limits). Comparing our model to NNR-NUVEL-1A and the newly available NNR-MORVEL56, we found better agreement with NNR-MORVEL56 than with NNR-NUVEL-1A for all plates, except for Australia where we observe an average residual rotation rate of 4 mm/a. Using our selection of sites, we found large global X-rotation rates between the two models (0.016°/Ma) and between our model and NNR-MORVEL56 of 0.023°/Ma, equivalent to 2.5 mm/a at the Earth surface.”Œyear”Œ2012”uŒ_keys”jŒ OrderedDict”“”)R”(jCŒjournal”j@CŒvolume”jBCŒnumber”jDCŒpages”jECŒkeywords”jGCŒdoi”jICŒ//url”jKCŒ//eprint”jMCŒabstract”jOCŒyear”uubŒpersons”j*C)”}”(j-C}”Œauthor”]”(j#CŒPerson”“”)”}”(Œ first_names”]”ŒZ.”aŒ middle_names”]”Œ prelast_names”]”Œ last_names”]”ŒAltamimi”aŒ lineage_names”]”ubjgC)”}”(jjC]”ŒL.”ajmC]”joC]”jqC]”Œ M{\'e}tivier”ajtC]”ubjgC)”}”(jjC]”ŒX.”ajmC]”joC]”jqC]”Œ Collilieux”ajtC]”ubesjQCjSC)R”jdCŒauthor”subŒkey”jþBubŒash_1972”j1C)”}”(j4CŒ techreport”j6CŒ techreport”j8Cj*C)”}”(j-C}”(Œtitle”Œ)Determination of {E}arth Satellite Orbits”Œ institution”Œ9Massachusetts Institute of Technology, Lincoln Laboratory”Œtype”ŒTechnical Note”Œnumber”Œ1972-5”Œ//month”ŒApril”Œyear”Œ1972”ujQCjSC)R”(j“CŒtitle”j•CŒ institution”j—CŒtype”j™CŒnumber”j›CŒ//month”jCŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”jgC)”}”(jjC]”ŒM.”ajmC]”ŒE.”ajoC]”jqC]”ŒAsh”ajtC]”ubasjQCjSC)R”j©CŒauthor”subjŠCjÿBubŒbar-sever_1996”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œyear”Œ1996”Œtitle”Œ"A new model for {GPS} yaw attitude”Œjournal”ŒJournal of Geodesy”Œpages”Œ714--723”Œvolume”Œ70”Œissue”Œ11”Œabstract”X­Modeling of the {GPS} satellite yaw attitude is a key element in high-precision geophysical applications. This fact is illustrated here as a new model for the {GPS} satellite yaw attitude is introduced. The model constitutes a significant improvement over the previously available model in terms of efficiency, flexibility and portability. The model is described in detail and implementation issues, including the proper estimation strategy, are addressed. The performance of the new model is analyzed and an error budget is presented. Finally, the implementation of the yaw bias on the {GPS} satellites is reviewed from its inception until it reached a steady state in November, 1995.”Œissn”Œ 1432-1394”Œ//url”Œ"https://doi.org/10.1007/BF00867149”Œdoi”Œ10.1007/BF00867149”ujQCjSC)R”(j¿CŒyear”jÁCŒtitle”jÃCŒjournal”jÅCŒpages”jÇCŒvolume”jÉCŒissue”jËCŒabstract”jÍCŒissn”jÏCŒ//url”jÑCŒdoi”uubj`Cj*C)”}”(j-C}”Œauthor”]”jgC)”}”(jjC]”ŒYoaz”ajmC]”ŒE.”ajoC]”jqC]”Œ Bar-Sever”ajtC]”ubasjQCjSC)R”jáCŒauthor”subjŠCjCubŒbeutler_et_al_1994a”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œ|The {I}nternational {GPS} {S}ervice for {G}eodynamics ({IGS}): Development and Start of Official Service on 1 {J}anuary 1994”Œjournal”ŒBulletin g{\'e}od{\'e}sique”Œvolume”Œ68”Œpages”Œ43--46”Œyear”Œ1994”Œissue”jwŒ//url”Œ"https://doi.org/10.1007/BF00806751”Œdoi”Œ10.1007/BF00806751”ujQCjSC)R”(j÷CŒtitle”jùCŒjournal”jûCŒvolume”jýCŒpages”jÿCŒyear”jDŒissue”jDŒ//url”jDŒdoi”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒGerhard”ajmC]”joC]”jqC]”ŒBeulter”ajtC]”ubjgC)”}”(jjC]”ŒIvan”ajmC]”ŒI.”ajoC]”jqC]”ŒMueller”ajtC]”ubjgC)”}”(jjC]”ŒRuth”ajmC]”ŒE.”ajoC]”jqC]”ŒNeilan”ajtC]”ubesjQCjSC)R”jDŒauthor”subjŠCjCubŒbeutler_et_al_1994b”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”ŒŸExtended orbit modeling techniques at the {CODE} processing center of the {I}nternational {GPS} {S}ervice for {G}eodynamics ({IGS}): theory and initial results”Œjournal”Œmanuscripta geodaetica”Œyear”Œ1994”Œvolume”Œ19”Œmonth”Œ01”Œnumber”Œ6”Œpages”Œ367-386”Œissn”Œ 0340-8825”ujQCjSC)R”(j;DŒtitle”j=DŒjournal”j?DŒyear”jADŒvolume”jCDŒmonth”jEDŒnumber”jGDŒpages”jIDŒissn”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒG.”ajmC]”joC]”jqC]”ŒBeutler”ajtC]”ubjgC)”}”(jjC]”ŒE.”ajmC]”joC]”jqC]”Œ Brockmann”ajtC]”ubjgC)”}”(jjC]”ŒW.”ajmC]”joC]”jqC]”ŒGurtner”ajtC]”ubjgC)”}”(jjC]”ŒU.”ajmC]”joC]”jqC]”Œ Hugentobler”ajtC]”ubjgC)”}”(jjC]”ŒL.”ajmC]”joC]”jqC]”ŒMervart”ajtC]”ubjgC)”}”(jjC]”ŒM.”ajmC]”joC]”jqC]”Œ Rothacher”ajtC]”ubjgC)”}”(jjC]”ŒA.”ajmC]”joC]”jqC]”ŒVerdun”ajtC]”ubesjQCjSC)R”jWDŒauthor”subjŠCjCubŒbeutler_et_al_1996”j1C)”}”(j4CŒ inproceedings”j6CŒ InProceedings”j8Cj*C)”}”(j-C}”(Œtitle”ŒHThe {I}nternational {GPS} {S}ervice for {G}eodynamics ({IGS}): The Story”Œ booktitle”ŒJ{GPS} Trends in Precise Terrestrial, Airborne, and Spaceborne Applications”Œyear”Œ1996”Œ publisher”ŒSpringer Berlin Heidelberg”Œaddress”ŒBerlin, Heidelberg”Œpages”Œ3--13”Œabstract”XŒThe primary goal of the {I}nternational {GPS} {S}ervice for {G}eodynamics ({IGS}) is to provide highly accurate orbits, earth rotation parameters, and station coordinates derived from observations of the {G}lobal {P}ositioning System ({GPS}) to the geodynamics community, which currently demand the highest accuracy. A further goal is the extension of the {IERS} {T}errestrial {R}eference {F}rame ({ITRF}) for the purpose of global accessibility. The data of the permanent {IGS} network consisting of about 80 stations are transmitted on a daily basis to regional and global data centers from where they are retrieved by the {IGS} {A}nalysis {C}enters.”Œisbn”Œ978-3-642-80133-4”ujQCjSC)R”(j¢DŒtitle”j¤DŒ booktitle”j¦DŒyear”j¨DŒ publisher”jªDŒaddress”j¬DŒpages”j®DŒabstract”j°DŒisbn”uubj`Cj*C)”}”(j-C}”(Œauthor”]”(jgC)”}”(jjC]”ŒGerhard”ajmC]”joC]”jqC]”ŒBeutler”ajtC]”ubjgC)”}”(jjC]”ŒIvan”ajmC]”ŒI.”ajoC]”jqC]”ŒMueller”ajtC]”ubjgC)”}”(jjC]”ŒRuth”ajmC]”ŒE.”ajoC]”jqC]”ŒNeilan”ajtC]”ubeŒeditor”]”(jgC)”}”(jjC]”ŒGerhard”ajmC]”joC]”jqC]”ŒBeutler”ajtC]”ubjgC)”}”(jjC]”ŒWilliam”ajmC]”ŒG.”ajoC]”jqC]”Œ Melbourne”ajtC]”ubjgC)”}”(jjC]”Œ G{\"u}nter”ajmC]”ŒW.”ajoC]”jqC]”ŒHein”ajtC]”ubjgC)”}”(jjC]”Œ G{\"u}nter”ajmC]”joC]”jqC]”ŒSeeber”ajtC]”ubeujQCjSC)R”(j¾DŒauthor”jÝDŒeditor”uubjŠCjCubŒ blewitt_1989”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”ŒvCarrier phase ambiguity resolution for the {G}lobal {P}ositioning {S}ystem applied to geodetic baselines up to 2000 km”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ94”Œnumber”ŒB8”Œpages”Œ 10187-10203”Œdoi”Œ10.1029/JB094iB08p10187”Œ//url”ŒGhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/JB094iB08p10187”Œ//eprint”ŒGhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/JB094iB08p10187”Œabstract”XðThe {G}lobal {P}ositioning {S}ystem ({GPS}) carrier phase data are biased by an integer number of cycles. A successful strategy has been developed and demonstrated for resolving these integer ambiguities for geodetic baselines of up to 2000 km in length, resulting in a factor of 3 improvement in baseline accuracy, and giving centimeter-level agreement with coordinates inferred by very long baseline interferometry in the western {U}nited {S}tates. For this experiment, a method using pseudorange data is shown to be more reliable than one using ionospheric constraints for baselines longer than 200 km. An automated algorithm exploits the correlations between the many phase biases of a {GPS} receiver network to enable the resolution of ambiguities for very long baselines. A method called bias optimizing has been developed, which, unlike traditional bias fixing, does not require an arbitrary confidence test. Bias optimizing is expected to be preferable to bias fixing for poorly configured networks. In order to enable ambiguity resolution for long baselines, it is recommended that future {GPS} networks have a wide spectrum of baseline lengths ranging from <100 to >1000 km and that {GPS} receivers be used which can acquire dual-frequency {P} code data.”Œyear”Œ1989”ujQCjSC)R”(jEŒtitle”jEŒjournal”jEŒvolume”jEŒnumber”jEŒpages”jEŒdoi”jEŒ//url”jEŒ//eprint”j EŒabstract”j"EŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”jgC)”}”(jjC]”ŒGeoffrey”ajmC]”joC]”jqC]”ŒBlewitt”ajtC]”ubasjQCjSC)R”j2EŒauthor”subjŠCjCubŒ blewitt_1990”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œ-An Automatic Editing Algorithm for {GPS} data”Œjournal”ŒGeophysical Research Letters”Œvolume”Œ17”Œnumber”Œ3”Œpages”Œ199-202”Œdoi”Œ10.1029/GL017i003p00199”Œ//url”ŒGhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/GL017i003p00199”Œ//eprint”ŒGhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/GL017i003p00199”Œabstract”X=An algorithm has been developed to edit automatically {G}lobal {P}ositioning {S}ystem data such that outlier deletion, cycle slip identification and correction are independent of clock instability, selective availability, receiver–satellite kinematics, and tropospheric conditions. This algorithm, called {T}urbo{E}dit, operates on undifferenced, dual frequency carrier phase data, and requires (1) the use of {P} code pseudorange data and (2) a smoothly varying ionospheric electron content. The latter requirement can be relaxed if the analysis software incorporates ambiguity resolution techniques to estimate unresolved cycle slip parameters. {T}urbo{E}dit was tested on the large data set from the {CASA} {U}no experiment, which contained over 2500 cycle slips. Analyst intervention was required on 1\% of the station–satellite passes, almost all of these problems being due to difficulties in extrapolating variations in the ionospheric delay. The algorithm is presently being adapted for real time data editing in the {R}ogue receiver for continuous monitoring applications.”Œyear”Œ1990”ujQCjSC)R”(jGEŒtitle”jIEŒjournal”jKEŒvolume”jMEŒnumber”jOEŒpages”jQEŒdoi”jSEŒ//url”jUEŒ//eprint”jWEŒabstract”jYEŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”jgC)”}”(jjC]”ŒGeoffrey”ajmC]”joC]”jqC]”ŒBlewitt”ajtC]”ubasjQCjSC)R”jiEŒauthor”subjŠCjCubŒbock_et_al_1986”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œ4Interferometric analysis of {GPS} phase observations”Œjournal”ŒManuscripta geodaetica”Œvolume”Œ11”Œpages”Œ282-288”Œyear”Œ1986”ujQCjSC)R”(j~EŒtitle”j€EŒjournal”j‚EŒvolume”j„EŒpages”j†EŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒYehuda”ajmC]”joC]”jqC]”ŒBock”ajtC]”ubjgC)”}”(jjC]”ŒSergei”ajmC]”ŒA”ajoC]”jqC]”Œ Gourevitch”ajtC]”ubjgC)”}”(jjC]”ŒCharles”ajmC]”j1MajoC]”jqC]”(Œ Counselman”ŒIII”ejtC]”ubjgC)”}”(jjC]”ŒRobert”ajmC]”ŒW”ajoC]”jqC]”ŒKing”ajtC]”ubjgC)”}”(jjC]”ŒRichard”ajmC]”ŒI”ajoC]”jqC]”ŒAbbot”ajtC]”ubesjQCjSC)R”j‘EŒauthor”subjŠCjCubŒboehm_et_al_2006a”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œ«Troposphere mapping functions for {GPS} and very long baseline interferometry from {E}uropean {C}entre for {M}edium-{R}ange {W}eather {F}orecasts operational analysis data”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ111”Œnumber”ŒB2”Œpages”hoŒkeywords”Œmapping function, VLBI, GPS”Œdoi”Œ10.1029/2005JB003629”Œ//url”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2005JB003629”Œ//eprint”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2005JB003629”Œabstract”XŠIn the analyses of geodetic very long baseline interferometry ({VLBI}) and {GPS} data the analytic form used for mapping of the atmosphere delay from zenith to the line of site is most often a three-parameter continued fraction in 1/sin(elevation). Using the 40 years reanalysis ({ERA}-40) data of the {E}uropean {C}entre for {M}edium-{R}ange {W}eather {F}orecasts for the year 2001, the b and c coefficients of the continued fraction form for the hydrostatic mapping functions have been redetermined. Unlike previous mapping functions based on data from numerical weather models (isobaric mapping functions ({N}iell, 2000) and {V}ienna mapping functions ({VMF}) ({B}oehm and {S}chuh, 2004)), the new c coefficients are dependent on the day of the year, and unlike the {N}iell mapping functions ({N}iell, 1996) they are no longer symmetric with respect to the equator (apart from the opposite phase for the two hemispheres). Compared to {VMF}, this causes an effect on the {VLBI} or {GPS} station heights that is constant and as large as 2 mm at the equator and that varies seasonally between 4 mm and 0 mm at the poles. The updated {VMF}, based on these new coefficients and called {VMF}1 hereinafter, yields slightly better baseline length repeatabilities for {VLBI} data. The hydrostatic and wet mapping functions are applied in various combinations with different kinds of a priori zenith delays in the analyses of all {VLBI} {I}nternational {VLBI} {S}ervice for {G}eodesy and {A}strometry ({IVS})-{R}1 and {IVS}-{R}4 24-hour sessions of 2002 and 2003; the investigations concentrate on baseline length repeatabilities, as well as on absolute changes of station heights.”Œyear”Œ2006”ujQCjSC)R”(jÎEŒtitle”jÐEŒjournal”jÒEŒvolume”jÔEŒnumber”jÖEŒpages”j×EŒkeywords”jÙEŒdoi”jÛEŒ//url”jÝEŒ//eprint”jßEŒabstract”jáEŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒJohannes”ajmC]”joC]”jqC]”ŒBoehm”ajtC]”ubjgC)”}”(jjC]”ŒBirgit”ajmC]”joC]”jqC]”ŒWerl”ajtC]”ubjgC)”}”(jjC]”ŒHarald”ajmC]”joC]”jqC]”ŒSchuh”ajtC]”ubesjQCjSC)R”jòEŒauthor”subjŠCjCubŒboehm_et_al_2006b”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œm{G}lobal {M}apping {F}unction ({GMF}): A new empirical mapping function based on numerical weather model data”Œjournal”ŒGeophysical Research Letters”Œvolume”Œ33”Œnumber”Œ7”Œpages”hoŒdoi”Œ10.1029/2005GL025546”Œ//url”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2005GL025546”Œ//eprint”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2005GL025546”Œabstract”X¯Troposphere mapping functions are used in the analyses of Global Positioning System and Very Long Baseline Interferometry observations to map a priori zenith hydrostatic and wet delays to any elevation angle. Most analysts use the Niell Mapping Function (NMF) whose coefficients are determined from site coordinates and the day of year. Here we present the Global Mapping Function (GMF), based on data from the global ECMWF numerical weather model. The coefficients of the GMF were obtained from an expansion of the Vienna Mapping Function (VMF1) parameters into spherical harmonics on a global grid. Similar to NMF, the values of the coefficients require only the station coordinates and the day of year as input parameters. Compared to the 6-hourly values of the VMF1 a slight degradation in short-term precision occurs using the empirical GMF. However, the regional height biases and annual errors of NMF are significantly reduced with GMF.”Œyear”Œ2006”ujQCjSC)R”(jFŒtitle”jFŒjournal”jFŒvolume”jFŒnumber”j!FŒpages”j"FŒdoi”j$FŒ//url”j&FŒ//eprint”j(FŒabstract”j*FŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒJ.”ajmC]”joC]”jqC]”ŒBoehm”ajtC]”ubjgC)”}”(jjC]”ŒA.”ajmC]”joC]”jqC]”ŒNiell”ajtC]”ubjgC)”}”(jjC]”ŒP.”ajmC]”joC]”jqC]”Œ Tregoning”ajtC]”ubjgC)”}”(jjC]”ŒH.”ajmC]”joC]”jqC]”ŒSchuh”ajtC]”ubesjQCjSC)R”j:FŒauthor”subjŠCjCubŒ colombo_1986”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œyear”Œ1986”Œtitle”Œ$Ephemeris errors of {GPS} satellites”Œjournal”ŒBulletin g{\'e}od{\'e}sique”Œpages”Œ64--84”Œvolume”Œ60”Œissue”jwŒabstract”X©Ephemeris errors are supposed to be a major factor limiting the usefulness of {GPS} in high precision geodesy. Considerations of orbital mechanics suggest that, regardless of their complexity, the uncertainties in the solar radiation pressure model, the gravity field model, and the estimated initial state, may have simple effects on the ephemeris. This possibility has been tested by fitting linear combinations of simple functions—chosen on theoretical grounds—to simulated errors of three-day ephemerides. With a set of five functions for the across-track component, six for the radial, and seven for the along-track, it has been possible to fit the position errors to better than 1\% of their r.m.s values, in all the caces studied. The simulations included—besides solar radiation pressure errors—gravity field model and initial state uncertainties, as well as an unknown constant force along the axis of the solar panels. The solar radiation force was calculated taking into account the shape, orientation, and physical properties (reflectivity and specularity) of the main parts of the spacecraft, under various conditions of illumination (continuous sunlight, eclipses, etc.).”Œissn”Œ 1432-1394”Œ//url”Œ"https://doi.org/10.1007/BF02519355”Œdoi”Œ10.1007/BF02519355”ujQCjSC)R”(jjFŒyear”jlFŒtitle”jnFŒjournal”jpFŒpages”jrFŒvolume”jtFŒissue”juFŒabstract”jwFŒissn”jyFŒ//url”j{FŒdoi”uubj`Cj*C)”}”(j-C}”Œauthor”]”jgC)”}”(jjC]”ŒOscar”ajmC]”ŒL.”ajoC]”jqC]”ŒColombo”ajtC]”ubasjQCjSC)R”j‹FŒauthor”subjŠCj CubŒdavis_et_al_2003”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”ŒaAssessment of {GPS} velocity accuracy for the {B}asin and {R}ange {G}eodetic {N}etwork ({BARGEN})”Œjournal”ŒGeophysical Research Letters”Œvolume”Œ30”Œnumber”j FŒpages”hoŒdoi”Œ10.1029/2003GL016961”Œ//url”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2003GL016961”Œ//eprint”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2003GL016961”Œabstract”XïWe assess the accuracy of horizontal velocity estimates from the Basin and Range Geodetic Network (BARGEN), a continuous GPS network that has been in operation since 1996. To make this quantitative assessment, we use a procedure that we term the “whole-error†method. In this method, the measure of the velocity errors is the root-mean-square (RMS) residual velocity relative to a simple geophysical model. This method produces a conservative estimate of the uncertainties, since errors in the geophysical models also contribute to the RMS residual. Using estimates from two different BARGEN subnetworks, the Northern Basin and Range and the Yucca Mountain Cluster, we determine velocity uncertainties of 0.1–0.2 mm yr−1. Since BARGEN covers a significant fraction of area of the proposed Plate Boundary Observatory component of EarthScope, our results indicate a good ability of this project to determine highly accurate long-term horizontal crustal velocities and deformation rates in this region.”Œyear”Œ2003”ujQCjSC)R”(j¡FŒtitle”j£FŒjournal”j¥FŒvolume”j§FŒnumber”j¨FŒpages”j©FŒdoi”j«FŒ//url”j­FŒ//eprint”j¯FŒabstract”j±FŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒJ.”ajmC]”ŒL.”ajoC]”jqC]”ŒDavis”ajtC]”ubjgC)”}”(jjC]”ŒR.”ajmC]”ŒA.”ajoC]”jqC]”ŒBennett”ajtC]”ubjgC)”}”(jjC]”ŒB.”ajmC]”ŒP.”ajoC]”jqC]”ŒWernicke”ajtC]”ubesjQCjSC)R”jÁFŒauthor”subjŠCj CubŒdixon_et_al_2000”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œ–Present-day motion of the {S}ierra {N}evada block and some tectonic implications for the {B}asin and {R}ange province, {N}orth {A}merican {C}ordillera”Œjournal”Œ Tectonics”Œvolume”Œ19”Œnumber”jwŒpages”Œ1--24”Œdoi”Œ10.1029/1998TC001088”Œ//url”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/1998TC001088”Œ//eprint”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/1998TC001088”Œabstract”X6{G}lobal {P}ositioning {S}ystem ({GPS}) data from five sites on the stable interior of the {S}ierra {N}evada block are inverted to describe its angular velocity relative to stable {N}orth {A}merica. The velocity data for the five sites fit the rigid block model with rms misfits of 0.3 mm/yr (north) and 0.8 mm/yr (east), smaller than independently estimated data uncertainty, indicating that the rigid block model is appropriate. The new {E}uler vector, 17.0°N, 137.3°W, rotation rate 0.28 degrees per million years, predicts that the block is translating to the northwest, nearly parallel to the plate motion direction, at 13--14 mm/yr, faster than previous estimates. Using the predicted {S}ierra {N}evada block velocity as a kinematic boundary condition and {GPS}, {VLBI} and other data from the interior and margins of the {B}asin and {R}ange, we estimate the velocities of some major boundary zone faults. For a transect approximately perpendicular to plate motion through northern {O}wens {V}alley, the eastern {C}alifornia shear zone (western boundary of the {B}asin and {R}ange province) accommodates 11±1 mm/yr of right-lateral shear primarily on two faults, the {O}wens {V}alley-{W}hite {M}ountain (3±2 mm/yr) and {F}ish {L}ake {V}alley (8±2 mm/yr) fault zones, based on a viscoelastic coupling model that accounts for the effects of the 1872 {O}wens {V}alley earthquake and the rheology of the lower crust. Together these two faults, separated by less than 50 km on this transect, define a region of high surface velocity gradient on the eastern boundary of the {S}ierra {N}evada block. The {W}asatch {F}ault zone accommodates less than 3±1 mm/yr of east-west extension on the eastern boundary of the {B}asin and {R}ange province. Remaining deformation within the {B}asin and {R}ange interior is also probably less than 3 mm/yr.”Œyear”Œ2000”ujQCjSC)R”(jëFŒtitle”jíFŒjournal”jïFŒvolume”jñFŒnumber”jòFŒpages”jôFŒdoi”jöFŒ//url”jøFŒ//eprint”júFŒabstract”jüFŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒTimothy”ajmC]”ŒH.”ajoC]”jqC]”ŒDixon”ajtC]”ubjgC)”}”(jjC]”ŒMeghan”ajmC]”joC]”jqC]”ŒMiller”ajtC]”ubjgC)”}”(jjC]”ŒFrederic”ajmC]”joC]”jqC]”ŒFarina”ajtC]”ubjgC)”}”(jjC]”ŒHongzhi”ajmC]”joC]”jqC]”ŒWang”ajtC]”ubjgC)”}”(jjC]”ŒDaniel”ajmC]”joC]”jqC]”ŒJohnson”ajtC]”ubesjQCjSC)R”j GŒauthor”subjŠCj CubŒdong_and_bock_1989”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œ‡{G}lobal {P}ositioning {S}ystem Network analysis with phase ambiguity resolution applied to crustal deformation studies in {C}alifornia”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ94”Œnumber”ŒB4”Œpages”Œ 3949-3966”Œdoi”Œ10.1029/JB094iB04p03949”Œ//url”ŒGhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/JB094iB04p03949”Œ//eprint”ŒGhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/JB094iB04p03949”Œabstract”X˜A 5-year campaign is in progress in central and southern California to monitor tectonic motions using observations of the Global Positioning System (GPS) satellites. Evidence from geological and space-geodetic data indicates that significant horizontal deformations of order 10 mm/yr are occurring west of the San Andreas fault along the California margin. We demonstrate, using data from initial epoch measurements in January 1987, that the goal of measuring horizontal deformations with an accuracy of 5 mm/yr over the duration of the campaign should be readily achievable. The GPS network was designed to span a wide range of baseline lengths within California and across North America to aid in phase ambiguity resolution, an important factor in achieving highest-accuracy baseline determinations. We present an efficient algorithm for multisession network analysis of GPS data with simultaneous orbit determination and ambiguity resolution. Using this algorithm with the California data, we demonstrate the improvement obtained in station position and satellite orbit estimation when the phase ambiguities are resolved. We demonstrate several millimeters +1 part in 108 short-term repeatability over five single-session (daily) analyses for horizontal baseline components and length and several tens of millimeters for the vertical. Comparison with the independently determined very long baseline interferometry baseline between Mojave and Owens Valley suggests that the accuracy is at the same level as the repeatability. We show that simultaneous multisession analyses with ambiguity resolution improve the baseline and satellite orbit estimates compared to the single-session analyses. With the single-session analyses we were able to resolve all phase ambiguities on baselines within California. With the multisession analyses we were able to resolve the phase ambiguities for most of the network, over regional and continental scales.”•Œyear”Œ1989”ujQCjSC)R”(jFGŒtitle”jHGŒjournal”jJGŒvolume”jLGŒnumber”jNGŒpages”jPGŒdoi”jRGŒ//url”jTGŒ//eprint”jVGŒabstract”jXGŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒDa-Nan”ajmC]”joC]”jqC]”ŒDong”ajtC]”ubjgC)”}”(jjC]”ŒYehuda”ajmC]”joC]”jqC]”ŒBock”ajtC]”ubesjQCjSC)R”jhGŒauthor”subjŠCj CubŒdong_et_al_1998”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œyear”Œ1998”Œtitle”ŒYEstimating regional deformation from a combination of space and terrestrial geodetic data”Œjournal”ŒJournal of Geodesy”Œpages”Œ200--214”Œvolume”Œ72”Œissue”Œ4”Œabstract”XWe discuss an approach for efficiently combining different types of geodetic data to estimate time-dependent motions of stations in a region of active deformation. The primary observations are analyzed separately to produce loosely constrained estimates of station positions and coordinate system parameters which are then combined with appropriate constraints to estimate velocities and coseismic displacements. We define noninteger degrees of freedom to handle the case of finite constraints and stochastic perturbation of parameters and develop statistical tests for determining compatibility between different data sets. With these developments, we show an example of combining space and terrestrial geodetic data to obtain the deformation field in southern {C}alifornia.”Œissn”Œ 1432-1394”Œ//url”Œ%https://doi.org/10.1007/s001900050161”Œdoi”Œ10.1007/s001900050161”ujQCjSC)R”(j†GŒyear”jˆGŒtitle”jŠGŒjournal”jŒGŒpages”jŽGŒvolume”jGŒissue”j’GŒabstract”j”GŒissn”j–GŒ//url”j˜GŒdoi”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒD.”ajmC]”joC]”jqC]”ŒDong”ajtC]”ubjgC)”}”(jjC]”ŒT.”ajmC]”ŒA.”ajoC]”jqC]”ŒHerring”ajtC]”ubjgC)”}”(jjC]”ŒR.”ajmC]”ŒW.”ajoC]”jqC]”ŒKing”ajtC]”ubesjQCjSC)R”j¨GŒauthor”subjŠCj CubŒfeigl_et_al_1993”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”ŒbSpace geodetic measurement of crustal deformation in central and southern {C}alifornia, 1984--1992”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ98”Œnumber”ŒB12”Œpages”Œ 21677-21712”Œdoi”Œ10.1029/93JB02405”Œ\\url”ŒAhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/93JB02405”Œ\\eprint”ŒAhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/93JB02405”Œabstract”XÇ We estimate the velocity field in central and southern California using Global Positioning System (GPS) observations from 1986 to 1992 and very long baseline interferometry (VLBI) observations from 1984 to 1991. Our core network includes 12 GPS sites spaced approximately 50 km apart, mostly in the western Transverse Ranges and the coastal Borderlands. The precision and accuracy of the relative horizontal velocities estimated for these core stations are adequately described by a 95\% confidence ellipse with a semiminor axis of approximately 2 mm/yr oriented roughly north-south, and a semimajor axis of approximately 3 mm/yr oriented east-west. For other stations, occupied fewer than 5 times, or occupied during experiments with poor tracking geometries, the uncertainty is larger. These uncertainties are calibrated by analyzing the scatter in three types of comparisons: (1) multiple measurements of relative position ("repeatability"), (2) independent velocity estimates from separate analyses of the GPS and VLBI data, and (3) rates of change in baseline length estimated from the joint GPS+VLBI solution and from a comparison of GPS with trilateration. The dominant tectonic signature in the velocity field is shear deformation associated with the San Andreas and Garlock faults, which we model as resulting from slip below a given locking depth. Removing the effects of this simple model from the observed velocity field reveals residual deformation that is not attributable to the San Andreas fault. Baselines spanning the eastern Santa Barbara Channel, the Ventura basin, the Los Angeles basin, and the Santa Maria Fold and Thrust Belt are shortening at rates of up to 5 ± 1, 5 ± 1, 5 ± 1, and 2 ± 1 mm/yr, respectively. North of the Big Bend, some compression normal to the trace of the San Andreas fault can be resolved on both sides of the fault. The rates of rotation about vertical axes in the residual geodetic velocity field differ by up to a factor of 2 from those inferred from paleomagnetic declinations. Our estimates indicate that the "San Andreas discrepancy" can be resolved to within the 3 mm/yr uncertainties by accounting for deformation in California between Vandenberg (near Point Conception) and the westernmost {B}asin and {R}ange. Strain accumulation of 1–2 mm/yr on structures offshore of Vandenberg is also allowed by the uncertainties. South of the Transverse Ranges, the deformation budget must include 5 mm/yr between the offshore islands and the mainland.”Œyear”Œ1993”ujQCjSC)R”(jÑGŒtitle”jÓGŒjournal”jÕGŒvolume”j×GŒnumber”jÙGŒpages”jÛGŒdoi”jÝGŒ\\url”jßGŒ\\eprint”jáGŒabstract”jãGŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒKurt”ajmC]”ŒL.”ajoC]”jqC]”ŒFeigl”ajtC]”ubjgC)”}”(jjC]”ŒDuncan”ajmC]”ŒC.”ajoC]”jqC]”ŒAgnew”ajtC]”ubjgC)”}”(jjC]”ŒYehuda”ajmC]”joC]”jqC]”ŒBock”ajtC]”ubjgC)”}”(jjC]”ŒDanan”ajmC]”joC]”jqC]”ŒDong”ajtC]”ubjgC)”}”(jjC]”ŒAndrea”ajmC]”joC]”jqC]”Œ Donnellan”ajtC]”ubjgC)”}”(jjC]”ŒBradford”ajmC]”ŒH.”ajoC]”jqC]”ŒHager”ajtC]”ubjgC)”}”(jjC]”ŒThomas”ajmC]”ŒA.”ajoC]”jqC]”ŒHerring”ajtC]”ubjgC)”}”(jjC]”ŒDavid”ajmC]”ŒD.”ajoC]”jqC]”ŒJackson”ajtC]”ubjgC)”}”(jjC]”ŒThomas”ajmC]”ŒH.”ajoC]”jqC]”ŒJordan”ajtC]”ubjgC)”}”(jjC]”ŒRobert”ajmC]”ŒW.”ajoC]”jqC]”ŒKing”ajtC]”ubjgC)”}”(jjC]”ŒShawn”ajmC]”joC]”jqC]”ŒLarsen”ajtC]”ubjgC)”}”(jjC]”ŒKristine”ajmC]”ŒM.”ajoC]”jqC]”ŒLarson”ajtC]”ubjgC)”}”(jjC]”ŒMark”ajmC]”ŒH.”ajoC]”jqC]”ŒMurray”ajtC]”ubjgC)”}”(jjC]”Œ Zhengkang”ajmC]”joC]”jqC]”ŒShen”ajtC]”ubjgC)”}”(jjC]”ŒFrank”ajmC]”ŒH.”ajoC]”jqC]”ŒWebb”ajtC]”ubesjQCjSC)R”jóGŒauthor”subjŠCjCubŒ feigl_1991”j1C)”}”(j4CŒ phdthesis”j6CŒ phdthesis”j8Cj*C)”}”(j-C}”(Œtitle”ŒDGeodetic measurement of tectonic deformation in central {C}alifornia”Œschool”Œ%Massachusetts Institute of Technology”Œyear”Œ1991”Œtype”ŒThesis”Œaddress”hoŒmonth”hoŒnote”hoŒannote”houjQCjSC)R”(jHŒtitle”j’HŒschool”j”HŒyear”j–HŒtype”j˜HŒaddress”j™HŒmonth”jšHŒnote”j›HŒannote”uubj`Cj*C)”}”(j-C}”Œauthor”]”jgC)”}”(jjC]”ŒKurt”ajmC]”ŒLewis”ajoC]”jqC]”ŒFeigl”ajtC]”ubasjQCjSC)R”j¨HŒauthor”subjŠCjCubŒherring_et_al_1990”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œ€Geodesy by radio interferometry: The application of {K}alman Filtering to the analysis of very long baseline interferometry data”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ95”Œnumber”ŒB8”Œpages”Œ 12561--12581”Œdoi”Œ10.1029/JB095iB08p12561”Œ//url”ŒGhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/JB095iB08p12561”Œ//eprint”ŒGhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/JB095iB08p12561”Œabstract”XRWe discuss the application of {K}alman filtering techniques to the analysis of very long baseline interferometry ({VLBI}) data. The {VLBI} observables are geometrically related to the geodetic and astrometric parameters which can be determined from them. However, contributions to the observables from the clocks at, and the atmospheres above, the {VLBI} sites must be accounted for if reliable estimates of geodetic and astrometric parameters are to be obtained. Here an implementation of a {K}alman filter to account for stochastic behavior on those parameters which vary during the course of a {VLBI} experiment is discussed. Both the nature of the stochastic processes which should be used in the model for the {VLBI} data and the implementation of the {K}alman filter estimator are considered. From the results obtained, we conclude that the {K}alman filter is appropriate for analyzing {VLBI} data. The choice of stochastic model does not unduly affect the estimates of the geodetic parameters and the quality of these estimates is higher than that for conventional weighted least squares estimators.”Œyear”Œ1990”ujQCjSC)R”(j¾HŒtitle”jÀHŒjournal”jÂHŒvolume”jÄHŒnumber”jÆHŒpages”jÈHŒdoi”jÊHŒ//url”jÌHŒ//eprint”jÎHŒabstract”jÐHŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒThomas”ajmC]”ŒA.”ajoC]”jqC]”ŒHerring”ajtC]”ubjgC)”}”(jjC]”ŒJames”ajmC]”ŒL.”ajoC]”jqC]”ŒDavis”ajtC]”ubjgC)”}”(jjC]”ŒIrwin”ajmC]”ŒI.”ajoC]”jqC]”ŒShapiro”ajtC]”ubesjQCjSC)R”jàHŒauthor”subjŠCjCubŒ kouba_2009”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œyear”Œ2009”Œtitle”Œ>A simplified yaw-attitude model for eclipsing {GPS} satellites”Œjournal”Œ{GPS} Solutions”Œpages”Œ1--12”Œvolume”Œ13”Œissue”jwŒabstract”XwA simplified yaw-attitude modeling, consistent with {B}ar-{S}ever (1996), has been implemented and tested in the {NRC}an {PPP} software. For {B}lock {IIR} {GPS} satellite it is possible to model yaw-attitude control during eclipsing periods by using the constant hardware yaw rate of 0.20°/s. The {B}lock {IIR} satellites maintain the nominal yaw attitude even during a shadow crossing ({Y}. {E}. {B}ar-{S}ever, private communication, 2007), except for the noon and shadow midnight turn maneuvers, both of which can be modeled and last up to 15 min. Thus, for {B}lock {IIR} satellites it is possible to maintain continuous satellite clock estimation even during eclipsing periods. For the {B}lock {II}/{IIA} satellites, it is possible to model satisfactorily the noon turns and also shadow crossing, thanks to the permanent positive yaw bias of 0.5°, implemented in {N}ovember 1995. However, in order to model the {B}lock {II}/{IIA} shadow crossings, satellite specific yaw rates should be used, either solved for or averaged yaw-rate solutions. These yaw rates as estimated by the {J}et {P}ropulsion {L}aboratory ({JPL}) can differ significantly from the nominal hardware values. The {B}lock {II}/{IIA} post-shadow recovery periods, which last about 30 min, should be considered uncertain and cannot be properly modeled. Data from post-shadow recovery periods should, therefore, not be used in precise global {GPS} analyses ({B}ar-{S}ever 1996). For high-precision applications, it is essential that users implement a yaw-attitude model, which is consistent with the generation of the satellite clocks. Initial testing and analyses, based on the {IGS} and {AC} {F}inal orbits and clocks have revealed that during eclipsing periods, significant inconsistencies in yaw-attitude modeling still exist amongst the {IGS} {A}nalyses {C}enters, which contribute to the errors of the {IGS} {F}inal clock combinations.”Œissn”Œ 1521-1886”Œ//url”Œ)https://doi.org/10.1007/s10291-008-0092-1”Œdoi”Œ10.1007/s10291-008-0092-1”ujQCjSC)R”(j IŒyear”j IŒtitle”jIŒjournal”jIŒpages”jIŒvolume”jIŒissue”jIŒabstract”jIŒissn”jIŒ//url”jIŒdoi”uubj`Cj*C)”}”(j-C}”Œauthor”]”jgC)”}”(jjC]”ŒJ.”ajmC]”joC]”jqC]”ŒKouba”ajtC]”ubasjQCjSC)R”j+IŒauthor”subjŠCjCubŒlagler_et_al_2013”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”ŒG{GPT}2: Empirical slant delay model for radio space geodetic techniques”Œjournal”ŒGeophysical Research Letters”Œvolume”Œ40”Œnumber”jFDŒpages”Œ 1069--1073”Œkeywords”Œ8Tropospheric delay, GNSSl, Tropospheric mapping function”Œdoi”Œ10.1002/grl.50288”Œ//url”ŒAhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1002/grl.50288”Œ//eprint”ŒAhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1002/grl.50288”Œabstract”XUp to now, state-of-the-art empirical slant delay modeling for processing observations from radio space geodetic techniques has been provided by a combination of two empirical models. These are {GPT} ({G}lobal {P}ressure and {T}emperature) and {GMF} ({G}lobal {M}apping {F}unction), both operating on the basis of long-term averages of surface values from numerical weather models. Weaknesses in {GPT}/{GMF}, specifically their limited spatial and temporal variability, are largely eradicated by a new, combined model {GPT}2, which provides pressure, temperature, lapse rate, water vapor pressure, and mapping function coefficients at any site, resting upon a global 5° grid of mean values, annual, and semi-annual variations in all parameters. Built on {ERA}-{I}nterim data, {GPT}2 brings forth improved empirical slant delays for geophysical studies. Compared to {GPT}/{GMF}, {GPT}2 yields a 40\% reduction of annual and semi-annual amplitude differences in station heights with respect to a solution based on instantaneous local pressure values and the {V}ienna mapping functions 1, as shown with a series of global {VLBI} ({V}ery {L}ong {B}aseline {I}nterferometry) solutions.”Œyear”Œ2013”ujQCjSC)R”(j@IŒtitle”jBIŒjournal”jDIŒvolume”jFIŒnumber”jGIŒpages”jIIŒkeywords”jKIŒdoi”jMIŒ//url”jOIŒ//eprint”jQIŒabstract”jSIŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒK.”ajmC]”joC]”jqC]”ŒLagler”ajtC]”ubjgC)”}”(jjC]”ŒM.”ajmC]”joC]”jqC]”Œ Schindelegger”ajtC]”ubjgC)”}”(jjC]”ŒJ.”ajmC]”joC]”jqC]”ŒBöhm”ajtC]”ubjgC)”}”(jjC]”ŒH.”ajmC]”joC]”jqC]”ŒKr{\'a}sn{\'a}”ajtC]”ubjgC)”}”(jjC]”ŒT.”ajmC]”joC]”jqC]”ŒNilsson”ajtC]”ubesjQCjSC)R”jdIŒauthor”subjŠCjCubŒmao_et_al_1999”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œ%Noise in {GPS} coordinate time series”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ104”Œnumber”ŒB2”Œpages”Œ 2797--2816”Œdoi”Œ10.1029/1998JB900033”Œ//url”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/1998JB900033”Œ//eprint”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/1998JB900033”Œabstract”X÷We assess the noise characteristics in time series of daily position estimates for 23 globally distributed {G}lobal {P}ositioning {S}ystem ({GPS}) stations with 3 years of data, using spectral analysis and {M}aximum {L}ikelihood {E}stimation. A combination of white noise and flicker noise appears to be the best model for the noise characteristics of all three position components. Both white and flicker noise amplitudes are smallest in the north component and largest in the vertical component. The white noise part of the vertical component is higher for tropical stations (±23° latitude) compared to midlatitude stations. Velocity error in a {GPS} coordinate time series may be underestimated by factors of 5--11 if a pure white noise model is assumed.”Œyear”Œ1999”ujQCjSC)R”(jIŒtitle”jŸIŒjournal”j¡IŒvolume”j£IŒnumber”j¥IŒpages”j§IŒdoi”j©IŒ//url”j«IŒ//eprint”j­IŒabstract”j¯IŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒAilin”ajmC]”joC]”jqC]”ŒMao”ajtC]”ubjgC)”}”(jjC]”Œ Christopher”ajmC]”(ŒG.”ŒA.”ejoC]”jqC]”ŒHarrison”ajtC]”ubjgC)”}”(jjC]”ŒTimothy”ajmC]”ŒH.”ajoC]”jqC]”ŒDixon”ajtC]”ubesjQCjSC)R”j¿IŒauthor”subjŠCjCubŒmccaffrey_et_al_2007”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”ŒT{Fault locking, block rotation and crustal deformation in the {P}acific {N}orthwest}”Œjournal”Œ!Geophysical Journal International”Œvolume”Œ169”Œnumber”jNEŒpages”Œ 1315--1340”Œyear”Œ2007”Œmonth”Œ06”Œabstract”XØ {We interpret {G}lobal {P}ositioning {S}ystem ({GPS}) measurements in the northwestern United States and adjacent parts of western Canada to describe relative motions of crustal blocks, locking on faults and permanent deformation associated with convergence between the Juan de Fuca and North American plates. To estimate angular velocities of the oceanic Juan de Fuca and Explorer plates and several continental crustal blocks, we invert the GPS velocities together with seafloor spreading rates, earthquake slip vector azimuths and fault slip azimuths and rates. We also determine the degree to which faults are either creeping aseismically or, alternatively, locked on the block-bounding faults. The Cascadia subduction thrust is locked mainly offshore, except in central Oregon, where locking extends inland. Most of Oregon and southwest Washington rotate clockwise relative to North America at rates of 0.4–1.0 ° Myr−1. No shear or extension along the Cascades volcanic arc has occurred at the mm/yr level during the past decade, suggesting that the shear deformation extending northward from the Walker Lane and eastern California shear zone south of Oregon is largely accommodated by block rotation in Oregon. The general agreement of vertical axis rotation rates derived from GPS velocities with those estimated from palaeomagnetic declination anomalies suggests that the rotations have been relatively steady for 10–15 Ma. Additional permanent dextral shear is indicated within the Oregon Coast Range near the coast. Block rotations in the Pacific Northwest do not result in net westward flux of crustal material—the crust is simply spinning and not escaping. On Vancouver Island, where the convergence obliquity is less than in Oregon and Washington, the contractional strain at the coast is more aligned with Juan de Fuca—North America motion. GPS velocities are fit significantly better when Vancouver Island and the southern Coast Mountains move relative to North America in a block-like fashion. The relative motions of the Oregon, western Washington and Vancouver Island crustal blocks indicate that the rate of permanent shortening, the type that causes upper plate earthquakes, across the Puget Sound region is 4.4 ± 0.3 mm yr−1. This shortening is likely distributed over several faults but GPS data alone cannot determine the partitioning of slip on them. The transition from predominantly shear deformation within the continent south of the Mendocino Triple Junction to predominantly block rotations north of it is similar to changes in tectonic style at other transitions from shear to subduction. This similarity suggests that crustal block rotations are enhanced in the vicinity of subduction zones possibly due to lower resisting stress.}”Œissn”Œ 0956-540X”Œdoi”Œ 10.1111/j.1365-246X.2007.03371.x”Œ//url”Œ0https://doi.org/10.1111/j.1365-246X.2007.03371.x”Œ//eprint”ŒRhttps://academic.oup.com/gji/article-pdf/169/3/1315/40633401/gji\_169\_3\_1315.pdf”ujQCjSC)R”(jéIŒtitle”jëIŒjournal”jíIŒvolume”jïIŒnumber”jðIŒpages”jòIŒyear”jôIŒmonth”jöIŒabstract”jøIŒissn”júIŒdoi”jüIŒ//url”jþIŒ//eprint”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒRobert”ajmC]”joC]”jqC]”Œ McCaffrey”ajtC]”ubjgC)”}”(jjC]”ŒAnthony”ajmC]”ŒI.”ajoC]”jqC]”ŒQamar”ajtC]”ubjgC)”}”(jjC]”ŒRobert”ajmC]”ŒW.”ajoC]”jqC]”ŒKing”ajtC]”ubjgC)”}”(jjC]”ŒRay”ajmC]”joC]”jqC]”ŒWells”ajtC]”ubjgC)”}”(jjC]”ŒGiorgi”ajmC]”joC]”jqC]”Œ Khazaradze”ajtC]”ubjgC)”}”(jjC]”ŒCharles”ajmC]”ŒA.”ajoC]”jqC]”ŒWilliams”ajtC]”ubjgC)”}”(jjC]”ŒColleen”ajmC]”ŒW.”ajoC]”jqC]”ŒStevens”ajtC]”ubjgC)”}”(jjC]”ŒJesse”ajmC]”ŒJ.”ajoC]”jqC]”ŒVollick”ajtC]”ubjgC)”}”(jjC]”ŒPeter”ajmC]”ŒC.”ajoC]”jqC]”ŒZwick”ajtC]”ubesjQCjSC)R”jJŒauthor”subjŠCjCubŒmcclusky_et_al_2000”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œz{G}lobal {P}ositioning {S}ystem constraints on plate kinematics and dynamics in the eastern {M}editerranean and {C}aucasus”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ105”Œnumber”ŒB3”Œpages”Œ 5695--5719”Œdoi”Œ10.1029/1999JB900351”Œ//url”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/1999JB900351”Œ//eprint”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/1999JB900351”Œabstract”XWe present and interpret Global Positioning System (GPS) measurements of crustal motions for the period 1988–1997 at 189 sites extending east-west from the Caucasus mountains to the Adriatic Sea and north-south from the southern edge of the Eurasian plate to the northern edge of the African plate. Sites on the northern Arabian platform move 18±2 mm/yr at N25°±5°W relative to Eurasia, less than the NUVEL-1A circuit closure rate (25±1 mm/yr at N21°±7°W). Preliminary motion estimates (1994–1997) for stations located in Egypt on the northeastern part of Africa show northward motion at 5–6±2 mm/yr, also slower than NUVEL-IA estimates (10±1 mm/yr at N2°±4°E). Eastern Turkey is characterized by distributed deformation, while central Turkey is characterized by coherent plate motion (internal deformation of <2 mm/yr) involving westward displacement and counterclockwise rotation of the Anatolian plate. The Anatolian plate is de-coupled from Eurasia along the right-lateral, strike-slip North Anatolian fault (NAF). We derive a best fitting Euler vector for Anatolia-Eurasia motion of 30.7°± 0.8°N, 32.6°± 0.4°E, 1.2°±0.1°/Myr. The Euler vector gives an upper bound for NAF slip rate of 24±1 mm/yr. We determine a preliminary GPS Arabia-Anatolia Euler vector of 32.9°±1.2°N, 40.3°±1.1°E, 0.8°±0.2°/Myr and an upper bound on left-lateral slip on the East Anatolian fault (EAF) of 9±1 mm/yr. The central and southern Aegean is characterized by coherent motion (internal deformation of <2 mm/yr) toward the SW at 30±1 mm/yr relative to Eurasia. Stations in the SE Aegean deviate significantly from the overall motion of the southern Aegean, showing increasing velocities toward the trench and reaching 10±1 mm/yr relative to the southern Aegean as a whole.”Œyear”Œ2000”ujQCjSC)R”(jsJŒtitle”juJŒjournal”jwJŒvolume”jyJŒnumber”j{JŒpages”j}JŒdoi”jJŒ//url”jJŒ//eprint”jƒJŒabstract”j…JŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒS.”ajmC]”joC]”jqC]”ŒMcClusky”ajtC]”ubjgC)”}”(jjC]”ŒS.”ajmC]”joC]”jqC]”Œ Balassanian”ajtC]”ubjgC)”}”(jjC]”ŒA.”ajmC]”joC]”jqC]”ŒBarka”ajtC]”ubjgC)”}”(jjC]”ŒC.”ajmC]”joC]”jqC]”ŒDemir”ajtC]”ubjgC)”}”(jjC]”ŒS.”ajmC]”joC]”jqC]”ŒErgintav”ajtC]”ubjgC)”}”(jjC]”ŒI.”ajmC]”joC]”jqC]”ŒGeorgiev”ajtC]”ubjgC)”}”(jjC]”ŒO.”ajmC]”joC]”jqC]”ŒGurkan”ajtC]”ubjgC)”}”(jjC]”ŒM.”ajmC]”joC]”jqC]”Œ Hamburger”ajtC]”ubjgC)”}”(jjC]”ŒK.”ajmC]”joC]”jqC]”ŒHurst”ajtC]”ubjgC)”}”(jjC]”ŒH.”ajmC]”joC]”jqC]”ŒKahle”ajtC]”ubjgC)”}”(jjC]”ŒK.”ajmC]”joC]”jqC]”ŒKastens”ajtC]”ubjgC)”}”(jjC]”ŒG.”ajmC]”joC]”jqC]”Œ Kekelidze”ajtC]”ubjgC)”}”(jjC]”ŒR.”ajmC]”joC]”jqC]”ŒKing”ajtC]”ubjgC)”}”(jjC]”ŒV.”ajmC]”joC]”jqC]”ŒKotzev”ajtC]”ubjgC)”}”(jjC]”ŒO.”ajmC]”joC]”jqC]”ŒLenk”ajtC]”ubjgC)”}”(jjC]”ŒS.”ajmC]”joC]”jqC]”ŒMahmoud”ajtC]”ubjgC)”}”(jjC]”ŒA.”ajmC]”joC]”jqC]”ŒMishin”ajtC]”ubjgC)”}”(jjC]”ŒM.”ajmC]”joC]”jqC]”ŒNadariya”ajtC]”ubjgC)”}”(jjC]”ŒA.”ajmC]”joC]”jqC]”ŒOuzounis”ajtC]”ubjgC)”}”(jjC]”ŒD.”ajmC]”joC]”jqC]”Œ Paradissis”ajtC]”ubjgC)”}”(jjC]”ŒY.”ajmC]”joC]”jqC]”ŒPeter”ajtC]”ubjgC)”}”(jjC]”ŒM.”ajmC]”joC]”jqC]”ŒPrilepin”ajtC]”ubjgC)”}”(jjC]”ŒR.”ajmC]”joC]”jqC]”Œ Reilinger”ajtC]”ubjgC)”}”(jjC]”ŒI.”ajmC]”joC]”jqC]”ŒSanli”ajtC]”ubjgC)”}”(jjC]”ŒH.”ajmC]”joC]”jqC]”ŒSeeger”ajtC]”ubjgC)”}”(jjC]”ŒA.”ajmC]”joC]”jqC]”ŒTealeb”ajtC]”ubjgC)”}”(jjC]”ŒM.”ajmC]”ŒN.”ajoC]”jqC]”Œ Toks{\"o}z”ajtC]”ubjgC)”}”(jjC]”ŒG.”ajmC]”joC]”jqC]”ŒVeis”ajtC]”ubesjQCjSC)R”j•JŒauthor”subjŠCjCubŒmontenbruck_et_al_2015”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”Œ-{GNSS} satellite geometry and attitude models”Œjournal”ŒAdvances in Space Research”Œvolume”Œ56”Œnumber”jFDŒpages”Œ 1015--1029”Œyear”Œ2015”Œissn”Œ 0273-1177”Œdoi”Œ10.1016/j.asr.2015.06.019”Œ//url”ŒChttps://www.sciencedirect.com/science/article/pii/S0273117715004378”Œkeywords”Œ=GNSS satellites, Attitude models, Antenna offsets, ANTEX, SLR”Œabstract”X8This article discusses the attitude modes employed by present {G}lobal (and {R}egional) {N}avigation {S}atellite {S}ystems ({GNSS}s) and the models used to describe them along with definitions of the constellation-specific spacecraft body frames. A uniform convention for the labeling of the principal spacecraft axes is proposed by the {I}nternational {GNSS} {S}ervice ({IGS}), which results in a common formulation of the nominal attitude of all {GNSS} satellites in yaw-steering mode irrespective of their specific orbit and constellation. The conventions defined within this document provide the basis for the specification of antenna phase center offsets and variations in a multi-{GNSS} version of the {IGS} absolute phase center model in the {ANTEX} (antenna exchange) format. To facilitate the joint analysis of {GNSS} observations and satellite laser ranging measurements, laser retroreflector array coordinates consistent with the {IGS}-specific spacecraft frame conventions are provided in addition to representative antenna offset values for all {GNSS} constellations.”ujQCjSC)R”(jžKŒtitle”j KŒjournal”j¢KŒvolume”j¤KŒnumber”j¥KŒpages”j§KŒyear”j©KŒissn”j«KŒdoi”j­KŒ//url”j¯KŒkeywords”j±KŒabstract”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒO.”ajmC]”joC]”jqC]”Œ Montenbruck”ajtC]”ubjgC)”}”(jjC]”ŒR.”ajmC]”joC]”jqC]”ŒSchmid”ajtC]”ubjgC)”}”(jjC]”ŒF.”ajmC]”joC]”jqC]”ŒMercier”ajtC]”ubjgC)”}”(jjC]”ŒP.”ajmC]”joC]”jqC]”Œ Steigenberger”ajtC]”ubjgC)”}”(jjC]”ŒC.”ajmC]”joC]”jqC]”ŒNoll”ajtC]”ubjgC)”}”(jjC]”ŒR.”ajmC]”joC]”jqC]”ŒFatkulin”ajtC]”ubjgC)”}”(jjC]”ŒS.”ajmC]”joC]”jqC]”ŒKogure”ajtC]”ubjgC)”}”(jjC]”ŒA.S.”ajmC]”joC]”jqC]”ŒGaneshan”ajtC]”ubesjQCjSC)R”jÂKŒauthor”subjŠCjCubŒpetrie_et_al_2010”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”ŒLHigher-order ionospheric effects on the {GPS} reference frame and velocities”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ115”Œnumber”ŒB3”Œpages”hoŒkeywords”Œ9higher-order ionospheric, reference frame, vertical rates”Œdoi”Œ10.1029/2009JB006677”Œ//url”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2009JB006677”Œ//eprint”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2009JB006677”Œabstract”XóWe describe how {GPS} time series are influenced by higher-order ionospheric effects over the last solar cycle (1995--2008) and examine implications for geophysical studies. Using 14 years of globally reprocessed solutions, we demonstrate the effect on the reference frame. Including second- and third-order ionospheric terms causes up to 10 mm difference in the smoothed transformation to the {I}nternational {T}errestrial {R}eference {F}rame ({ITRF}) 2005, with the {Z} translation term dominant. Scale is also slightly affected, with a change of up to ∼0.05 ppb. After transformation to {ITRF}2005, residual effects on vertical site velocities are as high as 0.34 mm yr−1. We assess the effect of the magnetic field model on the second-order term and find a time-varying difference of 0–2 mm in the {Z} translation. We also assess the effect of omitting the third-order term. We find that while the second-order term is responsible for almost all the {Z} translation effects, it is the combination of the second- and third-order terms that causes the effect on scale. Comparison of our {GPS} reprocessing with {ITRF}2005 suggests that {GPS} origin rates may vary with time period. For example, we find {Z} translation rates of −0.82 ± 0.17 mm yr−1 for 1995--2008 and 0.17 ± 0.24 mm yr−1 for 1995--2005. If {GPS} were to contribute to origin rate definition for future {ITRF}s, higher-order ionospheric corrections would need to be applied due to their effect on translation parameters during solar maximum.”Œyear”Œ2010”ujQCjSC)R”(jLŒtitle”jLŒjournal”jLŒvolume”jLŒnumber”jLŒpages”jLŒkeywords”j!LŒdoi”j#LŒ//url”j%LŒ//eprint”j'LŒabstract”j)LŒyear”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”Œ Elizabeth”ajmC]”ŒJ.”ajoC]”jqC]”ŒPetrie”ajtC]”ubjgC)”}”(jjC]”ŒMatt”ajmC]”ŒA.”ajoC]”jqC]”ŒKing”ajtC]”ubjgC)”}”(jjC]”ŒPhilip”ajmC]”joC]”jqC]”ŒMoore”ajtC]”ubjgC)”}”(jjC]”ŒDavid”ajmC]”ŒA.”ajoC]”jqC]”Œ Lavall{\'e}e”ajtC]”ubesjQCjSC)R”j:LŒauthor”subjŠCjCubŒschaffrin_and_bock_1988”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œyear”Œ1988”Œtitle”ŒBA unified scheme for processing {GPS} dual-band phase observations”Œjournal”ŒBulletin g{\'e}od{\'e}sique”Œpages”Œ142-160”Œvolume”Œ62”Œnumber”Œ2”Œabstract”XLA unified computational scheme is presented for sequential least-squares processing ofGPS dual-band carrier-beat-phase observations in network-mode positioning with orbit relaxation, and in orbit determination applications. This scheme is applicable to any spatial and temporal distribution of stations and satellites during a particularGPS experiment. Full covariance matrices can be specified for carrier-beat-phases and for weighted constraints on the ionosphere in order to improve phase ambiguity resolution. Physically meaningful choices for these covariance matrices are developed.”Œissn”Œ 1432-1394”Œ//url”Œ"https://doi.org/10.1007/BF02519222”Œdoi”Œ10.1007/BF02519222”ujQCjSC)R”(jmLŒyear”joLŒtitle”jqLŒjournal”jsLŒpages”juLŒvolume”jwLŒnumber”jyLŒabstract”j{LŒissn”j}LŒ//url”jLŒdoi”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒBurkhard”ajmC]”joC]”jqC]”Œ Schaffrin”ajtC]”ubjgC)”}”(jjC]”ŒYehuda”ajmC]”joC]”jqC]”ŒBock”ajtC]”ubesjQCjSC)R”jLŒauthor”subjŠCjCubŒschmid_et_al_2007”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œyear”Œ2007”Œtitle”ŒkGeneration of a consistent absolute phase-center correction model for {GPS} receiver and satellite antennas”Œjournal”ŒJournal of Geodesy”Œpages”Œ781--798”Œvolume”Œ81”Œissue”Œ12”Œabstract”XÂThe development and numerical values of the new absolute phase-center correction model for {GPS} receiver and satellite antennas, as adopted by the {I}nternational {GNSS} (global navigation satellite systems) {S}ervice, are presented. Fixing absolute receiver antenna phase-center corrections to robot-based calibrations, the {G}eo{F}orschungs{Z}entrum {P}otsdam ({GFZ}) and the {T}echnische {U}niversit{\"a}t {M}{\"u}nchen reprocessed more than 10 years of {GPS} data in order to generate a consistent set of nadir-dependent phase-center variations ({PCV}s) and offsets in the z-direction pointing toward the {E}arth for all {GPS} satellites in orbit during that period. The agreement between the two solutions estimated by independent software packages is better than 1 mm for the {PCV}s and about 4 cm for the z-offsets. In addition, the long time-series facilitates the study of correlations of the satellite antenna corrections with several other parameters such as the global terrestrial scale or the orientation of the orbital planes with respect to the {S}un. Finally, completely reprocessed {GPS} solutions using different phase-center correction models demonstrate the benefits from switching from relative to absolute antenna phase-center corrections. For example, tropospheric zenith delay biases between {GPS} and very long baseline interferometry ({VLBI}), as well as the drift of the terrestrial scale, are reduced and the {GPS} orbit consistency is improved.”Œissn”Œ 1432-1394”Œ//url”Œ)https://doi.org/10.1007/s00190-007-0148-y”Œdoi”Œ10.1007/s00190-007-0148-y”ujQCjSC)R”(j­LŒyear”j¯LŒtitle”j±LŒjournal”j³LŒpages”jµLŒvolume”j·LŒissue”j¹LŒabstract”j»LŒissn”j½LŒ//url”j¿LŒdoi”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒRalf”ajmC]”joC]”jqC]”ŒSchmid”ajtC]”ubjgC)”}”(jjC]”ŒPeter”ajmC]”joC]”jqC]”Œ Steigenberger”ajtC]”ubjgC)”}”(jjC]”ŒGerd”ajmC]”joC]”jqC]”ŒGendt”ajtC]”ubjgC)”}”(jjC]”ŒMaorong”ajmC]”joC]”jqC]”ŒGe”ajtC]”ubjgC)”}”(jjC]”ŒMarkus”ajmC]”joC]”jqC]”Œ Rothacher”ajtC]”ubesjQCjSC)R”jÏLŒauthor”subjŠCjCubŒ williams_2003”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œyear”Œ2003”Œtitle”Œ^The effect of coloured noise on the uncertainties of rates estimated from geodetic time series”Œjournal”ŒJournal of Geodesy”Œpages”Œ483--494”Œvolume”Œ76”Œissue”Œ9”Œabstract”Xð{Until recently, it was typically assumed that only white noise was present in geodetic time series. However, several data sets have now provided evidence for the presence of power-law noise. The uncertainty of any rates estimated from such data sets is dependent on the error model assumed for the data. Here a general form for the covariance matrix for any power-law noise model is introduced and simple equations that relate the rate uncertainty to the noise amplitude, sampling frequency and length of the time series are empirically derived. In addition, equations to analyse data sets and obtain a rate uncertainty when computational speed is at a premium are provided. These equations are tested against previously published geodetic data sets.}”Œissn”Œ 1432-1394”Œ//url”Œ)https://doi.org/10.1007/s00190-002-0283-4”Œdoi”Œ10.1007/s00190-002-0283-4”ujQCjSC)R”(jMŒyear”j MŒtitle”j MŒjournal”jMŒpages”jMŒvolume”jMŒissue”jMŒabstract”jMŒissn”jMŒ//url”jMŒdoi”uubj`Cj*C)”}”(j-C}”Œauthor”]”jgC)”}”(jjC]”ŒS.”ajmC]”(ŒD.”ŒP.”ejoC]”jqC]”ŒWilliams”ajtC]”ubasjQCjSC)R”j*MŒauthor”subjŠCjCubŒziebart_et_al_2002”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”ŒJModeling Photon Pressure: The Key to High-precision {GPS} Satellite Orbits”Œjournal”Œ {GPS} World”Œvolume”Œ13”Œnumber”jwŒyear”Œ2002”Œpages”Œ43–-50”ujQCjSC)R”(jAMŒtitle”jCMŒjournal”jEMŒvolume”jGMŒnumber”jHMŒyear”jJMŒpages”uubj`Cj*C)”}”(j-C}”Œauthor”]”(jgC)”}”(jjC]”ŒMarek”ajmC]”joC]”jqC]”ŒZiebart”ajtC]”ubjgC)”}”(jjC]”ŒPaul”ajmC]”joC]”jqC]”ŒCross”ajtC]”ubjgC)”}”(jjC]”ŒSima”ajmC]”joC]”jqC]”ŒAdhya”ajtC]”ubesjQCjSC)R”jVMŒauthor”subjŠCjCubŒkreemer_et_al_2018”j1C)”}”(j4CŒarticle”j6CŒarticle”j8Cj*C)”}”(j-C}”(Œtitle”ŒbA Robust Estimation of the 3-{D} Intraplate Deformation of the {N}orth {A}merican Plate From {GPS}”Œjournal”Œ,Journal of Geophysical Research: Solid Earth”Œvolume”Œ123”Œnumber”Œ5”Œpages”Œ 4388--4412”Œdoi”Œ10.1029/2017JB015257”Œ//url”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/abs/10.1029/2017JB015257”Œ//eprint”ŒDhttps://agupubs.onlinelibrary.wiley.com/doi/pdf/10.1029/2017JB015257”Œabstract”XyAbstract Glacial isostatic adjustment (GIA) is the main cause of deformation in intraplate North America. Here we use up to 3,271 Global Positioning System station velocities to image this 3-D deformation across the entire plate. We apply a new robust strain rate estimation algorithm (median estimation of local deformation), which does not require the assumption that part of the plate is unaffected by GIA, an assumption we show to be false. Our results show extension in the area underneath the Laurentide ice sheet, contrasted with a semiannular belt of horizontal contraction of up to ~4 × 10−9 yr−1 around the former ice sheet. This contractional belt is kinematically linked to an ~1–2 mm yr−1 far-field horizontal motion directed toward the ice sheet. Our results, together with a new robustly imaged vertical velocity field, are consistent with GIA as the main cause of deformation, although the contractional strain rates around the former ice sheet and the far-field horizontal velocities are significantly higher than those predicted by the ICE6G\_C(VM5a) model. This finding suggests that our results, including the location of reversal in sign of horizontal motion relative to the ice sheet, will be useful to reevaluate the mantle viscosity structure used by GIA models. Besides the GIA-attributed deformation, we find almost no other region with significant strain accumulation. 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Ash.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒDetermination of ”sbjsbejCNKrubjqNŒ3”ubj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒYoaz”sbj/Nj*N)”}”jöMŒ E. Bar-Sever.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒA new model for ”sbjsbejCNKrubjqNjOubt””jN(jÉ‹jçMjCjðCj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒGerhard Beulter, Ivan”sbj/Nj*N)”}”jöMŒI. Mueller, and Ruth”sbj/Nj*N)”}”jöMŒ E. Neilan.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒThe ”sbjsbejCNKäubjqNŒ4”ubj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒGerhard Beulter, Ivan”sbj/Nj*N)”}”jöMŒI. Mueller, and Ruth”sbj/Nj*N)”}”jöMŒ E. Neilan.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒThe ”sbjsbejCNKäubjqNj³Oubt””jN(jÓ‹jçMjCj4Dj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒG.”sbj/Nj*N)”}”jöMŒ Beutler, E.”sbj/Nj*N)”}”jöMŒ Brockmann, W.”sbj/Nj*N)”}”jöMŒ Gurtner, U.”sbj/Nj*N)”}”jöMŒHugentobler, L.”sbj/Nj*N)”}”jöMŒ Mervart, M.”sbj/Nj*N)”}”jöMŒRothacher, and A.”sbj/Nj*N)”}”jöMŒVerdun.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒ*Extended orbit modeling techniques at the ”sbjsbejCNKèubjqNŒ6”ubj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒGeoffrey Blewitt.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒ+Carrier phase ambiguity resolution for the ”sbjsbejCNKèubjqNj1Qubt””jN(jñ‹jçMjCj@Ej N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒGeoffrey Blewitt.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒ#An automatic editing algorithm for ”sbjsbejCNKŽubjqNŒ7”ubj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒGeoffrey Blewitt.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒ#An automatic editing algorithm for ”sbjsbejCNKŽubjqNj¥Qubt””jN(jû‹jçMjCjwEj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒYehuda Bock, Sergei”sbj/Nj*N)”}”jöMŒA Gourevitch, Charles”sbj/Nj*N)”}”jöMŒ C Counselman”sbj/Nj*N)”}”jöMŒ III, Robert”sbj/Nj*N)”}”jöMŒW King, and Richard”sbj/Nj*N)”}”jöMŒI Abbot.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒInterferometric analysis of ”sbjsbejCNKÜubjqNŒ9”ubj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒJ.”sbj/Nj*N)”}”jöMŒ Boehm, A.”sbj/Nj*N)”}”jöMŒ Niell, P.”sbj/Nj*N)”}”jöMŒTregoning, and H.”sbj/Nj*N)”}”jöMŒSchuh.”sbj.N)”}”(j1NjLNj3NjLN…”ubjsbejCNKÜubjqNj”Rubt””jN(jŒjçMjCjÇEj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒ.Johannes Boehm, Birgit Werl, and Harald Schuh.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒ"Troposphere mapping functions for ”sbjsbejCNM%ubjqNŒ10”ubj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒ.Johannes Boehm, Birgit Werl, and Harald Schuh.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒ"Troposphere mapping functions for ”sbjsbejCNM%ubjqNj>Subt””jN(jŒjçMj CjcFj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒOscar”sbj/Nj*N)”}”jöMŒ L. Colombo.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒEphemeris errors of ”sbjsbejCNKrubjqNŒ11”ubj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒOscar”sbj/Nj*N)”}”jöMŒ L. Colombo.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒEphemeris errors of ”sbjsbejCNKrubjqNjÚSubt””jN(j#ŒjçMj CjšFj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒJ.”sbj/Nj*N)”}”jöMŒ L. Davis, R.”sbj/Nj*N)”}”jöMŒA. Bennett, and B.”sbj/Nj*N)”}”jöMŒ P. Wernicke.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒAssessment of ”sbjsbejCNKÌubjqNŒ12”ubj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒJ.”sbj/Nj*N)”}”jöMŒ L. Davis, R.”sbj/Nj*N)”}”jöMŒA. Bennett, and B.”sbj/Nj*N)”}”jöMŒ P. Wernicke.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒAssessment of ”sbjsbejCNKÌubjqNjzTubt””jN(j-ŒjçMj CjäFj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒTimothy”sbj/Nj*N)”}”jöMŒKH. Dixon, Meghan Miller, Frederic Farina, Hongzhi Wang, and Daniel Johnson.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒPresent-day motion of the ”sbjsbejCNMubjqNŒ13”ubj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒTimothy”sbj/Nj*N)”}”jöMŒKH. Dixon, Meghan Miller, Frederic Farina, Hongzhi Wang, and Daniel Johnson.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒPresent-day motion of the ”sbjsbejCNMubjqNj7Uubt””jN(jAŒjçMj CjGj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒD.”sbj/Nj*N)”}”jöMŒDong, T.”sbj/Nj*N)”}”jöMŒA. Herring, and R.”sbj/Nj*N)”}”jöMŒW. King.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒZEstimating regional deformation from a combination of space and terrestrial geodetic data.”sbj¨UjXN)”}”(j1Nj[Nj3Nj[N…”j'N]”j*N)”}”jöMŒJournal of Geodesy”sbajCNKubj*N)”}”jöMŒ, 72:200–214, 1998.”sbj¨UjeN)”}”(jhNŒ%https://doi.org/10.1007/s001900050161”j3NjºU…”j'N]”j*N)”}”jöMŒdoi:10.1007/s001900050161”sbajCNKubj*N)”}”jöMj—>sbejCNKÃubjqNŒ14”ubj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒD.”sbj/Nj*N)”}”jöMŒDong, T.”sbj/Nj*N)”}”jöMŒA. Herring, and R.”sbj/Nj*N)”}”jöMŒW. King.”sbj.N)”}”(j1NjLNj3NjLN…”ubj*N)”}”jöMŒZEstimating regional deformation from a combination of space and terrestrial geodetic data.”sbjÔUjXN)”}”(j1Nj[Nj3Nj[N…”j'N]”j*N)”}”jöMŒJournal of Geodesy”sbajCNKubj*N)”}”jöMŒ, 72:200–214, 1998.”sbjÔUjeN)”}”(jhNŒ%https://doi.org/10.1007/s001900050161”j3NjæU…”j'N]”j*N)”}”jöMŒdoi:10.1007/s001900050161”sbajCNKubj*N)”}”jöMj—>sbejCNKÃubjqNjÂUubt””jN(j7ŒjçMj Cj?Gj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒDa-Nan Dong and Yehuda Bock.”sbj.N)”}”(j1NjLNj3NjLN…”ubjsbejCNMubjqNŒ15”ubj N)”}”(jŠCj Chñj$N)”}”(j'N]”(j*N)”}”jöMŒDa-Nan Dong and Yehuda Bock.”sbj.N)”}”(j1NjLNj3NjLN…”ubjVjXN)”}”(j1Nj[Nj3Nj[N…”j'N]”j*N)”}”jöMŒ,Journal of Geophysical Research: Solid Earth”sbajCNK,ubj*N)”}”jöMŒ , 94(B4):3949”sbj.N)”}”(j1Nj‚Pj3Nj‚P…”ubj*N)”}”jöMŒ 3966, 1989.”sbj>VjeN)”}”(jhNŒ'https://doi.org/10.1029/JB094iB04p03949”j3NjsV…”j'N]”j*N)”}”jöMŒdoi:10.1029/JB094iB04p03949”sbajCNKubj*N)”}”jöMj—>sbejCNMubjqNj5Vubt””jN(jKŒjçMjCjÊGj N)”}”(jŠCjChñj$N)”}”(j'N]”(j*N)”}”jöMŒKurt”sbj/Nj*N)”}”jöMŒL. 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