; VLBAEOPS ;--------------------------------------------------------------- ;! Corrects Earth orientation parameters ;# PROCEDURE VLBI UTILITY CALIBRATION ;----------------------------------------------------------------------- ;; Copyright (C) 2005-2007, 2012, 2013, 2017-2018, 2020 ;; Associated Universities, Inc. Washington DC, USA. ;; ;; This program is free software; you can redistribute it and/or ;; modify it under the terms of the GNU General Public License as ;; published by the Free Software Foundation; either version 2 of ;; the License, or (at your option) any later version. ;; ;; This program is distributed in the hope that it will be useful, ;; but WITHOUT ANY WARRANTY; without even the implied warranty of ;; MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the ;; GNU General Public License for more details. ;; ;; You should have received a copy of the GNU General Public ;; License along with this program; if not, write to the Free ;; Software Foundation, Inc., 675 Massachusetts Ave, Cambridge, ;; MA 02139, USA. ;; ;; Correspondence concerning AIPS should be addressed as follows: ;; Internet email: aipsmail@nrao.edu. ;; Postal address: AIPS Project Office ;; National Radio Astronomy Observatory ;; 520 Edgemont Road ;; Charlottesville, VA 22903-2475 USA ;----------------------------------------------------------------------- VLBAEOPS LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC VLBAEOPS: Procedure to fix EOPs used by the VLBA correlator INNAME Input file name INCLASS Input file class INSEQ Input file sequence number INDISK Disk number for input file EOPSFILE File with correct EOPS. '' => download autmatically VLBAEOPS is defined in the VLBAUTIL run file. ---------------------------------------------------------------- VLBAEOPS Type: Procedure Use: VLBAEOPS is a procedure that fixes the Earth Orientation Parameters (EOPs) used by the VLBA correlator. This requires the existence of a CT table (which contains the old EOPs). This is HIGHLY recommended if you are doing phase referencing and astrometry in particular. From 5-May-2003 to 9-Aug-2005 the VLBA correlator used old predicted EOPs which could be significantly wrong and will effect all phase referencing experiments. Before and after this time better predictions are used but there is still a chance for large error and almost certainly small errors exist, so it is recommended for all phase referencing experiments. See HELP CLCOR for more details on the fix. Type RUN VLBAUTIL to make the VLBAEOPS procedure available. ************************* WARNING: This function does not work well on data sets that have been concatenated with multiple days. Use it only on the initial 1-day sort of data set. ************************* Adverbs: INNAME.....The name of the file to be corrected. Wildcard characters are allowed. INCLASS....The class of the file to be corrected. Wildcard characters are allowed. INSEQ......The sequence number of the file to be corrected. Zero defaults to the highest sequence number matching INNAME, INCLASS, and INDISK. INDISK.....The disk drive number of the file to be corrected. Zero defaults to any disk. EOPSFILE...Input file. If ''=> file will be automatically downloaded. If there is a problem with automatic downloads (this can be a problem with some firewalls) the file can be can be picked up with the following command (all on 1 line!) curl -u anonymous:daip@nrao.edu --ftp-ssl ftp://gdc.cddis.eosdis.nasa.gov/vlbi/gsfc/ancillary/ solve_apriori/usno_finals.erp > /tmp/usno_finals.erp ---------------------------------------------------------------- VLBAEOPS: Procedure to correct the Earth Orientation Parameters used by the VLBA correlator Documentor: Amy Mioduszewski Related Programs: CLCOR, VLBAUTIL You should run VLBAEOPS after you have run VLBAFIX. It can be run anytime before the final fringe fit. VLBAEOPS corrects the Earth Orientation Parameters (EOPs) used by the VLBA correlator. It requires the existence of a CT table which has the EOPS used by the correlator and a file, supplied by USNO, which contains the final values. Having good EOPs is important for all phase referencing projects, especially astrometry. Particularly bad EOPs can cause position shifts and distortions in phase referenced images, some to the degree that the target could be smeared to the point of non-detection. This procedure will automatically download the USNO file, if EOPSFILE is blank and run CLCOR. It does the downloading with curl. If you do not have this comand on your computer or there is a firewall preventing downloads you can consult https://cddis.nasa.gov/Data_and_Derived_Products/CDDIS_Archive_Access.html You may have to create an account with cddis in order to download in some other fashion. The automatic download is done with the command curl -u anonymous:daip@nrao.edu --ftp-ssl ftp://gdc.cddis.eosdis. nasa.gov/vlbi/gsfc/ancillary/solve_apriori/usno_finals.erp > /tmp/usno_finals.erp (no blanks between ancillary/ and solve) and run VLBAEOPS with the EOPSFILE parameter set. VLBAEOPS is intended for all levels of VLBA users.