; OBPLT ;--------------------------------------------------------------- ;! Plot columns of an OB table. ;# TASK VLBI UV PLOT ;----------------------------------------------------------------------- ;; Copyright (C) 1995, 1997, 2014 ;; 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 ;----------------------------------------------------------------------- ;--------------------------------------------------------------- OBPLT LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC OBPLT: Task which sorts UV data INNAME Input UV file name (name) INCLASS Input UV file name (class) INSEQ 0.0 9999.0 Input UV file name (seq. #) INDISK Disk unit # of input UV data INVERS Version # of OB table to plot OPCODE X-Column title to plot OPTYPE Y-Column title to plot Choose from the following for X- [OPCODE], Y- [OPTYPE] axes TIME - UTC time DIST - distance, velocity VEL to earth center ANG1 - angle between sun and pointing center BECL - time since last EECL eclipse began/ended ORIE - parallactic angle APARM use to set X,Y axis range [default: to use full range] (1) X-axis minimum value (2) X-axis maximum value LTYPE label type [see HELP LTYPE] DOTV Use TV? [otherwise create PL] ---------------------------------------------------------------- OBPLT Type: Task Use: To plot a specified column of an OB table Adverbs: INNAME.....Input UV file name (name). Standard defaults. INCLASS....Input UV file name (class). Standard defaults. INSEQ......Input UV file name (seq. #). 0 => highest. INDISK.....Disk drive # of input UV. 0 => any. INVERS.....Version # of OB table to plot OPCODE.....X-Column title to plot OPTYPE.....Y-Column title to plot APARM......Use to explicitly set X,Y axis range, default is to use all points. LTYPE......Labelling type, see HELP LTYPE for details: 1 = border, 2 = no ticks, 3 or 7 = standard, 4 or 8 = relative to ref. pixel, 5 or 9 = relative to subimage (BLC, TRC) center, 6 or 10 = pixels. 7-10 all labels other than tick numbers and axis type are omitted. Less than 0 is the same except that the plot file version number and create time are omitted. Add n * 100 to alter the metric scaling. DOTV.......Use TV or create PL file ---------------------------------------------------------------- OBPLT: Task which plots data from OB table DOCUMENTOR: K.M.Desai (NRAO/VLA) RELATED PROGRAMS: SVLBI suite PURPOSE OBPLT will plot a specified column of the OB table against time. The OPCODE/OPTYPE codes and the corresponding OB table column titles are: ANT Antenna number SUB Subarray number TIME UTC time since ref. time XPOS X position rel Earth center YPOS Y position rel Earth center ZPOS Z position rel Earth center XVEL X velocity rel Earth center YVEL Y velocity rel Earth center ZVEL Z velocity rel Earth center ORIE Parallactic angle towards source ECL1 Elapsed time since beginning of last eclipse ECL2 Elapsed time since end of last eclipse ECL3 ECL4 ANG1 Sun angle ANG2 Sun angle ANG3 Sun angle DIST distance to Earth center VEL speed rel Earth center BECL Elapsed time since beginning of last eclipse EECL Elapsed time since end of last eclipse