; DOUVCOMP ;--------------------------------------------------------------- ;! selects use of compression in writing UV data to disk ;# ADVERB UV ;----------------------------------------------------------------------- ;; Copyright (C) 1995, 2010, 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 ;----------------------------------------------------------------------- DOUVCOMP LLLLLLLLLLLLUUUUUUUUUUUU CCCCCCCCCCCCCCCCCCCCCCCCCCCCC ---------------------------------------------------------------- DOUVCOMP Type: Adverb (Logical: <= 0 is false, > 0 is true) Use: Instructs tasks to write visibility data to disk in AIPS compressed format. This format has one correlator value (2 numbers) per floating word, magic value blanking, and a single weight per visibility record. This may result in a significant reduction in disk usage (up to a factor of 3). This comes at a cost - the data must be compressed and uncompressed as they are used which requires a multiply for every datum. There is only one weight for all IFs and polarizations which probably does not represent reality (even if all spectral channels do have the same weight). Furthermore, the full dynamic range of the numbers is 1 in 32768 which means that one bad value can turn all the rest of the numbers into pure 0. Null value: false (-1) Tasks: ATLOD.......Reads ATCA data in RPFITS dormat into AIPS. BLING.......Find residual rate and delay on individual baselines. DOUVCOMP refers to the format of scratch files. FILLM.......Reads VLA on-line/archive format uv data tapes (post Jan 88). FITAB.......Writes images / uv data w extensions to tape in FITS format. DOUVCOMP refers to the format in the output FITS UV table. FITLD.......Reads FITS files to load images or UV (IDI or UVFITS) data to disk. DOUVCOMP does not apply to input UV FITS tables. FIXWT.......Modify weights to reflect amplitude scatter of data. M3TAR.......Translate Haystack MKIII VLBI format "A" TAR's into AIPS. MK3IN.......Translate Haystack MKIII VLBI format "A" tapes into AIPS. OTFUV.......Translates on-the-fly single-dish SDD format to AIPS UV file. SPLAT.......Applies calibration and splits or assemble selected sources. SPLIT.......Converts multi-source to single-source UV files w calibration. UV2MS.......Append single-source file to multi-source file. UVLOD.......Read export or FITS data from a tape or disk. VLBIN.......Task to read VLBI data from an NRAO/MPI MkII correlator. "Verbs": BDF2AIPS....Read EVLA ASDM/BDF data into AIPS. Procedures: READISK.....Reads images / uv data w extensions in FITS format into AIPS. VLBALOAD....Loads VLBA data. VLBAMPHC....Applies VLBARUN calibration to additional phase stopping centers. DOUVCOMP is used only if data have to be loaded. VLBARUN.....Applies amplitude and phase calibration procs to VLBA data. The VLBA calibration, editing, imaging pipeline. ----------------------------------------------------------------