[daip] 31DEC09 LINUX midnite job (dave, 20090726.034609)

aipsmgr at nrao.edu aipsmgr at nrao.edu
Sat Jul 25 23:46:39 EDT 2009


dave update report for 31DEC09 on Sun Jul 26 03:46:39 UTC 2009 (UT)

Copies and compiles:

AIPSUPD - Using CVS for copying files.
UPDCVS - cvs copy of 31DEC09 begun, 1st character means
 - U added, P updated, M your file differs from master
 - C you have a changed file needing work (error!)
 - ? you have a file not on the master (ignore)
? 31DEC09/ERRORS
? 31DEC09/LINUX/SUM-EFAGRELI
? 31DEC09/SUL/SYSTEM/NRAOAOC
U 31DEC09/TIMESTAMP
P 31DEC09/APL/DEV/UNIX/ZATCVT.FOR
P 31DEC09/APL/DEV/UNIX/ZATIO.FOR
P 31DEC09/APL/DEV/UNIX/BELL/MACPPC/ZATCVT.FOR
P 31DEC09/APL/DEV/UNIX/BELL/MACPPC/ZATIO.FOR
P 31DEC09/APL/DEV/UNIX/BELL/SOL/ZATCVT.FOR
P 31DEC09/APL/DEV/UNIX/BELL/SOL/ZATIO.FOR
P 31DEC09/APL/PGM/NOTST/ATLOD.FOR
U 31DEC09/APL/PGM/NOTST/FARS.FOR
U 31DEC09/HELP/FARS.HLP
P 31DEC09/HELP/LSAPROPO.HLP
P 31DEC09/HIST/CHANGE.DOC
P 31DEC09/UPDATE/COMLNK.UPD
U 31DEC09/UPDATE/COMLNK.UPD.SUM
U 31DEC09/UPDATE/LASTCVS.DAT
P 31DEC09/UPDATE/PUTBCK.UPD
U 31DEC09/UPDATE/PUTBCK.UPD.SUM
P 31DEC09/UPDATE/REASONS.UPD
U 31DEC09/UPDATE/REASONS.UPD.SUM
UPDCVS - cvs update of 31DEC09 completed
UPDCVS - cvs update of TEXT completed
AIPSUPD - UPDCVS apparently worked

UPDCONTROL - /home/AIPS/31DEC09/LINUX/UPDATE/LASTREMOVE.DAT = 20090725.034340
UPDCONTROL - /home/AIPS/31DEC09/LINUX/UPDATE/LASTCOPY.DAT = 20090725.034340
UPDCONTROL - /home/AIPS/31DEC09/LINUX/UPDATE/LASTCOMRPL.DAT = 20090725.034340
UPDCONTROL - /home/AIPS/31DEC09/LINUX/UPDATE/LASTCOMLNK.DAT = 20090725.034340

UPDCONTROL - Everything seems in order

UPDCOMRPL: COMRPLs


UPDCOMRPL: currently in /home/AIPS/31DEC09/LINUX/UPDATE

UPDCOMLNK: COMLNKs

25-JUL-2009 21:53:08 20090725 TST APGNOT   FARS.FOR      lkogan

UPDCOMLNK: currently in /home/AIPS/31DEC09/LINUX/UPDATE
UPDCOMLNK: /home/AIPS/31DEC09/APL/PGM/NOTST/FARS.FOR


UPDCONTROL - Reasons for file updates on Sun Jul 26 03:46:32 UTC 2009 (UT)

25-JUL-2009 21:49:08 20090725 TST APGNOT   FARS.FOR      the new task to serve Faraday rotation synthesis
25-JUL-2009 21:51:20 20090725 TST HLPFIL   FARS.HLP      the new task to serve Faraday rotation synthesis
25-JUL-2009 22:22:25 20090725 TST HIST     CHANGE.DOC    the new task FARS to serve Faraday rotation synthesis

CHANGE.DOC entries:

12905.  July 25, 2009           FARS                    Leonia
        The new task FARS to serve the Faraday rotation synthesis.
        FARS read the two input image cubes.
        The first cube should correspond to the Q-linear polarization
        component.
        The second cube should correspond to the U-linear polarization
        component.
        The main purpose of the current release of the task is to get
        the Faraday rotation free (lambda=0) brightness and the Faraday
        depth of the media on the way from the source to the observer.
        The multi frequency observations  are required to get this purpose.
        The main ideas of the algorithm are  described by M.A.Brentjens
        and A.G.de Bruyn at:
        Astronomy&Astrophysics, 441, 1217-1228(2005).
        FARS carries out the Fourier transform along the frequency
        (lambda square) axis for each pixel at the image plane.
        This Fourier transform converts the observed complex brightness
        as a function of the lambda^2 to the output complex function of
        the Faraday depth. The real part of this output is recorded into
        the first output file and the imaginary part of this output is
        recorded in the second output file.
        The amplitude of this output or Rotation Measure Transfer Function
        (RMTF) can be recorded instead under control of input parameters.
        The eight parameters of the found maximum athe Fourier transform
        can be recorded at the output instead of the full Fourier transform.
        This option serves to the most typical case: one source and one
        rotating media.
        Moved nowhere.

12906.  July




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