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SCUCLKERR
- Determine the possible error in the times stored in the data header
- Description:
- This routine calculates the error in the times stored in the
data header. It performs a self-consistency check to determine
the local sidereal time from the Azimuth and elevation information
(that comes directly from the telescope) and compares this to
the LST stored in the header.
- Usage:
- scuclkerr filename
- Parameters:
-
-
CLOCKERR = REAL (Write)
-
On exit, the clock error, in seconds, determined from the header.
-
DANG = REAL (Write)
-
Error in the array rotation angle due to the clock error (degrees)
-
DR = REAL (Write)
-
Positional error at the edge of the array for this particular
observation. In arcseconds.
Edge is defined as a radius of 70 arcseconds.
-
IN = NDF (Read)
-
The name of the NDF containing to be tested.
-
MSG_FILTER = CHAR (Read)
-
Message filter level. Default is NORM.
-
LAG = REAL (Write).
-
The discrepancy between the LST stored in the FITS header
and the LST when data acquisition begins. This provides
a measure of the lag in starting up the observation (including
slew times). The value is stored in seconds.
-
MJD = DOUBLE (Write)
-
Modified Julian Date of start of observation corrected for the
lag time and the clock error.
- Notes:
- The calculated clock error is only accurate to about 15 seconds.
-
References
- Jenness, T., 2000, JCMT Technical Report TR/001/84
Next: SCUHELP - Gives help about SCUBA software
Up: Complete routine descriptions
Previous: SCUCLIP - Simple sigma clipping for each bolometer
SURF -- SCUBA User Reduction Facility
Starlink User Note 216
T. Jenness, J. F. Lightfoot
Joint Astronomy Centre, Hilo, Hawaii
3 April 2003
E-mail:ussc@star.rl.ac.uk
Copyright © 1997-2000,2003 Particle Physics and Astronomy Research Council