IRAF Help page for: BURST
BURST (Mar95) suntrans BURST (Mar95)
NAME
BURST -- break up multi-image mode coefficient files into paired-l
mode coefficient files for making interim time series
USAGE
burst inputl burstfile (nburst_sect nsup_start)
PARAMETERS
inputl
input image or list of images
burstfile
image name template for output paired-l mode coefficient files
(nburst_sect = 1)
number of l pairs per section of the mode coefficient files
(nsup_start = 1)
starting image number for output paired-l mode coefficient
files
IMAGE HEADER WORDS
LMAX
maximum l value for mode coefficients
SHT_HIST
spherical harmonic transform history line
PLM_LINE
trimming file history line
EPOCH
Time of time sample 0 in UT, format yyyy/mm/dd.hh:mm:ss
GRID_HIS
heliographic remapping history line
SITE
observation site abreviation
MTYPE
m value type (all or even) for time series files
UTTMI_i
observation date and time for image i within file
SLOTI_i
time sample number for image i within file
MWGTI_i
merge weight for image i within file
DESCRIPTION
Task BURST breaks multi-image mode coefficient files from the
spherical harmonic transform into paired-l mode coefficient files
for input to the time transpose.
EXAMPLES
1. Put the multi-image mode coefficient files listed in file
sunsup.lis into paired-l mode coefficient files named
junecal###l_###.
su> burst @sunsup.lis juncal
2. Put the multi-image mode coefficient files listed in file
sunsup.lis into paired-l mode coefficient files named
junecal###l_### and numbered starting with junecal006l_###.
su> burst @sunsup.lis juncal nsup_start=6
3. Put the multi-image mode coefficient files listed in file
sunsup.lis into paired-l mode coefficient files named
junecal###l_###. The paired-l mode coefficient files will contain
8 l pairs per file.
su> burst @sunsup.lis juncal nburst_sect=8
TIME REQUIREMENTS
Highly dependent upon file size and disk I/O capabilities. Not
negligible.
BUGS
None known.
SEE ALSO
otrans, sermake, im3dtrans
modecoef_file
Data Product Code Guide |
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