IRAF Help page for: COPIPE
COPIPE (Jun01)
pipeline
COPIPE (Jun01)
NAME
COPIPE -- Camera
Offset Pipeline. Computes
angular
cross-correlations between simultaneous
GONG images recorded at
different sites in order to
determine an optimal, internally
consistent, set of equations describing the rotation
of Solar North
at each instrument. A brief description of
the algorithm can be
found in: Toner and Harvey
1998 Sounding Solar and Stellar
Interiors, ed. J. Provost and F-X Schmider, Proceedings
IAU Symp.
181, Poster Volume, Nice, France, 57.
USAGE
copipe input start_date end_date
PARAMETERS
input
ASCII file containing
a list of path names to the images to be
cross-correlated
start_date = "010312"
Defines the starting date
over which one wants to compute
correlations between
simultaeous image. Format is: YYMMDD (ie
2-digit year, month, day).
end_date = "010317"
Defines the ending
date over which one wants to compute
correlations between
simultaeous image. Format is: YYMMDD (ie
2-digit year, month, day).
tsample = 10
Time sample spacing (minutes).
Select the "cadence" for the
cross-correlations (i.e.,
every 5 minutes, every 10 minutes,
etc..)
nannuli = 12
The number of annuli to
cross-correlate between simultaneous
images. Recommended
values: 10 for Classic images, 12 for Plus
images
nsectors = 1024
The number of sectors per annulus
Recommended values: 512 for
Classic images, 1024 for Plus
images
tbl_path ""
Path to offset (mrhiy*) tables.
dev = "lw20"
Graphics output device (i.e.,
where to send the output plots)
data_type = "vzi"
Image data type (vzi, izi, etc...)
image_type = "fits.gz"
Image type (imh, fits, fits.gz,
etc...)
pm_tbl = "home$driftdrift.dat"
Full name & path of PM data
table
compress = "gzip"
Type of image compression. Choices
are: none|gzip|compress
use_tc = no
Use TC data if available?
tlist = ""
For internal use by COPIPE
EXAMPLES
TIME REQUIREMENTS
BUGS
SEE ALSO
Data Product Code Guide | Back to GRASP Help Page