Description
This program applies a flat-field correction for each framelet based on the
band's filter number. In order to output in I/F units, the cube must have spice
data. This calibration problem follows the algorithms described the document titled:
Mars Reconnaissance Orbiter Mars Color Imager (MARCI):
Instrument Description, Calibration, and Performance
J.F. Bell III, M.J. Wolff, M.C. Malin, W.M. Calvin, B.A. Cantor,
M.A. Caplinger, R.T. Clancy, K.S. Edgett3, L.J. Edwards5, J. Fahle,
F. Ghaemi, R.M. Haberle, A. Hale, P.B. James, S.W. Lee,
T. McConnochie, E. Noe Dobrea1, M.A. Ravine, D. Schaeffer,
K.D. Supulver, and P.C. Thomas
Categories
History
| Steven Lambright | 2009-01-21 |
Original version
|
| Steven Lambright | 2009-03-03 |
Added lookup table
|
| Steven Lambright | 2009-04-09 |
Fixed a problem where segmentation faults would occur if run
with the option "IOF=false"
|
| Janet Barrett | 2014-07-01 |
Added code to obtain exposure times from $mro/calibration/marci/varexp.tab
so they can be used when calibrating the input image. Also had to handle
images that have been flipped by marci2isis. Fixes #1860.
|
| Moses Milazzo | 2014-12-08 |
Fixed a bug in exposure time accounting. Fixes #1860.
|
| Stuart Sides | 2019-11-08 |
Modified to use the exposure duration from the new label keywords added by
marci2isis. Related #2034
|
| Lauren Adoram-Kershner | 2022-07-15 |
Implimented step 3 of marci calibration description, where if normalized flatfile DN value
is less than 0.25, the output cube DN is set to 0.
|
|
