ISIS 3 Application Documentation
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Create the Line Scanner Sensor section of a SOCET Set Line Scanner support file
Description
Categories
Groups
History
MRO-HiRISE
MRO-HiRISE IDEAL (i.e., noproj'ed images)
MRO-HiRISE IDEAL Jitter Corrected (i.e., hijitter'ed images)
MRO-CTX
LRO-NACL
LRO-NACR
| Name | Description |
|---|---|
| FROM | Filename of a cube |
| TO | SOCET Set Support file keywords |
Level 1 Input Line Scanner cube with SPICE data attached. Supported instruments and derived products are MRO-HiRISE, MRO-HiRISE IDEAL, MRO-HiRISE IDEAL Jitter Corrected, MRO-CTX, LRO-NACL, and LRO-NACR.
| Type | cube |
|---|---|
| File Mode | input |
| Filter | *.cub |
Output text file of the SOCET Set USGSAstro Line Scaner section of a SOCET Set support file. This output file is one of the input files to USGSAstro SOCET Set program 'import_pushbroom.'
| Type | filename |
|---|---|
| File Mode | output |
| Internal Default | None |
| E. Howington-Kraus | 2008-10-23 | Original version |
| K. Edmundson | 2011-05-13 | Added NADIR_CENTER_TIME parameter |
| E. Howington-Kraus | 2011-08-04 | Changed default NADIR_CENTER_TIME from None to 0.0 |
| E. Howington-Kraus | 2012-04-26 | Added MOUNT_ANG_TBL option |
| O. Thomas | 2012-08-23 | Renamed program from calc_pushbroom_keywords to socetlinescankeywords, added quaternions, made changes from SOCET Set Generic Pushbroom sensor model to the USGSAsro Line Scanner sensor model, and removed the MOUNT_ANG_TBL option. Started modifications to meet ISIS coding standards. |
| E. Howington-Kraus | 2013-02-20 | Completed modifications to meet ISIS coding standards for formal installation into ISIS3. Added support for HiRISE jitter-corrected images created at U of A. Added check for needed SPICE data (blobs) attached to the cube label. Renamed parameter PUSHKEY to TO. Temporarily removed support for MEX-HSRC and MGS-MOC sensors until they are tested and working under the SOCET Set USGSAstro Line Scanner sensor model. References #1490. |
| E. Howington-Kraus | 2013-06-21 | Modified to (1) generate ephemeris points and quaternions at a closer time interval if the spacing of the attached SPICE data are too sparse for the SOCET Set USGSAstro Line Scanner sensor model; (2) increase the precision of the output SOCET Set keyword values; (3) redefine the pixel-location of the input image's center ephemeris time, and (4) compute spacecraft velocity values instead of using SPICE velocity data blobs. Fixes #1672. |
| Jesse Mapel | 2018-03-23 | Added SEMI_MAJOR_AXIS and ECCENTRICITY to the output. Fixes #5362. |