ISIS Application Documentation
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Fix data gap in MOC images
Description
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Groups
History
Name | Description |
---|---|
FROM | Input cube |
TO | Output cube |
Name | Description |
---|---|
MAXSD | Maximum allowable deviance |
This is the input cube to be procesed and fixed around detector 371. must be an Isis cube from the Mars Global Surveyor Orbital Camera, and it needs to have already been processed to a level 1 cube.
Type | cube |
---|---|
File Mode | input |
Filter | *.cub |
This is the cube to which we will output our data
Type | cube |
---|---|
File Mode | output |
Filter | *.cub |
This parameter describes how many standard deviations from the local average are considered valid for the purpose of filling in the gap.
Type | double |
---|---|
Default | 1.0 |
Janet Barrett | 2003-01-31 | Original version |
Brendan George | 2005-11-21 | Converted to Isis |
U.S. Department of the Interior | U.S. Geological Survey ISIS | Privacy & Disclaimers | Astrogeology Research Program To contact us, please post comments and questions on the USGS Astrogeology Discussion Board To report a bug, or suggest a feature go to: ISIS Github File Modified: 02/24/2025 16:09:17 |