ISIS Application Documentation
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Removes noise from MOC narrow angle images
Description
Categories
Groups
History
Description
MOC narrow angle images with a crosstrack summing mode of 1 exhibit diagnol noise patterns. This
program will statistically determine the pattern and remove it.
Categories
Related Objects and Documents
Applications
Parameter Groups
Files
| Name | Description |
|---|---|
| FROM | Input MOC cube |
| TO | Output cube |
Parameters
| Name | Description |
|---|---|
| WIDTH | Width around noise pattern to use when computing noise removal coefficients |
Files: FROM
Description
The MOC narrow angle cube to have the noise removed. It must have a crosstrack summing mode of 1.
| Type | cube |
|---|---|
| File Mode | input |
| Filter | *.cub |
Files: TO
Description
The resultant cube containing cleaned-up data.
| Type | cube |
|---|---|
| File Mode | output |
| Filter | *.cub |
Parameters: WIDTH
Description
After the noise pattern is detected, three correction coefficients are computed by examining the average around the noise. The width defines how many pixels around the noise that will be used for the average computation.
| Type | integer |
|---|---|
| Default | 5 |
| Minimum | 5 (inclusive) |
History
| Tracie Sucharski | 1999-02-19 | Original version |
| Jeff Anderson | 2003-12-03 | Converted to Isis 3.0 |
| Steven Lambright | 2008-05-13 | Removed references to CubeInfo |
| Jeannie Walldren | 2008-11-05 | Replaced reference to MocLabels::IsWideAngle() with MocLabels::WideAngle() |
| Jeannie Walldren | 2011-05-03 | Removed Mgs namespace scope. |
| 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: 02/21/2025 20:05:58 |