ISIS Application Documentation
hifurrows | Standard View | TOC | Home |
Null furrowed pixels
Description
Categories
Groups
History
Name | Description |
---|---|
FROM | Input file |
TO | Output cube |
NEW_VERSION | Updated furrows functionality from the hical pipeline |
Name | Description |
---|---|
CORRELATION | Correlation threshold |
Name | Description |
---|---|
LOWPASS | Run Lowpass filter if Furrows are found |
The cube to be corrected
Type | cube |
---|---|
File Mode | input |
Filter | *.cub |
The resultant cube containing the modified data.
Type | cube |
---|---|
File Mode | output |
Filter | *.cub |
This option uses the updated furrows functionality from the hical pipeline script version1.42
Type | boolean |
---|---|
Default | FALSE |
Exclusions |
|
Inclusions |
|
The maximum correlation from pixel to pixel. If the correlation between two pixels suddenly drops below this value, then a furrow has been detected.
Type | double |
---|---|
Default | 0.75 |
Minimum | 0.0 (inclusive) |
Exclusions |
|
Run Lowpass filter if Furrows are found
Type | boolean |
---|---|
Default | true |
Sean Crosby | 2007-04-03 | Original version |
Steven Lambright | 2008-05-12 | Removed references to CubeInfo |
Sharmila Prasad | 2011-09-02 | Added newer version of implementing hifurrows taken from the Version 1.42 of the original HiCal pipeline perl script. |
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 16:09:03 |