ISIS Application Documentation
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Apply a Sigma Stretch to a cube.
Description
Categories
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Examples
History
new_dn = (old_dn - avg) * (variance / stddev)where avg and stddev are the statistical average and standard deviation of all valid pixels in the current band. The variance is a user-specified parameter, VARIANCE, that affects how much the histogram of the image is widened, and does not represent the statistical variance of the image.
Name | Description |
---|---|
FROM | Input cube to stretch |
TO | Output cube |
Name | Description |
---|---|
VARIANCE | Non-uniformity of the output's histogram |
The input cube to which the sigma stretch will be applied.
Type | cube |
---|---|
File Mode | input |
Filter | *.cub |
The resultant cube containing the image after being stretched.
Type | cube |
---|---|
File Mode | output |
Pixel Type | real |
Filter | *.cub |
The nonuniformity of the output image's histogram. For values less than 1.0, the distribution will be closer to uniform. This value must be greater than 0.0.
Type | double |
---|---|
Default | 40.0 |
Minimum | 0.0 (exclusive) |
Two THEMIS Images
Travis Addair | 2011-09-08 | Original translation of Davinci's "sstretch" script into Isis 3. |
Steven Lambright | 2012-02-24 | This program now takes advantage of multiple global processing threads. |
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 21:48:33 |