ISIS Application Documentation
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Apply Hapke bidirectional reflectance model photometric correction to multiband cubes
Overview | Parameters |
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 19:28:12 |
Parameter GroupsFiles
Photometry
Other Options
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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 19:28:12 |
Use this parameter to select the input filename.
Type | cube |
---|---|
File Mode | input |
Filter | *.cub |
This file will contain the photometrically corrected image data after being corrected.
Type | cube |
---|---|
File Mode | output |
Pixel Type | real |
This file will contain the backplane data. It must have "Phase Angle", "Emission Angle", "Incidence Angle", "Latitude" and "Longitude".
Type | cube |
---|---|
File Mode | input |
Pixel Type | real |
Internal Default | Calculate the photometry on the fly |
This file will contain the photometric correction algorithm information. Here's an example pvl file for Hapke photometric correction:
Object = PhotometricModel Name = HapkeLROC Units = Degrees Incref = 60.0 Emiref = 0.0 Pharef = 60.0 Group = Parameters BandBinCenter = 321 Bands = (1, 2, 3, 4, 5, 6, 7, 8, 9) EndGroup EndObject
Type | filename |
---|---|
File Mode | input |
Default Path | $lro/calibration |
Default | $lro/calibration/WAC_hapke_full.????.pvl |
Filter | *.pvl |
This file will contain the parameters (in order) Wh, Hg1, Hg2, Bc0, hc, B0, Hh, Theta, phi. See the main program documentation for a full description.
Type | cube |
---|---|
File Mode | input |
Default | $lro/calibration/WAC_global_7bands_1x1_wbhs70NS_const_each_pole.????.cub |
Filter | *.cub |
Pixels which have a phase angle less than this value will be trimmed.
Type | double |
---|---|
Default | 0.0 |
Minimum | 0.0 (inclusive) |
Maximum | 180.0 (inclusive) |
Less Than or Equal | MAXPHASE |
Pixels which have a phase angle greater than this value will be trimmed.
Type | double |
---|---|
Default | 180.0 |
Minimum | 0.0 (inclusive) |
Maximum | 180.0 (inclusive) |
Greater Than or Equal | MINPHASE |
Pixels which have an emission angle less than this value will be trimmed.
Type | double |
---|---|
Default | 0.0 |
Minimum | 0.0 (inclusive) |
Maximum | 90.0 (inclusive) |
Less Than or Equal | MAXEMISSION |
Pixels which have a emission angle greater than this value will be trimmed.
Type | double |
---|---|
Default | 90.0 |
Minimum | 0.0 (inclusive) |
Maximum | 90.0 (inclusive) |
Greater Than or Equal | MINEMISSION |
Pixels which have an incidence angle less than this value will be trimmed.
Type | double |
---|---|
Default | 0.0 |
Minimum | 0.0 (inclusive) |
Maximum | 180.0 (inclusive) |
Less Than or Equal | MAXINCIDENCE |
Pixels which have a incidence angle greater than this value will be trimmed.
Type | double |
---|---|
Default | 90.0 |
Minimum | 0.0 (inclusive) |
Maximum | 180.0 (inclusive) |
Greater Than or Equal | MININCIDENCE |
Phase, Emission, and Incidence angles can be calculated from the elipsoid (default) or from the DEM. The difference is that using the DEM the surface roughness is taken into account.
Type | boolean |
---|---|
Default | False |
Only the photometry value will be written to the output cube, not the original image data. Used for testing photometry calculation.
Type | boolean |
---|---|
Default | False |
Set to False to cause the photometry value to not be normalized. Used for testing photometry calculation.
Type | boolean |
---|---|
Default | True |