ISIS Application Documentation
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Import Vicar image file into Isis format
Overview | Parameters | Example 1 |
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 19:28:14 |
Parameter GroupsFiles
Special Pixels
|
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 19:28:14 |
Use this parameter to select the Vicar filename. If multi-band, it is assumed to be in band sequential order.
Type | filename |
---|---|
File Mode | input |
Filter | *.img *.IMG *.vic |
Use this parameter to select the output filename
Type | cube |
---|---|
File Mode | output |
Filter | *.cub |
If this option is used input raw pixels below minimum and above maximum will be converted to LRS and HRS respectively. Otherwise pixels in the input raw file will be left unchanged in most cases. For example, importing a raw 8-bit file and outputing to a 16-bit or 32-bit real will cause 0 and 255 to be actual values. If left as 8-bit then 0 will be NULL and 255 will be HRS.
Type | boolean |
---|---|
Default | NO |
Inclusions |
|
Minimum valid value. Anything below this value will be set to LRS.
Type | double |
---|---|
Inclusions |
|
Maximum valid value. Anything above this value will be set to HRS.
Type | double |
---|---|
Inclusions |
|
If this option is used input raw pixels below minimum and above maximum will be converted to LRS and HRS respectively. Otherwise pixels in the input raw file will be left unchanged in most cases. For example, importing a raw 8-bit file and outputing to a 16-bit or 32-bit real will cause 0 and 255 to be actual values. If left as 8-bit then 0 will be NULL and 255 will be HRS.
Type | boolean |
---|---|
Default | NO |
Inclusions |
|
Minimum valid value. Anything below this value will be set to LRS.
Type | double |
---|---|
Inclusions |
|
Maximum valid value. Anything above this value will be set to HRS.
Type | double |
---|---|
Inclusions |
|
If this option is used input raw pixels below minimum and above maximum will be converted to LRS and HRS respectively. Otherwise pixels in the input raw file will be left unchanged in most cases. For example, importing a raw 8-bit file and outputing to a 16-bit or 32-bit real will cause 0 and 255 to be actual values. If left as 8-bit then 0 will be NULL and 255 will be HRS.
Type | boolean |
---|---|
Default | NO |
Inclusions |
|
Minimum valid value. Anything below this value will be set to LRS.
Type | double |
---|---|
Inclusions |
|
Maximum valid value. Anything above this value will be set to HRS.
Type | double |
---|---|
Inclusions |
|
Example 1Converting an vicar file to an Isis Cube Description
This example will show the conversion from a vicar file to a cube.
Command Line
vicar2isis FROM=input.img TO=out.cub
Convert the image input.img to the Isis Cube out.cub
GUI Screenshot
Data FileLinks open in a new window.
Output Image |
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 19:28:14 |