ISIS Application Documentation
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Outputs latitude/longitude at line/sample or reverse
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
Position
Coordinate System
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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 |
Input cube which must have a Mapping group in the labels.
Type | cube |
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File Mode | input |
Filter | *.cub |
A text file which will contain the results of this program. This file can be used in conjunction with the "getkey" program in order to pass the results to another program when developing scripts if the PVL format is selected.
Type | filename |
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File Mode | output |
Internal Default | None |
Format type for output file. Pvl format is default.
Type | string | |||||||||
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Default | PVL | |||||||||
Option List: |
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If this option is selected, the output from the application will be appended to the file. If it is not selected, any information in the TO file will be overwritten.
Type | boolean |
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Default | TRUE |
This parameter is used to select the type of coordinate which will be used to compute the other two remaining coordinates.
Type | string | ||||||||||||
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Default | IMAGE | ||||||||||||
Option List: |
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This is the sample position used to compute information about the camera state at the pixel.
Type | double |
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This is the line position used to compute information about the camera state at the pixel.
Type | double |
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This is the latitude value used to compute the other coordinate values. The latitude will be interpreted as either Planetographic or Planetocentric latitude depending on the option selected under coordinate system.
Type | double |
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This is the longitude value used to compute the other coordinate values. The longitude will be interpreted as either PositiveEast or PositiveWest longitude and -180 to 180 or 0 to 360 domain depending on the option selected under coordinate system.
Type | double |
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This is the x coordinate value used to compute the other coordinate values. It will be a projection X value in meters.
Type | double |
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This is the y coordinate value used to compute the other coordinate values. It will be a projection Y value in meters.
Type | double |
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Selecting this parameter will enable the 'COORDLIST' parameter in the GUI.
Note that this parameter is optional when running mappt on the command line.
Type | boolean |
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Default | FALSE |
Exclusions |
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Inclusions |
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An input comma-delimited flatfile of image, ground or projection coordinates. This allows the program to process multiple coordinates in a single run of mappt, and output the results to the specified output file.
Expected order for image coordinates: sample, line
Expected order for ground coordinates: latitude, longitude
Expected order for projection coordinates: X, Y
The "Error" keyword will only appear when using a coordinate list. The value of "Error" will then be NULL unless an error occurs during the processing of a coordinate in the coordinate list. Then, the value of this keyword will be the error message. This allows for mappt to continue processing the remaining coordinates in the coordinate list.
For the input of Latitude and Longitude, mappt expects Planetocentric Latitude (within -90 to 90 boundary) and Positive East Longitude (with 0-360 boundary) to find the location in the input camera image.
Type | filename |
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File Mode | input |
Internal Default | None |
Exclusions |
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The Allowoutside parameter influences how mappt will report resulting latitude/longitude and sample/line coordinates that fall outside the input cube pixel boundaries.
The default is set to True, which allows mappt to return the values that are outside the cube pixel boundaries, For example, a given latitude/longitude might return a sample location of -1.0 (a single whole pixel coordinate off the left side of the image). This is a feature of the ISIS camera models.
When set to False, if a returned coordinate is off the image, mappt will fail. This failure can be indicated and ignored within a batch script when only coordinates that fall within the image cube pixel boundaries are desired.
Type | boolean |
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Default | true |
This is the coordinate system the input latitude and longitude will be interpreted in. There are eight possible options with the variation of planetocentric or planetographic, positive east or west, 180 to -180 range or 0 to 360.
Type | string | |||||||||||||||
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Default | INPUTFILESYS | |||||||||||||||
Option List: |
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This file can be a cube or a simple hand produced map file. This file must contain a maping group and is how the coordinate system will be determined if selected.
Type | filename |
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File Mode | input |
Filter | *.map *.cub |
The latitude type for the projection. It can either be Planetocentric or Planetographic. PLANETOCENTRIC is the default.
Type | string | |||||||||
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Default | PLANETOCENTRIC | |||||||||
Option List: |
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The longitude direction for the projection. It can have a direction of Positive East or Positive West. POSITIVEEAST is the default.
Type | string | |||||||||
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Default | POSITIVEEAST | |||||||||
Option List: |
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The longitude domain for the projection. It can either have a domain of 180 or 360. 360 is the default.
Type | string | |||||||||
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Default | 360 | |||||||||
Option List: |
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