Home

Quick Links

Software Manual
GitHub
API Reference

Documentation Versions

Latest Release
Dev
8.3.0
8.2.0
8.1.0
8.0.0
7.2.0
7.1.0
7.0.0
6.0.0
3.9.0
3.5.0
USGS

ISIS Application Documentation

cam2cam

Printer Friendly View | TOC | Home

Convert camera image to a different camera image

Overview Parameters

Description

This program will convert a input camera cube to a different camera geometry. For example, given overlapping MGS MOC and Odyssey Themis cubes, this program can convert the MOC image to have the same geometric camera characteristics as the Themis cube (or vice versa). Another use is to align bands in a camera cube which has independent bands. For example, a raw Themis cube (after thm2isis) will not have aligned pixels. This program can be used to align the pixels without going to a map projection. To prevent pixels from falling off the edge of the cube you can run pad on the cube prior to this program.

Categories

Related Applications to Previous Versions of ISIS

This program replaces the following application existing in previous versions of ISIS:
  • lev1tolev1

History

Jeff Anderson2000-05-10 Original version
Jeff Anderson2004-01-19 Converted to Isis 3.0
Jacob Danton2005-12-05 Added an appTest.
Elizabeth Miller2006-03-23 Fixed appTest to reflect changes in all camera models
Debbie A. Cook2007-06-21 Corrected setting of output file labels so that the Spice comes from the match cube and not the input cube
Steven Lambright2007-06-22 Fixed typo in documentation
Steven Lambright2008-01-23 Fixed an access on an invalid pointer that caused segmentation faults on cubes in which the camera is band-dependant.
Jeff Anderson2008-02-12 Fixed problems with reference bands on band-dependent instruments
Steven Lambright2008-05-12 Removed references to CubeInfo
Jesse Mapel2018-05-17 Changed transform to use the local radius computed by the output camera instead of having the input camera re-compute it (sometimes incorrectly) from the latitude and longitude. Fixes #5425.
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 19:28:09
X

Files: FROM

Description

The camera cube which will be modified

Type cube
File Mode input
Filter *.cub
Close Window
X

Files: MATCH

Description

This is the camera cube which will be matched. It must be only one band so use the input attributes to select the band to match. For example, themis.cub+5.

Type cube
File Mode input
Filter *.cub
Close Window
X

Files: TO

Description

The resultant cube which will have the same camera geometry and image size as the match cube.

Type cube
File Mode output
Filter *.cub
Close Window
X

Options: REFBAND

Description

This is the reference band to be used in the MATCH cube. That is, all bands in the FROM cube will be matched to this band. The default is to use the middle band; however, the user can enter any band number which is valid for the instrument, regardless of whether the band is in the cube or not. This only applies to band dependent camera models such as Themis.

Type integer
Internal Default middle
Minimum 1 (inclusive)
Close Window
X

Options: INTERP

Description

This is the type of interpolation to be performed on the input.

Type string
Default CUBICCONVOLUTION
Option List:
Option Brief Description
NEARESTNEIGHBORNearest Neighbor Each output pixel will be set to the pixel nearest the calculated input pixel.
BILINEARBi-Linear interpolation Each output pixel will be set to the value calculated by a bi-linear interpolation of the calculated input pixel.
CUBICCONVOLUTIONCubic Convolution interpolation Each output pixel will be set to the value calculated by a cubic convolution interpolation of the calculated input pixel.
Close Window