ISIS 3 Application Documentation
Warp an image to another using control points
Description
Categories
Groups
History
Description
This program warps Apollo images using the reseau information. (note:
apollofindrx must be run first).
Categories
Parameter Groups
Files
|
Name
|
Description
|
| FROM |
Input cube to warp
|
| TO |
Output cube
|
Warp parameters
|
Name
|
Description
|
| DEGREE | Order of polynomial |
| WEIGHTED | Weight the control points using distance |
Interpolation
Files:
FROM
Description
Use this parameter to select the filename. All bands within the file
will be warped unless a specific band is specified.
|
Type
| cube |
|
File Mode
| input |
|
Filter
|
*.cub
|
Files:
TO
Description
This file will contain the results of the warping.
|
Type
| cube |
|
File Mode
| output |
Warp parameters:
DEGREE
Description
The order of the polynomial to be used in the linear regression fit.
|
Type
| integer |
|
Default
| 1 |
|
Minimum
| 1
(inclusive)
|
Warp parameters:
WEIGHTED
Description
The control points will be weighted based on distance if this option is selected.
If it is not selected, all control points will have a weight of 1, reguardless of distance.
|
Type
| boolean |
|
Default
| true |
Interpolation:
INTERPOLATION
Description
This is the type of interpolation to be performed on the input.
|
Type
| string |
|
Default
|
NEARESTNEIGHBOR
|
|
Option List:
|
|
Option |
Brief |
Description |
| NEARESTNEIGHBOR | Nearest Neighbor |
Each output pixel will be set to the pixel nearest the
calculated input pixel.
|
| BILINEAR | Bi-Linear interpolation |
Each output pixel will be set to the value calculated by
a bi-linear interpolation of the calculated input pixel.
|
| CUBICCONVOLUTION | Cubic Convolutioin interpolation |
Each output pixel will be set to the value calculated by
a cubic convolution interpolation of the calculated input pixel.
|
|
History
| Jacob Danton | 2007-01-30 |
Original version
|
| Kristin Berry | 2014-05-29 |
Updated to fix string conversion error. References #2043.
|