dewobble3
m (Dewobble3 moved to dewobble3) |
Revision as of 16:33, 3 March 2006
Contents: Description, Arguments, Usage, Images, Sub-Functions, Related Functions, Source Supported Under Version: >1.00
Description Calculate DN contribution due to THEMIS drift and wobble.
Arguments and Return Values Arguments: A THEMIS image and bandlist Return Value: The cleaned THEMIS image
Usage Syntax: dewobble3(image,bandlist) 'image' must be a 3 or 10 band THEMIS RDR data product 'bandlist' must be an Nx1x1 ordered list of THEMIS bands contained in the image Combines the functionality of undrift and dewobble2 into a single function. This function is called by uddw to remove long wavelength row-corellated noise due to temperature variations (aka wobble) and thermal drift in the THEMIS instrument. THEMIS band 10 is assumed to be a direct measurement of the Martian atmosphere which is further assumed to be thermally stable over large distances. The down-track radiance variations in band 10 are removed from all other bands, but band 10 is unaltered for reversibility.
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Recent Library Changes Created On: 02-15-2006 |