dewobble3

Contents: Description, Arguments, Usage, Images, Sub-Functions, Related Functions, Source Supported Under Version: >1.00 Current .dvrc Version: 1.04 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. Images 300px 300px

DavinciWiki Mini-Nav Bar Contents Functions Function Categories Common Procedures Glossary Download Davinci Change Log News Mailing List Contact Developers davinci-dev [AT] mars.asu.edu All other topics See navigation on the left Major Sub-Functions avg filtery Related Functions uddw themis_science.dvrc dewobble3() Recent Library Changes Change Log Created On: 02-15-2006 Modified On: 05-14-2013