dewobble3

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Citation

Bandfield, J. L., D. Rogers, M.D. Smith, P.R. Christensen (2004), Atmospheric correction and surface spectral unit mapping using Thermal Emission Imaging System data, J. Geophys. Res., 109, E10008, doi:10010.11029/12004JE002289.

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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Major Sub-Functions

Related Functions

Recent Library Changes

Created On: 02-15-2006
Modified On: 05-14-2013

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