dewobble3
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| − | {{DavinciWiki_Function | + | {{DavinciWiki_Function| |
| − | [[ | + | Calculate DN contribution due to THEMIS drift and wobble. |
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| + | Arguments: A THEMIS image and bandlist | ||
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| + | Return Value: The cleaned THEMIS image | ||
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| + | Syntax: dewobble3(image,bandlist) | ||
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| + | 'image' must be a 3 or 10 band THEMIS RDR data product | ||
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| + | 'bandlist' must be an Nx1x1 ordered list of THEMIS bands contained in the image | ||
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| + | 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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| + | [[Image:wobble.png|300px]] [[Image:dewobble3.png|300px]] | ||
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| + | *[[avg]] | ||
| + | *[[filtery]] | ||
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| + | *[[uddw]] | ||
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| + | [[Media:dewobble3.dvrc|dewobble3()]] | ||
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| + | }} | ||
[[category:Functions]] | [[category:Functions]] | ||
| + | [[category:User Defined Functions]] | ||
[[category:THEMIS Science]] | [[category:THEMIS Science]] | ||
Revision as of 14:37, 2 March 2006
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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 |
