autoradcorr

Contents: Citation, Description, Arguments, Usage, Examples, Images, Sub-Functions, Related Functions, Source Supported Under Version: > 1.04 Current .dvrc Version: 1.04 Citation Bandfield, J. L., D. Rogers, M. D. Smith, and P. R. Christensen (2004), Atmospheric correction and surface spectral unit mapping using Thermal Emission Imaging System data, J. Geophys. Res., 109, E10008, doi:10.1029/2004JE002289. Description Calculates a radiance correction for all 50x50 pixel boxes in the scene that meet the following criteria: greater than 3.0 degree standard deviation in temperature temperature of pixels must be greater than 225K box must contain 50 percent usable pixels box cannot overlap areas containing ghost signal radiation correction for a box cannot have negative correction values Boxes that meet all above criteria are given a Quality of 2 in the quality mask. Quality 1 boxes ignore criterium 5 - this allows for water cloud corrections. Arguments and Return Values Returns a structure containing: .avgdark 1x1x10 average radiance correction for entire image .blackmask XxYx1 mask of used pixels in calculations .dark (X/50)x(Y/50)x10 radiance corrections for every 50x50 box .darkcol 1xYx10 correction for entire image .data XxYx10 corrected data cube Usage Syntax: rc = autoradcorr(data [, bandlist = INT] [, b1 = INT] [, b2 = INT] [, sd = FLOAT] [, tempmin = FLOAT] [, pix_fraction = FLOAT] [, first_image = INT] [, ignore = FLOAT]) 'data' is the full projected hdf. You MUST supply this! 'bandlist' is the ordered list of THEMIS bands in the cube. Default is 1-10. 'b1 and b2' are the first and last z values to search for maxbtemp. Default is 3 and 9. 'sd' is the standard deviation of the temperature. Default is 3K. 'tempmin' is the minimum brightness temperature. Default is 225K. 'pix_fraction' is the fraction of usable pixels in a box. Default is 50 percent. 'first_image' = 1 is first 3600-line chunk of single data cube, = 0 is not. Default is 1. 'ignore' is null value of the black space. Default is -32768. Examples dv> a 345x1000x10 array of float, bsq format [13,800,000 bytes] dv> emissivity_before = thm.themis_emissivity(a) .struct, 2 elements emiss: 345x1000x10 array of float, bsq format [13,800,000 bytes] maxbtemp: 345x1000x1 array of float, bsq format [1,380,000 bytes] dv> rc = autoradcorr(a) ............................... struct, 4 elements avgdark: 1x1x10 array of float, bsq format [40 bytes] blackmask: 345x1000x1 array of byte, bsq format [345,000 bytes] dark: 7x20x10 array of float, bsq format [5,600 bytes] darkcol: 1x1000x10 array of float, bsq format [40,000 bytes] data: 345x1000x10 array of float, bsq format [13,800,000 bytes] dv> emissivity_after = thm.themis_emissivity(rc.data) .struct, 2 elements emiss: 345x1000x10 array of float, bsq format [13,800,000 bytes] maxbtemp: 345x1000x1 array of float, bsq format [1,380,000 bytes] Images The following images show dcs images of the radiance, emissivity before and emissvity after of an image that has been autoradcorr-ed.

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 thm.themis_emissivity thm.radcorr thm.column_fill thm.supersample Related Functions radcorr2 thm.radcorr themis_science.dvrc autoradcorr() Recent Library Changes Change Log Created On: 02-15-2006 Modified On: 02-22-2013