Published June 20, 2008 | Version v1
Journal article

Laboratory-based bidirectional reflectance distribution functions of radiometric tarps

Description

Laboratory-based bidirectional reflectance distribution functions (BRDFs) of radiometric tarp samples used in the vicarious calibration of Earth remote sensing satellite instruments are presented in this paper. The results illustrate the BRDF dependence on the orientation of the tarps' weft and warp threads. The study was performed using the GSFC scatterometer at incident zenith angles of 0 deg., 10 deg., and 30 deg.; scatter zenith angles from 0 deg. to 60 deg.; and scatter azimuth angles of 0 deg., 45 deg., 90 deg., 135 deg., and 180 deg.. The wavelengths were 485 nm, 550 nm, 633 nm, and 800 nm. The tarp's weft and warp dependence on BRDF is well defined at all measurement geometries and wavelengths. The BRDF difference can be as high as 8% at 0 deg. incident angle and 12% at 30 deg. incident angle. The fitted BRDF data show a very small discrepancy from the measured ones. New data on the forward and backscatter properties of radiometric tarps are reported. The backward scatter is well pronounced for the white samples. The black sample has well-pronounced forward scatter. The provided BRDF characterization of radiometric tarps is an excellent reference for anyone interested in using tarps for radiometric calibrations. The results are NIST traceable

Additional details

Identifiers

Publishing Information

Journal Title
Applied Optics
Journal Volume
47
Journal Issue
18
Journal Page Range
p. 3313-3323
ISSN
0003-6935
CODEN
APOPAI

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
40003325
Subject category
S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
Descriptors DEI
CALIBRATION; DISTRIBUTION FUNCTIONS; GEOMETRY; LIGHT SCATTERING; MEASURING METHODS; REMOTE SENSING; SATELLITES; TESTING; WAVELENGTHS
Descriptors DEC
FUNCTIONS; MATHEMATICS; SCATTERING

Optional Information

Notes
(c) 2008 Optical Society of America