2012
DOI: 10.1016/j.rse.2012.07.012
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Accuracy assessments of cloud droplet size retrievals from polarized reflectance measurements by the research scanning polarimeter

Abstract: We present an algorithm for the retrieval of cloud droplet size distribution parameters (effective radius and variance) from the Research Scanning Polarimeter (RSP) measurements. The RSP is an airborne prototype for the Aerosol Polarimetery Sensor (APS), which was on-board of the NASA Glory satellite. This instrument measures both polarized and total reflectance in 9 spectral channels with central wavelengths ranging from 410 to 2260 nm. The cloud droplet size retrievals use the polarized reflectance in the sc… Show more

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Cited by 111 publications
(164 citation statements)
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“…The second step is to fit the observed polarized reflectances (OPRs) with the polarized phase functions (P P ) in the LUT, which is based on the following expression of Bréon and Doutriaux-Boucher (2005): where λ is the wavelength, is the scattering angle, and the empirical fitting parameters a, b, and c represent the polarized contributions from multiple scattering, Rayleigh scattering, aerosol extinction, ground surface reflectance of thin clouds, and effects caused by rotation to the scattering plane. The parameter cos 2 ( ) is used to account for the Rayleigh scattering contributions (Alexandrov et al, 2012a). We adopt the multiple linear regression fit method of Bevington and Robinson (1969) to calculate the parameters a, b, and c for every CDR and EV combination.…”
Section: Retrieval Methodsmentioning
confidence: 99%
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“…The second step is to fit the observed polarized reflectances (OPRs) with the polarized phase functions (P P ) in the LUT, which is based on the following expression of Bréon and Doutriaux-Boucher (2005): where λ is the wavelength, is the scattering angle, and the empirical fitting parameters a, b, and c represent the polarized contributions from multiple scattering, Rayleigh scattering, aerosol extinction, ground surface reflectance of thin clouds, and effects caused by rotation to the scattering plane. The parameter cos 2 ( ) is used to account for the Rayleigh scattering contributions (Alexandrov et al, 2012a). We adopt the multiple linear regression fit method of Bevington and Robinson (1969) to calculate the parameters a, b, and c for every CDR and EV combination.…”
Section: Retrieval Methodsmentioning
confidence: 99%
“…The Rayleigh optical thickness for different wavelengths was set according to the results of Bodhaine et al (1999). The solar zenith angle was assumed to be 20 • , and the relative azimuth angle was 180 • (the sensor was in front of the sun), which avoids potential error induced by the rotation to the scattering plane (Hansen and Travis, 1974;Alexandrov et al, 2012a).…”
Section: Polder-like Observations Simulated With the Rt3 Modelmentioning
confidence: 99%
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