Radiative transfer models for retrieval of cloud parameters from EPIC/DSCOVR measurements. (July 2018)

• Record Type: Journal Article
• Authors: Molina García, Víctor; Sasi, Sruthy; Efremenko, Dmitry S.; Doicu, Adrian; Loyola, Diego
• Is Part Of: Journal of quantitative spectroscopy & radiative transfer. Volume 213(2018)
• Page Start: 228
• Page End: 240
• Publication Date: 2018-07
• Subjects: Backscattering -- PCA -- Correlated k-distribution -- Asymptotic theory -- EPIC; Spectrum analysis -- Periodicals; Radiation -- Periodicals; Analyse spectrale -- Périodiques; Rayonnement -- Périodiques; Radiation; Spectrum analysis; Periodicals; 543.0858
• DOI: 10.1016/j.jqsrt.2018.03.014
• Languages: English
• ISSNs: 0022-4073

Abstract

Highlights: The requirements of the radiative transfer model for EPIC sensor are considered. The efficiency of exact and approximate models applied to EPIC is analyzed. The k -distribution method is used together with the principal component analysis. The performance is enhanced by four orders of magnitude with 1.5% of accuracy. Abstract: In this paper we analyze the accuracy and efficiency of several radiative transfer models for inferring cloud parameters from radiances measured by the Earth Polychromatic Imaging Camera (EPIC) on board the Deep Space Climate Observatory (DSCOVR). The radiative transfer models are the exact discrete ordinate and matrix operator methods with matrix exponential, and the approximate asymptotic and equivalent Lambertian cloud models. To deal with the computationally expensive radiative transfer calculations, several acceleration techniques such as, for example, the telescoping technique, the method of false discrete ordinate, the correlated k -distribution method and the principal component analysis (PCA) are used. We found that, for the EPIC oxygen A-band absorption channel at 764 nm, the exact models using the correlated k -distribution in conjunction with PCA yield an accuracy better than 1.5% and a computation time of 18 s for radiance calculations at 5 viewing zenith angles.