Revised and extended benchmark results for Rayleigh scattering of sunlight in spherical atmospheres

dc.contributor.authorKorkin, Sergey
dc.contributor.authorYang, Eun-Su
dc.contributor.authorSpurr, Robert
dc.contributor.authorEmde, Claudia
dc.contributor.authorKrotkov, Nickolay
dc.contributor.authorVasilkov, Alexander
dc.contributor.authorHaffner, David
dc.contributor.authorMok, Jungbin
dc.contributor.authorLyapustin, Alexei
dc.date.accessioned2023-07-20T18:46:23Z
dc.date.available2023-07-20T18:46:23Z
dc.date.issued2020-08-11
dc.description.abstractWhile most of traditional Earth-atmosphere satellite remote sensing relies on radiative transfer (RT) in the plane parallel geometry, effects of sphericity are important at high sun and view zenith angles. Broad understanding of these effects is limited and, contrary to the plane-parallel case, finding accurate numerical results to test spherical RT codes is not easy. This paper aims to partially fill in this gap. Using the full-spherical RT code MYSTIC (Monte Carlo), and the plane-parallel RT code VLIDORT (discrete ordinates) corrected for atmospheric sphericity in the single and multiple scattering, we reproduced with better accuracy and extended the benchmark results by Adams & Kattawar [1].en_US
dc.description.sponsorshipThe work of S. Korkin was supported by the NASA's Earth Science Division under Grant 17-TASNPP17–0116, and in part by the USRA Internal Research & Development (R&D) program. He is also thankful to James Limbacher (SSAI and NASA GSFC) for discussion of many related topics from RT and Monte Carlo, to parallel computing in Python, and to Corey Bettenhausen (Adnet and NASA GSFC) for help with libRadtran setup. We are grateful to three anonymous reviewers for their comments and suggestions.en_US
dc.description.urihttps://www.sciencedirect.com/science/article/pii/S0022407320303976en_US
dc.format.extent16 pagesen_US
dc.genrejournal articlesen_US
dc.identifierdoi:10.13016/m2wla0-42so
dc.identifier.citationKorkin, Sergey, et al. "Revised and extended benchmark results for Rayleigh scattering of sunlight in spherical atmospheres." Journal of Quantitative Spectroscopy and Radiative Transfer 254, 107181 (11 August, 2020). https://doi.org/10.1016/j.jqsrt.2020.107181.en_US
dc.identifier.urihttps://doi.org/10.1016/j.jqsrt.2020.107181
dc.identifier.urihttp://hdl.handle.net/11603/28813
dc.language.isoen_USen_US
dc.publisherElsevieren_US
dc.relation.isAvailableAtThe University of Maryland, Baltimore County (UMBC)
dc.relation.ispartofUMBC GESTAR II Collection
dc.relation.ispartofUMBC Faculty Collection
dc.rightsThis work was written as part of one of the author's official duties as an Employee of the United States Government and is therefore a work of the United States Government. In accordance with 17 U.S.C. 105, no copyright protection is available for such works under U.S. Law.en_US
dc.rightsPublic Domain Mark 1.0*
dc.rights.urihttp://creativecommons.org/publicdomain/mark/1.0/*
dc.titleRevised and extended benchmark results for Rayleigh scattering of sunlight in spherical atmospheresen_US
dc.typeTexten_US
dcterms.creatorhttps://orcid.org/0000-0003-4690-3232en_US

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