An empirical line-by-line model for the infrared solar transmittance spectrum from 700 to 5000 cm- 1

Journal of Quantitative Spectroscopy and Radiative Transfer

Volumn 102, Issue 3, 2006, Pages 450-463

  Hase, F ^a   Demoulin, P ^b   Sauval, A J ^c   Toon, G C ^d   Bernath, P F ^e   Goldman, A ^f   Hannigan, J W ^g   Rinsland, C P ^h  

^a KARLSRUHE INSTITUTE OF TECHNOLOGY   (Germany)

^b UNIVERSITY OF LIÈGE   (Belgium)

^c ROYAL OBSERVATORY OF BELGIUM   (Belgium)

^d CALIFORNIA INSTITUTE OF TECHNOLOGY   (United States)

^e UNIVERSITY OF WATERLOO   (Canada)

^f UNIVERSITY OF DENVER   (United States)

^g NATIONAL CENTER FOR ATMOSPHERIC RESEARCH   (United States)

^h NASA LANGLEY RESEARCH CENTER   (United States)

Author keywords

Atmospheric trace gases; Infrared spectroscopy; Radiative transfer; Retrieval algorithms; Solar spectrum

Indexed keywords

ALGORITHMS; INFRARED SPECTROSCOPY; MATHEMATICAL MODELS; SOLAR RADIATION; SPECTRUM ANALYSIS;

ATMOSPHERIC TRACE GASES; RADIATIVE TRANSFER; RETRIEVAL ALGORITHMS; SOALR SPECTRUM;

SUN;

ATMOSPHERIC MODELING; EMPIRICAL ANALYSIS; INFRARED RADIATION; RADIATIVE TRANSFER; REMOTE SENSING; SOLAR RADIATION; SPECTRAL ANALYSIS; TRACE GAS; TRANSMITTANCE;

EID: 33747621411     PISSN: 00224073     EISSN: None     Source Type: Journal    
DOI: 10.1016/j.jqsrt.2006.02.026     Document Type: Article

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