Application of the spectrally integrated Voigt function to line-by-line radiative transfer modelling

被引:13
|
作者
Quine, B. M. [1 ,2 ]
Abrarov, S. M. [1 ]
机构
[1] Dept Earth & Space Sci & Engn, 4700 Keele St, Toronto, ON M3J 1P3, Canada
[2] Dept Phys & Astron, 4700 Keele St, Toronto, ON M3J 1P3, Canada
关键词
Radiance; Spectral radiance; Spectrally integrated Voigt function; Line-by-line radiative transfer model; Spectral line broadening; IMPLEMENTATION; APPROXIMATIONS; TRANSMITTANCE; COMPUTATION; ALGORITHM; SERIES;
D O I
10.1016/j.jqsrt.2013.04.020
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
We show that a new approach based on the spectrally integrated Voigt function (SIVF) enables the computation of line-by-line (LBL) radiative transfer at reduced spectral resolution without loss of accuracy. The algorithm provides rapid and accurate computation of area under the Voigt function in a way that preserves spectral radiance and, consequently, radiant intensity. The error analysis we provide shows the high-accuracy of the proposed SIVF approximations. A comparison of the performance of the method with that of the traditional LBL approach is presented. Motivations for the use and advantage of the SIVF as a replacement for conventional line function computations in radiative transfer are discussed. (C) 2013 Elsevier Ltd. All rights reserved.
引用
收藏
页码:37 / 48
页数:12
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