Efficient line-by-line calculation of absorption coefficients to high numerical accuracy

被引:42
作者
Sparks, L
机构
[1] Atmosph., Oceanic and Planet. Phys., Clarendon Laboratory, University of Oxford, Oxford OX1 3PU, Parks Road
[2] Jet Propulsion Laboratory, California Institute of Technology, Pasadena
基金
美国国家航空航天局;
关键词
D O I
10.1016/S0022-4073(96)00154-9
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Modeling radiative transfer at high resolution is computationally expensive due to the need to evaluate spectral absorption coefficients on a line-by-line basis. A simple yet efficient method is presented here for calculating these coefficients to high numerical accuracy. For each spectral line retained in the model, this method evaluates a contribution to absorption over the entire frequency range of interest (i.e., the far wings of each line are not truncated). The accuracy achieved is independent of the size of the sampling interval. The level of accuracy may be varied continuously over many orders of magnitude, thereby permitting the user to trade accuracy for speed and rendering it easy to perform convergence studies that quantify the numerical error. The method is applicable to any analytic model of the spectral line shape. (C) 1997 Elsevier Science Ltd.
引用
收藏
页码:631 / 650
页数:20
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