The k-distribution method and correlated-k approximation for a shortwave radiative transfer model

被引:223
|
作者
Kato, S [1 ]
Ackerman, TP [1 ]
Mather, JH [1 ]
Clothiaux, EE [1 ]
机构
[1] Penn State Univ, Dept Meteorol, University Pk, PA 16802 USA
基金
美国国家航空航天局;
关键词
D O I
10.1016/S0022-4073(98)00075-2
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
Absorption cross sections are tabulated for water vapor, including continuum absorption, ozone, oxygen and carbon dioxide in the solar spectral region by adopting the k-distribution method. These tables are generated based on line-by-line code results for ranges of total pressure, temperature and water vapor concentration typical of values throughout the troposphere. These tables are incorporated into a shortwave radiative transfer code, which has 32 wavelength intervals across the solar spectrum, by using the correlated-k approximation in order to evaluate the accuracy in the broad band direct normal irradiance computation. A comparison of the direct normal irradiance with MODTRAN3 demonstrates that these tables can be used for shortwave broad band irradiance computations; the difference in the transmissivity is within 0.01 throughout most of the solar spectral region. (C) 1999 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码:109 / 121
页数:13
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