Standard problem of radiative transfer in a vibration-rotation band in a planetary atmosphere under non-LTE conditions

被引：0

作者：

Semenov, AO ^{[1
]}

Shved, GM ^{[1
]}

机构：

[1] St Petersburg State Univ, Dept Atmospher Phys, St Petersburg 198504, Russia

来源：

IRS 2000: CURRENT PROBLEMS IN ATMOSPHERIC RADIATION | 2001年

关键词：

D O I：

暂无

中图分类号：

X [环境科学、安全科学];

学科分类号：

08 ; 0830 ;

摘要：

We attempt here to lay foundations of general theory of radiative transfer in a vibration-rotation band in a planetary atmosphere by formulating and solving corresponding standard problem that is an integral equation for the source function. We introduce a convenient dimensionless vertical coordinate and four similarity parameters to describe the dependence of the source function on height. We propose formulas approximating the calculations of the source function.

引用

页码：337 / 340

页数：4

共 22 条

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Shved, GM
Semenov, AO
SOLAR SYSTEM RESEARCH, 2001, 35 (03) : 212 - 226
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A. O. Semenov
Solar System Research, 2001, 35 : 212 - 226
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[5] RADIATIVE-TRANSFER IN 15-MU-M CO2 BAND WITH NON-LTE IN EARTHS ATMOSPHERE
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[8] Non-LTE radiative transfer in the 4.7 and 2.3 μm bands of CO: Vibration-rotational non-LTE and its effects on limb radiance
Institut für Astronomie and Astrophysik, Universität München, ScheinerStr. 1, München
81679, Germany
不详
76021, Germany
J. Quant. Spectrosc. Radiat. Transf., 3 (317-339):
[9] STUDYING THE PHYSICAL CONDITIONS IN BE STAR DISKS USING NON-LTE RADIATIVE TRANSFER CODES
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Jones, C. E.
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INTERFEROMETRIC VIEW ON HOT STARS, 2010, 38 : 85 - 86
[10] A fast computation of radiative heating rates under non-LTE in a CO2 atmosphere
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IRS 2000: CURRENT PROBLEMS IN ATMOSPHERIC RADIATION, 2001, : 319 - 322

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