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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[15] An Improved Optical Model for the Non-LTE Problem for the CO2 Molecule in the Atmosphere of Mars: Nighttime Populations of Vibrational States and the Rate of Radiative Cooling of the Atmosphere
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[16] An improved optical model for the non-LTE problem for the CO2 molecule in the atmosphere of Mars:: Nighttime populations of vibrational states and the rate of radiative cooling of the atmosphere
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[17] AN APPROXIMATE METHOD FOR THE SOLUTION OF THE RADIATION TRANSFER PROBLEM IN THE 4,3 MU-M CO2 BAND IN AN OPTICALLY THICK ATMOSPHERE WITH THE RELATIONAL NON-LTE
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[19] PARAMETERIZATION OF IR COOLING IN A MIDDLE ATMOSPHERE DYNAMICS MODEL .2. NON-LTE RADIATIVE-TRANSFER AND THE GLOBALLY AVERAGED TEMPERATURE OF THE MESOSPHERE AND LOWER THERMOSPHERE
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