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

[21] Non-LTE models for synthetic spectra of type Ia supernovae/hot stars with extremely extended atmospheres II. Improved lower boundary conditions for the numerical solution of the radiative transfer
Sauer, D. N.
Hoffmann, T. L.
Pauldrach, A. W. A.
ASTRONOMY & ASTROPHYSICS, 2006, 459 (01) : 229 - 240
[22] A NON-LTE RADIATIVE-TRANSFER MODEL FOR INFRARED BANDS IN THE MIDDLE ATMOSPHERE .2. CO2 (2.7 AND 4.3 MU-M) AND WATER-VAPOR (6.3 MU-M) BANDS AND N2(1) AND O2(1) VIBRATIONAL LEVELS
LOPEZPUERTAS, M
RODRIGO, R
LOPEZMORENO, JJ
TAYLOR, FW
JOURNAL OF ATMOSPHERIC AND TERRESTRIAL PHYSICS, 1986, 48 (08): : 749 - 764

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