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恒星大气吸收线内转移方程的反变层模型解
引用本文:骆宏悌.恒星大气吸收线内转移方程的反变层模型解[J].湖南师范大学自然科学学报,1986(2).
作者姓名:骆宏悌
摘    要:本文首先引入恒星大气的反变层模型,在反变层的特定条件下,得出相应的吸收线内的辐射转移方程,再引入与方向无关的近似条件和将普朗克函数按光学深度展开,分别求出对于累积辐射而言的剩余强度和对点的辐射而言的剩余强度。

关 键 词:空间物理学  恒星大气  吸收谱  辐射转移  方程解

REVERSING LAYER MODEL SULUTION FOR TRANSPORT EQUATION IN STELLAR ATMOSPHERE ABSORPTION LINES
Luo Hongti.REVERSING LAYER MODEL SULUTION FOR TRANSPORT EQUATION IN STELLAR ATMOSPHERE ABSORPTION LINES[J].Journal of Natural Science of Hunan Normal University,1986(2).
Authors:Luo Hongti
Abstract:In this paper,the reversing layer model of stellar atmosphere is introduced at first.Thenon a special condition of reversing layer the radiative transport equations in absorption lineare obtained.At last,on presenting an approximate condition which has no relation todirection and expanding planck function according to optical depth,the residual intensityfor accumulative transmition and point transmition are found respectively.
Keywords:space physics  stellar atmosphere  absorption spectra  radiative transfer  solution of equation
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