Inhomogeneous radiative model of refractive and dispersive semi-transparent stellar atmospheres

被引：9
|
作者：
Ben-Abdallah, P [1 ]
Le Dez, V
Lemonnier, D
Fumeron, S
Charette, A
机构：
[1] Univ Quebec, Grp Rech Ingn Procedes & Syst, Chicoutimi, PQ G7H 2B1, Canada
[2] Ecole Natl Super Mecan & Aerotech, UMR CNRS 6608, Lab Etud Therm, F-86960 Futuroscope, France
来源：
JOURNAL OF QUANTITATIVE SPECTROSCOPY & RADIATIVE TRANSFER | 2001年 / 69卷 / 01期
关键词：
D O I：
10.1016/S0022-4073(00)00062-5
中图分类号：
O43 [光学];
学科分类号：
070207 ; 0803 ;
摘要：
A time-independent radiative model for the inhomogeneous semi-transparent stellar atmospheres is developed taking into account a continuous variation of both the refractive index and the absorption coefficient. The medium considered is supposed to have an internal space-dependent energy source and a purely reflective boundary illuminated by an external flux. The integral forms of the radiative transfer equation with any spatially continuous refractive index and any phase function are derived from its integro-differential form. (C) 2001 Elsevier Science Ltd. All rights reserved.
引用
收藏
页码：61 / 80
页数：20
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