BACKWARD AND FORWARD MONTE CARLO METHOD IN POLARIZED RADIATIVE TRANSFER

被引:24
|
作者
Yong, Huang [1 ]
Guo-Dong, Shi [1 ,2 ]
Ke-Yong, Zhu [1 ]
机构
[1] Beihang Univ, Sch Aeronaut Sci & Engn, Beijing 100191, Peoples R China
[2] Aviat Univ Air Force, Changchun 130022, Peoples R China
来源
ASTROPHYSICAL JOURNAL | 2016年 / 820卷 / 01期
基金
美国国家科学基金会;
关键词
methods: numerical; polarization; radiative transfer; TRANSFER MODELS; DISCRETE-ORDINATE; SUCCESSIVE ORDER; SCATTERING; ATMOSPHERE; LIGHT; INDEX; TRANSPORT; SIMULATIONS; RADIANCE;
D O I
10.3847/0004-637X/820/1/9
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
In general, the Stocks vector cannot be calculated in reverse in the vector radiative transfer. This paper presents a novel backward and forward Monte Carlo simulation strategy to study the vector radiative transfer in the participated medium. A backward Monte Carlo process is used to calculate the ray trajectory and the endpoint of the ray. The Stocks vector is carried out by a forward Monte Carlo process. A one-dimensional graded index semi-transparent medium was presented as the physical model and the thermal emission consideration of polarization was studied in the medium. The solution process to non-scattering, isotropic scattering, and the anisotropic scattering medium, respectively, is discussed. The influence of the optical thickness and albedo on the Stocks vector are studied. The results show that the U, V-components of the apparent Stocks vector are very small, but the Q-component of the apparent Stocks vector is relatively larger, which cannot be ignored.
引用
收藏
页数:11
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