Forward Monte Carlo computations of fully polarized microwave radiation in non-isotropic media

被引:28
作者
Battaglia, A
Mantovani, S
机构
[1] Univ Ferrara, Dept Phys, I-44100 Ferrara, Italy
[2] ISAC, CNR, Inst Atmospher Sci & Climate, I-40129 Bologna, Italy
基金
美国国家航空航天局;
关键词
radiative transfer; non-spherical particles; biasing technique;
D O I
10.1016/j.jqsrt.2004.12.002
中图分类号
O43 [光学];
学科分类号
070207 ; 0803 ;
摘要
A completely forward Monte Carlo radiative transfer code has been developed with biasing techniques to efficiently solve the polarized radiative transfer equation for the full Stokes vector. The code has been adapted to accommodate plane parallel/3-D vertically/horizontally inhomogeneous scattering atmospheres in Cartesian geometries. Particular attention has been paid in stochastically treating the propagation, the emission and the scattering through anisotropic media particularly suited for clouds containing perfectly or partially oriented particles. Our modelling is very appealing because all its biasing techniques do not introduce unphysical Stokes vector. Numerical results and comparisons with benchmark tests are presented for verification. (c) 2005 Elsevier Ltd. All rights reserved.
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收藏
页码:285 / 308
页数:24
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