期刊
ASTRONOMY & ASTROPHYSICS
卷 417, 期 3, 页码 793-805出版社
EDP SCIENCES S A
DOI: 10.1051/0004-6361:20040017
关键词
radiative transfer; stars : circumstellar matter; methods : numerical
We present benchmark problems and solutions for the continuum radiative transfer (RT) in a 2D disk configuration. The reliability of three Monte-Carlo and two grid-based codes is tested by comparing their results for a set of well-defined cases which differ for optical depth and viewing angle. For all the configurations, the overall shape of the resulting temperature and spectral energy distribution is well reproduced. The solutions we provide can be used for the verification of other RT codes. We also point out the advantages and disadvantages of the various numerical techniques applied to solve the RT problem.
作者
我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。
推荐
暂无数据