On the solution of the radiative transfer equations for polarized radiation

On the solution of the radiative transfer equations for polarized radiation
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偏振辐射辐射传输方程的求解

DOI:
10.1007/bf00165988
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发表时间:
1985
期刊:
影响因子:
2.8
通讯作者:
M. L. Degl'innocenti
M. L. Degl'innocenti
中科院分区:
物理与天体物理3区
文献类型:
--
作者:
E. L. Degl'innocenti;M. L. Degl'innocenti

文献摘要

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当Stokes参数的吸收Mueller矩阵沿射线路径为常数时,给出了极化辐射传递方程解析解的一般形式。然后,将该形式应用于寻找典型色球线的Stokes参数剖面的解析近似,该线具有光深依赖于源函数的形式S(τ) = (ν + δ)1/2(1 + ν)1/2。
A general formalism is presented to obtain an analytical solution of the radiative transfer equations for polarized radiation when the absorption Mueller matrix for the Stokes parameters is constant along the ray-path. The formalism is then applied to find an analytical approximation of the Stokes parameters profiles for a typical chromospheric line having an optical-depth dependence of the source function of the form S(τ) = (ɛ + δ)1/2(1 + ɛ)1/2.