辐射转移方程

对含有磁场的相对论热等离子体的同步加速辐射，考虑等离子体的自吸收，求解辐射转移方程，得到等离子体表面向外的同步加速辐射的辐射强度。

In solving the radiative transfer equation , we have found the specific intensity of synchrotron emission in relativistic hot plasma with self - absorption .

本文根据偏振辐射转移方程组就形成于有磁场的恒星大气中的Stokes轮廓的一些特征量与磁场强度大小的关系从理论上进行了探讨。

The relation between some of the characteristic quantities of the Stokes profiles of the stellar atmosphere with the magnetic field and the magnetic field strength is theoretically explored .

对恒星力学平衡方程及辐射转移方程的一点修正

Corrections to the mechanical equilibrium equation for a star and to the transfer equation of stellar radiation

本文首先介绍了等离子体关于波的衰变和合成过程中，高频电磁波的湍动辐射转移方程，然后通过谱线的非湍动辐射转移理论。

In this paper one of the very important nonlinear process in plasma & the decay and synthesis of the waves and the turbulent radiation displacement equation of the high-frequency electromagnetic waves in the process is introduced at first .