Stellar atmosphere

A point worth emphasizing is that hydrostatic equilibrium is fulfilled with great accuracy in stellar atmosphere .

值得强调指出，在恒星大气中，流体静力平衡是非常精确地成立的。

Line Formation Calculation for an Expanding stellar Atmosphere using the Linearized Separation Method

用线性化分离法计算膨胀恒星大气的谱线形成

Reversing layer model sulution for transport equation in stellar atmosphere absorption lines

恒星大气吸收线内转移方程的反变层模型解

A Study of the Characteristic Quantities of the Stokes Profiles of the Stellar Atmosphere in the Magnetic Field

在磁场条件下恒星大气Stokes轮廓特征量的研究

The conditions and elements present in the stellar atmosphere will dictate the chemical composition of the dust .

尘埃的化学成分受恒星大气呈现的状态与成分支配。

Absorption and scattering of stellar atmosphere

恒星大气的吸收和散射

The propagation of perturbations in the stellar atmosphere stratified due to gravity with steep density drop

在重力分层、密度陡降的恒星大气中扰动的传播

Principles and practice of the iterative alter - nating projection algorithm : the solution for non-LTE stellar atmosphere model with linear separate method

交互投影迭代算法的原理与实践：用线性化分离方法求解Non-LTE恒星大气模型

The physical parameters of stellar atmosphere , including the effective temperature , surface gravity and chemical abundance , are three main important factors leading to the differences of stellar spectra .

恒星大气物理参数，包括恒星的有效温度、表面重力、化学丰度，是导致恒星光谱差异的重要因素。

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 .

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 algorithms to measure the physical parameters of stellar atmosphere based on the template matching method are mainly studied , and the effectiveness of several template matching algorithms is demonstrated through the experiments on different measured data . 3 .

重点研究通过模板匹配方法测量恒星大气物理参数的算法，并通过对不同的实测数据的实验表明了几种模板匹配算法的有效性。