| On the Line Formation in Stellar Magnetized Atmospheres |
| |
| 作者姓名： | Zhong-Quan Qu Xiao-Yu Zhang and Zhi Xu |
| |
| 作者单位： | 1 Yunnan Observatory，Chinese Academy of Sciences，Kunming 650011 2 National Astronomical Observatories，Chinese Academy of Sciences，Beijing 100012 |
| |
| 摘 要： | 1 INTRODUCTIONIn the previous paper (on et al. 1999, hereafter Paper I), we investigated the wavelength-dependence of four colltribution functions (CFs) derived from dmerent formal solutions andreferring to different emergellt quantities in the unpolarized case. Because one cannot generallyassign a single formation region to the whole line band in a real stellar atmosphere, e.g., the solaratmosphere, instead, the line formation region can be defined as the layers deviating farthestfrom t…
|
| 关 键 词： | 太阳观测 大气 太阳黑子 磁场 |
On the Line Formation in Stellar Magnetized Atmospheres |
| |
| Zhong-Quan Qu,Xiao-Yu Zhang and Zhi Xu.On the Line Formation in Stellar Magnetized Atmospheres[J].Chinese Journal of Astronomy and Astrophysics,2001,1(2):161-175. |
| |
| Authors: | Zhong-Quan Qu Xiao-Yu Zhang and Zhi Xu |
| |
| Abstract: | |
| |
| Keywords: | line: formation - radiative transfer - Sun: atmosphere - sunspots Sun: magnetic fields |
| 本文献已被 CNKI 等数据库收录！ |
