首页 | 官方网站   微博 | 高级检索  
     

多条太阳光球FeI线在磁场中形成及形成深度的综合分析(Ⅰ)
引用本文:宋慰鸿,艾国祥,张洪起,李孝昌.多条太阳光球FeI线在磁场中形成及形成深度的综合分析(Ⅰ)[J].中国天文和天体物理学报,1990(1).
作者姓名:宋慰鸿  艾国祥  张洪起  李孝昌
作者单位:成都科技大学高温高压物理所 (宋慰鸿),中国科学院北京天文台 (艾国祥,张洪起),成都科技大学高温高压物理所(李孝昌)
摘    要:针对多通道滤光器太阳磁场望远镜的磁场观测定标及掌握(所采用的)谱线特征之需要,取VAL宁静太阳大气模型计算了7条Fel光球线的Stokes轮廓、形成深度、贡献函数分布,从而较为系统地对多条反常及正常Zeeman线的特征及性质作出了分析与总结,解释了在磁光效应影响下Stokes Q,U参量的形成深度曲线在近线心区域处出现陡峭峰值的原因。

关 键 词:太阳  磁场  谱线

AN ANALYSIS FOR THE FORMATION AND THE FORMATION DEPTH OF SEVERAL SOLAR PHOTOSPHERIC FeI LINES IN MAGNETIC FIELD
Song Weihong.AN ANALYSIS FOR THE FORMATION AND THE FORMATION DEPTH OF SEVERAL SOLAR PHOTOSPHERIC FeI LINES IN MAGNETIC FIELD[J].Chinese Journal of Astronomy and Astrophysics,1990(1).
Authors:Song Weihong
Abstract:In order to meet the demand of the magnetic field observation calibration for the multichannel birefrigence filter, VAL quiet sun atmosphere model is adopted to compute Stokes profile, formation depth and distribution of contribution function for 7 Pel lines.The features and properties of some normal and anormalous Zeeman lines are analyzed, compared and summarized. The causes of sharp peaks of the Stokes Q and U curve under the influence of magnetic optical effect in the close line-center region are discussed.
Keywords:Sun (the): magnetic field-Spectral lines
本文献已被 CNKI 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司    京ICP备09084417号-23

京公网安备 11010802026262号