NAOC Open IR
用斯托克斯轮廓推导太阳矢量磁场和热力学参量的三维结构
陈学昆; 张霄宇; 屈中权; 丁有济
1996
Source Publication天文学报
ISSN0001-5245
Volume037Issue:002Pages:201
Abstract一种根据斯托克斯轮廓分析推导太阳矢量磁场和热力学参量的空间三维结构的新方法在本文中提出。在不考虑散射和原子偏振的假设下,该方法由三个具有不同功能的操作分别作用于太阳大气中一层或二层斯托克斯轮廓组成。这三个操作构成一个运行单元。
Language英语
Document Type期刊论文
Identifierhttp://ir.bao.ac.cn/handle/114a11/39404
Collection中国科学院国家天文台
Affiliation中国科学院国家天文台
First Author AffilicationNational Astronomical Observatories, Chinese Academy of Sciences
Recommended Citation
GB/T 7714
陈学昆,张霄宇,屈中权,等. 用斯托克斯轮廓推导太阳矢量磁场和热力学参量的三维结构[J]. 天文学报,1996,037(002):201.
APA 陈学昆,张霄宇,屈中权,&丁有济.(1996).用斯托克斯轮廓推导太阳矢量磁场和热力学参量的三维结构.天文学报,037(002),201.
MLA 陈学昆,et al."用斯托克斯轮廓推导太阳矢量磁场和热力学参量的三维结构".天文学报 037.002(1996):201.
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