PMO OpenIR  > 期刊(老文献)
论白光太阳磁象仪的原理
叶式辉,金介海
1987
Source PublicationChinese Journal of Astronomy and Astrophysics
ISSN1009-9271
Volume7Issue:3Pages:238-248
Abstract现有的天体磁场测量方法主要根据磁场敏感谱线的塞曼效应,而解释观测资料的理论基础是斯托克斯(Stokes)参数的形成及其转移方程的求解。近年来,为了观测太阳的向量磁场和精细结构磁场,仪器技术和理论分析都得到迅速发展,这突出表现在斯托克斯偏振量度学的诞生。本文对这些情况作扼要的综合介绍。
Keyword天文仪器 太阳磁象仪
Subject Area天文和天体物理
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/7623
Collection期刊(老文献)
Recommended Citation
GB/T 7714
叶式辉,金介海. 论白光太阳磁象仪的原理[J]. Chinese Journal of Astronomy and Astrophysics,1987,7(3):238-248.
APA 叶式辉,金介海.(1987).论白光太阳磁象仪的原理.Chinese Journal of Astronomy and Astrophysics,7(3),238-248.
MLA 叶式辉,金介海."论白光太阳磁象仪的原理".Chinese Journal of Astronomy and Astrophysics 7.3(1987):238-248.
Files in This Item:
File Name/Size DocType Version Access License
1987445论白光太阳磁象仪的原理.p(2963KB) 开放获取LicenseView Application Full Text
Related Services
Recommend this item
Bookmark
Usage statistics
Export to Endnote
Google Scholar
Similar articles in Google Scholar
[叶式辉,金介海]'s Articles
Baidu academic
Similar articles in Baidu academic
[叶式辉,金介海]'s Articles
Bing Scholar
Similar articles in Bing Scholar
[叶式辉,金介海]'s Articles
Terms of Use
No data!
Social Bookmark/Share
File name: 1987445论白光太阳磁象仪的原理.pdf
Format: Adobe PDF
All comments (0)
No comment.
 

Items in the repository are protected by copyright, with all rights reserved, unless otherwise indicated.