The determination of the solar vector magnetic field at the surface from Stokes profiles | |
Qu ZQ(屈中权); Ding YJ(丁有济); Xuan JY(宣家余) | |
刊名 | ASTROPHYSICS AND SPACE SCIENCE
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1993-10 | |
卷号 | 208期号:2页码:229-244 |
ISSN号 | 0004-640X |
通讯作者 | Qu, ZQ |
产权排序 | 第一完成单位 |
英文摘要 | A simple method is proposed to infer the vector magnetic field at the surface of the Sun from Stokes profiles. This is based on the assumption that the variations of thermodynamical and magnetic field parameters with depth near the surface are so small that the displacements of the wavelengths at which the Stokes profiles reach their extrema can be ignored. And hence the polarized radiative transfer equations are greatly reduced to a set of non-linear equations with vector magnetic field parameters (H, gamma, chi) which can be solved by a numerical iteration method. By fitting the synthetic profiles, it is shown that this proposed method can produce information on the vector field at the surface. It is also used to revise the observed profiles and it is found that the observed sunspot has the magnetic field structure of the fan model with the lines of magnetic field twisted. |
学科主题 | Astronomy & Astrophysics |
WOS标题词 | Science & Technology ; Physical Sciences |
类目[WOS] | Astronomy & Astrophysics |
研究领域[WOS] | Astronomy & Astrophysics |
关键词[WOS] | INVERSION ; LINES |
收录类别 | SCI |
原文出处 | http://link.springer.com/article/10.1007%2FBF00657938 |
语种 | 英语 |
WOS记录号 | WOS:A1993MR94900005 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/5102] ![]() |
专题 | 云南天文台_光纤阵列太阳光学望远镜研究组 |
作者单位 | Yunnan Astronomical Observatory, Kunming, P.R. China |
推荐引用方式 GB/T 7714 | Qu ZQ,Ding YJ,Xuan JY. The determination of the solar vector magnetic field at the surface from Stokes profiles[J]. ASTROPHYSICS AND SPACE SCIENCE,1993,208(2):229-244 . |
APA | Qu ZQ,Ding YJ,&Xuan JY.(1993).The determination of the solar vector magnetic field at the surface from Stokes profiles.ASTROPHYSICS AND SPACE SCIENCE,208(2),229-244 . |
MLA | Qu ZQ,et al."The determination of the solar vector magnetic field at the surface from Stokes profiles".ASTROPHYSICS AND SPACE SCIENCE 208.2(1993):229-244 . |
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