Correlation analysis between vector magnetograms measured by (ST)-T-3 and MSFC | |
Liang, HF1,2![]() ![]() ![]() ![]() | |
刊名 | NEW ASTRONOMY
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2007-08 | |
卷号 | 12期号:6页码:497-506 |
关键词 | polarization radiative transfer Sun : sunspots Sun : vector magnetic field |
ISSN号 | 1384-1076 |
通讯作者 | Liang, HF (reprint author), Yunnan Normal Univ, Kunming 650011, Peoples R China. |
产权排序 | 第二完成单位 |
英文摘要 | By quantitative analysis of AR NOAA 10484 two-dimensional Stokes spectra obtained from the Solar Stokes Spectral Telescope (S(3)7) at the Yunnan Observatory, we have derived three components, the flux intensity B, the inclination gamma and the azimuth chi of the vector magnetic fields in the AR. The contours of the flux intensity B have a basic agreement to the morphological configuration of the sunspot group in white-light. Comparing the vector magnetograms obtained by (ST)-T-3 and by the NASA/Marshall Space Flight Center (MSFC), basic agreement on the longitudinal and transverse components between the S3T and MSFC magnetograms is found, resulting in correlation coefficients rho(B parallel to) = 0.904, rho(B1) = 0.749 and rho(az), = 0.941. There is a split of 241 m angstrom between the two sigma lines of Fe I 6302.5 angstrom which implies the field flux intensity near the center of the west umbra is 2600 G. This value is consistent with the result obtained by fitting the Stokes profiles. (C) 2007 Elsevier B.V. All rights reserved. |
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] | STOKES PROFILE ANALYSIS ; MAGNETIC-FIELDS ; CURRENT HELICITY ; ACTIVE REGIONS ; LINES ; MEES ; INVERSION ; HALEAKALA ; HUAIROU |
收录类别 | SCI ; EI |
原文出处 | http://www.sciencedirect.com/science/article/pii/S1384107607000188 |
语种 | 英语 |
WOS记录号 | WOS:000246728100010 |
公开日期 | 2016-05-03 |
内容类型 | 期刊论文 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/6102] ![]() |
专题 | 云南天文台_太阳物理研究组 |
作者单位 | 1.Yunnan Normal University, Kunming 650011, China 2.National Astronomical Observatories/Yunnan Observatory, CAS, Kunming 650011, China 3.National Satellite Meteorological Center, China Meteorological Administration, Beijing 100081, China 4.Xiangtan University, Hunan, China |
推荐引用方式 GB/T 7714 | Liang, HF,Qu ZQ,Zhao, HJ,et al. Correlation analysis between vector magnetograms measured by (ST)-T-3 and MSFC[J]. NEW ASTRONOMY,2007,12(6):497-506. |
APA | Liang, HF,Qu ZQ,Zhao, HJ,&Xiang, FY.(2007).Correlation analysis between vector magnetograms measured by (ST)-T-3 and MSFC.NEW ASTRONOMY,12(6),497-506. |
MLA | Liang, HF,et al."Correlation analysis between vector magnetograms measured by (ST)-T-3 and MSFC".NEW ASTRONOMY 12.6(2007):497-506. |
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