CHROMOSPHERIC MAGNETIC FIELDS OF AN ACTIVE REGION FILAMENT
文献类型:会议论文
作者 | Xu Z(徐稚)1![]() |
出版日期 | 2012 |
会议名称 | 4th Frech-Chinese Meeting on Solar Physics |
会议日期 | 2011-11-15 |
会议地点 | Nice, FRANCE |
卷号 | 55 |
页码 | 163-168 |
通讯作者 | Xu, Z (reprint author), Chinese Acad Sci, Yunnan Astron Observ, Kunming 650011, Yunnan, Peoples R China. |
英文摘要 | Vector magnetic fields of an active region filament are co-spatially and co-temporally mapped in photosphere and upper chromosphere, by using spectro-polaximetric observations made by Tenerife Infrared Polarimeter (TIP II) at the German Vacuum Tower Telescope (VTT). A Zeeman-based ME inversion is performed on the full Stokes vectors of both the photospheric Si I 1082.7 nm and the chromospheric He I 1083.0 nm lines. We found that the strong magnetic fields, with the field strength of 600-800 G in the He I line formation height, are not uncommon among AR filaments. But such strong magnetic field is not always found in AR filaments. |
收录类别 | CPCI |
产权排序 | 第一完成单位 |
会议网址 | http://www.eas-journal.org/articles/eas/abs/2012/03/eas1255022/eas1255022.html |
会议录 | EAS Publications Series - UNDERSTANDING SOLAR ACTIVITY: ADVANCES AND CHALLENGES
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会议录出版者 | E D P SCIENCES |
学科主题 | Astronomy & Astrophysics |
会议录出版地 | 17 AVE DU HOGGAR PARC D ACTIVITES COUTABOEUF BP 112, F-91944 CEDEX A, FRANCE |
语种 | 英语 |
ISSN号 | 1633-4760 |
ISBN号 | 978-2-7598-0752-9 |
WOS记录号 | WOS:000312967500022 |
研究领域[WOS] | Astronomy & Astrophysics |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4853] ![]() |
专题 | 云南天文台_抚仙湖太阳观测站 |
作者单位 | 1.Yunnan Astronomical Observatory, CAS, Kunming, 650011 Yunnan, China 2.Max-Planck-Institut für Sonnensystemforschung, Max-Planck-Strasse 2, 37191 Katlenburg-Lindau, Germany |
推荐引用方式 GB/T 7714 | Xu Z,Solanki, S,Lagg, A. CHROMOSPHERIC MAGNETIC FIELDS OF AN ACTIVE REGION FILAMENT[C]. 见:4th Frech-Chinese Meeting on Solar Physics. Nice, FRANCE. 2011-11-15.http://www.eas-journal.org/articles/eas/abs/2012/03/eas1255022/eas1255022.html. |
入库方式: OAI收割
来源:云南天文台
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