中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
CHROMOSPHERIC MAGNETIC FIELDS OF AN ACTIVE REGION FILAMENT

文献类型:会议论文

作者Xu Z(徐稚)1; Solanki, S2; Lagg, A2
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
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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