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The coronal magnetic field reversal observed by the SOLARC instrument
Liu Y(刘煜); Shen YD(申远灯); Liu, Y (reprint author), Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Peoples R China.
会议录名称SCIENCE IN CHINA SERIES G-PHYSICS MECHANICS & ASTRONOMY
2009-11
卷号52
期号11
页码1696-1701
DOI10.1007/s11433-009-0248-1
产权排序第1完成单位
收录类别SCI ; EI ; CPCI
会议名称Solar Workshop on Solar Magnetism, Corona and Space Weather - Chinese Space Solar Telescope Science
会议日期2008-07-28
会议地点Jiuquan, PEOPLES R CHINA
关键词Solar Corona Magnetic Field Infrared Wavelength Extrapolation
摘要High-sensitivity measurements for mapping coronal magnetic field have become possible since the recent development of infrared detection techniques. One urgent task that arises from the routine infrared observations is to interpret what the Stokes signals could indicate for coronal magnetic fields. It is the first time for us to successfully reveal the coronal field structure above a simple and stable sunspot on the photosphere using profiles of full Stokes parameters. In this paper, the author further points out the deficiency in any conclusions/judgements just based on incomplete polarization data. A magnetic flux reversal feature, observed from circular polarization data, may correspond to one or more coronal tubes with their front or farside arching apex there, more complicated than people imagined before. To exactly locate the infrared radiation sources, we need both circular and linear polarization data for an integrated analysis of them.
语种英语
学科领域Physics
文章类型Article; Proceedings Paper
出版者SCIENCE PRESS
出版地16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA
ISSN号1672-1799
URL查看原文
归档日期2009-11-10
WOS记录号WOS:000271718600011
WOS研究方向Physics
WOS类目Physics, Multidisciplinary
关键词[WOS]POLARIZATION
WOS标题词Science & Technology ; Physical Sciences
引用统计
被引频次:3[WOS]   [WOS记录]     [WOS相关记录]
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/7216
专题选址与日冕观测组
通讯作者Liu, Y (reprint author), Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Peoples R China.
作者单位National Astronomical Observatories, Yunnan Astronomical Observatory, Kunming, 650011, China
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Liu Y,Shen YD,Liu, Y . The coronal magnetic field reversal observed by the SOLARC instrument[C]. 16 DONGHUANGCHENGGEN NORTH ST, BEIJING 100717, PEOPLES R CHINA:SCIENCE PRESS,2009:1696-1701.
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