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Radio observations of the fine structure inside a post-CME current sheet
Gao GN(高冠男)1,2,3; Wang M(汪敏)1,3,4; Lin J(林隽)1; Wu, N5; Tan, CM4; Berhard Kliem1,6; Su, Y7; Gao, GN (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China.
发表期刊RESEARCH IN ASTRONOMY AND ASTROPHYSICS
2014-07
卷号14期号:7页码:843-854
DOI10.1088/1674-4527/14/7/006
产权排序第1完成单位
收录类别SCI
关键词Sun: Coronal Mass Ejections (Cmes) Sun: Flares Sun: Solar Radio Bursts Sun: Magnetic Reconnection
摘要A solar radio burst was observed in a coronal mass ejection/flare event by the Solar Broadband Radio Spectrometer at the Huairou Solar Observing Station on 2004 December 1. The data exhibited various patterns of plasma motions, suggestive of the interaction between sunward moving plasmoids and the flare loop system during the impulsive phase of the event. In addition to the radio data, the associated white-light, H alpha, extreme ultraviolet light, and soft and hard X-rays were also studied.
项目资助者National Basic Research Program of China (973 program) [2011CB811403, 2013CBA01503] ; National Natural Science Foundation of China [11273055, 11173010, 11333007, 10978006, 11103044, 11273030] ; CAS [KJCX2-EW-T07, XDB09040202] ; DFG ; European Community Framework Programme 7, High Energy Solar Physics Data in Europe (HESPE) [263086] ; Key Laboratory of Solar Activity, National Astronomical Observatories, CAS ; Chinese Academy of Sciences [2012T1J0017]
语种英语
学科领域Astronomy & Astrophysics
文章类型Article
ISSN1674-4527
URL查看原文
归档日期2014-09-10
WOS记录号WOS:000339102700006
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]SOLAR-FLARE ; MAGNETIC RECONNECTION ; CHROMOSPHERIC EVAPORATION ; ELECTRON ACCELERATION ; CORONAL LOOP ; DECEMBER 1 ; MOTIONS ; SPECTROMETER ; SHRINKAGE ; ERUPTION
引用统计
被引频次:7[WOS]   [WOS记录]     [WOS相关记录]
文献类型期刊论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/5629
专题射电天文研究组
中国科学院天体结构与演化重点实验室
通讯作者Gao, GN (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China.
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
2.University of Chinese Academy of Sciences, Beijing 100049, China
3.Key Laboratory for the Structure and Evolution of Celestial Objects, Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China
4.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China
5.School of Tourism and Geography, Yunnan Normal University, Kunming 650031, China
6.Institute of Physics and Astronomy, University of Potsdam, Potsdam 14476, Germany
7.IGAM-Kanzelhöhe Observatory, Institute of Physics, University of Graz, Universitätsplatz 5, 8010 Graz, Austria
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GB/T 7714
Gao GN,Wang M,Lin J,et al. Radio observations of the fine structure inside a post-CME current sheet[J]. RESEARCH IN ASTRONOMY AND ASTROPHYSICS,2014,14(7):843-854.
APA Gao GN.,Wang M.,Lin J.,Wu, N.,Tan, CM.,...&Gao, GN .(2014).Radio observations of the fine structure inside a post-CME current sheet.RESEARCH IN ASTRONOMY AND ASTROPHYSICS,14(7),843-854.
MLA Gao GN,et al."Radio observations of the fine structure inside a post-CME current sheet".RESEARCH IN ASTRONOMY AND ASTROPHYSICS 14.7(2014):843-854.
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