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 | |
发表期刊 | RESEARCH IN ASTRONOMY AND ASTROPHYSICS |
2014-07 | |
卷号 | 14期号:7页码:843-854 |
DOI | 10.1088/1674-4527/14/7/006 |
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. |
资助项目 | National Basic Research Program of China (973 program)[2011CB811403] ; National Basic Research Program of China (973 program)[2013CBA01503] ; National Natural Science Foundation of China[11273055] ; National Natural Science Foundation of China[11173010] ; National Natural Science Foundation of China[11333007] ; National Natural Science Foundation of China[10978006] ; National Natural Science Foundation of China[11103044] ; National Natural Science Foundation of China[11273030] ; CAS[KJCX2-EW-T07] ; CAS[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] |
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 | 天文学 ; 射电天文学 ; 太阳与太阳系 |
文章类型 | Article |
出版者 | NATL ASTRONOMICAL OBSERVATORIES, CHIN ACAD SCIENCES |
出版地 | 20A DATUN RD, CHAOYANG, BEIJING, 100012, PEOPLES R CHINA |
ISSN | 1674-4527 |
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 | |
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(高冠男) |
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 |
第一作者单位 | 中国科学院云南天文台 |
通讯作者单位 | 中国科学院云南天文台 |
推荐引用方式 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.,...&Su, Y.(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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