中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
INITIATION PROCESSES FOR THE 2013 MAY 13 X1.7 LIMB FLARE

文献类型:期刊论文

作者Shen, Jinhua1,2; Wang, Ya3,4; Zhou, Tuanhui3,5; Ji, Haisheng3,5
刊名ASTROPHYSICAL JOURNAL
出版日期2017-01-20
卷号835期号:1
ISSN号0004-637X
关键词Sun: activity Sun: flares sunspots
英文摘要For the X1.7 class flare on 2013 May 13 (SOL2013-05-13T01: 53), its initiation process was well observed by the Atmospheric Imaging Assembly (AIA) on board the Solar Dynamic Observatory. and the Extreme UltraViolet Imager (EUVI) on board STEREO-B. The initiation process incorporates the following phenomena: an X-ray precursor that started similar to 9 minutes before flare onset, two hot magnetic loops (as seen with AIA hot channels) forming a sigmoidal core magnetic structure (as seen with the EUVI), a rapidly formed magnetic flux rope (MFR) that expands outward, and a flare loop that contracts inward. The two hot magnetic loops were activated after the occurrence of the X-ray precursor. After activation, magnetic reconnection occurred between the two hot magnetic loops (inside the sigmoid structure), which produced the expanding MFR and the contracting flare loop (CFL). The MFR and CFL can only be seen with AIA hot and cool channels, respectively. For this flare, the real initiation time can be regarded as being from the starting time of the precursor, and its impulsive phase started when the MFR began its fast expansion. In addition, the CFL and the growing postflare magnetic loops are different loop systems, and the CFL was the product of magnetic reconnection between sheared magnetic fields that also produced the MFR.
WOS标题词Science & Technology ; Physical Sciences
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]CORONAL MASS EJECTIONS ; MAGNETIC-FLUX ROPE ; SOLAR-FLARES ; X-RAY ; FILAMENT ERUPTION ; CONVERGING MOTION ; PHASE ; LOOPS ; RECONNECTION ; PROMINENCES
收录类别SCI
语种英语
WOS记录号WOS:000393455400043
源URL[http://ir.xao.ac.cn/handle/45760611-7/1424]  
专题新疆天文台_光学天文与技术应用研究室
作者单位1.Chinese Acad Sci, Xinjiang Astron Observ, Urumqi 830011, Peoples R China
2.Chinese Acad Sci, NAO, Key Lab Solar Act, Beijing 100012, Peoples R China
3.Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Jiangsu, Peoples R China
4.Univ Chinese Acad Sci, Beijing 100049, Peoples R China
5.Chinese Acad Sci, Key Lab DMSA, Nanjing 210008, Jiangsu, Peoples R China
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Shen, Jinhua,Wang, Ya,Zhou, Tuanhui,et al. INITIATION PROCESSES FOR THE 2013 MAY 13 X1.7 LIMB FLARE[J]. ASTROPHYSICAL JOURNAL,2017,835(1).
APA Shen, Jinhua,Wang, Ya,Zhou, Tuanhui,&Ji, Haisheng.(2017).INITIATION PROCESSES FOR THE 2013 MAY 13 X1.7 LIMB FLARE.ASTROPHYSICAL JOURNAL,835(1).
MLA Shen, Jinhua,et al."INITIATION PROCESSES FOR THE 2013 MAY 13 X1.7 LIMB FLARE".ASTROPHYSICAL JOURNAL 835.1(2017).

入库方式: OAI收割

来源:新疆天文台

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