Rotating Magnetic Structures Associated with a Quasi-circular Ribbon Flare | |
Li HD(李海东)1,2; Jiang YC(姜云春)1; Yang JY(杨家艳)1; Yang B(杨波)1,2; Xu Z(徐喆)1,2; Hong JC(洪俊超)1; Bi Y(毕以)1,2 | |
发表期刊 | ASTROPHYSICAL JOURNAL |
2017-02-20 | |
卷号 | 836期号:2 |
DOI | 10.3847/1538-4357/aa5eac |
产权排序 | 第1完成单位 |
收录类别 | SCI |
关键词 | Sun: Activity Sun: Corona Sun: Filaments Sun: Flares Sun: Magnetic Fields Supporting Material: Animations |
摘要 | We present the detection of a small eruption and the associated quasi-circular ribbon flare during the emergence of a bipole occurring on 2015 February 3. Under a fan dome, a sigmoid was rooted in a single magnetic bipole, which was encircled by negative polarity. The nonlinear force-free field extrapolation shows the presence of twisted field lines, which can represent a sigmoid structure. The rotation of the magnetic bipole may cause the twisting of magnetic field lines. An initial brightening appeared at one of the footpoints of the sigmoid, where the positive polarity slides toward a nearby negative polarity field region. The sigmoid displayed an ascending motion and then interacted intensively with the spine-like field. This type of null point reconnection in corona led to a violent blowout jet, and a quasi-circular flare ribbon was also produced. The magnetic emergence and rotational motion are the main contributors to the energy buildup for the flare, while the cancellation and collision might act as a trigger. |
资助项目 | Natural Science Foundation of China[11333007] ; Natural Science Foundation of China[11403098] ; Natural Science Foundation of China[11473065] ; Natural Science Foundation of China[11573012] ; Natural Science Foundation of China[11503081] ; Natural Science Foundation of China[11503082] ; Natural Science Foundation of China[11633008] ; CAS |
项目资助者 | Natural Science Foundation of China[11333007, 11403098, 11473065, 11573012, 11503081, 11503082, 11633008] ; CAS |
语种 | 英语 |
学科领域 | 天文学 ; 太阳与太阳系 ; 太阳物理学 |
文章类型 | Article |
出版者 | IOP PUBLISHING LTD |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
ISSN | 0004-637X |
URL | 查看原文 |
WOS记录号 | WOS:000401169200003 |
WOS研究方向 | Astronomy & Astrophysics |
WOS类目 | Astronomy & Astrophysics |
关键词[WOS] | SOLAR ACTIVE-REGION ; SLIP-RUNNING RECONNECTION ; RAPID SUNSPOT ROTATION ; SEPARATRIX LAYERS ; X-RAY ; MULTIWAVELENGTH OBSERVATIONS ; RESOLUTION OBSERVATIONS ; CORONAL JETS ; FLUX ROPES ; FIELD |
引用统计 | |
文献类型 | 期刊论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/10063 |
专题 | 太阳物理研究组 |
通讯作者 | Li HD(李海东) |
作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, China 2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, 100012, China |
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 | Li HD,Jiang YC,Yang JY,et al. Rotating Magnetic Structures Associated with a Quasi-circular Ribbon Flare[J]. ASTROPHYSICAL JOURNAL,2017,836(2). |
APA | Li HD.,Jiang YC.,Yang JY.,Yang B.,Xu Z.,...&Bi Y.(2017).Rotating Magnetic Structures Associated with a Quasi-circular Ribbon Flare.ASTROPHYSICAL JOURNAL,836(2). |
MLA | Li HD,et al."Rotating Magnetic Structures Associated with a Quasi-circular Ribbon Flare".ASTROPHYSICAL JOURNAL 836.2(2017). |
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Rotating Magnetic St(3244KB) | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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