中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Magnetic field evolution leading to solar flares I. Cases with low magnetic shear and flux emergence

文献类型:期刊论文

作者Li, H; Sakurai, T; Ichimoto, K; UeNo, S
刊名PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
出版日期2000
卷号52期号:3页码:465-481
关键词Sun : flares Sun : magnetic fields Sun : X-rays
ISSN号0004-6264
英文摘要We picked up five solar flares larger than GOES X-ray class M/H alpha importance 1, and studied the magnetic evolution of the corresponding active regions. In particular, we investigated the spatial relationships among H alpha flare ribbons, soft X-ray (SXR) hare loops, and magnetic configurations. Our results show that all of these flares are not associated with high magnetic shear, but with emerging flux, indicating that flux emergence is a common phenomenon in this kind of solar flare with low magnetic shear. The maximum values of the transverse magnetic fields on the neutral lines responsible for these hares are 300-800 G. All of these flares but one have multiple (more than two) H alpha ribbons, and almost all of these ribbons are located at the footpoints of SXR flare loops. The flare-related shear changes, which can be both positive and negative, may be determined by the balance of the energy carried by the emerging flux and that required to power the flare.
WOS标题词Science & Technology ; Physical Sciences
学科主题Astronomy & Astrophysics
类目[WOS]Astronomy & Astrophysics
研究领域[WOS]Astronomy & Astrophysics
关键词[WOS]X-RAY TELESCOPE ; A MISSION ; MULTIWAVELENGTH OBSERVATIONS ; ACTIVE REGIONS ; RECONNECTION ; CONFIGURATION ; CURRENTS ; TOPOLOGY ; SYSTEM ; SITES
收录类别SCI
语种英语
WOS记录号WOS:000088014000008
公开日期2013-02-01
源URL[http://libir.pmo.ac.cn/handle/332002/8261]  
专题紫金山天文台_太阳高能及相关物理过程研究团组
作者单位1.Chinese Acad Sci, Natl Astron Observ, Purple Mt Observ, Nanjing 210008, Peoples R China
2.Natl Astron Observ, Mitaka, Tokyo 1818588, Japan
3.Kyoto Univ, Hida Observ, Gifu 5061317, Japan
推荐引用方式
GB/T 7714
Li, H,Sakurai, T,Ichimoto, K,et al. Magnetic field evolution leading to solar flares I. Cases with low magnetic shear and flux emergence[J]. PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,2000,52(3):465-481.
APA Li, H,Sakurai, T,Ichimoto, K,&UeNo, S.(2000).Magnetic field evolution leading to solar flares I. Cases with low magnetic shear and flux emergence.PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN,52(3),465-481.
MLA Li, H,et al."Magnetic field evolution leading to solar flares I. Cases with low magnetic shear and flux emergence".PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN 52.3(2000):465-481.

入库方式: OAI收割

来源:紫金山天文台

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