Where do flare ribbons stop?
文献类型：期刊论文
| 作者 | Chen PengFei1,2; Su JiangTao2 ; Guo Yang1; Deng YuanYong2
|
| 刊名 | CHINESE SCIENCE BULLETIN
 |
| 出版日期 | 2012-04-01 |
| 卷号 | 57期号:12页码:1393-1396 |
| 关键词 | solar flares magnetic field separatrix |
| 英文摘要 | The standard flare model, which was proposed based on observations and magnetohydrodynamic theory, can successfully explain many observational features of solar flares. However, this model is just a framework, with many details awaiting to be filled in, including how reconnection is triggered. In this paper, we address an unanswered question: where do flare ribbons stop? With the data analysis of the 2003 May 29 flare event, we tentatively confirmed our conjecture that flare ribbons finally stop at the intersection of separatrices (or quasi-separatrix layer in a general case) with the solar surface. Once verified, such a conjecture can be used to predict the final size and even the lifetime of solar flares. |
| 收录类别 | SCI |
| 语种 | 英语 |
| WOS记录号 | WOS:000303218800007 |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/6191]  |
| 专题 | 国家天文台_太阳物理研究部 |
| 作者单位 | 1.Nanjing Univ, Dept Astron, Nanjing 210093, Jiangsu, Peoples R China 2.Chinese Acad Sci, Natl Astron Observ, Key Lab Solar Phys, Beijing 100012, Peoples R China |
| 推荐引用方式 GB/T 7714 | Chen PengFei,Su JiangTao,Guo Yang,et al. Where do flare ribbons stop?[J]. CHINESE SCIENCE BULLETIN,2012,57(12):1393-1396. |
| APA | Chen PengFei,Su JiangTao,Guo Yang,&Deng YuanYong.(2012).Where do flare ribbons stop?.CHINESE SCIENCE BULLETIN,57(12),1393-1396. |
| MLA | Chen PengFei,et al."Where do flare ribbons stop?".CHINESE SCIENCE BULLETIN 57.12(2012):1393-1396. |
入库方式： OAI收割
来源：国家天文台
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