THE FORMATION OF AN INVERSE S-SHAPED ACTIVE-REGION FILAMENT DRIVEN BY SUNSPOT MOTION AND MAGNETIC RECONNECTION
文献类型：期刊论文
| 作者 | Yan XL(闫晓理)1 ; Priest, E. R.2; Guo, Q. L.3; Xue ZK(薛志科)1,4; Wang JC(王金成)1; Yang LH(杨丽恒)1,4
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| 刊名 | ASTROPHYSICAL JOURNAL
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| 出版日期 | 2016-11-20 |
| 卷号 | 832期号:1 |
| 关键词 | Sun: activity Sun: filaments, prominences Sun: magnetic fields Sun: photosphere sunspots Supporting material: animations |
| ISSN号 | 0004-637X |
| 产权排序 | 第一完成单位 |
| 通讯作者 | Yan, XL (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650011, Peoples R China. |
| 英文摘要 | We present a detailed study of the formation of an inverse S-shaped filament prior to its eruption in active region NOAA 11884 from 2013 October 31 to November 2. In the initial stage, clockwise rotation of a small positive sunspot around the main negative trailing sunspot formed a curved filament. Then the small sunspot cancelled with the negative magnetic flux to create a longer active-region filament with an inverse S-shape. At the cancellation site a brightening was observed in UV and EUV images and bright material was transferred to the filament. Later the filament erupted after cancellation of two opposite polarities below the upper part of the filament. Nonlinear force-free field extrapolation of vector photospheric fields suggests that the filament may have a twisted structure, but this cannot be confirmed from the current observations. |
| 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] | VACUUM SOLAR TELESCOPE ; CORONAL MASS EJECTIONS ; HELICAL FLUX ROPE ; PROMINENCE FORMATION ; HIGH-RESOLUTION ; FORCE-FREE ; SPECKLE MASKING ; QUIET SUN ; DYNAMICS ; FIELD |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/article/10.3847/0004-637X/832/1/23/meta |
| 语种 | 英语 |
| WOS记录号 | WOS:000388603600005 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/9785]  |
| 专题 | 云南天文台_抚仙湖太阳观测站 |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650011, China 2.Mathematics Institute, University of St Andrews, St Andrews, KY16 9SS, UK 3.College of Mathematics Physics and Information Engineering, Jiaxing University, Jiaxing 314001, China 4.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China |
| 推荐引用方式 GB/T 7714 | Yan XL,Priest, E. R.,Guo, Q. L.,et al. THE FORMATION OF AN INVERSE S-SHAPED ACTIVE-REGION FILAMENT DRIVEN BY SUNSPOT MOTION AND MAGNETIC RECONNECTION[J]. ASTROPHYSICAL JOURNAL,2016,832(1). |
| APA | Yan XL,Priest, E. R.,Guo, Q. L.,Xue ZK,Wang JC,&Yang LH.(2016).THE FORMATION OF AN INVERSE S-SHAPED ACTIVE-REGION FILAMENT DRIVEN BY SUNSPOT MOTION AND MAGNETIC RECONNECTION.ASTROPHYSICAL JOURNAL,832(1). |
| MLA | Yan XL,et al."THE FORMATION OF AN INVERSE S-SHAPED ACTIVE-REGION FILAMENT DRIVEN BY SUNSPOT MOTION AND MAGNETIC RECONNECTION".ASTROPHYSICAL JOURNAL 832.1(2016). |
入库方式： OAI收割
来源：云南天文台
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