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Observing the release of twist by magnetic reconnection in a solar filament eruption
文献类型：期刊论文
| 作者 | Xue ZK(薛志科)1,2 ; Yan XL(闫晓理)1; Cheng, Xin3; Yang LH(杨丽恒)1,2; Su, Yingna4; Bernhard Kliem1,5; Zhang, Jun2; Liu Z(刘忠)1; Bi Y(毕以)1; Xiang YY(向永源)1
|
| 刊名 | NATURE COMMUNICATIONS
 |
| 出版日期 | 2016-06-01 |
| 卷号 | 7 |
| ISSN号 | 2041-1723 |
| 通讯作者 | Yan, XL (reprint author), Chinese Acad Sci, Yunnan Observ, Kunming 650216, Yunnan, Peoples R China. |
| 产权排序 | 第一完成单位 |
| 英文摘要 | Magnetic reconnection is a fundamental process of topology change and energy release, taking place in plasmas on the Sun, in space, in astrophysical objects and in the laboratory. However, observational evidence has been relatively rare and typically only partial. Here we present evidence of fast reconnection in a solar filament eruption using high-resolution H-alpha images from the New Vacuum Solar Telescope, supplemented by extreme ultraviolet observations. The reconnection is seen to occur between a set of ambient chromospheric fibrils and the filament itself. This allows for the relaxation of magnetic tension in the filament by an untwisting motion, demonstrating a flux rope structure. The topology change and untwisting are also found through nonlinear force-free field modelling of the active region in combination with magnetohydrodynamic simulation. These results demonstrate a new role for reconnection in solar eruptions: the release of magnetic twist. |
| 学科主题 | Science & Technology - Other Topics |
| WOS标题词 | Science & Technology |
| 类目[WOS] | Multidisciplinary Sciences |
| 研究领域[WOS] | Science & Technology - Other Topics |
| 关键词[WOS] | X-RAY TELESCOPE ; DYNAMICS-OBSERVATORY SDO ; CORONAL MASS EJECTIONS ; 2010 APRIL 8 ; ACTIVE REGIONS ; CURRENT SHEET ; FLUX ROPE ; FLARE ; LOOP ; MODEL |
| 收录类别 | SCI ; EI |
| 原文出处 | http://www.nature.com/ncomms/2016/160616/ncomms11837/full/ncomms11837.html |
| 语种 | 英语 |
| WOS记录号 | WOS:000378812000001 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/9616]  |
| 专题 | 云南天文台_抚仙湖太阳观测站 云南天文台_太阳物理研究组 |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan 650216, China 2.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China 3.School of Astronomy and Space Science, Nanjing University, Nanjing, Jiangsu 210093, China 4.Key Laboratory for Dark Matter and Space Science, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, Jiangsu 210008, China 5.Institute of Physics and Astronomy, University of Potsdam, Potsdam 14476, Germany |
| 推荐引用方式 GB/T 7714 | Xue ZK,Yan XL,Cheng, Xin,et al. Observing the release of twist by magnetic reconnection in a solar filament eruption[J]. NATURE COMMUNICATIONS,2016,7. |
| APA | Xue ZK.,Yan XL.,Cheng, Xin.,Yang LH.,Su, Yingna.,...&Zhao L.(2016).Observing the release of twist by magnetic reconnection in a solar filament eruption.NATURE COMMUNICATIONS,7. |
| MLA | Xue ZK,et al."Observing the release of twist by magnetic reconnection in a solar filament eruption".NATURE COMMUNICATIONS 7(2016). |
入库方式： OAI收割
来源：云南天文台
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