ERUPTION OF A SOLAR FILAMENT CONSISTING OF TWO THREADS
文献类型：期刊论文
| 作者 | Bi Y(毕以) ; Jiang YC(姜云春); Li HD(李海东); Hong JC(洪俊超); Zheng RS(郑瑞生)
|
| 刊名 | ASTROPHYSICAL JOURNAL
 |
| 出版日期 | 2012-10-10 |
| 卷号 | 758期号:1页码:42-47 |
| ISSN号 | 0004-637X |
| 关键词 | Sun: filaments Sun: magnetic topology prominences |
| 通讯作者 | Bi, Y (reprint author), Chinese Acad Sci, Natl Astron Observ, Yunnan Astron Observ, Kunming 650011, Peoples R China. |
| 产权排序 | 第一完成单位 |
| 英文摘要 | The trigger and driving mechanism for the eruption of a filament consisting of two dark threads was studied with unprecedented high cadence and resolution of He II 304 angstrom observations made by the Atmospheric Imagining Assembly (AIA) on board the Solar Dynamics Observatory (SDO) and the observations made by the Solar Magnetic Activity Research Telescope and the Extreme Ultraviolet Imager (EUVI) telescope on board the Solar Terrestrial Relations Observatory Ahead (STEREO-A). The filament was located at the periphery of the active region NOAA 11228 and erupted on 2011 June 6. At the onset of the eruption, a turbulent filament thread was found to be heated and to elongate in stride over a second one. After it rose slowly, most interestingly, the elongating thread was driven to contact and interact with the second one, and it then erupted with its southern leg being wrapped by a newly formed thread produced by the magnetic reconnection between fields carried by the two threads. Combining the observations from STEREO-A/EUVI and SDO/AIA 304 angstrom images, the three-dimensional shape of the axis of the filament was obtained and it was found that only the southern leg of the eruptive filament underwent rotation. We suggest that the eruption was triggered by the reconnection of the turbulent filament thread and the surrounding magnetic field, and that it was mainly driven by the kink instability of the southern leg of the eruptive filament that possessed a more twisted field introduced by the reconnection-produced thread. |
| 学科主题 | Astronomy & Astrophysics |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 类目[WOS] | Astronomy & Astrophysics |
| 研究领域[WOS] | Astronomy & Astrophysics |
| 关键词[WOS] | CORONAL MASS EJECTIONS ; MAGNETIC-FLUX ; ROPES ; RECONNECTION ; PROMINENCES ; CATASTROPHE ; HELICITY ; SIGMOIDS ; KINKING ; FIELD |
| 收录类别 | SCI |
| 原文出处 | http://iopscience.iop.org/article/10.1088/0004-637X/758/1/42/meta |
| 语种 | 英语 |
| WOS记录号 | WOS:000309520500042 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6190]  |
| 专题 | 云南天文台_太阳物理研究组 |
| 作者单位 | National Astronomical Observatories/Yunnan Astronomical Observatory, Chinese Academy of Sciences, Kunming 650011, China |
| 推荐引用方式 GB/T 7714 | Bi Y,Jiang YC,Li HD,et al. ERUPTION OF A SOLAR FILAMENT CONSISTING OF TWO THREADS[J]. ASTROPHYSICAL JOURNAL,2012,758(1):42-47. |
| APA | Bi Y,Jiang YC,Li HD,Hong JC,&Zheng RS.(2012).ERUPTION OF A SOLAR FILAMENT CONSISTING OF TWO THREADS.ASTROPHYSICAL JOURNAL,758(1),42-47. |
| MLA | Bi Y,et al."ERUPTION OF A SOLAR FILAMENT CONSISTING OF TWO THREADS".ASTROPHYSICAL JOURNAL 758.1(2012):42-47. |
入库方式： OAI收割
来源：云南天文台
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。