Stereoscopic Observations of an Erupting Mini-filament-driven Two-sided-loop Jet and the Applications for Diagnosing a Filament Magnetic Field
文献类型：期刊论文
| 作者 | Shen,Yuandeng1,2; Qu,Zhining3; Yuan,Ding4; Chen,Huadong5,6 ; Duan,Yadan7; Zhou,Chengrui1,5; Tang,Zehao1,5; Huang,Jin1,5; Liu,Yu1
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| 刊名 | The Astrophysical Journal
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| 出版日期 | 2019-09-25 |
| 卷号 | 883期号:1 |
| ISSN号 | 0004-637X |
| 关键词 | Solar activity Solar flares Solar filaments Solar coronal mass ejections Solar magnetic fields |
| DOI | 10.3847/1538-4357/ab3a4d |
| 英文摘要 | Abstract Ubiquitous solar jets or jet-like activities are generally regarded as an important source of energy and mass input to the upper solar atmosphere and the solar wind. However, their triggering and driving mechanisms are not completely understood. By taking advantage of stereoscopic observations with high temporal and spatial resolutions taken by the Solar Dynamic Observatory (SDO) and the Solar Terrestrial Relations Observatory (STEREO), we report an intriguing two-sided-loop jet that occurred on 2013 June 02, and was dynamically associated with the eruption of a mini-filament below an overlying large filament. Additionally, two distinct reconnection processes are identified during the formation stage. The SDO observations reveal that the two-sided-loop jet showed a concave shape with a projection speed of about 80–136 km s?1. From the other view angle, the STEREO observations clearly showed that the trajectories of the two arms of the two-sided-loop were along the cavity magnetic field lines hosting the large filament. Contrary to the well-accepted theoretical model, the present observation sheds new light on our understanding of the formation mechanism of two-sided-loop jets. Moreover, the eruption of the two-sided-loop jet not only supplied mass to the overlying large filament, but also provided a rare opportunity to diagnose the magnetic structure of the overlying large filament via the method of three-dimensional reconstruction. |
| 语种 | 英语 |
| 出版者 | The American Astronomical Society |
| WOS记录号 | IOP:0004-637X-883-1-AB3A4D |
| 源URL | [http://ir.bao.ac.cn/handle/114a11/27886]  |
| 专题 | 中国科学院国家天文台 |
| 作者单位 | 1.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, People’s Republic of China; ydshen@ynao.ac.cn 2.Center for Astronomical Mega-Science, Chinese Academy of Sciences, Beijing, 100012, People’s Republic of China 3.School of Automation and Information Engineering, Sichuan University of Science & Engineering, Zigong 643000, People’s Republic of China 4.Institute of Space Science and Applied Technology, Harbin Institute of Technology, Shenzhen, 518055, People’s Republic of China 5.University of Chinese Academy of Sciences, Beijing, People’s Republic of China 6.Key Laboratory of Solar Activity, National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, People’s Republic of China 7.Yunnan Normal University, Department of Physics, Kunming 650500, People’s Republic of China |
| 推荐引用方式 GB/T 7714 | Shen,Yuandeng,Qu,Zhining,Yuan,Ding,et al. Stereoscopic Observations of an Erupting Mini-filament-driven Two-sided-loop Jet and the Applications for Diagnosing a Filament Magnetic Field[J]. The Astrophysical Journal,2019,883(1). |
| APA | Shen,Yuandeng.,Qu,Zhining.,Yuan,Ding.,Chen,Huadong.,Duan,Yadan.,...&Liu,Yu.(2019).Stereoscopic Observations of an Erupting Mini-filament-driven Two-sided-loop Jet and the Applications for Diagnosing a Filament Magnetic Field.The Astrophysical Journal,883(1). |
| MLA | Shen,Yuandeng,et al."Stereoscopic Observations of an Erupting Mini-filament-driven Two-sided-loop Jet and the Applications for Diagnosing a Filament Magnetic Field".The Astrophysical Journal 883.1(2019). |
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来源：国家天文台
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