Onset mechanism of an inverted U-shaped solar filament eruption revealed by NVST, SDO, and STEREO-A observations
文献类型：期刊论文
| 作者 | Wang JC(王金成)5,6 ; Yan XL(闫晓理)5,6; Cai, Qiangwei4; Xue ZK(薛志科)5,6; Yang LH(杨丽恒)5,6; Li, Qiaoling3; Xu Z(徐喆)5,6; Cai YF(蔡云芳)5,6; Yang LP(杨丽平)2,6; Peng Y(彭洋)2,6
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| 刊名 | Astronomy and Astrophysics
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| 出版日期 | 2024-04-01 |
| 卷号 | 684 |
| 关键词 | Sun: activity Sun: filaments prominences |
| ISSN号 | 0004-6361 |
| DOI | 10.1051/0004-6361/202347962 |
| 产权排序 | 第1完成单位 |
| 文献子类 | Journal article (JA) |
| 英文摘要 | Context. Solar filaments, also called solar prominences when appearing on the solar limb, consist of dense, cool plasma suspended in the hot and tenuous corona. They are the main potential sources of solar storms. Aims. To understand the onset mechanism of solar filaments, we investigated the eruption process of an inverted U-shaped solar filament and two precursory jet-like activities. Methods. Using observations from the New Vacuum Solar Telescope (NVST), the Solar Dynamics Observatory (SDO), and the Solar Terrestrial Relations Observatory-Ahead (STEREO-A), we investigated the event from two distinct observational perspectives: on the solar disk using NVST and SDO, and on the solar limb using STEREO-A. We employed both a nonlinear force-free field model and a potential field model to reconstruct the coronal magnetic field with the aim to understand its magnetic properties. Results. Two precursor jet-like activities were observed before the eruption, displaying an untwisted rotation. The second activity released an estimated twist of over two turns. During these two jet-like activities, Y-shaped brightenings, which are newly emerging magnetic flux accompanied by magnetic cancellation, and the formation of newly moving fibrils were identified. When these observational features are combined, it can be inferred that these two precursor jet-like activities released the magnetic field that constrained the filament and were caused by newly emerging magnetic flux. Before the filament eruption, it was observed that some moving flows had been ejected from the site as the onset of two jet-like activities, indicating the same physical process as in the two jet-like activities. Extrapolations revealed that the filament was below the height of the decay index of 1.0 and had a strong magnetic field (540 Gauss) and a high twist number (2.4 turns) before the eruption. An apparent rotational motion was observed during the filament eruption. Conclusions. We deduce that the solar filament, exhibiting an inverted U-shape, is a significantly twisted flux rope. The eruption of the filament was initiated by the release of constraining magnetic fields through continuous magnetic reconnection. This reconnection process was caused by the emergence of new magnetic flux. © 2024 EDP Sciences. All rights reserved. |
| 学科主题 | 天文学 ; 太阳与太阳系 |
| URL标识 | 查看原文 |
| 资助项目 | N/A |
| 语种 | 英语 |
| 资助机构 | N/A |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/27046]  |
| 专题 | 云南天文台_抚仙湖太阳观测站 |
| 通讯作者 | Wang JC(王金成) |
| 作者单位 | 1.School of Physics and Electronic Information Technology, Yunnan Normal University, Kunming, 650500, China 2.University of Chinese Academy of Sciences, Yuquan Road, Shijingshan Block, Beijing, 100049, China; 3.Department of Physics, Yunnan University, Kunming, 650091, China; 4.Institute of Space Physics, Luoyang Normal University, Luoyang, 471934, China; 5.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming, 650011, China; 6.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, 650216, China; |
| 推荐引用方式 GB/T 7714 | Wang JC,Yan XL,Cai, Qiangwei,et al. Onset mechanism of an inverted U-shaped solar filament eruption revealed by NVST, SDO, and STEREO-A observations[J]. Astronomy and Astrophysics,2024,684. |
| APA | 王金成.,闫晓理.,Cai, Qiangwei.,薛志科.,杨丽恒.,...&Zhou YA.(2024).Onset mechanism of an inverted U-shaped solar filament eruption revealed by NVST, SDO, and STEREO-A observations.Astronomy and Astrophysics,684. |
| MLA | 王金成,et al."Onset mechanism of an inverted U-shaped solar filament eruption revealed by NVST, SDO, and STEREO-A observations".Astronomy and Astrophysics 684(2024). |
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来源：云南天文台
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