Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament
文献类型:期刊论文
作者 | Chen, Hechao1,2,3; Tian, Hui2; Zhang, Quanhao4; Li, Chuan5,6; Xia, Chun1,3; Bai, Xianyong7; Hou, Zhenyong2; Ji KF(季凯帆)8![]() |
刊名 | ASTROPHYSICAL JOURNAL
![]() |
出版日期 | 2025-04-20 |
卷号 | 983期号:2 |
ISSN号 | 0004-637X |
DOI | 10.3847/1538-4357/adc12a |
产权排序 | 第8完成单位 |
文献子类 | Article |
英文摘要 | Filament eruptions are magnetically driven violent explosions commonly observed on the Sun and late-type stars, sometimes leading to monster coronal mass ejections that directly affect the nearby planets' environments. More than a century of research on solar filaments suggests that the slow evolution of photospheric magnetic fields plays a decisive role in initiating filament eruptions, but the underlying mechanism remains unclear. Using high-resolution observations from the Chinese H alpha Solar Explorer, the Solar Upper Transition Region Imager, and the Solar Dynamics Observatory, we present direct evidence that a giant solar filament eruption is triggered by a series of minifilament eruptions occurring beneath it. These minifilaments, which are homologous to the giant filament but on a smaller tempo-spatial scale, sequently form and erupt due to extremely weak mutual flux disappearance of opposite-polarity photospheric magnetic fields. Through multifold magnetic interactions, these erupting minifilaments act as the last straw to break the force balance of the overlying giant filament and initiate its ultimate eruption. The results unveil a possible novel pathway for small-scale magnetic activities near the stellar surface to initiate spectacular filament eruptions, and provide new insight into the magnetic coupling of filament eruptions across different tempo-spatial scales. |
学科主题 | 天文学 ; 太阳与太阳系 |
URL标识 | 查看原文 |
出版地 | TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND |
WOS关键词 | CORONAL MASS EJECTION ; MAGNETIC-FLUX CANCELLATION ; TRANSVERSE OSCILLATIONS ; JET DRIVEN ; RECONNECTION ; PROMINENCE ; MODEL ; ROPES ; INITIATION ; FLARES |
资助项目 | NSFC[12425301]; NSFC[12103005]; NSFC[12333009]; NSFC[12073022]; NSFC[12373115]; NSFC[42188101]; NSFC[42174213]; National Key R&D Program of China[2021YFA0718600]; Yunnan Key Laboratory of Solar Physics and Space Science[YNSPCC202210]; Yunnan Key Laboratory of Solar Physics and Space Science[202205AG070009]; Yunnan Provincial Basic Research Project[202401CF070165]; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000]; China National Space Administration; Precision Mechanics of CAS; Innovation Academy for Microsatellites of CAS |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
WOS记录号 | WOS:001468695200001 |
出版者 | IOP Publishing Ltd |
资助机构 | NSFC[12425301, 12103005, 12333009, 12073022, 12373115, 42188101, 42174213] ; National Key R&D Program of China[2021YFA0718600] ; Yunnan Key Laboratory of Solar Physics and Space Science[YNSPCC202210, 202205AG070009] ; Yunnan Provincial Basic Research Project[202401CF070165] ; Strategic Priority Research Program of the Chinese Academy of Sciences[XDB0560000] ; China National Space Administration ; Precision Mechanics of CAS ; Innovation Academy for Microsatellites of CAS |
版本 | 出版稿 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/28261] ![]() |
专题 | 天文技术实验室 |
作者单位 | 1.School of Physics and Astronomy, Yunnan University, Kunming, 650500, People's Republic of China; 2.School of Earth and Space Sciences, Peking University, Beijing, 100871, People's Republic of China; 3.Yunnan Key Laboratory of the Solar Physics and Space Science, Kunming, 650216, People's Republic of China; 4.CAS Key Laboratory of Geospace Environment, Department of Geophysics and Planetary Sciences, University of Science and Technology of China, Hefei, 230026, People's Republic of China; 5.School of Astronomy and Space Science, Nanjing University, Nanjing 210023, People's Republic of China; 6.Institute of Science and Technology for Deep Space Exploration, Suzhou Campus, Nanjing University, Suzhou 215163, People's Republic of China; 7.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, People's Republic of China; 8.Yunnan Observatories, Chinese Academy of Sciences, 396 Yangfangwang, Guandu District, Kunming, 650216, People's Republic of China |
推荐引用方式 GB/T 7714 | Chen, Hechao,Tian, Hui,Zhang, Quanhao,et al. Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament[J]. ASTROPHYSICAL JOURNAL,2025,983(2). |
APA | Chen, Hechao.,Tian, Hui.,Zhang, Quanhao.,Li, Chuan.,Xia, Chun.,...&Hu, Ziyao.(2025).Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament.ASTROPHYSICAL JOURNAL,983(2). |
MLA | Chen, Hechao,et al."Minifilament Eruptions as the Last Straw to Break the Equilibrium of a Giant Solar Filament".ASTROPHYSICAL JOURNAL 983.2(2025). |
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。