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Observation of a Large-Scale Filament Eruption Initiated by Two Small-Scale Erupting Filaments Pushing Out from Below
Song, Yongliang1,2; Su, Jiangtao1,2,3; Zhang, Qingmin4; Zhang, Mei1,2,3; Deng, Yuanyong1,2,3; Bai, Xianyong1,2,3; Liu, Suo1,2; Yang, Xiao1,2; Chen, Jie1,2; Xu, Haiqing1,2; Ji KF(季凯帆)5; Hu, Ziyao1,2,3
发表期刊SOLAR PHYSICS
2024-06
卷号299期号:6
DOI10.1007/s11207-024-02327-6
产权排序第5完成单位
收录类别SCI
关键词Active region Flare Filament eruption CME
摘要Filament eruptions often result in flares and coronal mass ejections (CMEs). Most studies attribute the filament eruptions to their instabilities or magnetic reconnection. In this study, we report a unique observation of a filament eruption whose initiation process has not been reported before. This large-scale filament, with a length of about 360 Mm crossing an active region, is forced to erupt by two small-scale erupting filaments pushing out from below. This process of multifilament eruption results in an M6.4 flare in the active region NOAA 13229 on 25 February 2023. The whole process can be divided into three stages: the eruptions of two active-region filaments, F1 and F2; the interactions between the erupting F1, F2, and the large-scale filament F3; and the eruption of F3. Though this multifilament eruption occurs near the northwest limb of the solar disk, it produces a strong halo CME that causes a significant geomagnetic disturbance. Our observations present a new filament eruption mechanism in which the initial kinetic energy of the eruption is obtained from and transported to by other erupting structures. This event provides us a unique insight into the dynamics of multifilament eruptions and their corresponding effects on the interplanetary space.
资助项目Strategic Priority Research Program on Space Science of CAS[XDA15320000]; China National Space Administration (CNSA); Star Program of NASA; Precision Mechanics of CAS; Innovation Academy for Microsatellites of CAS
项目资助者Strategic Priority Research Program on Space Science of CAS[XDA15320000] ; China National Space Administration (CNSA) ; Star Program of NASA ; Precision Mechanics of CAS ; Innovation Academy for Microsatellites of CAS
语种英语
学科领域天文学 ; 太阳与太阳系
文章类型Article
出版者SPRINGER
出版地VAN GODEWIJCKSTRAAT 30, 3311 GZ DORDRECHT, NETHERLANDS
ISSN0038-0938
URL查看原文
WOS记录号WOS:001250431900001
WOS研究方向Astronomy & Astrophysics
WOS类目Astronomy & Astrophysics
关键词[WOS]FLUX ROPE ; SOLAR ; RECONNECTION ; MISSION
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文献类型期刊论文
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条目标识符http://ir.ynao.ac.cn/handle/114a53/27409
专题天文技术实验室
作者单位1.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
2.Key Laboratory of Solar Activity and Space Weather, National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China;
3.School of Astronomy and Space Sciences, University of Chinese Academy of Sciences, Beijing, 100049, China;
4.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Nanjing, 210023, China;
5.Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, 650216, China
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Song, Yongliang,Su, Jiangtao,Zhang, Qingmin,et al. Observation of a Large-Scale Filament Eruption Initiated by Two Small-Scale Erupting Filaments Pushing Out from Below[J]. SOLAR PHYSICS,2024,299(6).
APA Song, Yongliang.,Su, Jiangtao.,Zhang, Qingmin.,Zhang, Mei.,Deng, Yuanyong.,...&Hu, Ziyao.(2024).Observation of a Large-Scale Filament Eruption Initiated by Two Small-Scale Erupting Filaments Pushing Out from Below.SOLAR PHYSICS,299(6).
MLA Song, Yongliang,et al."Observation of a Large-Scale Filament Eruption Initiated by Two Small-Scale Erupting Filaments Pushing Out from Below".SOLAR PHYSICS 299.6(2024).
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