KMS of Xinjiang Astronomical Observatory, CAS
| High-resolution Observation and Magnetic Modeling of a Solar Minifilament: The Formation, Eruption, and Failing Mechanisms | |
Teng, Weilin1,2; Su, Yingna1,2; Liu, Rui3,4,5; Chen, Jialin6; Liu, Yanjie1,2; Dai, Jun1,7; Cao, Wenda8; Shen, Jinhua9 ; Ji, Haisheng1,2
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| 2024-08-01 | |
| Source Publication | ASTROPHYSICAL JOURNAL
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| ISSN | 0004-637X |
| Volume | 970Issue:2Pages:100 |
| Contribution Rank | 9 |
| Abstract | Minifilaments are widespread small-scale structures in the solar atmosphere. To better understand their formation and eruption mechanisms, we investigate the entire life of a sigmoidal minifilament located below a large quiescent filament observed by Big Bear Solar Observatory/Goode Solar Telescope on 2015 August 3. The H alpha structure initially appears as a group of arched threads, then transforms into two J-shaped arcades, and finally forms a sigmoidal shape. Solar Dynamics Observatory (SDO)/Atmospheric Imaging Assembly observations in 171 & Aring; show that two coronal jets occur around the southern footpoint of the minifilament before the minifilament eruption. The minifilament eruption starts from the southern footpoint, then interacts with the overlying filament and fails. The aforementioned observational changes correspond to three episodes of flux cancellations observed by SDO/Helioseismic and Magnetic Imager. Unlike previous studies, the flux cancellation occurs between the polarity where the southern footpoint of the minifilament is rooted and an external polarity. We construct two magnetic field models before the eruption using the flux rope insertion method and find a hyperbolic flux tube above the flux cancellation site. The observation and modeling results suggest that the eruption is triggered by the external magnetic reconnection between the core field of the minifilament and the external fields due to flux cancellations. This study reveals a new triggering mechanism for minifilament eruptions and a new relationship between minifilament eruptions and coronal jets. |
| DOI | 10.3847/1538-4357/ad50d0 |
| Indexed By | SCI |
| Language | 英语 |
| WOS Keyword | X-RAY JETS ; ACTIVE-REGION ; CORONAL JETS ; FLUX-ROPE ; FILAMENT ERUPTIONS ; MINI-FILAMENT ; FIELDS ; RECONNECTION ; DYNAMICS ; FLARE |
| Funding Project | National Key R&D Program of China[2021YFA1600502] ; National Key R&D Program of China[2021YFA1600500] ; National Key R&D Program of China[2022YFF0503001] ; National Key R&D Program of China[2022YFF0503000] ; NSFC[12173092] ; NSFC[11925302] ; NSFC[12273101] ; NSFC[11790302] ; NSFC[11790300] ; Strategic Priority Research Program on Space Science, CAS[XDA15052200] ; Strategic Priority Research Program on Space Science, CAS[XDA15320301] ; Natural Science Foundation of Xinjiang Uygur Autonomous Region for Outstanding Youth ; High-level Flexible Talent Program of Xinjiang Uygur Autonomous Region ; US NSF[AGS-2309939] ; US NSF[AGS-1821294] ; US NSF[AST-2108235] ; US NSF[1821294] ; Korea Astronomy and Space Science Institute ; Seoul National University |
| WOS Research Area | Astronomy & Astrophysics |
| WOS Subject | Astronomy & Astrophysics |
| WOS ID | WOS:001273725400001 |
| Publisher | IOP Publishing Ltd |
| Funding Organization | National Key R&D Program of China ; NSFC ; Strategic Priority Research Program on Space Science, CAS ; Natural Science Foundation of Xinjiang Uygur Autonomous Region for Outstanding Youth ; High-level Flexible Talent Program of Xinjiang Uygur Autonomous Region ; US NSF ; Korea Astronomy and Space Science Institute ; Seoul National University |
| Citation statistics | |
| Document Type | 期刊论文 |
| Identifier | http://ir.xao.ac.cn/handle/45760611-7/6881 |
| Collection | 太阳物理研究团组 |
| Corresponding Author | Su, Yingna |
| Affiliation | 1.Univ Chinese Acad Sci, Purple Mt Observ, Key Lab Dark Matter & Space Astron, Nanjing 210023, Peoples R China 2.Univ Sci & Technol China, Dept Astron & Space Sci, Hefei 230026, Anhui, Peoples R China 3.Univ Sci & Technol China, Dept Geophys & Planetary Sci, CAS Key Lab Geospace Environm, Hefei 230026, Peoples R China 4.Univ Sci & Technol China, CAS Ctr Excellence Comparat Planetol, Hefei 230026, Peoples R China 5.Univ Sci & Technol China, Mengcheng Natl Geophys Observ, Mengcheng 233500, Peoples R China 6.Hanjiang Normal Univ, Sch Phys & Elect Engn, 18 South Beijing Rd, Shiyan 442000, Hubei, Peoples R China 7.Kyoto Univ, Astron Observ, Sakyo, Kyoto, Japan 8.New Jersey Inst Technol, Big Bear Solar Observ, 40386 North Shore Lane, Big Bear City, CA 92314 USA 9.Chinese Acad Sci, Xinjiang Astron Observ, 150 Sci 1 St, Urumqi 830011, Xinjiang, Peoples R China |
| Recommended Citation GB/T 7714 | Teng, Weilin,Su, Yingna,Liu, Rui,et al. High-resolution Observation and Magnetic Modeling of a Solar Minifilament: The Formation, Eruption, and Failing Mechanisms[J]. ASTROPHYSICAL JOURNAL,2024,970(2):100. |
| APA | Teng, Weilin.,Su, Yingna.,Liu, Rui.,Chen, Jialin.,Liu, Yanjie.,...&Ji, Haisheng.(2024).High-resolution Observation and Magnetic Modeling of a Solar Minifilament: The Formation, Eruption, and Failing Mechanisms.ASTROPHYSICAL JOURNAL,970(2),100. |
| MLA | Teng, Weilin,et al."High-resolution Observation and Magnetic Modeling of a Solar Minifilament: The Formation, Eruption, and Failing Mechanisms".ASTROPHYSICAL JOURNAL 970.2(2024):100. |
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| Teng-2024-High-resol（3687KB） | 期刊论文 | 出版稿 | 开放获取 | CC BY-NC-SA | View Application Full Text | |
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