中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Quasiperiodic Slipping Motion of Flare Ribbon Fine Structures Anchored in a Sunspot Light Bridge

文献类型:期刊论文

作者Chen TY(陈添源)1,3; Yan XL(闫晓理)1,2; Xue ZK(薛志科)1,2; Wang JC(王金成)1,2; Xu Z(徐喆)1,2; Yang LH(杨丽恒)1,2; Duan YD(段雅丹)1,2; Zhou YA(周羿安)1; Wu ZY(吴宗银)1,3; Dong QF(董起帆)1,3
刊名ASTROPHYSICAL JOURNAL
出版日期2026-04-01
卷号1000期号:2
ISSN号0004-637X
DOI10.3847/1538-4357/ae4d10
产权排序第1完成单位
文献子类Article
英文摘要We used high-resolution observations from the New Vacuum Solar Telescope and the Solar Dynamics Observatory to perform a detailed multiwavelength analysis of the fine structures in the flare ribbon of a C3.9-class flare on 2021 April 22. A segment of the flare ribbon was rooted in a sunspot light bridge and exhibited discrete substructures that we term burrs, with equivalent diameters of 233-895 km and intercore separations of 1129-1739 km. These structures are characterized by discrete redshifted cores, accompanied by tails (length 700-1370 km and width 310-600 km) exhibiting faint blueshifts. These structures exhibit systematic slipping motions along the ribbon, with apparent velocities decelerating from about 40-21 km s-1, and display a distinct quasiperiodicity of similar to 6 minutes in H alpha and extreme-ultraviolet passbands. Differential emission measure (DEM) analysis confirms the emitting plasma is multithermal, dominated by temperatures of 1-2 MK. The observed morphology and kinematics are consistent with the scenario of impulsive energy deposition by precipitating plasmoids (oblique flux ropes) originating from tearing-mode fragmentation in the coronal current sheet. The specific spatiotemporal correlation between the tails and blueshifts supports the hypothesis of untwisting magnetic flux ropes. Furthermore, the similar to 6 minute periodicity suggests that the reconnection process may be modulated by photospheric p-mode oscillations coupled with the tearing-mode instability. Our findings provide observational evidence that these light-bridge-anchored fine structures constitute elementary units of flare energy release.
学科主题天文学 ; 太阳与太阳系
URL标识查看原文
出版地No.2 The Distillery, Glassfields, Avon Street, Bristol, ENGLAND
WOS关键词3-DIMENSIONAL MAGNETIC RECONNECTION ; DIFFERENTIAL EMISSION MEASURE ; RUNNING RECONNECTION ; SEPARATRIX LAYERS ; SOLAR-TELESCOPE ; DYNAMICS ; EVOLUTION ; MODEL ; PROMINENCES ; PULSATIONS
资助项目MOST divided by National Key Research and Development Program of China (NKPs)[No.2024YFA1612001]
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001720963300001
出版者IOP Publishing Ltd
资助机构MOST divided by National Key Research and Development Program of China (NKPs)[No.2024YFA1612001]
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/29066]  
专题云南天文台_抚仙湖太阳观测站
通讯作者Yan XL(闫晓理)
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, People’s Republic of China; yanxl@ynao.ac.cn;
2.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming 650216, People’s Republic of China
3.University of Chinese Academy of Sciences, Beijing 100049, People’s Republic of China;
推荐引用方式
GB/T 7714
Chen TY,Yan XL,Xue ZK,et al. Quasiperiodic Slipping Motion of Flare Ribbon Fine Structures Anchored in a Sunspot Light Bridge[J]. ASTROPHYSICAL JOURNAL,2026,1000(2).
APA 陈添源.,闫晓理.,薛志科.,王金成.,徐喆.,...&张鑫生.(2026).Quasiperiodic Slipping Motion of Flare Ribbon Fine Structures Anchored in a Sunspot Light Bridge.ASTROPHYSICAL JOURNAL,1000(2).
MLA 陈添源,et al."Quasiperiodic Slipping Motion of Flare Ribbon Fine Structures Anchored in a Sunspot Light Bridge".ASTROPHYSICAL JOURNAL 1000.2(2026).

入库方式: OAI收割

来源:云南天文台

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