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Two successive EUV waves and a transverse oscillation of a quiescent prominence

文献类型：期刊论文

作者Zhang, Q M6,7; Lin, M S5,7; Yan XL(闫晓理)4,6; Dai, J3,7; Hou, Z Y2; Li, Y7; Qiu, Y1
刊名MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
出版日期2024-09-03
卷号533期号:3页码:3255-3262
关键词Sun: coronal mass ejections (CMEs) Sun: filaments, prominences Sun: flares Sun: oscillations
ISSN号0035-8711
DOI10.1093/mnras/stae1936
产权排序第4完成单位
文献子类Article
英文摘要In this paper, we carry out multiwavelength observations of two successive extreme-ultraviolet (EUV) waves originating from active region (AR) NOAA 13575 and a transverse oscillation of a columnar quiescent prominence on 2024 February 9. A hot channel eruption generates an X3.4 class flare and the associated full-halo coronal mass ejection (CME), which drives the first EUV wave front (WF1) at a speed of similar to 835 km s(-1). WF1 propagates in the south-east direction and interacts with the prominence, causing an eastward displacement of the prominence immediately. Then, a second EUV wave front (WF2) is driven by a coronal jet at a speed of similar to 831 km s(-1). WF2 follows WF1 and decelerates from similar to 788 to similar to 603 km s(-1) before arriving at and touching the prominence. After reaching the maximum displacement, the prominence turns back and swings for 1-3 cycles. The transverse oscillation of horizontal polarization is most evident in 304 & Aring;. The initial displacement amplitude, velocity in the plane of the sky, period, and damping time fall in the ranges of 12-34 Mm, 65-143 km s(-1), 18-27 min, and 33-108 min, respectively. There are strong correlations among the initial amplitude, velocity, period, and height of the prominence. Surprisingly, the oscillation is also detected in 1600 & Aring;, which is totally in phase with that in 304 & Aring;.
学科主题天文学 ; 太阳与太阳系
URL标识查看原文
出版地GREAT CLARENDON ST, OXFORD OX2 6DP, ENGLAND
WOS关键词CORONAL LOOP OSCILLATIONS ; H-ALPHA OBSERVATIONS ; MAGNETIC-FLUX-ROPE ; II RADIO-BURST ; MORETON WAVE ; VERTICAL OSCILLATION ; SOLAR PROMINENCES ; EIT WAVE ; FILAMENT OSCILLATIONS ; MASS EJECTION
资助项目NSFC; China National Space Administration (CNSA); Precision Mechanics of CAS; Innovation Academy for Microsatellites of CAS; Strategic Priority Research Program on Space Science, Chinese Academy of Sciences[XDB0560000]; Strategic Priority Research Program of the Chinese Academy of Sciences[2021YFA1600500 (2021YFA1600502)]; Strategic Priority Research Program of the Chinese Academy of Sciences[2022YFF0503003]; Strategic Priority Research Program of the Chinese Academy of Sciences[2022YFF0503000]; National Key R&D Program of China[12373065]; National Key R&D Program of China[12325303]; National Key R&D Program of China[12273115]; National Key R&D Program of China[12303057]; NSFC[BK20231510]; Natural Science Foundation of Jiangsu Province[202205AG070009]; Natural Science Foundation of Jiangsu Province[YNSPCC202206]; Yunnan Key Laboratory of Solar Physics and Space Science[2023M733734]; Special Research Assistant Project of Chinese Academy of Sciences - China Post-doctoral Science Foundation
WOS研究方向Astronomy & Astrophysics
语种英语
WOS记录号WOS:001304246500004
出版者OXFORD UNIV PRESS
资助机构NSFC ; China National Space Administration (CNSA) ; Precision Mechanics of CAS ; Innovation Academy for Microsatellites of CAS ; Strategic Priority Research Program on Space Science, Chinese Academy of Sciences[XDB0560000] ; Strategic Priority Research Program of the Chinese Academy of Sciences[2021YFA1600500 (2021YFA1600502), 2022YFF0503003, 2022YFF0503000] ; National Key R&D Program of China[12373065, 12325303, 12273115, 12303057] ; NSFC[BK20231510] ; Natural Science Foundation of Jiangsu Province[202205AG070009, YNSPCC202206] ; Yunnan Key Laboratory of Solar Physics and Space Science[2023M733734] ; Special Research Assistant Project of Chinese Academy of Sciences - China Post-doctoral Science Foundation
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27580]  
专题云南天文台_抚仙湖太阳观测站
作者单位1.Institute of Science and Technology for Deep Space Exploration, Suzhou Campus, Nanjing University, Suzhou 215163, China
2.School of Earth and Space Sciences, Peking University, Beijing 100871, China;
3.Astronomical Observatory, Kyoto University, Sakyo, Kyoto 606-8502, Japan;
4.Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China;
5.School of Astronomy and Space Science, University of Science and Technology of China, Hefei 230026, China;
6.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming 650216, China;
7.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Nanjing 210023, China;
推荐引用方式
GB/T 7714		 Zhang, Q M,Lin, M S,Yan XL,et al. Two successive EUV waves and a transverse oscillation of a quiescent prominence[J]. MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,2024,533(3):3255-3262.
APA Zhang, Q M.,Lin, M S.,闫晓理.,Dai, J.,Hou, Z Y.,...&Qiu, Y.(2024).Two successive EUV waves and a transverse oscillation of a quiescent prominence.MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY,533(3),3255-3262.
MLA Zhang, Q M,et al."Two successive EUV waves and a transverse oscillation of a quiescent prominence".MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 533.3(2024):3255-3262.

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