中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
Negative-energy Waves in the Vertical Threads of a Solar Prominence

文献类型:期刊论文

作者Wang JC(王金成)1,2; Li, Dong2,3; Li, Chuan4,5,6; Hou, Yijun2,7; Xue ZK(薛志科)1,2; Xu Z(徐喆)1,2; Yang LH(杨丽恒)1,2; Li, Qiaoling8
刊名ASTROPHYSICAL JOURNAL LETTERS
出版日期2024-04-01
卷号965期号:2
ISSN号2041-8205
DOI10.3847/2041-8213/ad3af8
产权排序第1完成单位
文献子类Article
英文摘要Solar prominences, intricate structures on the Sun's limb, have been a subject of fascination owing to their threadlike features and dynamic behaviors. Utilizing data from the New Vacuum Solar Telescope, Chinese H alpha Solar Explorer, and Solar Dynamics Observatory, this study investigates the transverse swaying motions observed in the vertical threads of a solar prominence during its eruption onset on 2023 May 11. The transverse swaying motions were observed to propagate upward, accompanied by upflowing materials at an inclination of 31 degrees relative to the plane of the sky. These motions displayed small-amplitude oscillations with corrected velocities of around 3-4 km s-1 and periods of 13-17 minutes. Over time, the oscillations of swaying motion exhibited an increasing pattern in displacement amplitudes, oscillatory periods, and projected velocity amplitudes. Their phase velocities are estimated to be about 26-34 km s-1. An important finding is that these oscillations' phase velocities are comparable to the upward flow velocities, measured to be around 30-34 km s-1. We propose that this phenomenon is associated with negative-energy wave instabilities, which require comparable velocities of the waves and flows, as indicated by our findings. This phenomenon may contribute to the instability and observed disruption of the prominence. By using prominence seismology, the Alfven speed and magnetic field strength of the vertical threads have been estimated to be approximately 21.5 km s-1 and 1-3G, respectively. This study reveals the dynamics and magnetic properties of solar prominences, contributing to our understanding of their behavior in the solar atmosphere.
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TRANSVERSE MAGNETOHYDRODYNAMIC WAVES ; RESONANT ABSORPTION ; MAGNETIC-STRUCTURE ; KINK OSCILLATIONS ; PROPAGATION ; SEISMOLOGY ; HINODE/SOT ; TELESCOPE ; TOPOLOGY ; DYNAMICS
资助项目MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809; China National Space Administration (CNSA)[XDB0560000]; Strategic Priority Research Program of the Chinese Academy of Sciences[2023063]; Youth Innovation Promotion Association CAS[12003064]; Youth Innovation Promotion Association CAS[12333009]; Youth Innovation Promotion Association CAS[12003068]; Youth Innovation Promotion Association CAS[12325303]; Youth Innovation Promotion Association CAS[12203020]; Youth Innovation Promotion Association CAS[12203097]; Youth Innovation Promotion Association CAS[12273110]; Youth Innovation Promotion Association CAS[12273060]; National Science Foundation of China (NSFC)[2019YFA0405000]; National Key R&D Program of China[202205AG070009]; Yunnan Key Laboratory of Solar Physics and Space Science[YNSPCC202211]; Open Research Program of Yunnan Key Laboratory of Solar Physics and Space Science[202301AT070347]; Open Research Program of Yunnan Key Laboratory of Solar Physics and Space Science[202201AT070194]; Open Research Program of Yunnan Key Laboratory of Solar Physics and Space Science[202001AU070077]; Yunnan Science Foundation of China[202001AV070004]; Yunnan Science Foundation for Distinguished Young Scholars[202305AS350029]; Yunnan Science Foundation for Distinguished Young Scholars[202305AT350005]; Yunnan Revitalization Talent Support Program; Group for Innovation of Yunnan province
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP Publishing Ltd
WOS记录号WOS:001204902600001
资助机构MOST divided by National Natural Science Foundation of China (NSFC)https://doi.org/10.13039/501100001809 ; China National Space Administration (CNSA)[XDB0560000] ; Strategic Priority Research Program of the Chinese Academy of Sciences[2023063] ; Youth Innovation Promotion Association CAS[12003064, 12333009, 12003068, 12325303, 12203020, 12203097, 12273110, 12273060] ; National Science Foundation of China (NSFC)[2019YFA0405000] ; National Key R&D Program of China[202205AG070009] ; Yunnan Key Laboratory of Solar Physics and Space Science[YNSPCC202211] ; Open Research Program of Yunnan Key Laboratory of Solar Physics and Space Science[202301AT070347, 202201AT070194, 202001AU070077] ; Yunnan Science Foundation of China[202001AV070004] ; Yunnan Science Foundation for Distinguished Young Scholars[202305AS350029, 202305AT350005] ; Yunnan Revitalization Talent Support Program ; Group for Innovation of Yunnan province
版本出版稿
源URL[http://ir.ynao.ac.cn/handle/114a53/27127]  
专题云南天文台_抚仙湖太阳观测站
作者单位1.Yunnan Observatories, Chinese Academy of Sciences, Kunming Yunnan 650216, People's Republic of China; wangjincheng@ynao.ac.cn;
2.Yunnan Key Laboratory of Solar Physics and Space Science, Kunming 650216, People's Republic of China;
3.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, People's Republic of China;
4.School of Astronomy and Space Science, Nanjing University, Nanjing 210023, People's Republic of China;
5.Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, 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.Department of Physics, Yunnan University, Kunming 650091, People's Republic of China
推荐引用方式
GB/T 7714
Wang JC,Li, Dong,Li, Chuan,et al. Negative-energy Waves in the Vertical Threads of a Solar Prominence[J]. ASTROPHYSICAL JOURNAL LETTERS,2024,965(2).
APA 王金成.,Li, Dong.,Li, Chuan.,Hou, Yijun.,薛志科.,...&Li, Qiaoling.(2024).Negative-energy Waves in the Vertical Threads of a Solar Prominence.ASTROPHYSICAL JOURNAL LETTERS,965(2).
MLA 王金成,et al."Negative-energy Waves in the Vertical Threads of a Solar Prominence".ASTROPHYSICAL JOURNAL LETTERS 965.2(2024).

入库方式: OAI收割

来源:云南天文台

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