Negative-energy Waves in the Vertical Threads of a Solar Prominence

doi:10.3847/2041-8213/ad3af8

YNAO OpenIR > 抚仙湖太阳观测和研究基地

	Negative-energy Waves in the Vertical Threads of a Solar Prominence
	Wang JC(王金成)1,2 ; Li, Dong 2,3; Li, Chuan 4,5,6; Hou, Yijun 2,7; Xue ZK(薛志科)1,2 ; Xu Z(徐喆)1,2 ; Yang LH(杨丽恒)1,2 ; Li, Qiaoling 8
发表期刊	ASTROPHYSICAL JOURNAL LETTERS
	2024-04-01
卷号	965 期号:2
DOI	10.3847/2041-8213/ad3af8
产权排序	第1完成单位
收录类别	SCI
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.
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
项目资助者	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
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	IOP Publishing Ltd
出版地	TEMPLE CIRCUS, TEMPLE WAY, BRISTOL BS1 6BE, ENGLAND
ISSN	2041-8205
URL	查看原文
WOS记录号	WOS:001204902600001
WOS研究方向	Astronomy & Astrophysics
WOS类目	Astronomy & Astrophysics
关键词[WOS]	TRANSVERSE MAGNETOHYDRODYNAMIC WAVES ; RESONANT ABSORPTION ; MAGNETIC-STRUCTURE ; KINK OSCILLATIONS ; PROPAGATION ; SEISMOLOGY ; HINODE/SOT ; TELESCOPE ; TOPOLOGY ; DYNAMICS
引用统计
文献类型	期刊论文
版本	出版稿
条目标识符	http://ir.ynao.ac.cn/handle/114a53/27127
专题	抚仙湖太阳观测和研究基地
作者单位	1.Yunnan Observatories, Chinese Academy of Sciences, Kunming Yunnan 650216, People's Republic of China; [email protected]; 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
第一作者单位	中国科学院云南天文台
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).

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