Simultaneous detection of flare-associated kink oscillations and extreme-ultraviolet waves

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外文摘要：Kink oscillations,which are frequently observed in coronal loops and prominences,are often accompanied by extreme-ultraviolet(EUV)waves.However,much more needs to be explored regarding the causal relationships between kink oscillations and EUV waves.In this article,we report the simultaneous detection of kink oscillations and EUV waves that are both associated with an X2.1 flare on 2023 March 03(SOL2023-03-03T17:39).The kink oscillations,which are almost perpendicular to the axes of loop-like structures,are observed in three coronal loops and one prominence.One short loop shows in-phase oscillation within the same period of 5.2 min at three positions.This oscillation could be triggered by the pushing of an expanding loop and interpreted as the standing kink wave.Time lags are found between the kink oscillations of the short loop and two long loops,suggesting that the kink wave travels in different loops.The kink oscillations of one long loop and the prominence are possibly driven by the disturbance of the coronal mass ejection(CME),and that of another long loop might be attributed to the interaction of the EUV wave.The onset time of the kink oscillation of the short loop is nearly same as the beginning of an EUV wave.This fact demonstrates that they are almost simultaneous.The EUV wave is most likely excited by the expanding loop structure and shows two components.The leading component is a fast coronal wave,and the trailing one could be due to the stretching magnetic field lines.

外文关键词：

coronal loopssolar flaressolar prominencesolar oscillationsextreme-ultraviolet wavemagnetohydrodynamic

作者：

LI Dong、HOU ZhenYong、BAI XianYong、LI Chuan、FANG Matthew、ZHAO HaiSheng、WANG JinCheng、NING ZongJun

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作者单位：

Key Laboratory of Dark Matter and Space Astronomy,Purple Mountain Observatory,Chinese Academy of Sciences,Nanjing 210023,China

Yunnan Key Laboratory of the Solar Physics and Space Science,Kunming 650216,China

School of Earth and Space Sciences,Peking University,Beijing 100871,China

National Astronomical Observatories,Chinese Academy of Sciences,Beijing 100101,China

School of Astronomy and Space Science,University of Chinese Academy of Sciences,Beijing 100049,China

School of Astronomy and Space Science,Nanjing University,Nanjing 210023,China

Key Laboratory of Modern Astronomy and Astrophysics,Ministry of Education,Nanjing University,Nanjing 210023,China

Columbus Academy,Gahanna 0hio 43230,USA

Key Laboratory of Particle Astrophysics,Institute of High Energy Physics,Chinese Academy of Sciences,Beijing 100049,China

Yunnan Observatories,Chinese Academy of Sciences,Kunming 650216,China

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基金：

National Key R&D Program of ChinaNational Key R&D Program of ChinaNational Natural Science Foundation of ChinaNational Natural Science Foundation of ChinaNational Natural Science Foundation of ChinaNational Natural Science Foundation of ChinaSurface Project of Jiangsu ProvinceYunnan Key Laboratory of Solar Physics and Space ScienceNational Astronomical Observatories of CASPeking UniversityTongji UniversityXi'an Institute of Optics and Precision Mechanics of CASInnovation Academy for Microsatellites of CASChina National Space Administration(CNSA)

项目编号：

2021YFA16005022021YFA160050011973092120730811200306412333009BK20211402YN-SPCC202207

出版年：

2024

DOI：

10.1007/s11431-023-2534-8

中国科学:技术科学(英文版)

中国科学院

中国科学:技术科学(英文版)

CSTPCDEI

影响因子：1.056

ISSN：1674-7321

年,卷(期)：2024.67(5)