Three-dimensional Propagation of the Global Extreme-ultraviolet Wave Associated with a Solar Eruption on 2021 October 28

We present a case study for the global extreme-ultraviolet (EUV) wave and its chromospheric counterpart the Moreton-Ramsey Wave associated with the second X-class flare in Solar Cycle 25 and a halo coronal mass ejection (CME). The EUV wave was observed in the H α and EUV passbands with different cha...

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Published inThe Astrophysical journal Vol. 928; no. 2; pp. 98 - 107
Main Authors Hou, Zhenyong, Tian, Hui, Wang, Jing-Song, Zhang, Xiaoxin, Song, Qiao, Zheng, Ruisheng, Chen, Hechao, Chen, Bo, Bai, Xianyong, Chen, Yajie, He, Lingping, Song, Kefei, Zhang, Peng, Hu, Xiuqing, Dun, Jinping, Zong, Weiguo, Song, Yongliang, Xu, Yu, Tan, Guangyu
Format Journal Article
LanguageEnglish
Published Philadelphia The American Astronomical Society 01.04.2022
IOP Publishing
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Summary:We present a case study for the global extreme-ultraviolet (EUV) wave and its chromospheric counterpart the Moreton-Ramsey Wave associated with the second X-class flare in Solar Cycle 25 and a halo coronal mass ejection (CME). The EUV wave was observed in the H α and EUV passbands with different characteristic temperatures. In the 171 Å and 193/195 Å images, the wave propagates circularly with an initial velocity of 600–720 km s −1 and a deceleration of 110–320 m s −2 . The local coronal plasma is heated from log( T/K ) ≈ 5.9 to log( T/K ) ≈ 6.2 during the passage of the wave front. The H α and 304 Å images also reveal signatures of wave propagation with a velocity of 310–540 km s −1 . With multiwavelength and dual-perspective observations, we found that the wave front likely propagates forwardly inclined to the solar surface with a tilt angle of ∼53°.2. Our results suggest that this EUV wave is a fast-mode magnetohydrodynamic wave or shock driven by the expansion of the associated CME, whose wave front is likely a dome-shaped structure that could impact the upper chromosphere, transition region, and corona.
Bibliography:AAS36977
The Sun and the Heliosphere
ObjectType-Article-1
SourceType-Scholarly Journals-1
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ISSN:0004-637X
1538-4357
DOI:10.3847/1538-4357/ac590d