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 in | The Astrophysical journal Vol. 928; no. 2; pp. 98 - 107 |
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Main Authors | , , , , , , , , , , , , , , , , , , |
Format | Journal Article |
Language | English |
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01.04.2022
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Abstract | 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. |
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AbstractList | 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. 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 Hα 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 Hα 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. |
Author | Wang, Jing-Song He, Lingping Zhang, Peng Xu, Yu Tan, Guangyu Zhang, Xiaoxin Zheng, Ruisheng Chen, Hechao Hou, Zhenyong Chen, Yajie Zong, Weiguo Song, Qiao Song, Yongliang Hu, Xiuqing Dun, Jinping Tian, Hui Song, Kefei Chen, Bo Bai, Xianyong |
Author_xml | – sequence: 1 givenname: Zhenyong orcidid: 0000-0003-4804-5673 surname: Hou fullname: Hou, Zhenyong organization: Peking University School of Earth and Space Sciences, Beijing, 100871, People's Republic of China – sequence: 2 givenname: Hui orcidid: 0000-0002-1369-1758 surname: Tian fullname: Tian, Hui organization: Chinese Academy of Sciences National Astronomical Observatories, Beijing, 100012, People's Republic of China – sequence: 3 givenname: Jing-Song surname: Wang fullname: Wang, Jing-Song organization: National Center for Space Weather Key Laboratory of Space Weather, China Meteorological Administration, Beijing 100081, People's Republic of China – sequence: 4 givenname: Xiaoxin surname: Zhang fullname: Zhang, Xiaoxin organization: National Center for Space Weather Key Laboratory of Space Weather, China Meteorological Administration, Beijing 100081, People's Republic of China – sequence: 5 givenname: Qiao orcidid: 0000-0003-3568-445X surname: Song fullname: Song, Qiao organization: National Center for Space Weather Key Laboratory of Space Weather, China Meteorological Administration, Beijing 100081, People's Republic of China – sequence: 6 givenname: Ruisheng orcidid: 0000-0002-2734-8969 surname: Zheng fullname: Zheng, Ruisheng organization: Shandong University School of Space Science and Physics, Institute of Space Sciences, Weihai, Shandong, 264209, People's Republic of China – sequence: 7 givenname: Hechao orcidid: 0000-0001-7866-4358 surname: Chen fullname: Chen, Hechao organization: Peking University School of Earth and Space Sciences, Beijing, 100871, People's Republic of China – sequence: 8 givenname: Bo surname: Chen fullname: Chen, Bo organization: Chinese Academy of Sciences Changchun Institute of Optics, Fine Mechanics and Physics, Changchun 130033, People's Republic of China – sequence: 9 givenname: Xianyong orcidid: 0000-0003-2686-9153 surname: Bai fullname: Bai, Xianyong organization: Chinese Academy of Sciences National Astronomical Observatories, Beijing, 100012, People's Republic of China – sequence: 10 givenname: Yajie orcidid: 0000-0001-5494-4339 surname: Chen fullname: Chen, Yajie organization: Peking University School of Earth and Space Sciences, Beijing, 100871, People's Republic of China – sequence: 11 givenname: Lingping surname: He fullname: He, Lingping organization: Chinese Academy of Sciences Changchun Institute of Optics, Fine Mechanics and Physics, Changchun 130033, People's Republic of China – sequence: 12 givenname: Kefei surname: Song fullname: Song, Kefei organization: Chinese Academy of Sciences Changchun Institute of Optics, Fine Mechanics and Physics, Changchun 130033, People's Republic of China – sequence: 13 givenname: Peng surname: Zhang fullname: Zhang, Peng organization: Innovation Center for Fengyun Meteorological Satellite , National Satellite Meteorological Center, China Meteorological Administration, Beijing 100081, People's Republic of China – sequence: 14 givenname: Xiuqing surname: Hu fullname: Hu, Xiuqing organization: Innovation Center for Fengyun Meteorological Satellite , National Satellite Meteorological Center, China Meteorological Administration, Beijing 100081, People's Republic of China – sequence: 15 givenname: Jinping surname: Dun fullname: Dun, Jinping organization: National Center for Space Weather Key Laboratory of Space Weather, China Meteorological Administration, Beijing 100081, People's Republic of China – sequence: 16 givenname: Weiguo surname: Zong fullname: Zong, Weiguo organization: National Center for Space Weather Key Laboratory of Space Weather, China Meteorological Administration, Beijing 100081, People's Republic of China – sequence: 17 givenname: Yongliang surname: Song fullname: Song, Yongliang organization: Chinese Academy of Sciences National Astronomical Observatories, Beijing, 100012, People's Republic of China – sequence: 18 givenname: Yu surname: Xu fullname: Xu, Yu organization: Peking University School of Earth and Space Sciences, Beijing, 100871, People's Republic of China – sequence: 19 givenname: Guangyu surname: Tan fullname: Tan, Guangyu organization: Peking University School of Earth and Space Sciences, Beijing, 100871, People's Republic of China |
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Snippet | We present a case study for the global extreme-ultraviolet (EUV) wave and its chromospheric counterpart the
Moreton-Ramsey Wave
associated with the second... We present a case study for the global extreme-ultraviolet (EUV) wave and its chromospheric counterpart the Moreton-Ramsey Wave associated with the second... |
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StartPage | 98 |
SubjectTerms | Alfven waves Astrophysics Chromosphere Corona Coronal mass ejection Deceleration Fluid flow Magnetohydrodynamic waves Magnetohydrodynamics Propagation velocity Solar activity Solar corona Solar coronal mass ejections Solar coronal waves Solar cycle Solar surface Wave fronts Wave propagation |
Title | Three-dimensional Propagation of the Global Extreme-ultraviolet Wave Associated with a Solar Eruption on 2021 October 28 |
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