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 |
Published |
Philadelphia
The American Astronomical Society
01.04.2022
IOP Publishing |
Subjects | |
Online Access | Get full text |
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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. |
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Bibliography: | AAS36977 The Sun and the Heliosphere ObjectType-Article-1 SourceType-Scholarly Journals-1 ObjectType-Feature-2 content type line 14 |
ISSN: | 0004-637X 1538-4357 |
DOI: | 10.3847/1538-4357/ac590d |