Three-dimensional Propagation of the Global EUV Wave associated with a solar eruption on 2021 October 28

Abstract

We present a case study for the global extreme ultraviolet (EUV) wave and its chromospheric counterpart `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$\alpha$ 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 wavefront. The H$\alpha$ and 304 Å images also reveal signatures of wave propagation with a velocity of 310-540 km s${}^{-1}$. With multi-wavelength and dual-perspective observations, we found that the wavefront likely propagates forwardly inclined to the solar surface with a tilt angle of ~53.2${}^{\circ }$. Our results suggest that this EUV wave is a fast-mode magnetohydrodynamic wave or shock driven by the expansion of the associated CME, whose wavefront is likely a dome-shaped structure that could impact the upper chromosphere, transition region and corona.

Accepted by ApJ, 15 pages, and 7 figures

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• Why "solar tsunamis" rarely leave their imprints in the chromosphere
• A Data-constrained Magnetohydrodynamic Simulation of the X1.0 Solar Flare of 2021 October 28
• Observations of a Flare-ignited broad Quasi-periodic Fast-propagating wave train
• On the three-dimensional relation between the coronal dimming, erupting filament and CME. Case study of the 28 October 2021 X1.0 event
• The multi-spacecraft high-energy solar particle event of 28 October 2021
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• On some features of the solar proton event on 2021 October 28 (GLE73)
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• Limb Observations of Global Solar Coronal Extreme-ultraviolet Wavefronts: The Inclination, Kinematics, Coupling with the Expanding Coronal Mass Ejections, and Connection with the Coronal Mass Ejection Driven Shocks
• Implications for additional plasma heating driving the extreme-ultraviolet late phase of a solar flare with microwave imaging spectroscopy
• Global Coronal Plasma Diagnostics Based on Multi-slit EUV Spectroscopy
• Freely propagating flanks of wide coronal-mass-ejection-driven shocks: Modelling and observational insights
• Investigation of the Two-Dimensional Velocity Field of the Large-Scale Coronal Wave from September 6, 2011 using the SOLERwave Tool