Kinematic Relationship Between Solar Extreme Ultraviolet Waves and Type II Metric Radio Bursts

arXiv:2609.00930 · astro-ph.SR · Submitted 2026-09-01 · Read on arXiv

astro-ph.SR

Submitted: 2026-09-01

Updated: 2026-09-01

Terminology

• Solar Dynamics Observatory — 6× in this paper
• Atmospheric Imaging Assembly — 3× in this paper
• Radio Solar Telescope Network — 3× in this paper
• Hybrid Model — 2× in this paper · explained in 2 episodes
• Active Regions — 1× in this paper · explained in 1 episode
• Benchmark — 1× in this paper · explained in 2 episodes
• Consistency — 1× in this paper · explained in 3 episodes
• Sun Earth Connection Coronal and Heliospheric Investigation — 1× in this paper

Sources

• Large-scale Coronal Propagating Fronts in Solar Eruptions as Observed by the Atmospheric Imaging Assembly on Board the Solar Dynamics Observatory\,--\,An Ensemble Study
• Observational Characteristics of solar EUV waves
• EUV Waves Driven by the Sudden Expansion of Transequatorial Loops Caused by Coronal Jets
• A type II solar radio burst without a coronal mass ejection
• Extreme-Ultraviolet Wave and Accompanying Loop Oscillations
• First Evidence of Coexisting EIT Wave and Coronal Moreton Wave from SDO/AIA Observations
• Dynamics and Kinematics of the EUV Wave Event on 6 May 2019
• Numerical Simulation of an EUV Coronal Wave Based on the February 13, 2009 CME Event Observed by STEREO
• Understanding CME and associated shock in the solar corona by merging multi wavelengths observation
• Coronal Signatures of Flare Generated Fast Mode Wave at EUV and Radio wavelengths
• Source location and evolution of a multi-lane type II radio burst
• Dependence of the intensity of the nonwave component of EUV waves on coronal magnetic field configuration
• Solar Energetic Particles and Associated EIT Disturbances in Solar Cycle 23

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