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Observational Characteristics of solar EUV waves

By Ramesh Chandra and others at
LogoKumaun University
and
LogoASTRON
Extreme-ultraviolet (EUV) waves are one of the large-scale phenomena on the Sun. They are defined as large propagating fronts in the low corona with speeds ranging from a few tens km/s to a multiple of 1000 km/s. They are often associated with solar filament eruptions, flares, or coronal mass ejections... Show more
October 19, 2023
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Observational Characteristics of solar EUV waves
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