Extreme Ultraviolet Waves in Solar Corona
A special issue of Galaxies (ISSN 2075-4434).
Deadline for manuscript submissions: closed (18 February 2022) | Viewed by 2762
Special Issue Editor
Special Issue Information
Dear Colleagues,
Extreme ultraviolet (EUV) waves are impressive coronal propagating disturbances that are best seen as intensity enhancements in EUV emission. EUV waves are also called “EIT waves”, “coronal bright fronts”, and “large-scale coronal propagating fronts”. EUV waves can provide potential diagnostics on coronal magnetic field strengths and coronal plasma parameters. Since the discovery of the first case, the EUV wave has been strongly debated in relation to the physical nature of a true wave or a pseudo wave. On the other hand, it is widely recognized that EUV waves are always associated with a variety of energetic eruptions, such as CMEs, flares, and filament eruptions. Benefiting from high resolution observations from the Solar Terrestrial Relations Observatory (STEREO) and the Solar Dynamics Observatory (SDO), an increasing number of EUV waves are being easily captured, including many small-scale cases that are associated with weak eruptions and present many new observational characteristics.
The proposed issue is scheduled for gathering new results of EUV waves in solar corona and aims to pave the way for better understanding the physical nature and driving mechanisms of solar EUV waves.
Prof. Dr. Ruisheng Zheng
Guest Editor
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Keywords
- extreme ultraviolet
- EIT waves
- solar corona
