Stellar Flares, Superflares, and Coronal Mass Ejections—Entering the Big Data Era

Flares, sometimes accompanied by coronal mass ejections (CMEs), are the result of sudden changes in the magnetic field of stars with high energy release through magnetic reconnection, which can be observed across a wide range of the electromagnetic spectrum from radio waves to the optical range to X...

Полное описание

Библиографические подробности

Главные авторы:	Krisztián Vida, Zsolt Kővári, Martin Leitzinger, Petra Odert, Katalin Oláh, Bálint Seli, Levente Kriskovics, Robert Greimel, Anna Mária Görgei
Формат:	Artigo
Язык:	Inglês
Опубликовано:	MDPI AG 2024-07-01
Серии:	Universe
Предметы:	late-type stars stellar magnetic activity starspots stellar flares superflares stellar coronal mass ejections
Online-ссылка:	https://www.mdpi.com/2218-1997/10/8/313
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