Stellar corona
In astronomy, a corona (pl.: coronas or coronae) is the outermost layer of a star's atmosphere. It is a region filled with relatively hot, tenuous plasma that is structured by the star's magnetic field.
In astronomy, a corona (pl.: coronas or coronae) is the outermost layer of a star's atmosphere. It is a region filled with relatively hot, tenuous plasma that is structured by the star's magnetic field.
In astronomy, a corona (pl.: coronas or coronae) is the outermost layer of a star's atmosphere. It is a region filled with relatively hot, tenuous plasma that is structured by the star's magnetic field.
Source: Wikipedia "Stellar corona" · CC BY-SA 4.0
Share this article: X · Bluesky