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Paper: Plasma Ejections from Coronae of Red Dwarfs
Volume: 518, Physics of Magnetic Stars
Page: 222
Authors: Kiikov, S. O.
Abstract: The formation of plasma ejections from coronae of flare red dwarf stars is being studied. It is assumed that under certain conditions such a process can be due to manifestation of plasmoids in the coronal plasma of these stars. The conditions contributing to this process can occur during magnetic reconnection in the current sheets of coronal plasma of red dwarfs and lead to the formation of plasmoids. Some plasmoids are ejected from the corona, but others are destroyed because of resonant and shock waves. The destruction of plasmoids can lead to the formation of plasma ejections. The parameters of plasma ejections are estimated.
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