Hot and Cool Plasmoid Ejections Associated with a Solar Flare
Author(s) -
M. Ohyama,
Kazunari Shibata
Publication year - 2008
Publication title -
publications of the astronomical society of japan
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.99
H-Index - 110
eISSN - 2053-051X
pISSN - 0004-6264
DOI - 10.1093/pasj/60.1.85
Subject(s) - plasmoid , physics , flare , protein filament , astrophysics , solar flare , coronal mass ejection , h alpha , plasma , solar prominence , astronomy , magnetic reconnection , solar wind , nuclear physics , emission spectrum , magnetic field , biology , quantum mechanics , genetics , spectral line
A 1993 May 14 flare was associated with both X-ray plasma ejection as hot plasmoid ejection and H$\alpha$ filament eruption as cool plasma ejection. The flare proceeded through two stages according to a GOES soft X-ray observation. In the first stage, an X-ray plasma ejection, an H$\alpha$ filament eruption, and a chain of pointlike H$\alpha$ brightenings occurred. In the second stage, an H$\alpha...
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