The Electrostatic Wave Instability as a Heating Mechanism in the Hot Phase of Solar Flares and Coronal Transients
The Electrostatic Wave Instability as a Heating Mechanism in the Hot Phase of Solar Flares and Coronal Transients
Document information
The Electrostatic Wave Instability as a Heating Mechanism in the Hot Phase of Solar Flares and Coronal Transients
International symposium, X-ray solar physics from Yohkoh ; 1993 ; Kanagawa; Japan
1994-01-01
4 pages
Conference paper
English
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