Escape of Flare-accelerated Particles in Solar Eruptive Events

Impulsive solar energetic particle events are widely believed to be due to the prompt escape into the interplanetary medium of flare-accelerated particles produced by solar eruptive events. According to the standard model for such events, however, particles accelerated by the flare reconnection shou...

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Veröffentlicht in:	The Astrophysical journal 2019-10, Vol.884 (2), p.143
Hauptverfasser:	Masson, S., Antiochos, S. K., DeVore, C. R.
Format:	Artikel
Sprache:	eng
Schlagworte:	Acceleration Astrophysics Computational fluid dynamics Computer simulation Corona Coronal mass ejection Dipoles Ejecta Energetic particles Fluctuations Fluid flow Flux Interplanetary medium Magnetic reconnection Magnetohydrodynamic simulation Physics Solar coronal mass ejections Solar magnetic reconnection Solar Physics Solar wind Standard model (particle physics) Three dimensional models
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