AbstractNumerical simulations of two types of flares indicate that magnetic reconnection can provide environments favorable for various particle acceleration mechanisms to work. This paper reviews recent test particle simulations of DC electric field mechanism, and discusses how the flare particles can escape into the interplanetary space under different magnetic configurations.
Magnetic reconnection configurations and particle acceleration in solar flares
Advances in Space Research ; 39 , 9 ; 1421-1426
2007-02-20
6 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
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