Numerical studies of particle acceleration at turbulent, oblique shocks with an application to prompt ion acceleration during solar flares

1986 ◽  
Vol 306 ◽  
pp. 710 ◽  
Author(s):  
R. B. Decker ◽  
L. Vlahos
1994 ◽  
Vol 142 ◽  
pp. 719-728
Author(s):  
Bernhard Kliem

AbstractTest particle orbits in the two-dimensional Fadeev equilibrium with a perpendicular electric field added are analyzed to show that impulsive bursty reconnection, which has been proposed as a model for fragmentary energy release in solar flares, may account also for particle acceleration to (near) relativistic energies within a fraction of a second. The convective electric field connected with magnetic island dynamics can play an important role in the acceleration process.Subject headings: acceleration of particles — MHD — plasmas — Sun: corona — Sun: flares


1986 ◽  
Vol 305 ◽  
pp. 909 ◽  
Author(s):  
W. Droege ◽  
R. Schlickeiser

1993 ◽  
Vol 415 ◽  
pp. 342 ◽  
Author(s):  
Jurgen Steinacker ◽  
Uwe Jaekel ◽  
Reinhard Schlickeiser

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