scholarly journals Test Particle Acceleration in Three-dimensional Magnetohydrodynamic Turbulence

2003 ◽  
Vol 597 (1) ◽  
pp. L81-L84 ◽  
Author(s):  
P. Dmitruk ◽  
W. H. Matthaeus ◽  
N. Seenu ◽  
M. R. Brown
1999 ◽  
Vol 6 (11) ◽  
pp. 4318-4327 ◽  
Author(s):  
Rüdiger Schopper ◽  
Guido T. Birk ◽  
Harald Lesch

2016 ◽  
Vol 23 (8) ◽  
pp. 082305 ◽  
Author(s):  
C. A. González ◽  
P. Dmitruk ◽  
P. D. Mininni ◽  
W. H. Matthaeus

2014 ◽  
Vol 783 (2) ◽  
pp. 143 ◽  
Author(s):  
S. Dalena ◽  
A. F. Rappazzo ◽  
P. Dmitruk ◽  
A. Greco ◽  
W. H. Matthaeus

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


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