scholarly journals On the compressibility effect in test particle acceleration by magnetohydrodynamic turbulence

2016 ◽  
Vol 23 (8) ◽  
pp. 082305 ◽  
Author(s):  
C. A. González ◽  
P. Dmitruk ◽  
P. D. Mininni ◽  
W. H. Matthaeus
2003 ◽  
Vol 597 (1) ◽  
pp. L81-L84 ◽  
Author(s):  
P. Dmitruk ◽  
W. H. Matthaeus ◽  
N. Seenu ◽  
M. R. Brown

2017 ◽  
Vol 29 (3) ◽  
pp. 035105 ◽  
Author(s):  
Yan Yang ◽  
William H. Matthaeus ◽  
Yipeng Shi ◽  
Minping Wan ◽  
Shiyi Chen

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


1999 ◽  
Vol 6 (11) ◽  
pp. 4318-4327 ◽  
Author(s):  
Rüdiger Schopper ◽  
Guido T. Birk ◽  
Harald Lesch

1989 ◽  
Vol 16 (9) ◽  
pp. 1027-1030 ◽  
Author(s):  
D. Sachsenweger ◽  
M. Scholer ◽  
E. Möbius

2006 ◽  
Vol 2 (14) ◽  
pp. 88-88
Author(s):  
Miroslav Bárta ◽  
Marian Karlický

AbstractStarting from 2.5D MHD modelling of solar flares on a global scale we calculate (using the PIC and test-particle simulations) the radio and X-ray emissions generated in solar flare reconnection. Our results – the radio and X-ray spectra and brightness distributions, and their dynamics – are directly comparable with observations providing thus a test of particle acceleration models as well as of the ‘standard’ global flare scenario.


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