Astronomy and Astrophysics – Astrophysics
Scientific paper
Jun 1990
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990apjs...73..313o&link_type=abstract
(NASA and University of New Hampshire, Workshop on Impulsive Solar Flares, 2nd, Durham, NH, Sept. 26-28, 1988) Astrophysical Jou
Astronomy and Astrophysics
Astrophysics
2
Ion Beams, Magnetoelastic Waves, Particle Acceleration, Relativistic Particles, Shock Waves, Electric Fields, Mach Number, Magnetic Fields, Solar Flares, Trapped Particles, Wave Propagation
Scientific paper
The rapid acceleration of ions by a large-amplitude magnetosonic wave is discussed. Theory and relativistic particle simulation show that a large-amplitude magnetosonic wave (such as a shock wave) can trap some fraction of ions and resonantly accelerate them in the direction perpendicular to the ambient magnetic field. In a rather strong magnetic field, those resonant ions gain relativistic energies (above 1 GeV) in a short time period (much shorter than 1 s). The condition for the ion trapping is also studied; a few percent of ions can be strongly accelerated, and more than 10 percent of ions can be mildly accelerated for the shock with the Alfven Mach number of about 2.
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