Astronomy and Astrophysics – Astrophysics
Scientific paper
Aug 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...438..391k&link_type=abstract
Astronomy and Astrophysics, Volume 438, Issue 2, August I 2005, pp.391-402
Astronomy and Astrophysics
Astrophysics
12
Acceleration Of Particles, Shock Waves, Diffusion
Scientific paper
We discuss an acceleration mechanism of charged particles by magnetohydrodynamic (MHD) structures, such as quasi-parallel shocks and short-large amplitude magnetic structures (SLAMS). In the presence of electromagnetic waves and an electrostatic electric field, particles are accelerated efficiently in the perpendicular direction to the background magnetic field by the combination of two effects, the trapping of particles by the wave and the dragging by the electrostatic field to keep the resonance condition. This allows particles to propagate downstream even when they initially have smaller kinetic energy than the potential. We show the fundamental properties of this mechanism, referred to as gyroresonant surfing.
Krasnoselskikh Vladimir
Kuramitsu Yasuhiro
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