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Stochastic acceleration by multi-island contraction during turbulent magnetic reconnection

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arxiv 1302.6090 v1 pith:BROTIKLD submitted 2013-02-25 astro-ph.SR physics.plasm-ph

classification astro-ph.SRphysics.plasm-ph
keywords accelerationcompressionparticlesprocessduringratemagneticmodel
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The acceleration of charged particles in magnetized plasmas is considered during turbulent multi-island magnetic reconnection. The particle acceleration model is constructed for an ensemble of islands which produce adiabatic compression of the particles. The model takes into account the statistical fluctuations in the compression rate experienced by the particles during their transport in the acceleration region. The evolution of the particle distribution function is described as a simultaneous first and second-order Fermi acceleration process. While the efficiency of the first-order process is controlled by the average rate of compression, the second order process involves the variance in the compression rate. Moreover, the acceleration efficiency associated with the second-order process involves both the Eulerian properties of the compression field and the Lagrangian properties of the particles. The stochastic contribution to the acceleration is non-resonant and can dominate the systematic part in the case of a large variance in the compression rate. The model addresses the role of the second-order process, how the latter can be related to the large-scale turbulent transport of particles and explains some features of the numerical simulations of particle acceleration by multi-island contraction during magnetic reconnection.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. A Brief Review on Particle Acceleration in Multi-island Magnetic Reconnection

    astro-ph.SR 2019-08 conditional novelty 1.0 of 10

    The paper concludes that multi-island magnetic reconnection, while theoretically able to produce power-law particle spectra, fails in mildly relativistic simulations and cannot yet explain observed solar wind and flar...

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