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AGU: Journal of Geophysical Research, Space Physics

 

Keywords

  • Hall MHD
  • particle acceleration
  • turbulence

Index Terms

  • Solar Physics, Astrophysics, and Astronomy: Energetic particles
  • Solar Physics, Astrophysics, and Astronomy: Magnetic reconnection
  • Space Plasma Physics: Turbulence
  • Space Plasma Physics: Charged particle motion and acceleration
Abstract
Cited By (7)
 

Abstract

JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 111, A12110, 11 PP., 2006
doi:10.1029/2006JA011988

Test particle acceleration in three-dimensional Hall MHD turbulence

P. Dmitruk

Bartol Research Institute, University of Delaware, Newark, Delaware, USA

W. H. Matthaeus

Bartol Research Institute, University of Delaware, Newark, Delaware, USA

Numerical experiments of test particle acceleration are performed using turbulent magnetic and electric fields obtained from direct numerical solutions of the compressible three-dimensional Hall magnetohydrodynamic (MHD) equations. Comparisons are made of the results for the test particle momentum distribution function with and without the Hall term in the MHD solution. Electrons and protons are considered for the test particles at short times before particles leave the simulation box (with length size of the order of a few turbulent correlation lengths). The particles momentum distribution functions develop long tails in a short time. For electrons, no substantial difference it is found between results with and without the Hall term in the MHD solution, while for protons differences are seen in the low momentum part of the distributions. When a background uniform magnetic field (guide field) is added, the particle acceleration is anisotropic. Electrons develop large parallel momentum, while protons develop large perpendicular momentum. A discussion of the basic particle acceleration mechanisms in this system is made.

Received 25 July 2006; accepted 13 October 2006; published 21 December 2006.

Citation: Dmitruk, P., and W. H. Matthaeus (2006), Test particle acceleration in three-dimensional Hall MHD turbulence, J. Geophys. Res., 111, A12110, doi:10.1029/2006JA011988.

Cited By

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