Experimental Observation of Energetic Ions Accelerated by Three-dimensional Magnetic Reconnection in a Laboratory Plasma

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Published 2002 August 30 © 2002. The American Astronomical Society. All rights reserved. Printed in U.S.A.
, , Citation M. R. Brown et al 2002 ApJ 577 L63 DOI 10.1086/344145

1538-4357/577/1/L63

Abstract

Magnetic reconnection is widely believed responsible for heating the solar corona as well as for generating X-rays and energetic particles in solar flares. On astrophysical scales, reconnection in the intergalactic plasma is a prime candidate for a local source (<100 Mpc) of cosmic rays exceeding the Greisen-Zatsepin-Kúzmin cutoff (~1019 eV). In a laboratory astrophysics experiment, we have made the first observation of particles accelerated by magnetic reconnection events to energies significantly above both the thermal and the characteristic magnetohydrodynamic energies. These particles are correlated temporally and spatially with the formation of three-dimensional magnetic structures in the reconnection region.

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10.1086/344145