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FAST MAGNETIC RECONNECTION AND SPONTANEOUS...
Journal article

FAST MAGNETIC RECONNECTION AND SPONTANEOUS STOCHASTICITY

Abstract

Magnetic field lines in astrophysical plasmas are expected to be frozen-in at scales larger than the ion gyroradius. The rapid reconnection of magnetic-flux structures with dimensions vastly larger than the gyroradius requires a breakdown in the standard Alfvén flux-freezing law. We attribute this breakdown to ubiquitous MHD plasma turbulence with power-law scaling ranges of velocity and magnetic energy spectra. Lagrangian particle trajectories …

Authors

Eyink GL; Lazarian A; Vishniac ET

Journal

The Astrophysical Journal, Vol. 743, No. 1,

Publisher

American Astronomical Society

Publication Date

December 10, 2011

DOI

10.1088/0004-637x/743/1/51

ISSN

0004-637X