Catastrophic onset of fast magnetic reconnection with a guide field
Phys. Plasmas 14, 054502 (2007); doi:10.1063/1.2734948
Published 11 May 2007
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It was recently shown that the slow (collisional) Sweet-Parker and the fast (collisionless) Hall magnetic reconnection solutions simultaneously exist for a wide range of resistivities; reconnection is bistable [Cassak, Shay, and Drake, Phys. Rev. Lett., 95, 235002 (2005)]. When the thickness of the dissipation region becomes smaller than a critical value, the Sweet-Parker solution disappears and fast reconnection ensues, potentially explaining how large amounts of magnetic free energy can accrue without significant release before the onset of fast reconnection. Two-fluid numerical simulations extending the previous results for anti-parallel reconnection (where the critical thickness is the ion skin depth) to component reconnection with a large guide field (where the critical thickness is the thermal ion Larmor radius) are presented. Applications to laboratory experiments of magnetic reconnection and the sawtooth crash are discussed.
©2007 American Institute of Physics
| History: | Received 25 January 2007; accepted 4 April 2007; published 11 May 2007 |
| Permalink: |
http://link.aip.org/link/?PHPAEN/14/054502/1 |
KEYWORDS and PACS
magnetic reconnection,
plasma magnetohydrodynamics,
plasma transport processes,
plasma simulation,
sawtooth instability
- 52.35.Vd
Magnetic reconnection in plasmas - 52.30.Cv
Plasma magnetohydrodynamics including electron magnetohydrodynamics - 52.25.Fi
Plasma transport properties - 52.30.Ex
Two-fluid and multi-fluid plasmas - 52.65.Kj
Magnetohydrodynamic and fluid equation (plasma simulation) - 52.35.Py
Plasma macroinstabilities (hydromagnetic) e.g., kink, fire-hose, mirror, ballooning, tearing, trapped-particle, flute, Rayleigh-Taylor instabilities, etc - YEAR: 2007
RELATED DATABASES
PUBLICATION DATA
1070-664X (print)
1089-7674 (online)
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