Published June 2010 | Version v1
Journal article

Fundamental role of ion viscosity on fast magnetic reconnection in large-guide-field regimes

  • 1. Theoretical Division, Los Alamos National Laboratory, Los Alamos, New Mexico 87545 (United States) and Max-Planck-Institut fuer Plasmaphysik, 17491 Greifswald (Germany)
  • 2. Fusion Energy Division, Oak Ridge National Laboratory, Oak Ridge, Tennessee 37830 (United States)
  • 3. Culham Centre for Fusion Energy, Abingdon, Oxon OX14 3DB, United Kingdom and Rudolf Peierls Centre for Theoretical Physics, University of Oxford, Oxford OX1 3NP (United Kingdom)

Description

Nonlinear analytical theory of magnetic reconnection with a large guide field is presented for the first time. We confirm that two distinct steady-state reconnection regimes are possible depending on the relative size of the diffusion region thickness δ versus the sound gyroradius ρs. The reconnection is slow (Sweet-Parker-like) for δ > or approx. ρs, and fast otherwise. However, unlike earlier work, we find that ion viscosity μ plays a fundamental role in the fast regime. In particular, for δ<ρs we obtain δ∝Ha-1, with Ha∝1/√(ημ) as the Hartmann number, and the reconnection rate Ez∝Pr-1/2, with Pr=μ/η as the Prandtl number and η as the resistivity. If the perpendicular ion viscosity is employed for μ, the reconnection rate becomes independent of plasma β and collision frequencies, and therefore potentially fast.

Additional details

Identifiers

Publishing Information

Journal Title
Physics of Plasmas
Journal Volume
17
Journal Issue
6
Journal Page Range
p. 060701-060701.4
ISSN
1070-664X
CODEN
PHPAEN

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
41108460
Subject category
S70: PLASMA PHYSICS AND FUSION TECHNOLOGY;
Descriptors DEI
COLLISIONS; ION ACOUSTIC WAVES; IONS; MAGNETIC RECONNECTION; NONLINEAR PROBLEMS; PLASMA; STEADY-STATE CONDITIONS; VISCOSITY
Descriptors DEC
CHARGED PARTICLES; ION WAVES; PLASMA WAVES

Optional Information

Notes
(c) 2010 American Institute of Physics