Fundamental role of ion viscosity on fast magnetic reconnection in large-guide-field regimes
Creators
- 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
- DOI
- 10.1063/1.3449589;
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