Exact solutions for steady-state, planar, magnetic reconnection in an incompressible viscous plasma
- 1 June 1996
- journal article
- Published by AIP Publishing in Physics of Plasmas
- Vol. 3 (6) , 2243-2247
- https://doi.org/10.1063/1.871932
Abstract
The exact planar reconnection analysis of Craig and Henton [Astrophys. J. 450, 280 (1995)] is extended to include the finite viscosity of the fluid and the presence of nonplanar components in the magnetic and velocity fields. It is shown that fast reconnection can be achieved for sufficiently small values of the kinematic viscosity. In particular, the dissipation rate is sustained by the strong amplification of planar magnetic field components advected toward the neutral point. By contrast, nonplanar field components are advected without amplification and so dissipate energy at the slow Sweet–Parker rate.Keywords
This publication has 13 references indexed in Scilit:
- Exact Solutions for Steady State Incompressible Magnetic ReconnectionThe Astrophysical Journal, 1995
- Linear theory of fast reconnection at an X-type neutral pointThe Astrophysical Journal, 1993
- Reconnection of stressed magnetic fieldsThe Astrophysical Journal, 1992
- Fast dynamic reconnection at X-type neutral pointsThe Astrophysical Journal, 1992
- A family of two‐dimensional nonlinear solutions for magnetic field annihilationJournal of Geophysical Research, 1992
- Dynamic magnetic reconnection at an X-type neutral pointThe Astrophysical Journal, 1991
- Planar MHD stagnation-point flows with velocity shearPlanetary and Space Science, 1990
- MHD stagnation point flows in the presence of resistivity and viscosityJournal of Geophysical Research, 1988
- A comparison of analytical and numerical models for steadily driven magnetic reconnectionReviews of Geophysics, 1987
- Resistive MHD stagnation-point flows at a current sheetJournal of Plasma Physics, 1975