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Magnetic reconnection via current sheets

Journal Article · · Phys. Fluids; (United States)
DOI:https://doi.org/10.1063/1.865670· OSTI ID:5937776
A general picture of magnetic reconnection in the framework of 2-D incompressible resistive magnetohydrodynamic theory is presented. Numerical studies of (quasi-) steady-state driven reconnection reveal current sheet formation for Mach numbers M = u/v/sub A/ exceeding the Sweet--Parker reconnection rate M/sub SP/ = (eta/Lv/sub A/)/sup 1//sup ///sup 2/. Since the thickness delta of the current sheet is found to be invariant to a change of the resistivity eta, its length ..delta.. increases rapidly with decreasing eta or increasing M, which can be written in the form ..delta..approx.(M/M/sub SP/)/sup 4/, so that ..delta.. reaches the global system size L within a short range of the parameter M/M/sub SP/. The results are rather insensitive to the particular choice of boundary conditions. Because of the presence of a current sheet, the overall reconnection process is quite slow. This picture essentially agrees with Syrovatsky's (Sov. Phys. JETP 33, 933 (1971)) theory and disproves Petschek's (AAS/NASA Symposium on the Physics of Solar Flares, (NASA, Washington, DC, 1964) p. 425) mechanism of fast magnetic reconnection. A theory of the solution in the external and in the diffusion region is developed and analytical expressions in agreement with the simulation results are obtained by means of a variational principle.
Research Organization:
Max-Planck-Institut fuer Plasmaphysik,8046 Garching bei Muenchen, Federal Republic of Germany
OSTI ID:
5937776
Journal Information:
Phys. Fluids; (United States), Journal Name: Phys. Fluids; (United States) Vol. 29:5; ISSN PFLDA
Country of Publication:
United States
Language:
English