Current sheet formation along three-dimensional magnetic separators
- 1 August 1996
- journal article
- Published by AIP Publishing in Physics of Plasmas
- Vol. 3 (8) , 2885-2897
- https://doi.org/10.1063/1.871627
Abstract
It was shown by Syrovatskii [Sov. Phys. JETP 33, 933 (1971)] that a perfectly conducting two‐dimensional magnetic field stressed externally develops a current sheet at an X point. A generalization of this analysis shows that a generic three‐dimensional magnetic field develops a closed ribbon of current along separators already existing in the field. A separator is a field line that begins and ends at different magnetic null points. A current ribbon will occur if there are two distinct separators beginning and ending at the same two nulls, thus forming a loop. The magnetic field containing the current ribbon is in force‐free equilibrium. An expression is found for the net current induced in the ribbon, and the magnetic energy stored by it, in terms of the amount of external stress. An electric field parallel to the current will facilitate reconnection and will dissipate the current and release the stored energy.Keywords
This publication has 19 references indexed in Scilit:
- Magnetic reconnectionPhysics Reports, 1994
- Nonlinear dynamics of them=1 instability and fast sawtooth collapse in high-temperature plasmasPhysical Review Letters, 1993
- Fast magnetic reconnection and the coalescence instabilityPhysics of Fluids B: Plasma Physics, 1993
- Does fast magnetic reconnection exist?Journal of Geophysical Research, 1992
- Collisionless reconnection and the sawtooth crashPhysical Review Letters, 1991
- Current sheet formation in a sheared force-free-magnetic fieldThe Astrophysical Journal, 1989
- A theoretical foundation of general magnetic reconnectionJournal of Geophysical Research, 1988
- Magnetic reconnection via current sheetsPhysics of Fluids, 1986
- Electric currents in the solar corona and the existence of magnetostatic equilibriumThe Astrophysical Journal, 1985
- Topological Dissipation and the Small-Scale Fields in Turbulent GasesThe Astrophysical Journal, 1972