Hall current effects in dynamic magnetic reconnection solutions
- 18 July 2003
- journal article
- Published by AIP Publishing in Physics of Plasmas
- Vol. 10 (8) , 3120-3130
- https://doi.org/10.1063/1.1590980
Abstract
The impact of Hall current contributions on flow driven planar magnetic merging solutions is discussed. The Hall current is important if the dimensionless Hall parameter (or normalized ion skin depth) satisfies cH>η where η is the inverse Lundquist number for the plasma. A dynamic analysis of the problem shows, however, that the Hall current initially manifests itself, not by modifying the planar reconnection field, but by inducing a non-reconnecting perpendicular "separator" component in the magnetic field. Only if the stronger condition c2/H > η is satisfied can Hall currents be expected to affect the planar merging. These analytic predictions are then tested by performing a series of numerical experiments in periodic geometry, using the full system of planar magnetohydrodynamic (MHD) equations. The numerical results confirm that the nature of the merging changes dramatically when the Hall coupling satisfies c2/H > η. In line with the analytic treatment of sheared reconnection, the coupling provided by the Hall term leads to the emergence of multiple current layers that can enhance the global Ohmic dissipation at the expense of the reconnection rate. However, the details of the dissipation depend critically on the symmetries of the simulation, and when the merging is "head-on" (i.e., comprises fourfold symmetry) the reconnection rate can be enhancedKeywords
This publication has 13 references indexed in Scilit:
- Magnetic Reconnection Solutions Based on a Generalized Ohm's lawSolar Physics, 2003
- Recent developments in collisionless reconnection theory: Applications to laboratory and space plasmasPhysics of Plasmas, 2001
- Geospace Environmental Modeling (GEM) Magnetic Reconnection ChallengeJournal of Geophysical Research, 2001
- Flare Energy Release by Flux Pile‐up Magnetic Reconnection in a Turbulent Current SheetThe Astrophysical Journal, 2000
- Exact solutions for reconnective magnetic annihilationProceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, 2000
- Impulsive reconnection dynamics in collisionless laboratory and space plasmasJournal of Geophysical Research, 1999
- Magnetic Energy Release in Dynamic Fan Reconnection ModelsThe Astrophysical Journal, 1999
- Dynamic magnetic reconnection in three space dimensions: Fan current solutionsPhysics of Plasmas, 1998
- Exact Solutions for Steady State Incompressible Magnetic ReconnectionThe Astrophysical Journal, 1995
- Resistive MHD stagnation-point flows at a current sheetJournal of Plasma Physics, 1975