English

A model of Hall reconnection

Astrophysics 2009-12-11 v2

Abstract

The rate of quasi-stationary, two-dimensional magnetic reconnection is calculated in the framework of incompressible Hall magnetohydrodynamics (MHD). The calculation is based on the solution of Hall-MHD equations that include Hall and electron pressure terms for electric current. These equations are solved in a local region across the reconnection electron layer, including only the upstream region and the layer center. In the case when the ion inertial length d_i is larger than the Sweet-Parker reconnection layer thickness, the dimensionless reconnection rate is found to be independent of the electrical resistivity and equal to d_i/L, where L is the scale length of the external magnetic field in the upstream region outside the electron layer.

Keywords

Cite

@article{arxiv.0810.3278,
  title  = {A model of Hall reconnection},
  author = {Leonid M. Malyshkin},
  journal= {arXiv preprint arXiv:0810.3278},
  year   = {2009}
}

Comments

4 pages, 1 figure

R2 v1 2026-06-21T11:32:17.907Z