Model of two-fluid reconnection
Solar and Stellar Astrophysics
2009-12-11 v3 Earth and Planetary Astrophysics
Abstract
A theoretical model of quasi-stationary, two-dimensional magnetic reconnection is presented in the framework of incompressible two-fluid magnetohydrodynamics (MHD). The results are compared with recent numerical simulations and experiment.
Keywords
Cite
@article{arxiv.0904.0660,
title = {Model of two-fluid reconnection},
author = {Leonid M. Malyshkin},
journal= {arXiv preprint arXiv:0904.0660},
year = {2009}
}
Comments
4 pages, 1 figure, accepted to Physical Review Letters