Turbulent Magnetic Reconnection in Two Dimensions
Solar and Stellar Astrophysics
2015-05-13 v2 Plasma Physics
Space Physics
Abstract
Two-dimensional numerical simulations of the effect of background turbulence on 2D resistive magnetic reconnection are presented. For sufficiently small values of the resistivity () and moderate values of the turbulent power (), the reconnection rate is found to have a much weaker dependence on than the Sweet-Parker scaling of and is even consistent with an independent value. For a given value of , the dependence of the reconnection rate on the turbulent power exhibits a critical threshold in above which the reconnection rate is significantly enhanced.
Keywords
Cite
@article{arxiv.0904.0823,
title = {Turbulent Magnetic Reconnection in Two Dimensions},
author = {N. F. Loureiro and D. A. Uzdensky and A. A. Schekochihin and S. C. Cowley and T. A. Yousef},
journal= {arXiv preprint arXiv:0904.0823},
year = {2015}
}
Comments
Accepted to MNRAS