English

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 (η\eta) and moderate values of the turbulent power (ϵ\epsilon), the reconnection rate is found to have a much weaker dependence on η\eta than the Sweet-Parker scaling of η1/2\eta^{1/2} and is even consistent with an η\eta-independent value. For a given value of η\eta, the dependence of the reconnection rate on the turbulent power exhibits a critical threshold in ϵ\epsilon 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

R2 v1 2026-06-21T12:48:24.541Z