English

Fast magnetic reconnection in three dimensional MHD simulations

Plasma Physics 2015-05-18 v1 Solar and Stellar Astrophysics Computational Physics Fluid Dynamics

Abstract

We present a constructive numerical example of fast magnetic reconnection in a three dimensional periodic box. Reconnection is initiated by a strong, localized perturbation to the field lines. The solution is intrinsically three dimensional, and its gross properties do not depend on the details of the simulations. 50\sim 50% of the magnetic energy is released in an event which lasts about one Alfven time, but only after a delay during which the field lines evolve into a critical configuration. We present a physical picture of the process. The reconnection regions are dynamical and mutually interacting. In the comoving frame of these regions, reconnection occurs through an X-like point, analogous to Petschek reconnection. The dynamics appear to be driven by global flows, not local processes.

Keywords

Cite

@article{arxiv.1003.0105,
  title  = {Fast magnetic reconnection in three dimensional MHD simulations},
  author = {Bijia Pang and Ue-Li Pen and Ethan T. Vishniac},
  journal= {arXiv preprint arXiv:1003.0105},
  year   = {2015}
}

Comments

10 pages, 14 figures, submitted to Physics of Plasmas

R2 v1 2026-06-21T14:51:56.938Z