Sub-Grid-Scale Description of Turbulent Magnetic Reconnection in Magnetohydrodynamics

@article{Widmer2015SubGridScaleDO,
  title={Sub-Grid-Scale Description of Turbulent Magnetic Reconnection in Magnetohydrodynamics},
  author={F. Widmer and Jorg Buchner and N. Yokoi},
  journal={arXiv: Plasma Physics},
  year={2015}
}
Magnetic reconnection requires, at least locally, a non-ideal plasma response. In collisionless space and astrophysical plasmas, turbulence could permit this instead of the too rare binary collisions. We investigated the influence of turbulence on the reconnection rate in the framework of a single fluid compressible MHD approach. The goal is to find out, whether unresolved, sub-grid for MHD simulations, turbulence can enhance the reconnection process in high Reynolds number astrophysical plasma… 
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