English

Flow-turbulence interaction in magnetic reconnection

Solar and Stellar Astrophysics 2015-05-28 v2 Earth and Planetary Astrophysics Fluid Dynamics

Abstract

Roles of turbulence in the context of magnetic reconnection are investigated with special emphasis on the mutual interaction between flow (large-scale inhomogeneous structure) and turbulence. In order to evaluate the effective transport due to turbulence, in addition to the {\it intensity} information of turbulence represented by the turbulent energy, the {\it structure} information represented by pseudoscalar statistical quantities (helicities) is important. On the basis of the evolution equation, mechanisms that provide turbulence with cross helicity are presented. Magnetic-flux freezing in highly turbulent media is considered with special emphasis on the spatial distribution of the turbulent cross helicity. The cross-helicity effects in the context of magnetic reconnection are also investigated. It is shown that the large-scale flow and magnetic-field configurations favorable for the cross-helicity generation is compatible with the fast reconnection. In this sense, turbulence and large-scale structures promote magnetic reconnection mediated by the turbulent cross helicity.

Keywords

Cite

@article{arxiv.1105.6343,
  title  = {Flow-turbulence interaction in magnetic reconnection},
  author = {Nobumitsu Yokoi and Masahiro Hoshino},
  journal= {arXiv preprint arXiv:1105.6343},
  year   = {2015}
}

Comments

15 pages, 10 figures

R2 v1 2026-06-21T18:15:31.105Z