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Turbulent magnetic Prandtl number and magnetic diffusivity quenching from simulations

T. A. Yousef, A. Brandenburg, G. Rüdiger

astro-pharXiv:astro-ph/0302425

Abstract

Forced turbulence simulations are used to determine the turbulent kinematic viscosity, nut, from the decay rate of a large scale velocity field. Likewise, the turbulent magnetic diffusivity, etat, is determined from the decay of a large scale magnetic field. In the kinematic regime, when the field is weak, the turbulent magnetic Prandtl number, nut/etat, is about unity. When the field is nonhelical, etat is quenched when magnetic and kinetic energies become comparable. For helical fields the quenching is stronger and can be described by a dynamical quenching formula.

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