Abstract
A subgrid-scale (SGS) model is proposed to enable the numerical simulation of magnetohydrodynamic (MHD) turbulence at very high kinetic and magnetic Reynolds numbers in fusion plasma physics and astro/geophysics. The model supplements the SGS energy dissipation process with the aid of the SGS turbulent viscosity, the SGS anomalous resistivity, etc., which are written in terms of the grid-scale magnetic field and velocity.
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