Search NASA⌕ Search

NASA NTRS · 19910061953

Renormalization group analysis of reduced magnetohydrodynamics with application to subgrid modeling

Abstract

The technique for obtaining a subgrid model for Navier-Stokes turbulence, based on renormalization group analysis (RNG), is extended to the reduced magnetohydrodynamic (RMND) equations. It is shown that a RNG treatment of the Alfven turbulence supported by the RMHD equations leads to effective values of the viscosity and resistivity at large scales, k yields 0, dependent on the amplitude of turbulence. The effective viscosity and resistivity become independent of the molecular quantities when the RNG analysis is augmented by the Kolmogorov argument for energy cascade. A self-contained system of equations is derived for the range of scales, k = 0-K, where K = pi/Delta is the maximum wave number for a grid size Delta. Differential operators, whose coefficients depend upon the amplitudes of the large-scale quantities, represent in this system the resistive and viscous dissipation.

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Longcope, D. W., Sudan, R. N.. 1991-08-01. Renormalization group analysis of reduced magnetohydrodynamics with application to subgrid modeling. https://ntrs.nasa.gov/citations/19910061953

Cite the original work for its findings. Save a collection to share your selection of sources.