Abstract

In this paper we study a well-known three--dimensional turbulence model, the filtered Clark model, or Clark-alpha model. This is Large Eddy Simulation (LES) tensor-diffusivity model of turbulent flows with an additional spatial filter of width alpha (α\alpha). We show the global well-posedness of this model with constant Navier-Stokes (eddy) viscosity. Moreover, we establish the existence of a finite dimensional global attractor for this dissipative evolution system, and we provide an anaytical estimate for its fractal and Hausdorff dimensions. Our estimate is proportional to (L/ld)3(L/l_d)^3, where LL is the integral spatial scale and ldl_d is the viscous dissipation length scale. This explicit bound is consistent with the physical estimate for the number of degrees of freedom based on heuristic arguments. Using semi-rigorous physical arguments we show that the inertial range of the energy spectrum for the Clark-a˚\aa model has the usual k−5/3k^{-5/3} Kolmogorov power law for wave numbers ka˚≪1k\aa \ll 1 and k−3k^{-3} decay power law for ka˚≫1.k\aa \gg 1. This is evidence that the Clark−α-\alpha model parameterizes efficiently the large wave numbers within the inertial range, ka˚≫1k\aa \gg 1, so that they contain much less translational kinetic energy than their counterparts in the Navier-Stokes equations.Comment: 11 pages, no figures, submitted to J of Turbulenc

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