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National Center for Atmospheric Research

 

 

SCD/CSS SEMINAR:

 

  Revisiting turbulence at large Reynolds numbers

 

Speaker and Affiliation: Pablo Mininni ~ IMAGe/TNT
 

Abstract:
Several of the numerical investigations of turbulent flows are done in a rather abstract framework: that of three-dimensional rectangular periodic boundary conditions. This has happened for several reasons, an important one of which is that one of the best existing numerical techniques for investigating turbulence has been the Orszag-Patterson pseudospectral method that relies heavily on the fast Fourier transform. The method is non-dissipative, non-dispersive, and high-order. These are essential features for the study of turbulent flows. Another reason is that the results of such computations appear in a form that compares easily with homogeneous and isotropic turbulence theory predictions in the Kolmogorov theory. Several techniques have been developed to parallelize efficiently this method on distributed memory computers. In this talk we will discuss the methods and results from high-resolution simulations of hydrodynamic (HD) and magneto hydrodynamic (MHD) turbulence with Taylor Reynolds numbers up to 1200, done at NCAR and PSC. A pseudo spectral code that scales up to thousands of processors was used. We have re-investigated some familiar turbulence problems with the intent of revising some of the prevailing assumptions about the locality of interactions between spatial scales in Kolmogorov theory.

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Date, Time, and Location:

 


 
Tuesday, April 11, 2006

10:30 AM – 11:30 AM

NCAR Mesa Lab, Damon Room