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Solutions of the Taylor-Green Vortex Problem Using High-Resolution Explicit Finite Difference MethodsA computational fluid dynamics code that solves the compressible Navier-Stokes equations was applied to the Taylor-Green vortex problem to examine the code s ability to accurately simulate the vortex decay and subsequent turbulence. The code, WRLES (Wave Resolving Large-Eddy Simulation), uses explicit central-differencing to compute the spatial derivatives and explicit Low Dispersion Runge-Kutta methods for the temporal discretization. The flow was first studied and characterized using Bogey & Bailley s 13-point dispersion relation preserving (DRP) scheme. The kinetic energy dissipation rate, computed both directly and from the enstrophy field, vorticity contours, and the energy spectra are examined. Results are in excellent agreement with a reference solution obtained using a spectral method and provide insight into computations of turbulent flows. In addition the following studies were performed: a comparison of 4th-, 8th-, 12th- and DRP spatial differencing schemes, the effect of the solution filtering on the results, the effect of large-eddy simulation sub-grid scale models, and the effect of high-order discretization of the viscous terms.
Document ID
20130011044
Acquisition Source
Glenn Research Center
Document Type
Technical Memorandum (TM)
Authors
DeBonis, James R.
(NASA Glenn Research Center Cleveland, OH, United States)
Date Acquired
August 27, 2013
Publication Date
February 1, 2013
Subject Category
Fluid Mechanics And Thermodynamics
Report/Patent Number
NASA/TM-2013-217850
E-18637
Report Number: NASA/TM-2013-217850
Report Number: E-18637
Meeting Information
Meeting: 51st Aerospace Sciences Meeting
Location: Grapevine, TX
Country: United States
Start Date: January 7, 2013
End Date: January 10, 2013
Sponsors: American Inst. of Aeronautics and Astronautics
Funding Number(s)
WBS: WBS 561581.02.08.03.48.01
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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