NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Dilatation-dissipation corrections for advanced turbulence modelsThis paper analyzes dilatation-dissipation based compressibility corrections for advanced turbulence models. Numerical computations verify that the dilatation-dissipation corrections devised by Sarkar and Zeman greatly improve both the k-omega and k-epsilon model predicted effect of Mach number on spreading rate. However, computations with the k-gamma model also show that the Sarkar/Zeman terms cause an undesired reduction in skin friction for the compressible flat-plate boundary layer. A perturbation solution for the compressible wall layer shows that the Sarkar and Zeman terms reduce the effective von Karman constant in the law of the wall. This is the source of the inaccurate k-gamma model skin-friction predictions for the flat-plate boundary layer. The perturbation solution also shows that the k-epsilon model has an inherent flaw for compressible boundary layers that is not compensated for by the dilatation-dissipation corrections. A compressibility modification for k-gamma and k-epsilon models is proposed that is similar to those of Sarkar and Zeman. The new compressibility term permits accurate predictions for the compressible mixing layer, flat-plate boundary layer, and a shock separated flow with the same values for all closure coefficients.
Document ID
19930030547
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Wilcox, David C.
(DCW Industries, Inc. La Canada, CA, United States)
Date Acquired
August 15, 2013
Publication Date
November 1, 1992
Publication Information
Publication: AIAA Journal
Volume: 30
Issue: 11
ISSN: 0001-1452
Subject Category
Fluid Mechanics And Heat Transfer
Accession Number
93A14544
Funding Number(s)
CONTRACT_GRANT: DAAL03-89-C-0032
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available