NASA NTRS ยท 19870033623
Comparison of pressure-strain correlation models for the flow behind a disk
Abstract
Attention is given to the behavior of Reynolds stresses in the separated wake region behind a disk that is attached in a normal fashion to a long cylinder of small diameter. Computations of the turbulent flow were made in a region beyond a disk by using the second-order closure model of turbulence. It is found that the models of Naot et al. (1970) and Launder et al. (1975) yield similar results and are reliable; the energy distribution may nevertheless be improved for the case of reattaching shear flows by taking the effects of mean strain into account.
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Amano, R. S.. 1986-11-01. Comparison of pressure-strain correlation models for the flow behind a disk. https://ntrs.nasa.gov/citations/19870033623
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