Search NASAโŒ• Search

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.

Keep this discovery

Explore connections, maps & timelines

BibTeXRIS

Amano, R. S.. 1986-11-01. Comparison of pressure-strain correlation models for the flow behind a disk. https://ntrs.nasa.gov/citations/19870033623

Cite the original work for its findings. Save a collection to share your selection of sources.