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NASA NTRS · 19890037864

3D computational analyses for SSME internal flows

Abstract

Two qualities of the turbulent flow of hot gases in liquid fueled rocket engines that affect the selection and performance of turbulence models used in computational fluid analyses of the flow are curvature of the flow passages and rotation of the flow. Three configurations which represent these conditions and for which experimental data are available are subjected to three dimensional computational analyses using both the standard k - epsilon and a multiple-time-scale turbulence models. It is found that the multiple-time-scale model is better able to predict overall flow features, especially where regions of separated flow are present.

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BibTeXRIS

Chen, C. P., Schafer, Charles F.. 1989-01-01. 3D computational analyses for SSME internal flows. https://ntrs.nasa.gov/citations/19890037864

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