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NASA NTRS · 19840035193

The computation of rotational conical flows

Abstract

A method based on the Clebsch velocity decomposition is presented to solve the steady, inviscid, supersonic flow field about arbitrary conical geometries. The system of equations developed, although formally equivalent to the Euler equations, retains the computational efficiency of type-dependent potential flow solutions. Accurate rotational-flow solutions are developed using shock-fitting procedures at the bow and imbedded waves along with special treatment of the vortical layer. Solutions are presented for several high Mach number conical flows and compared with existing Euler solutions and experimental data.

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BibTeXRIS

Grossman, B., Choi, S. K.. 1984-01-01. The computation of rotational conical flows. https://ntrs.nasa.gov/citations/19840035193

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