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NASA NTRS · 19860015192

Nonisentropic unsteady three dimensional small disturbance potential theory

Abstract

Modifications that allow for more accurate modeling of flow fields when strong shocks are present were made into three dimensional transonic small disturbance (TSD) potential theory. The Engquist-Osher type-dependent differencing was incorporated into the solution algorithm. The modified theory was implemented in the XTRAN3S computer code. Steady flows over a rectangular wing with a constant NACA 0012 airfoil section and an aspect ratio of 12 were calculated for freestream Mach numbers (M) of 0.82, 0.84, and 0.86. The obtained results are compared using the modified and unmodified TSD theories and the results from a three dimensional Euler code are presented. Nonunique solutions in three dimensions are shown to appear for the rectangular wing as aspect ratio increases. Steady and unsteady results are shown for the RAE tailplane model at M = 0.90. Calculations using unmodified theory, modified theory and experimental data are compared.

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BibTeXRIS

Gibbons, M. D., Whitlow, W., Jr., Williams, M. H.. 1986-04-01. Nonisentropic unsteady three dimensional small disturbance potential theory. https://ntrs.nasa.gov/citations/19860015192

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