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NASA NTRS · 19920014110

High-Order Polynomial Expansions (HOPE) for flux-vector splitting

Abstract

The Van Leer flux splitting is known to produce excessive numerical dissipation for Navier-Stokes calculations. Researchers attempt to remedy this deficiency by introducing a higher order polynomial expansion (HOPE) for the mass flux. In addition to Van Leer's splitting, a term is introduced so that the mass diffusion error vanishes at M = 0. Several splittings for pressure are proposed and examined. The effectiveness of the HOPE scheme is illustrated for 1-D hypersonic conical viscous flow and 2-D supersonic shock-wave boundary layer interactions.

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BibTeXRIS

Liou, Meng-Sing, Steffen, Chris J., Jr.. 1991-10-01. High-Order Polynomial Expansions (HOPE) for flux-vector splitting. https://ntrs.nasa.gov/citations/19920014110

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