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NASA NTRS ยท 19840052563

Flux-vector splitting for the Euler equations

Abstract

Flux-vector splitting is shown to be the simplest way of implementing upwind differencing for the full or isenthalpic Euler equations combined with the ideal-gas law. The scheme presented produces steady shock profiles with two interior zones. A disadvantage in using flux-vector splitting is that it leads to numerical diffusion of a contact discontinuity at rest. This diffusion, however, can be removed, and present research is aimed at achieving this with minimal computational effort.

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BibTeXRIS

Van Leer, B.. 1982-01-01. Flux-vector splitting for the Euler equations. https://ntrs.nasa.gov/citations/19840052563

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