NASA NTRS · 19850039711
Spectral methods for the Euler equations. II - Chebyshev methods and shock fitting
Abstract
The Chebyshev spectral collocation method for the Euler gasdynamic equations is described. It is used with shock fitting to compute several two-dimensional gasdynamic flows. Examples include a shock/acoustic wave interaction, a shock/vortex interaction, and the classical blunt-body problem. With shock fitting, the spectral method has a clear advantage over second-order finite differences in that equivalent accuracy can be obtained with far fewer grid points.
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Hussaini, M. Y., Kopriva, D. A., Salas, M. D., Zang, T. A.. 1985-02-01. Spectral methods for the Euler equations. II - Chebyshev methods and shock fitting. https://ntrs.nasa.gov/citations/19850039711
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