NASA NTRS · 19910058094
Stable boundary conditions for Cartesian grid calculations
Abstract
The inviscid Euler equations in complicated geometries are solved using a Cartesian grid. This requires solid wall boundary conditions in the irregular grid cells near the boundary. Since these cells may be orders of magnitude smaller than the regular grid cells, stability is a primary concern. An approach to this problem is presented and its use is illustrated.
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Berger, M. J., Leveque, R. J.. 1990-01-01. Stable boundary conditions for Cartesian grid calculations. https://ntrs.nasa.gov/citations/19910058094
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