NASA NTRS · 19900012428
Three-dimensional simulation of vortex breakdown
Abstract
The integral form of the complete, unsteady, compressible, three-dimensional Navier-Stokes equations in the conservation form, cast in generalized coordinate system, are solved, numerically, to simulate the vortex breakdown phenomenon. The inviscid fluxes are discretized using Roe's upwind-biased flux-difference splitting scheme and the viscous fluxes are discretized using central differencing. Time integration is performed using a backward Euler ADI (alternating direction implicit) scheme. A full approximation multigrid is used to accelerate the convergence to steady state.
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Kuruvila, G., Salas, M. D.. 1990-06-01. Three-dimensional simulation of vortex breakdown. https://ntrs.nasa.gov/citations/19900012428
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