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NASA NTRS · 19950021496

A numerical method for solving the three-dimensional parabolized Navier-Stokes equations

Abstract

A numerical technique that solves the parabolized form of the Navier-Stokes equations is presented. Such a method makes it possible to obtain very detailed descriptions of the flowfield in a relatively modest CPU time. The present approach is based on a space-marching technique, uses a finite volume discretization and an upwind flux-difference splitting scheme for the evaluation of the inviscid fluxes. Second order accuracy is achieved following the guidelines of the the ENO schemes. The methodology is used to investigate three-dimensional supersonic viscous flows over symmetric corners. Primary and secondary streamwise vortical structures embedded in the boundary layer and originated by the interaction with shock waves are detected and studied. For purpose of validation, results are compared with experimental data extracted from literature. The agreement is found to be satisfactory. In conclusion, the numerical method proposed seems to be promising as it permits, at a reasonable computational expense, investigation of complex three-dimensional flowfields in great detail.

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BibTeXRIS

Dambrosio, Domenic, Marsilio, Robert. 1995-05-01. A numerical method for solving the three-dimensional parabolized Navier-Stokes equations. https://ntrs.nasa.gov/citations/19950021496

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