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Numerical Simulation of the Entire Transition Path Caused by an Oblique Breakdown at Mach 3

Numerical Simulation of the Entire Transition Path Caused by an Oblique Breakdown at Mach 3
Chair:

AIAA Fluid Mechanics Conference
AIAA Paper 2008-4398

Place:Seattle, WA
Date:2008
Author:

Mayer,C.S.J.
Von Terzi,D.A.
Fasel,H.F.

Abstract

A pair of oblique waves at low amplitudes is introduced in a supersonic flat-plate boundary layer. Its downstream development and the concomitant process of laminar to turbulent transition is then investigated numerically using Direct Numerical Simulations (DNS). Data and analysis exist from the early linear stages to breakdown to turbulence.
In the present paper, first the linear regime is studied in great detail. Comparisons to linear stability theory clearly determine that the so-called “oblique breakdown” mechanism is initiated.
The focus of the second part is the nonlinear regime. It is shown how the spectrum is filled up, what kind of flow structures arise and how these structures locally break down to small scales.
Finally, a logarithmic region of the mean streamwise velocity profile is formed indicating the begin of a fully turbulent flow region. The simulations demonstrate that oblique breakdown is a viable path to turbulence.