Simulation and stability analysis of oblique shock-wave/boundary-layer interactions at Mach 5.92

Nathaniel Hildebrand, Anubhav Dwivedi, Joseph W. Nichols, Mihailo R. Jovanović, Graham V. Candler

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We investigate flow instability created by an oblique shock wave impinging on a Mach 5.92 laminar boundary layer at a transitional Reynolds number. The adverse pressure gradient of the oblique shock causes the boundary layer to separate from the wall, resulting in the formation of a recirculation bubble. For sufficiently large oblique shock angles, the recirculation bubble is unstable to three-dimensional perturbations and the flow bifurcates from its original laminar state. We utilize direct numerical simulation (DNS) and global stability analysis to show that this first occurs at a critical shock angle of θ=12.9. At bifurcation, the least-stable global mode is nonoscillatory and it takes place at a spanwise wave number β=0.25, in good agreement with DNS results. Examination of the critical global mode reveals that it originates from an interaction between small spanwise corrugations at the base of the incident shock, streamwise vortices inside the recirculation bubble, and spanwise modulation of the bubble strength. The global mode drives the formation of long streamwise streaks downstream of the bubble. While the streaks may be amplified by either the lift-up effect or by Görtler instability, we show that centrifugal instability plays no role in the upstream self-sustaining mechanism of the global mode. We employ an adjoint solver to corroborate our physical interpretation by showing that the critical global mode is most sensitive to base flow modifications that are entirely contained inside the recirculation bubble.

Original languageEnglish (US)
Article number013906
JournalPhysical Review Fluids
Issue number1
StatePublished - Jan 2018

Bibliographical note

Funding Information:
We are grateful to the Office of Naval Research for their support of this study through Grant No. N00014-15-1-2522.

Publisher Copyright:
© 2018 American Physical Society.


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