Second-mode Waves in Hypersonic Transition: Energy Balance, Kinematics and Mechanics
Speaker: Carlo Scalo, Program Manager, Defense Sciences Office, DARPA
Presentation
Seminar Slide Deck (PDF-8.1MB)
Abstract
This seminar presents recent advances in the understanding of the fundamental structure of second-mode waves in hypersonic transition published by Roy & Scalo, J. Fluid Mech. (2025-2026). Reference flow conditions are taken from a Mach 6 boundary layer over a 3◦ cone at zero angle of attack, with varying degrees of wall-to-adiabatic temperature ratios, ranging from strongly cooled, Tw/Tad = 0.25, to highly heated, Tw/Tad =1.75.
It was found that second-mode instabilities comprise two decks, separated by the pressure node location, i.e., the point of zero pressure fluctuation, y=y_π. The upper deck (y > y_π) is characterised by temperature and density fluctuations sustaining the bulk of the second-mode energy production, peaking between the critical layer, y=y_c, and the generalised inflection point, y=y_i. The nature of the wave at this location is NOT acoustic, but rather akin to a vortical roll-up of density gradients, ultimately visible in Schlieren imaging as the famous rope waves.
Slightly below the inflection point, a downward-oriented energy flux develops, sustaining acoustic energy accumulation in the lower deck, i.e., y < y_π, ultimately leading to the fluctuating pressure footprint of second-mode waves that is measured by experimental techniques such as wall-mounted PCBs or pressure sensitive paints (PSP). Colder walls (Tw/Tad << 1) enhance the temperature gradient in the second-mode energy production term, strengthening the flux from the upper to the lower deck. Ray tracing also reveals that colder walls, entailing stronger base flow velocity gradients, are more effective at kinematically trapping acoustic wave paths emanating from the wall, hence enabling eigenmode growth.
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