Theory of turbulence augmentation across hypersonic shock waves

ORAL

Abstract

The interaction between a weakly turbulent free stream and a hypersonic shock wave is investigated theoretically by using linear interaction analysis (LIA). Modified Rankine-Hugoniot jump conditions that account for dissociation and vibrational excitation are derived and employed in a Fourier analysis of a hypersonic shock interacting with three-dimensional isotropic vortical disturbances. Besides confirming known endothermic effects of hypersonic thermochemistry in decreasing the mean post-shock temperature and velocity, these LIA results indicate that the enstrophy, anisotropy, intensity, and turbulent kinetic energy of the fluctuations are much more amplified through the shock than in the calorically perfect case. Additionally, the turbulent Reynolds number is amplified across the shock at hypersonic Mach numbers in the presence of dissociation and vibrational excitation, as opposed to the attenuation observed in the calorically perfect case. These results suggest that turbulence may persist and get augmented across hypersonic shock waves despite the high post-shock temperatures.

*C.H. was funded by a 2019 Leonardo Grant for Researchers and Cultural Creators awarded by the BBVA Foundation, and by the MICINN Grant no. PID2019-108592RB-C41. J.U. acknowledges funding from the Hypersonic Aerothermodynamics portfolio of the U.S. Air Force Office of Scientific Research (AFOSR), Grant no. FA9550-16-1-0319, and by the U.S. Department of Energy's National Nuclear Security Administration (NNSA) via the Stanford PSAAP-III Center, Grant no.DE-NA0003968

Presenters

  • Alberto Cuadra Lara

    • Univ Carlos III de Madrid

Authors

  • Alberto Cuadra Lara

    • Univ Carlos III de Madrid
  • Cesar Huete

    • Univ Carlos III De Madrid
    • Univ Carlos III de Madrid
  • Marcos Vera

    • Universidad Carlos III de Madrid
    • Univ Carlos III de Madrid
  • Javier Urzay

    • Center for Turbulence Research, Stanford University, USA
    • Center for Turbulence Research, Stanford University
    • Stanford Univ