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Internal energy balance and aerodynamic heating predictions for hypersonic turbulent boundary layers

Matthew Barone*

Gary L. Nicholson and Lian Duan

  • Aerosciences Department, Sandia National Laboratories, Albuquerque, New Mexico 87185, USA

  • Department of Mechanical and Aerospace Engineering, Ohio State University, Columbus, Ohio 43210, USA

  • *mbarone@sandia.gov

Phys. Rev. Fluids 7, 084604 – Published 19 August, 2022

DOI: https://doi.org/10.1103/PhysRevFluids.7.084604

Abstract

The elemental equation governing heat transfer in aerodynamic flows is the internal energy equation. For a boundary layer flow, a double integration of the Reynolds-averaged form of this equation provides an expression of the wall heat flux in terms of the integrated effects, over the boundary layer, of various physical processes: turbulent dissipation, mean dissipation, turbulent heat flux, etc. Recently available direct numerical simulation data for a Mach 11 cold-wall turbulent boundary layer allows a comparison of the exact contributions of these terms in the energy equation to the wall heat flux with their counterparts modeled in the Reynolds-averaged Navier-Stokes (RANS) framework. Various approximations involved in RANS, both closure models as well as approximations involved in adapting incompressible RANS models to a compressible form, are assessed through examination of the internal energy balance. There are a number of potentially problematic assumptions and terms identified through this analysis. The effect of compressibility corrections of the dilatational dissipation type is explored, as is the role of the modeled turbulent dissipation, in the context of wall heat flux predictions. The results indicate several potential avenues for RANS model improvement for hypersonic cold-wall boundary-layer flows.

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