4.7 Article

Direct numerical simulation of hypersonic turbulent boundary layers: effect of spatial evolution and Reynolds number

Journal

JOURNAL OF FLUID MECHANICS
Volume 937, Issue -, Pages -

Publisher

CAMBRIDGE UNIV PRESS
DOI: 10.1017/jfm.2022.80

Keywords

compressible boundary layers; hypersonic flow; turbulent boundary layers

Funding

  1. Office of Naval Research [N00014-20-1-2194]
  2. National Science Foundation [CBET 2001127]
  3. NASA Hypersonic Technology Project
  4. DOE Office of Science User Facility [DE-AC02-06CH11357]

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This study investigates the spatial evolution of flat-plate zero-pressure-gradient turbulent boundary layers over long streamwise domains at high Mach numbers and cold-wall conditions using direct numerical simulations. The study monitors the settlement of turbulence statistics into a fully developed equilibrium state and characterizes the streamwise evolution of various important variables.
Direct numerical simulations (DNS) are performed to investigate the spatial evolution of flat-plate zero-pressure-gradient turbulent boundary layers over long streamwise domains (>300 delta(i), with delta(i) the inflow boundary-layer thickness) at three different Mach numbers, 2.5, 4.9 and 10.9, with the surface temperatures ranging from quasiadiabatic to highly cooled conditions. The settlement of turbulence statistics into a fully developed equilibrium state of the turbulent boundary layer has been carefully monitored, either based on the satisfaction of the von Karman integral equation or by comparing runs with different inflow turbulence generation techniques. The generated DNS database is used to characterize the streamwise evolution of multiple important variables in the high-Mach-number, cold-wall regime, including the skin friction, the Reynolds analogy factor, the shape factor, the Reynolds stresses, and the fluctuating wall quantities. The data confirm the validity of many classic and newer compressibility transformations at moderately high Reynolds numbers (up to friction Reynolds number Re-tau approximate to 1200) and show that, with proper scaling, the sizes of the near-wall streaks and superstructures are insensitive to the Mach number and wall cooling conditions. The strong wall cooling in the hypersonic cold-wall case is found to cause a significant increase in the size of the near-wall turbulence eddies (relative to the boundary-layer thickness), which leads to a reduced-scale separation between the large and small turbulence scales, and in turn to a lack of an outer peak in the spanwise spectra of the streamwise velocity in the logarithmic region.

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