Abstract

Direct numerical simulations of turbulent boundary layers with a nominal free-stream Mach number of $6$ and a Reynolds number of $Re_{\unicode[STIX]{x1D70F}}\approx 450$ are conducted at a wall-to-recovery temperature ratio of $T_{w}/T_{r}=0.25$ and compared with a previous database for $T_{w}/T_{r}=0.76$ in order to investigate pressure fluctuations and their dependence on wall temperature. The wall-temperature dependence of widely used velocity and temperature scaling laws for high-speed turbulent boundary layers is consistent with previous studies. The near-wall pressure-fluctuation intensities are dramatically modified by wall-temperature conditions. At different wall temperatures, the variation of pressure-fluctuation intensities as a function of wall-normal distance is dramatically modified in the near-wall region but remains almost intact away from the wall. Wall cooling also has a strong effect on the frequency spectrum of wall-pressure fluctuations, resulting in a higher dominant frequency and a sharper spectrum peak with a faster roll-off at both the high- and low-frequency ends. The effect of wall cooling on the free-stream noise spectrum can be largely accounted for by the associated changes in boundary-layer velocity and length scales. The pressure structures within the boundary layer and in the free stream evolve less rapidly as the wall temperature decreases, resulting in an increase in the decorrelation length of coherent pressure structures for the colder-wall case. The pressure structures propagate with similar speeds for both wall temperatures. Due to wall cooling, the generated pressure disturbances undergo less refraction before they are radiated to the free stream, resulting in a slightly steeper radiation wave front in the free stream. Acoustic sources are largely concentrated in the near-wall region; wall cooling most significantly influences the nonlinear (slow) component of the acoustic source term by enhancing dilatational fluctuations in the viscous sublayer while damping vortical fluctuations in the buffer and log layers.

Highlights

  • An understanding of the physics of pressure fluctuations induced by high-speed turbulent boundary layers is important to the structural design of hypersonic vehicles and to the testing and evaluation of hypersonic vehicles in noisy hypersonic facilities

  • The objective of the current paper is to investigate the dependence of boundarylayer-induced pressure fluctuations on wall temperature for hypersonic Mach numbers

  • Direct numerical simulations of Mach 5.86 turbulent boundary layers with two wall temperatures (Tw/Tr = 0.25, 0.76) are compared to investigate the effect of wall cooling on the pressure fluctuations generated by hypersonic turbulent boundary layers

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Summary

Introduction

An understanding of the physics of pressure fluctuations induced by high-speed turbulent boundary layers is important to the structural design of hypersonic vehicles and to the testing and evaluation of hypersonic vehicles in noisy hypersonic facilities. Duan et al (2010) performed direct numerical simulations (DNS) of turbulent boundary layers at Mach 5 over a broad range of wall-to-recovery temperature ratios (Tw/Tr = 0.18–1.0) and focused on assessing the validity of Morkonvin’s hypothesis in the high-Mach-number cold-wall regime. To the best of the knowledge of the authors, no existing studies have been conducted in the high-Mach-number cold-wall regime that provide the off-wall fluctuating pressure field including the free-stream acoustic pressure fluctuations. In a previous paper by the present authors (Duan et al 2016), the successful application of DNS in capturing the global fluctuating pressure field has been demonstrated for a spatially developing flat-plate nominally Mach 6 turbulent boundary layer with a wall-to-recovery temperature ratio of Tw/Tr = 0.76.

Simulation details
Assessment of DNS data
Boundary-layer-induced pressure fluctuations
Root mean square of pressure fluctuations
Frequency spectra of pressure fluctuations
10–1 M6Tw025 M6Tw076
Spatial correlation of pressure fluctuations
Propagation and evolution of pressure structures
Free-stream acoustic radiation
Findings
Summary and conclusions

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