An improved method for performing measurements of turbulent quantities and spectra in hypersonic wind tunnel flows, using a miniature pitot probe, is presented. The results of an extensive investigation of velocity fluctuation spectra, performed in the weakly compressible, decaying turbulent field established in the test section of a small scale hypersonic (Mach 6) wind-tunnel, at low enthalpy conditions, are also presented. A discussion of the fundamental assumptions is provided, together with experimental and theoretical considerations of applicability and limits of the proposed method. The measured one-dimensional spectra exhibits a non-Kolmogorov power-law behaviour over a significant wavenumber range, with a –11/3 exponent which is not predicted by available scaling relations for compressible turbulence. On the other hand, such power-law exponent is in agreement with EDQNM and LES results for the irrotational component of velocity fluctuations in weakly compressible flows [1,2]. Based on these results, a new dimensionally-based scaling relation is obtained for the compressible energy spectrum, which is in agreement with the numerically observed radiative behaviour for weakly compressible turbulence.

Compressibility Effects in Weakly Turbulent Hypersonic Flow Fields

D'AGOSTINO, LUCA
2001-01-01

Abstract

An improved method for performing measurements of turbulent quantities and spectra in hypersonic wind tunnel flows, using a miniature pitot probe, is presented. The results of an extensive investigation of velocity fluctuation spectra, performed in the weakly compressible, decaying turbulent field established in the test section of a small scale hypersonic (Mach 6) wind-tunnel, at low enthalpy conditions, are also presented. A discussion of the fundamental assumptions is provided, together with experimental and theoretical considerations of applicability and limits of the proposed method. The measured one-dimensional spectra exhibits a non-Kolmogorov power-law behaviour over a significant wavenumber range, with a –11/3 exponent which is not predicted by available scaling relations for compressible turbulence. On the other hand, such power-law exponent is in agreement with EDQNM and LES results for the irrotational component of velocity fluctuations in weakly compressible flows [1,2]. Based on these results, a new dimensionally-based scaling relation is obtained for the compressible energy spectrum, which is in agreement with the numerically observed radiative behaviour for weakly compressible turbulence.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11568/178997
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