Active and inactive contributions to the wall pressure and wall-shear stress in turbulent boundary layers

A phenomenological description is presented to explain the intermediate and low-frequency/large-scale contributions to the wall-shear-stress ( ${\tau }_w$ ) and wall-pressure ( $\,{p}_w$ ) spectra of canonical turbulent boundary layers, both of which are well known to increase with Reynolds number, albeit in a distinct manner. The explanation is based on the concept of active and inactive motions (Townsend, J. Fluid Mech. , vol. 11, issue 1, 1961, pp. 97–120) associated with the attached-eddy hypothesis. Unique data sets of simultaneously acquired ${\tau }_w$ , ${p}_w$ and velocity-fluctuation time series in the log region are considered, across a friction-Reynolds-number ( $Re_{\tau }$ ) range of $ {O}(10^3) \lesssim Re_{\tau } \lesssim {O}(10^6)$ . A recently proposed energy-decomposition methodology (Deshpande et al. , J. Fluid Mech. , vol. 914, 2021, A5) is implemented to reveal the active and inactive contributions to the ${\tau }_w$ - and $p_w$ -spectra. Empirical evidence is provided in support of Bradshaw's ( J. Fluid Mech. , vol. 30, issue 2, 1967, pp. 241–258) hypothesis that the inactive motions are responsible for the non-local wall-ward transport of the large-scale inertia-dominated energy, which is produced in the log region by active motions. This explains the large-scale signatures in the ${\tau }_w$ -spectrum, which grow with $Re_{\tau }$ despite the statistically weak signature of large-scale turbulence production, in the near-wall region. For wall pressure, active and inactive motions respectively contribute to the intermediate and large scales of the $p_w$ -spectrum. Both these contributions are found to increase with increasing $Re_{\tau }$ owing to the broadening and energization of the wall-scaled (attached) eddy hierarchy. This potentially explains the rapid $Re_{\tau }$ -growth of the $p_w$ -spectra relative to ${\tau }_w$ , given the dependence of the latter only on the inactive contributions.

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Publication Details

Journal
Journal of Fluid Mechanics
Published
2025-01-16
DOI
https://doi.org/10.1017/jfm.2024.1218
Citations
5
Primary Topic
Fluid Dynamics and Turbulent Flows
Type
article
Field-Weighted Citation Impact
6.67

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article

Active and inactive contributions to the wall pressure and wall-shear stress in turbulent boundary layers

Joseph Klewicki, Ricardo Vinuesa, Rahul Deshpande, Ivan Marušič
5 citations
Journal of Fluid Mechanics
Fluid Dynamics and Turbulent Flows
6.67
article

Active and inactive contributions to the wall pressure and wall-shear stress in turbulent boundary layers

Joseph Klewicki, Ricardo Vinuesa, Rahul Deshpande, Ivan Marušič
article en
5 citations

Abstract

A phenomenological description is presented to explain the intermediate and low-frequency/large-scale contributions to the wall-shear-stress ( ${\tau }_w$ ) and wall-pressure ( $\,{p}_w$ ) spectra of canonical turbulent boundary layers, both of which are well known to increase with Reynolds number, albeit in a distinct manner. The explanation is based on the concept of active and inactive motions (Townsend, J. Fluid Mech. , vol. 11, issue 1, 1961, pp. 97–120) associated with the attached-eddy hypothesis. Unique data sets of simultaneously acquired ${\tau }_w$ , ${p}_w$ and velocity-fluctuation time series in the log region are considered, across a friction-Reynolds-number ( $Re_{\tau }$ ) range of $ {O}(10^3) \lesssim Re_{\tau } \lesssim {O}(10^6)$ . A recently proposed energy-decomposition methodology (Deshpande et al. , J. Fluid Mech. , vol. 914, 2021, A5) is implemented to reveal the active and inactive contributions to the ${\tau }_w$ - and $p_w$ -spectra. Empirical evidence is provided in support of Bradshaw's ( J. Fluid Mech. , vol. 30, issue 2, 1967, pp. 241–258) hypothesis that the inactive motions are responsible for the non-local wall-ward transport of the large-scale inertia-dominated energy, which is produced in the log region by active motions. This explains the large-scale signatures in the ${\tau }_w$ -spectrum, which grow with $Re_{\tau }$ despite the statistically weak signature of large-scale turbulence production, in the near-wall region. For wall pressure, active and inactive motions respectively contribute to the intermediate and large scales of the $p_w$ -spectrum. Both these contributions are found to increase with increasing $Re_{\tau }$ owing to the broadening and energization of the wall-scaled (attached) eddy hierarchy. This potentially explains the rapid $Re_{\tau }$ -growth of the $p_w$ -spectra relative to ${\tau }_w$ , given the dependence of the latter only on the inactive contributions.

Journal of Fluid MechanicsVol. 1003
The University of Melbourne (AU), KTH Royal Institute of Technology (SE)
European Commission, Australian Research Council, Office of Naval Research, Office of Naval Research Global
Openalex Percentile: Top 4%
Fluid Dynamics and Turbulent Flows
6.67
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