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

被引:0
|
作者
Deshpande, Rahul [1 ]
Vinuesa, Ricardo [2 ]
Klewicki, Joseph [1 ]
Marusic, Ivan [1 ]
机构
[1] Univ Melbourne, Dept Mech Eng, Parkville, Vic 3010, Australia
[2] KTH Royal Inst Technol, FLOW, Eng Mech, S-10044 Stockholm, Sweden
基金
欧洲研究理事会;
关键词
turbulent boundary layers; boundary layer structure; AMPLITUDE-MODULATION; FLUCTUATIONS; SIMULATION; FLOWS; MODEL;
D O I
10.1017/jfm.2024.1218
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
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.
引用
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页数:19
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