Analysis of wall-pressure fluctuation sources from DNS of turbulent channel flow

Abstract

The sources of wall-pressure fluctuations in turbulent channel flow are studied using a novel framework. The wall-pressure power spectral density (PSD) (φpp(ω)) is expressed as an integrated contribution from all wall-parallel plane pairs, φpp(ω)=∫-δ+δ∫-δ+δ(r,s,ω)\,dr\,ds, using the Green's function. Here, (r,s,ω) is termed the net source cross spectral density (CSD) between two wall-parallel planes, y=r and y=s and δ is the half channel height. Direct Numerical Simulation (DNS) data at friction Reynolds number of 180 and 400 are used to compute (r,s,ω). Analysis of the net source CSD, (r,s,ω) reveals that the location of dominant sources responsible for the premultiplied peak in the power spectra at ω+≈ 0.35 and the wavenumber spectra at λ+≈ 200 is in the buffer layer at y+≈ 16.5 and 18.4 for Reτ=180 and 400, respectively. The contribution from a wall-parallel plane (located at distance y+ from the wall) to wall-pressure PSD is log-normal in y+ for ω+>0.35. A dominant inner-overlap region interaction of the sources is observed at low frequencies. Further, the decorrelated features of the wall-pressure fluctuation sources are analyzed using spectral Proper Orthogonal Decomposition (POD). We require the modes to be orthogonal in an inner product with a symmetric positive definite kernel. Spectral POD supports the case that the net source is composed of two decorrelated components - active (dominant mode) and inactive (remaining modes). The structure represented by the dominant POD mode at the premultiplied wall-pressure PSD peak inclines in the downstream direction. At the low-frequency linear PSD peak, the dominant mode resembles a large scale vertical pattern.

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