On the wavenumber-frequency spectra of wall pressure fluctuations in turbulent channel flows
Bowen Yang, Guowei He, Zixuan Yang

TL;DR
This study uses DNS to analyze wall pressure spectra in turbulent channel flows, revealing a valley-like feature and quantifying errors from common assumptions, especially in three-dimensional spectra across various Reynolds numbers.
Contribution
It provides the first quantitative evaluation of neglecting the cross spectral density between rapid and slow pressure components in wall pressure spectra.
Findings
Valley-like behavior in total pressure spectra contours.
Neglecting CSD introduces significant errors in 3D spectra.
Large errors (up to 5dB) occur in the sub-convective region across Reynolds numbers.
Abstract
The characteristics of the wavenumber-frequency spectra of the rapid, slow and total wall pressure fluctuations are investigated using direct numerical simulation (DNS) of turbulent channel flow up to . For the wavenumber-frequency spectra of the total wall pressure fluctuations, a valley-like behavior of contour lines in the sub-convective region is found, which may be linked to the Kraichnan-Phillips theorem. For the decomposition of the wall pressure spectra, it is commonly assumed in previous studies that the cross spectral density (CSD) between the rapid and slow components of the wall pressure fluctuations can be neglected. Yet no experimental or numerical evidence is available for either confirming or disproving this assumption. In this paper, we use DNS data to quantitatively evaluate this assumption. Emphasizes are put on the error in decibel scale caused…
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Taxonomy
TopicsFluid Dynamics and Turbulent Flows · Aerodynamics and Acoustics in Jet Flows · Heat Transfer Mechanisms
