Bulletin of the American Physical Society
71st Annual Meeting of the APS Division of Fluid Dynamics
Volume 63, Number 13
Sunday–Tuesday, November 18–20, 2018; Atlanta, Georgia
Session F29: Turbulent and Planetary Boundary Layers
8:00 AM–10:10 AM,
Monday, November 19, 2018
Georgia World Congress Center
Room: B401
Chair: William Anderson, University of Texas, Dallas
Abstract ID: BAPS.2018.DFD.F29.6
Abstract: F29.00006 : Relation between pressure and spanwise velocity fluctuations in turbulent channel flows
9:05 AM–9:18 AM
Presenter:
Ali Mehrez
(Nagoya Univ)
Authors:
Ali Mehrez
(Nagoya Univ)
Yoshinobu Yamamoto
(Yamanashi Univ)
Yoshiyuki Tsuji
(Nagoya Univ)
We study the logarithmic behavior of the mean-square pressure fluctuations ⟨p+2⟩ in fully developed turbulent channel flows. Data of direct numerical simulation of channel flow is used in the present research for Reynolds number flows up to Reτ=4000 . The profile of ⟨p+2⟩ is found to follow a logarithmic behavior at some distances from the wall which is similar to that of the mean-square spanwise velocity fluctuations ⟨w+2⟩ at the same Reynolds number. The results are also emphasized for the higher-order moments of p and w where the logarithmic behavior is confirmed. Spectral analysis in the streamwise and spanwise directions indicate that the ridge of the spectra of p and w are overlapping each other within the regions where ⟨p+2⟩ and ⟨w2⟩ show the log-trends. In addition, within these regions, the shape of the two-dimensional spectra of p and w collapse with each other, and the contours of the spectra at a constant level are bounded by a linear relationship between the streamwise and spanwise length scales This linear relation indicates that p and w may be associated with geometrically shaped self-similar eddies. The shape of these self-similar eddies is investigated, and the scaling of their sizes with the distance from the wall are discussed.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DFD.F29.6
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