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Experimental Investigation of Longitudinal Space-Time Correlations of the Velocity Field in Turbulent Rayleigh-Bénard Convection

We report an experimental investigation of the longitudinal space-time cross-correlation function of the velocity field, $C(r,τ)$, in a cylindrical turbulent Rayleigh-Bénard convection cell using the particle image velocimetry (PIV) technique. We show that while the Taylor's frozen-flow hypothesis does not hold in turbulent thermal convection, the recent elliptic model advanced for turbulent shear flows [He & Zhang, \emph{Phys. Rev. E} \textbf{73}, 055303(R) (2006)] is valid for the present velocity field for all over the cell, i.e., the isocorrelation contours of the measured $C(r,τ)$ have a shape of elliptical curves and hence $C(r,τ)$ can be related to $C(r_E,0)$ via $r_E^2=(r-βτ)^2+γ^2τ^2$ with $β$ and $γ$ being two characteristic velocities. We further show that the fitted $β$ is proportional to the mean velocity of the flow, but the values of $γ$ are larger than the theoretical predictions. Specifically, we focus on two representative regions in the cell: the region near the cell sidewall and the cell's central region. It is found that $β$ and $γ$ are approximately the same near the sidewall, while $β\simeq0$ at cell center.

preprint2011arXivOpen access

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