On the nature of fluctuations in turbulent Rayleigh-Benard convection at large Prandtl numbers

We report experimental results for the power spectra, variance, skewness and kurtosis of temperature fluctuations in turbulent Rayleigh-Benard convection (RBC) of a fluid with Prandtl number Pr = 12.3 in cylindrical samples with aspect ratios (diameter D over height L) of 0.50 and 1.00. The measurements were primarily for the radial positions xi = 1 - r/(D/2) = 1.00 and xi = 0.063. In both cases, data were obtained at several vertical locations z = L. For all locations, there is a frequency range of about a decade over which the spectra can be described well by the power law P(f) similar to f (alpha). For all xi and Gamma the alpha value is less than one near the top and bottom plates and increases as z/L or 1 - z/L increase from 0.01 to 0.5. This differs from the finding for Pr = 0.8 (He et al., Phys. Rev. Lett., vol. 112, 2014, 174501) and the expectation for the downstream velocity of turbulent wall-bounded shear flow (Rosenberg, J. Fluid Mech., vol. 731, 2013, pp. 46-63), where alpha = 1 is found or expected in an inner layer (0.01 less than or similar to z/L less than or similar to 0.1) near the wall but in the bulk. The variance is described better by a power law sigma(2) similar to (z/L)(-zeta) than by the logarithmic dependence found or expected for Pr = 0.8 and for turbulent shear flow. For both Gamma, we found that, independent of Rayleigh number, zeta similar or equal to 2/3 near the sidewall (xi = 0.063), where plumes primarily rise or fall and the large- scale circulation (LSC) dynamics is most influential. This result agrees with a model due to Priestley (Turbulent Transfer in the Lower Atmosphere, 1959, University of Chicago Press) for convection over a horizontal heated surface. However, we found zeta similar or equal to 1 along the sample centreline (xi = 1.00), where there are relatively few plumes moving vertically and the LSC dynamics is expected to be less important; that result is consistent with one of two possible interpretations by Adrian (Intl J. Heat Mass Transfer, vol. 39, 1996, pp. 2303- 2310) of a model due to Libchaber et al. (J. Fluid Mech., vol. 204, 1989, pp. 1- 30). We discuss the composite nature of fluctuations in turbulent RBC, with contributions from intrinsic background fluctuations, plumes, the stochastic dynamics of the LSC, and the sloshing and torsional mode of the LSC. None of the models advanced so far explicitly consider all of these contributions.