4.7 Article

Turbulent flow in the bulk of Rayleigh-Benard convection: small-scale properties in a cubic cell

Journal

JOURNAL OF FLUID MECHANICS
Volume 722, Issue -, Pages 596-617

Publisher

CAMBRIDGE UNIV PRESS
DOI: 10.1017/jfm.2013.74

Keywords

Benard convection; isotropic turbulence; turbulent convection

Funding

  1. Hong Kong Research Grants Council (RGC) [CUHK 404409]
  2. RGC Direct Grant [2060441]
  3. NSFC/RGC Joint Research Scheme [N_CUHK462/11]
  4. EU Science and Technology Fellowship Programme China
  5. Research Grant Council
  6. University Grant Committee of the HKSAR
  7. Hong Kong Baptist University
  8. Leibnitz Rechenzentrum Munich

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The Rayleigh number (Ra) scaling of the global Bolgiano length scale L-B,L-global and the local Bolgiano length scale L-B,L-centre in the centre region of turbulent Rayleigh-Benard convection are investigated for Prandtl numbers Pr = 0.7 and 4.38 and 3 x 10(5) <= Ra <= 3 x 10(9). It is found that L-B,L-centre does not necessarily exhibit the same scaling as L-B,L-global. While L-B,L-global is monotonically deceasing as L-B,L-global similar to Ra-0.10 for both Pr, L-B,L-centre shows a steep increase beyond a certain Ra value. The complex scaling of the local Bolgiano length scale in the centre is a result of the different behaviour of the temperature-variance dissipation rate, epsilon(T), and the turbulent-kinetic-energy dissipation rate, epsilon(u). This shows that for sufficiently high Ra the flow is well-mixed and hence temperature is passively advected. It is also observed that the Ra-range in which L-B,L-centre exhibits the same scaling as the global Bolgiano length scale is increasing with increasing Pr. It is further observed that for Pr = 4.38 and Ra <= 3 x 10(7) the local vertical heat flux in the centre region is balanced by the turbulent-kinetic-energy dissipation rate. For higher Ra we find that the local heat flux is decreasing. At Pr = 0.7 we do not observe such a balance, as the measured heat flux is between the heat fluxes estimated through the turbulent-kinetic-energy dissipation rate and the temperature-variance dissipation rate. We therefore suggest that the balance of the local heat flux might be Prandtl-number dependent. The conditional average of the local vertical heat flux < Nu vertical bar epsilon(u,) epsilon(T)>(centre) in the core region of the flow reveals that the highest vertical heat flux occurs for rare events with very high dissipation rates, while the joint most probable dissipation rates are associated with very low values of vertical heat flux. It is also observed that high values of epsilon(u) and epsilon(T) tend to occur together. It is further observed that the longitudinal velocity structure functions approach Kolmogorov K41 scaling. The temperature structure functions appear to approach Bolgiano-Obukhov BO59 scaling for r > L-B,L-centre, while a scaling exponent smaller than the BO59 scaling is observed for separations r < L-B,L-centre. The mixed velocity and temperature structure function for Ra = 1 x 10(9) and Pr = 4.38 shows a short 4/5-scaling for r > L-B,L-centre. Our results suggest that BO59 scaling might be more clearly observable at higher Prandtl and moderate Rayleigh numbers.

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