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Turbulent thermal convection over rough plates with varying roughness geometries

Published online by Cambridge University Press:  21 July 2017

Yi-Chao Xie
Affiliation:
Department of Physics, The Chinese University of Hong Kong, Shatin, Hong Kong, China
Ke-Qing Xia*
Affiliation:
Department of Physics, The Chinese University of Hong Kong, Shatin, Hong Kong, China
*
†Email address for correspondence: kxia@cuhk.edu.hk

Abstract

We present a systematic investigation of the effects of roughness geometry on turbulent Rayleigh–Bénard convection (RBC) over rough plates with pyramid-shaped and periodically distributed roughness elements. Using a parameter $\unicode[STIX]{x1D706}$ defined as the height of a roughness element over its base width, the heat transport, the flow dynamics and the local temperatures are measured for the Rayleigh number range $7.50\times 10^{7}\leqslant Ra\leqslant 1.31\times 10^{11}$ and Prandtl numbers $Pr$ from 3.57 to 23.34 at four values of $\unicode[STIX]{x1D706}$ (0.5, 1.0, 1.9 and 4.0). It is found that the heat transport scaling, i.e. $Nu\sim Ra^{\unicode[STIX]{x1D6FC}}$ where $Nu$ is the Nusselt number, may be classified into three regimes in turbulent RBC over rough plates. In Regime I, the system is in a dynamically smooth state. The heat transport scaling is the same as that in a smooth cell. In Regimes II and III, the heat transport is enhanced. When $\unicode[STIX]{x1D706}$ is increased from 0.5 to 4.0, $\unicode[STIX]{x1D6FC}$ increases from 0.36 to 0.59 in Regime II and it increases from 0.30 to 0.50 in Regime III. The experiment thus clearly demonstrates that the heat transport scaling in turbulent RBC can be manipulated using $\unicode[STIX]{x1D706}$ in the heat transport enhanced regime. Previous studies suggest that the transition to heat transport enhanced regime, i.e. from Regime I to Regime II, occurs when the thermal boundary layer (BL) thickness becomes smaller than the roughness height. Direct measurements of the viscous BL in the present study suggest that the transition from Regime II to Regime III is likely a result of the viscous BL thickness becoming smaller than the roughness height. The scaling exponent of the Reynolds number $Re$ with respect to $Ra$ changes from 0.471 to 0.551 when $\unicode[STIX]{x1D706}$ is increased from 0.5 to 4.0, suggesting a change of the dynamics of the large-scale circulation. Interestingly, the transition from Regime II to Regime III in terms of the heat transport scaling is not reflected in the $Re$ scaling with $Ra$ . It is also found that increasing $\unicode[STIX]{x1D706}$ increases the clustering of thermal plumes which effectively increases the plume lifetime. This leads to a great increase in the probability of observing large temperature fluctuations in the bulk flow, which corresponds to the formation of more coherent plumes or plume clusters that are ultimately responsible for the enhanced heat transport.

Information

Type
Papers
Copyright
© 2017 Cambridge University Press 
Figure 0

Figure 1.Photos of the bottom plate of a rough cell with $\unicode[STIX]{x1D706}=1.0$. (a) Top view; (b) side view. The red heater connection wires can be seen at the top of (a). Plates with $\unicode[STIX]{x1D706}$ values of 0.5, 1.9 and 4.0 have the same design.

Figure 1

Figure 2.$Ra$–$Pr$ phase space explored for different values of $\unicode[STIX]{x1D706}$. The case for $\unicode[STIX]{x1D706}=0.5$ is only studied for $Pr=23.34$. All experiments were conducted in convection cells with roughness height $h=8$ mm, except for the ones corresponding to hexagons that were conducted in convection cell with $h=4~\text{mm}$.

Figure 2

Figure 3.(a) $Nu$ as a function of $Ra$ in a rough cell with a roughness elements height of 4 mm. The down-pointing triangles are taken from Funfschilling et al. (2005) ($\unicode[STIX]{x1D6E4}=1.0,Pr=4.38$), the hexagons are taken from Sun et al. (2005) ($\unicode[STIX]{x1D6E4}=2.0,Pr=4.34$), the stars are taken from Wei et al. (2014) ($\unicode[STIX]{x1D6E4}=1.0,Pr=4.34$). (b) The compensated plot of the same data as in (a).

Figure 3

Figure 4.(a,d,g,j) $Nu$ as a function of $Ra$ in rough cells for (a) $\unicode[STIX]{x1D706}=4.0$; (d) $\unicode[STIX]{x1D706}=1.9$; (g) $\unicode[STIX]{x1D706}=1.0$ and ($j$) $\unicode[STIX]{x1D706}=0.5$. The down-pointing triangles are from Funfschilling et al. (2005) ($\unicode[STIX]{x1D6E4}=1.0,Pr=4.38$), the hexagons are from Sun et al. (2005) ($\unicode[STIX]{x1D6E4}=2.0,Pr=4.34$) and the stars are from Wei et al. (2014) ($\unicode[STIX]{x1D6E4}=1.0,Pr=4.38$). Data at $Pr=4.34$ in $(j)$ are from Wei et al. (2014); $Nu$ at $Pr=23.34$ at $\unicode[STIX]{x1D706}=4.0$ and 1.9 are larger than those at $Pr=3.57$ at the same $Ra$. For a better comparison, they are shifted downwards respectively by 1.5 and 1.34 and displayed using squares with a cross. The solid lines are power-law fits to the data larger and smaller than $Ra^{\ast }\sim 4\times 10^{9}$. (b,c,e,f,h,i,k,l) The compensated plots of $Nu$ with the fitted $Ra$ scaling for $Ra$ larger and smaller than $Ra\sim 4\times 10^{9}$ from (a,d,g,j).

Figure 4

Table 1.Measured scaling law of the Nusselt number $Nu$ and normalised temperature fluctuations $\unicode[STIX]{x1D70E}_{T}/\unicode[STIX]{x0394}T$ in Regime III for different values of $\unicode[STIX]{x1D706}$.

Figure 5

Figure 5.The scaling exponent $\unicode[STIX]{x1D6FC}$ from power-law fits to $Nu$ versus $Ra$, i.e. $Nu\sim Ra^{\unicode[STIX]{x1D6FC}}$, in Regime II (circles) and Regime III (triangles) as a function of $\unicode[STIX]{x1D706}$. Also plotted in the figure is the scaling exponent $\unicode[STIX]{x1D6FD}$ from power-law fits to $Re$ versus $Ra$ (squares), i.e. $Re\sim Ra^{\unicode[STIX]{x1D6FD}}$, as a function of $\unicode[STIX]{x1D706}$. The solids lines are empirical power-law fits to the respective data sets: $\unicode[STIX]{x1D6FC}_{II}=0.43\unicode[STIX]{x1D706}^{0.24\pm 0.02}$, $\unicode[STIX]{x1D6FC}_{III}=0.37\unicode[STIX]{x1D706}^{0.23\pm 0.02}$ and $\unicode[STIX]{x1D6FD}=0.49\unicode[STIX]{x1D706}^{0.08\pm 0.01}$.

Figure 6

Figure 6.The heat transport enhancements in Regime II (open symbols) and Regime III (solid symbols) as a function of $\unicode[STIX]{x1D706}$.

Figure 7

Figure 7.The instantaneous (a) and time-averaged (b) velocity fields measured near the bottom plate within the large-scale circulation plane ($Ra=4.22\times 10^{9}$, $Pr=4.34$ and $\unicode[STIX]{x1D706}=1.0$). The velocity magnitude (in units of $\text{mm}~\text{s}^{-1}$) is colour coded with the colour bar nearby each figure and is also represented by the length of the vectors. The velocity field is not accessible experimentally below the dashed lines.

Figure 8

Figure 8.(a) Typical time-averaged horizontal velocity $U$ and root-mean-square horizontal velocity $\unicode[STIX]{x1D70E}_{u}$ profiles ($Ra=4.22\times 10^{9}$, $\unicode[STIX]{x1D706}=1.0$ and $Pr=4.34$). The vertical dashed line indicates the location of the viscous boundary layer. (b) Normalised viscous boundary layer thickness $\unicode[STIX]{x1D6FF}_{v}/H$ versus $Ra$. The dashed line marks the height of the roughness elements. The datum at the highest $Ra$ (symbols with cross, $\unicode[STIX]{x0394}T=29.83~\text{K}$) shows different behaviours with other data points which we believe is an artefact due to the strong optical distortion of the images used for PIV analysis.

Figure 9

Figure 9.$Nu$ as a function of $Re$ measured in rough cells with different values of $\unicode[STIX]{x1D706}$ at (a) $Pr=23.34$ (b) $Pr=6.14$ (c) $Pr=4.34$ and (d) $Pr=3.57$.

Figure 10

Figure 10.Autocorrelation function of the temperature measured ${\sim}1$ cm away from side wall in a rough cell with $\unicode[STIX]{x1D706}=4.0$ at $Ra=1.01\times 10^{11}$ and $Pr=23.34$. Here $T_{f}$ is the turnover time of the LSC.

Figure 11

Figure 11.Reynolds number $Re$ as a function of $Ra$ and $Pr$ in rough cells for (a) $\unicode[STIX]{x1D706}=4.0$, (c) $\unicode[STIX]{x1D706}=1.9$, (e) $\unicode[STIX]{x1D706}=1.0$ and (g) $\unicode[STIX]{x1D706}=0.5$. To determine more precisely the scaling exponent of $Re$ with respect to $Ra$, data measured at $Pr=3.53,4.34$ and $6.14$ in (a,c,e,g) are multiplied by a $Pr$-dependent constant $f(Pr)$ to collapse with data at $Pr=23.34$. The shifted data are shown in the main plot in the right panels (b,d,f,g) with power-law fit $Re\,f(Pr)\sim Ra^{\unicode[STIX]{x1D6FD}}$ shown as solid lines. The insets in (b,d,f,g) show the compensated plot $ReRa^{-\unicode[STIX]{x1D6FD}}$ with respect to $Pr$ with the solid lines representing power-law fits to the data. See table 1 for the fitted power laws.

Figure 12

Figure 12.Reynolds number $Re$ as a function of $RaNu$ for different values of $\unicode[STIX]{x1D706}$ with the solid line representing a power-law fit to the data irrespective of $\unicode[STIX]{x1D706}$. (a) $Pr=23.34$ and $Re=0.076\times (RaNu)^{0.36\pm 0.01}$; (b) $Pr=6.14$ and $0.266\times (RaNu)^{0.35\pm 0.01}$; (c) $Pr=4.34$ and $0.281\times (RaNu)^{0.36\pm 0.01}$; (d) $Pr=3.57$ and $Re=0.340\times (RaNu)^{0.36\pm 0.01}$.

Figure 13

Figure 13.Probability density functions (PDFs) of the standardised temperature measured (a) at the cell centre and (b) near the side wall for different values of $\unicode[STIX]{x1D706}$ ($Ra=2.1\times 10^{10}$ and $Pr=23.34$). The r.m.s. temperatures as a function of $\unicode[STIX]{x1D706}$ at the cell centre and side wall are plotted in (c) and (d), respectively.

Figure 14

Figure 14.$\unicode[STIX]{x1D706}$-dependence of the normalised r.m.s. temperature as a function of $Ra$ at (a) the cell centre and (b) the side wall. The solid lines are power-law fits to the individual data set with the scaling exponents displayed nearby each data set. The data are measured at $Pr=23.34$.

Figure 15

Figure 15.Probability density function of the temperature deviation from the mean $T-\langle T\rangle$ normalised by the applied temperature between the top and bottom plate $\unicode[STIX]{x0394}T$ at (a) the cell centre and (b) the side wall ($Ra=2.1\times 10^{10}$, $Pr=23.34$).

Figure 16

Figure 16.Shadowgraph images of the instantaneous flow fields in a rough cell with (a) $\unicode[STIX]{x1D706}=0.0$, (b) $\unicode[STIX]{x1D706}=1.0$ and (c) $\unicode[STIX]{x1D706}=4.0$. The images were taken at $Ra=1.22\times 10^{11}$ and $Pr=23.34$.

Figure 17

Figure 17.(a) The time-averaged plume amplitude $\langle A\rangle$ normalised by $\unicode[STIX]{x0394}T$ and (b) the time-averaged plume width $\langle w\rangle$ normalised by the large-scale circulation turnover time $T_{f}$ as a function of $Ra$ extracted from the temperature time series measured at the side wall at $Pr=23.34$. The solid lines are power-law fits to individual data sets with the scaling exponents displayed nearby each data set.

Figure 18

Figure 18.(a) $Nu$ as a function of $Ra$ and $Pr$ at fixed $\unicode[STIX]{x1D706}=4.0$ measured in rough cells with roughness height $h$ of 4 mm and 8 mm. The down-pointing triangles are from Funfschilling et al. (2005) and the hexagons are from Sun et al. (2005) for smooth cells. The solid lines are power-law fits to the respective data set. The power-law fitting in cell with $h=8$ mm is extrapolated to $Ra=2\times 10^{11}$. (b) Compensated plot of the same data as in (a).

Figure 19

Figure 19.$Re$ as a function of $Ra$ in rough cells with $h=8~\text{mm}$ (solid symbols) and 4 mm (open symbols) at $Pr=4.34$ (triangles) and 23.34 (squares), respectively. In both cells $\unicode[STIX]{x1D706}=4.0$. The solid lines are power-law fits to each data set. For $Pr=4.34$, $Re=0.028R^{0.56}$ ($h=8~\text{mm}$) $Re=0.014R^{0.58}$ ($h=4~\text{mm}$); and for $Pr=23.34$$Re=0.013R^{0.55}$ ($h=8~\text{mm}$) $Re=0.0035R^{0.59}$ ($h=4~\text{mm}$).