Effect of Prandtl number on heat transport enhancement in Rayleigh-Benard convection under geometrical confinement

被引:58
作者
Chong, Kai Leong [1 ]
Wagner, Sebastian [2 ]
Kaczorowski, Matthias [1 ]
Shishkina, Olga [2 ]
Xia, Ke-Qing [1 ]
机构
[1] Chinese Univ Hong Kong, Dept Phys, Shatin, Hong Kong, Peoples R China
[2] Max Planck Inst Dynam & Self Org, Fassberg 17, D-37077 Gottingen, Germany
来源
PHYSICAL REVIEW FLUIDS | 2018年 / 3卷 / 01期
关键词
TURBULENT THERMAL-CONVECTION; ASPECT-RATIO DEPENDENCE; SMALL-SCALE PROPERTIES; UNIFYING THEORY; BOUNDARY-LAYER; ROUGH SURFACES; FLOW; PLATES; CELLS; BULK;
D O I
10.1103/PhysRevFluids.3.013501
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
We study, using direct numerical simulations, the effect of geometrical confinement on heat transport and flow structure in Rayleigh-Benard convection in fluids with different Prandtl numbers. Our simulations span over two decades of Prandtl number Pr, 0.1 <= Pr <= 40, with the Rayleigh number Ra fixed at 10(8). The width-to-height aspect ratio Gamma spans between 0.025 and 0.25, while the length-to-height aspect ratio is fixed at one. We first find that for Pr >= 0.5, geometrical confinement can lead to a significant enhancement in heat transport as characterized by the Nusselt number Nu. For those cases, Nu is maximal at a certain Gamma = Gamma(opt) and the maximal relative enhancement generally increases with Pr over the explored parameter range. As opposed to the situation of Pr >= 0.5, confinement-induced enhancement in Nu is not realized for smaller values of Pr, such as 0.1 and 0.2. The Pr dependence of the heat transport enhancement can be understood in its relation to the coverage area of the thermal plumes over the thermal boundary layer (BL) where larger coverage is observed for larger Pr due to a smaller thermal diffusivity. We further show that Gamma(opt) is closely related to the crossing of thermal and momentum BLs and find thatNu declines sharply when the thickness ratio of the thermal and momentum BLs exceeds a certain value of about one. In addition, through examining the temporally averaged flow fields and two-dimensional mode decomposition, it is found that for smaller Pr the large-scale circulation is robust against the geometrical confinement of the convection cell. We further found that Gamma(opt) exhibits a power-law relation with Pr as Gamma(opt) = 0.11 Pr-0.060 +/- 0.004. Together with the result Gamma(opt) = 29.37 Ra-0.31 found by Chong et al. [Phys. Rev. Lett. 115, 264503 (2015)], our findings provide a more complete picture of the geometrical confinement.
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页数:17
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共 57 条
[1]   Effect of a Polymer Additive on Heat Transport in Turbulent Rayleigh-Benard Convection [J].
Ahlers, Guenter ;
Nikolaenko, Alexei .
PHYSICAL REVIEW LETTERS, 2010, 104 (03)
[2]   Heat transfer and large scale dynamics in turbulent Rayleigh-Benard convection [J].
Ahlers, Guenter ;
Grossmann, Siegfried ;
Lohse, Detlef .
REVIEWS OF MODERN PHYSICS, 2009, 81 (02) :503-537
[3]   Aspect ratio dependence of heat transfer and large-scale flow in turbulent convection [J].
Bailon-Cuba, J. ;
Emran, M. S. ;
Schumacher, J. .
JOURNAL OF FLUID MECHANICS, 2010, 655 :152-173
[4]   Low-dimensional model of turbulent mixed convection in a complex domain [J].
Bailon-Cuba, Jorge ;
Shishkina, Olga ;
Wagner, Claus ;
Schumacher, Joerg .
PHYSICS OF FLUIDS, 2012, 24 (10)
[5]   TEMPERATURE AND VELOCITY BOUNDARY-LAYERS IN TURBULENT CONVECTION [J].
BELMONTE, A ;
TILGNER, A ;
LIBCHABER, A .
PHYSICAL REVIEW E, 1994, 50 (01) :269-279
[6]   Heat transport by laminar boundary layer flow with polymers [J].
Benzi, Roberto ;
Ching, Emily S. C. ;
Chu, Vivien W. S. .
JOURNAL OF FLUID MECHANICS, 2012, 696 :330-344
[7]   Effect of Polymer Additives on Heat Transport in Turbulent Thermal Convection [J].
Benzi, Roberto ;
Ching, Emily S. C. ;
De Angelis, Elisabetta .
PHYSICAL REVIEW LETTERS, 2010, 104 (02)
[8]   Reorientation of the large-scale circulation in turbulent Rayleigh-Benard convection [J].
Brown, E ;
Nikolaenko, A ;
Ahlers, G .
PHYSICAL REVIEW LETTERS, 2005, 95 (08)
[9]   DIFFERENTIAL ROTATION IN STELLAR CONVECTION ZONES [J].
BUSSE, FH .
ASTROPHYSICAL JOURNAL, 1970, 159 (02) :629-&
[10]   Dynamics and symmetries of flow reversals in turbulent convection [J].
Chandra, Mani ;
Verma, Mahendra K. .
PHYSICAL REVIEW E, 2011, 83 (06)