Similarities between characteristics of convective turbulence in confined and extended domains

被引:6
|
作者
Pandey, Ambrish [1 ]
Krasnov, Dmitry [2 ]
Schumacher, Joerg [2 ,3 ]
Samtaney, Ravi [4 ]
Sreenivasan, Katepalli R. [1 ,3 ,5 ,6 ]
机构
[1] New York Univ Abu Dhabi, Ctr Space Sci, Abu Dhabi 129188, U Arab Emirates
[2] Tech Univ Ilmenau, Inst Thermodynam & Fluid Mech, D-98684 Ilmenau, Germany
[3] NYU, Tandon Sch Engn, New York, NY 11201 USA
[4] King Abdullah Univ Sci & Technol, Div Phys Sci & Engn, Thuwal 239556900, Saudi Arabia
[5] NYU, Dept Phys, New York, NY 11201 USA
[6] NYU, Courant Inst Math Sci, New York, NY 11201 USA
基金
英国工程与自然科学研究理事会;
关键词
High Rayleigh number convection; Convection at variable Prandtl numbers; Aspect ratio dependence; RAYLEIGH-BENARD CONVECTION; HEAT-TRANSFER; PRANDTL-NUMBER; FLOW;
D O I
10.1016/j.physd.2022.133537
中图分类号
O29 [应用数学];
学科分类号
070104 ;
摘要
To understand turbulent convection at very high Rayleigh numbers typical of natural phenomena, computational studies in slender cells are an option if the needed resources have to be optimized within available limits. However, the accompanying horizontal confinement affects some properties of the flow. Here, we explore the characteristics of turbulent fluctuations in the velocity and temperature fields in a cylindrical convection cell of aspect ratio 0.1 by varying the Prandtl number Pr between 0.1 and 200 at a fixed Rayleigh number Ra = 3 x 1010, and find that the fluctuations weaken with increasing Pr, quantitatively as in aspect ratio 25. The probability density function (PDF) of temperature fluctuations in the bulk region of the slender cell remains mostly Gaussian, but increasing departures occur as Pr increases beyond unity. We assess the intermittency of the velocity field by computing the PDFs of velocity derivatives and of the kinetic energy dissipation rate, and find increasing intermittency as Pr decreases. In the bulk region of convection, a common result applicable to the slender cell, large aspect ratio cells, as well as in 2D convection, is that the turbulent Prandtl number decreases as Pr-1/3.
引用
收藏
页数:11
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