Towards the ultimate regime in Rayleigh-Darcy convection

被引:25
|
作者
Pirozzoli, Sergio [1 ]
De Paoli, Marco [2 ]
Zonta, Francesco [2 ]
Soldati, Alfredo [2 ,3 ]
机构
[1] Sapienza Univ Roma, Dipartimento Ingn Meccan & Aerospaziale, I-00184 Rome, Italy
[2] TU Wien, Inst Fluid Mech & Heat Transfer, A-1060 Vienna, Austria
[3] Univ Udine, Polytech Dept, I-33100 Udine, Italy
关键词
convection in porous media; plumes/thermals; COLUMNAR CONVECTION; NUMBER CONVECTION; POROUS-MEDIA; FLUID; STABILITY; PART;
D O I
10.1017/jfm.2020.1178
中图分类号
O3 [力学];
学科分类号
08 ; 0801 ;
摘要
Numerical simulations are used to probe Rayleigh-Darcy convection in fluid-saturated porous media towards the ultimate regime. The present three-dimensional dataset, up to Rayleigh-Darcy number Ra = 8 x 10(4), suggests that the appropriate scaling of the Nusselt number is Nu = 0.0081Ra + 0.067Ra(0.61), fitting the computed data for Ra greater than or similar to 10(3). Extrapolation of current predictions to the ultimate linear regime yields the asymptotic law Nu = 0.0081Ra, about 16% less than indicated in previous studies. Upon examination of the flow structures near the boundaries, we confirm previous indications of small flow cells hierarchically nesting into supercells, and we show evidence that the supercells at the boundary are the footprints of the megaplumes that dominate the interior part of the flow. The present findings pave the way for more accurate modelling of geophysical systems, with special reference to geological CO2 sequestration.
引用
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页数:13
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