Stochastic self-energy subgrid model for the large eddy simulation of turbulent channel flows

被引:3
作者
Kitsios, V. [1 ,2 ]
Sillero, J. A. [3 ]
Soria, J. [1 ,4 ]
Frederiksen, J. S. [2 ]
机构
[1] Monash Univ, Dept Mech & Aerosp Engn, Lab Turbulence Res Aerosp & Combust, Clayton, Vic 3800, Australia
[2] CSIRO Marine & Atmospher Res, Ctr Australian Weather & Climate Res, Aspendale, Vic 3195, Australia
[3] Univ Politecn Madrid, Sch Aeronaut, E-28040 Madrid, Spain
[4] King Abdulaziz Univ, Dept Aeronaut Engn, Jeddah, Saudi Arabia
来源
1ST MULTIFLOW SUMMER WORKSHOP | 2014年 / 506卷
基金
欧洲研究理事会; 澳大利亚研究理事会;
关键词
SCALE PARAMETERIZATIONS; ISOTROPIC TURBULENCE; VISCOSITY; BACKSCATTER; CLOSURE; ELIMINATION; LAWS;
D O I
10.1088/1742-6596/506/1/012001
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
This paper presents the large eddy simulation (LES) of turbulent channel flow using a self-energy (SE) subgrid model with coefficients determined from reference direct numerical simulations (DNSs). In contrast to standard approaches that develop subgrid models based upon physical hypotheses, in the present SE approach the model coefficients are determined from the subgrid statistics of a DNS, with physical interpretations made apostiori. This technique is applied here for the first time to wall-bounded flows, specifically channel flow. The stochastic SE subgrid model consists of a meanfield shift, deterministic drain dissipation acting on the resolved field and a stochastic backscatter force. The deterministic SE subgrid model comprises of a net dissipation representing the net effect of the drain and backscatter. We present LESs that reproduce the time-averaged kinetic energy spectra of the DNS within the resolved scales. The direction and magnitude of the energy transfers in scale space can then be determined from the coefficients of the SE subgrid model. Results are presented for friction velocity based Reynolds numbers up to Re-r = 950.
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页数:15
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