The "zeroth law" of turbulence: Isotropic turbulence simulations revisited
Bruce R. Pearson, Tarek A. Yousef, Nils Erland L. Haugen, Axel Brandenburg, Per A. Krogstad
Abstract
The dimensionless kinetic energy dissipation rate Cepsilon is estimated from numerical simulations of statistically stationary isotropic box turbulence that is slightly compressible. The Taylor microscale Reynolds number Relambda range is 20 < Relambda < 220 and the statistical stationarity is achieved with a random phase forcing method. The strong Relambda dependence of Cepsilon abates when Relambda approx. 100 after which Cepsilon slowly approaches approx 0.5 a value slightly different to previously reported simulations but in good agreement with experimental results. If Cepsilon is estimated at a specific time step from the time series of the quantities involved it is necessary to account for the time lag between energy injection and energy dissipation. Also, the resulting value can differ from the ensemble averaged value by up to +-30%. This may explain the spread in results from previously published estimates of Cepsilon.
Create a lesson
Related papers
Onset condition of the ramified-jet regime: an experimental and theoretical study
Bor Zupan, Jernej Kušar, Božidar Šarler
Fingering instability of thin films with an inclined contact line
Ze-Hui Gao, Er-Qiang Li, Peng Gao
A ghost-cell immersed boundary method for the shallow water equations on Cartesian grids: mass conservation and wetting and drying over variable topography
Yuta Yaegashi
Nonlocal generalization of the Chapman-Enskog method and hydrodynamic equations. Nonlocal vorticity transport in a turbulent medium
A. B. Kukushkin
Planar intrusions from a narrow, jet-like source in a linearly stratified ambient
Hai Duc Vu, Murray Rudman, Anja Slim
Wave-driven geostrophic vortices in rotating turbulence
Vladimir Parfenyev, Sergey Vergeles