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Space-time correlation and two-time, two point closure An important concept on turbulence is that small-scale eddies are progressively decorrelated in time. This decorrelation progress can be characterized by two-time, two-point correlations of fluctuating velocities, or simply, space-time correlations. Over the years, several space-time correlation models have been developed to provide the necessary time scales for turbulence closure theory and used as the staple methods to analyze spatial and temporal data from experiments and numerical simulations, such as Taylor frozen-flow model and Kraichnan random sweeping model. We are developing the space-time correlation models for turbulent flows in both Eulerian and Lagrangian frames. 1. X. Zhao and
G.W. He, Space-time correlations of fluctuating velocities in turbulent
shear flows, Phys. Rev. E 79 (4): 046316 (2009).
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Time-accurate large-eddy simulation (LES) The increasing applications of LES to compute sound sources and particle-laden turbulence require that LES with a sub-grid scale (SGS) model could accurately predict space-time correlations. Most of currently existing SGS models are based on energy-budget equations. Therefore, they are able to correctly predict energy spectra at large scales, but they may in-correctly predict space-time correlations. We are investigating the effects of SGS models on space-time correlations and developing time-accurate SGS models. 1.
G.W. He, R. Rubinstein and L.P. Wang, Effects of subgrid-scale modeling
on time correlations in large eddy simulation, Phys. Fluids 14: 2186 -
2193 (2002).
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AI and turbulence modeling 1. Zhang Fengshun, Zhou
Zhideng, Yang Xiaolei, He Guowei. Knowledge-integrated additive
learning for consistent near-wall modelling of turbulent flows. JFM
Rapids, 2025, 1011: R1. |