Turbulent Transition Models
All of the previously described models are incapable of predicting boundary layer transition. To include the effects of transition additional equations are necessary.
Transitional flows can be found in many industrial application cases including gas turbine blades, airplane wings and wind turbines. It is known that conventional turbulence models over predict the wall shear stress for transitional flows. Thus, transition models can be used to improve the accuracy of CFD solutions when flows encounter turbulent transition of the boundary layer.
γ-Reθ Model
Langtry and Menter (2009) proposed one of the most commonly used transition models in industrial CFD applications. The γ−Reθ model is a correlation based intermittency model that predicts natural, bypass and separation induced transition mechanisms.
The γ−Reθ model is coupled with the Shear Stress Transport (SST) turbulence model and requires two additional transport equations for the turbulence intermittency (γ) and transition momentum thickness Reynolds number (Reθ). The turbulence intermittency is a measure of the flow regime and is defined as γ=tturbulenttlaminar+tturbulent where tturbulent represents the time that the flow is turbulent at a given location, while tlaminar represents the time that the flow is laminar.
For example, while the intermittency value is zero, the flow is considered to be laminar. A value of one is for fully turbulent flow. The transition momentum thickness Reynolds number is responsible for capturing the non local effects of turbulence intensity and is defined as Reθ=ρˉu θμ where the momentum thickness is θ=δ∫0uˉu(1−uˉu)dy.
To couple with the SST model, Langtry and Menter (2009) modified the production term and dissipation term of the turbulent kinetic energy to account for the changes in the flow intermittency.
Transport Equations
Production Modeling
- Production Pk=μtS2
- Strain rate magnitude S=√2SijSij
- Strain rate tensor Sij=12(∂¯ui∂xj+∂¯uj∂xi)
- Constant β*
- Blending function for specifying constants α=α1F1+α2(1−F1)
- α1=59 for the inner layer
- α2 = 0.44 for the outer layer.
Turbulent Intermittency γ
where Fonset=max{min(max[Reν2.193 Reθ0,(Reν2.193 Reθ0)4],2)−max(1−(RT2.5)3,0)} Reν=Sd2ν, RT=kνω
Transition Momentum Thickness Reynolds Number Reθ
where Fθ=min(max[Fwakee−(dδ)4, 1−(γ−1/Ce21−1/Ce2)2],1), Fwake=e−(Reω1E+5)2, Reω=ωd2ν, δ=50ΩdˉuδBL, δBL=7.5θBL, θBL=¯Reθνˉu
Dissipation Modeling
where Fturbulent=e(−RT4)4
Modeling of Turbulent Viscosity μt
- The second blending function F2=tanh(max(2√kβ*ω d, 500νd2ω))2,
- Fluid kinematic viscosity ν,
- Constant β*.
Correlations
where λθ=θ2νdˉuds is the pressure gradient.
Model Coefficients
β* = 0.09.
The following constants for SST are computed by a blending function ϕ=ϕ1F1+ϕ2(1−F1): σω1 = 0.5, σω2 = 0.856, σk1 = 0.85, σk2 = 1.00, β1=340, β2 = 0.0828. Ce1 = 1.0, Ce2 = 50, Ca1 = 2.0, Ca2 = 0.06, Cθ1 = 1.0, Cθ2 = 2.0, σf = 1.0.