Coupling with Turbulence Models

The intermittency solved by the Gamma ReTheta transition model and the Gamma transition model is used to scale the turbulence equation of the SST (Menter) K-Omega model and the Spalart-Allmaras model.

Coupling with SST (Menter) K-Omega Model

The Gamma ReTheta transition model and the Gamma transition model enter the transport equation for the turbulent kinetic energy k and the specific dissipation rate ω (see SST (Menter) K-Omega Model) as follows:

1. EQUATION_DISPLAY
t(ρk)+∇⋅[ρk(v¯vg)]=∇⋅[(μ+σkμt)k]+Pkγρβ*fβ*(ωkω0k0)+Sk
(1576)
2. EQUATION_DISPLAY
t(ρω)+∇⋅(ρωv¯)=∇⋅[((μ+σωμt)ω]+Pωγρβfβ(ω2ω02)+Sω
(1577)

where the production term Pk is defined as:

3. EQUATION_DISPLAY
Pk=γtrans(Gk+Gnl+Gb)+Gklim
(1578)

and:

4. EQUATION_DISPLAY
γ={0,1,γtrans<0.9γtrans0.9
(1579)

where:

5. EQUATION_DISPLAY
γtrans={γefffor the Gamma ReTheta transition modelγfor the Gamma transition model
(1580)

γeff and γ are provided by the Gamma ReTheta Transition Model and Gamma Transition Model), respectively.

γtrans and γ are unity if no transition model is activated.

The Gamma transition model introduces an additional production term Gklim to ensure proper generation of k at transition points for low values of free-stream turbulence:

6. EQUATION_DISPLAY
Gklim=5max(γ0.2,0)(1γ)Fonlimmax(3μμt,0)SW
(1581)

where:

7. EQUATION_DISPLAY
Fonlim=min(max(Reν2.211001,0),3)
(1582)

and:

  • S and W are modulus of the mean strain rate tensor and the modulus of the mean vorticity tensor. See Eqn. (1129) and Eqn. (1131), respectively.
  • Reν is the strain-rate Reynolds number given by Eqn. (1139).

The additional production term is set to zero if the Gamma transition model is not activated.

Coupling with Spalart-Allmaras Model

The SA Gamma transition model enters the transport equation for the modified diffusivity ν˜ (see Spalart-Allmaras Model) as follows:

t(ρν˜)+∇⋅(ρν˜v¯)=1σν˜∇⋅[(μ+ρν˜)ν˜]+γPν˜max(γ,0.1)Dν˜+Sν˜
(1583)