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:

图 1. EQUATION_DISPLAY
∂∂t(ρk)+∇⋅[ρk(v¯−vg)]=∇⋅[(μ+σkμt)∇k]+Pk−γ′ρβ*fβ*(ωk−ω0k0)+Sk
(1576)
图 2. EQUATION_DISPLAY
∂∂t(ρω)+∇⋅(ρωv¯)=∇⋅[((μ+σωμt)∇ω]+Pω−γ′ρβfβ(ω2−ω02)+Sω
(1577)

where the production term Pk is defined as:

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

and:

图 4. EQUATION_DISPLAY
γ′={0,1,γtrans<0.9γtrans≥0.9
(1579)

where:

图 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:

图 6. EQUATION_DISPLAY
Gklim⁡=5max⁡(γ−0.2,0)(1−γ)Fonlim⁡max⁡(3μ−μt,0)SW
(1581)

where:

图 7. EQUATION_DISPLAY
Fonlim⁡=min⁡(max⁡(Reν2.2⋅1100−1,0),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)