Intermittency Transport Equation

The transport equation for the intermittency γ is formulated as:

Figure 1. EQUATION_DISPLAY
ddt(ργ)+∇⋅ργv¯=∇⋅[(μ+μtσf)γ]+PγEγ
(1500)

where:

Production Term

The transition production term is defined as:

Figure 2. EQUATION_DISPLAY
Pγ=FlengthC  a1ρS[γFonset]1/2(1-Ce1γ)
(1501)

where Fonset is a trigger function that describes the initiation of intermittency for the different modes of transition:

Figure 3. EQUATION_DISPLAY
Fonset=max(Fonset2-Fonset3,0)
(1502)

with:

Figure 4. EQUATION_DISPLAY
Fonset2=min[max((Fonset14,Fonset1),2)]
(1503)
Figure 5. EQUATION_DISPLAY
Fonset3=max[1-(Ret/2.5)3,0]
(1504)
Figure 6. EQUATION_DISPLAY
Fonset1=ReνConset1Reθc
(1505)

and:

Destruction Term

The destruction/relaminarization term is defined as:

Figure 7. EQUATION_DISPLAY
Eγ=Ca2ρWγFturb(Ce2γ-1)
(1506)

where:

Fturb=exp[-(Ret4)4]
(1507)

and:

Separation-Induced Transition Modification

The modification for separation-induced transition is:

Figure 8. EQUATION_DISPLAY
γsep=min[s1max(0,Reν3.235Reθc-1)Freattach,2]Fθt
(1508)

where:

F r e a t t a c h = exp [ ( Re t 20 ) 4 ]
(1509)

where Ret is given by Eqn. (1136).

Effective Intermittency

The effective intermittency that enters the turbulence transport equations is defined as:

Figure 9. EQUATION_DISPLAY
γeff=max(γ,γsep)
(1510)

For details on how γeff enters the turbulence transport equations, see Coupling with SST (Menter) K-Omega Model.

Model Coefficients

σf Ce1 Ca1 Ce2 Ca2 Conset1 s1
1 1 2 50 0.06 2.193 2