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4.6.2 Transport Equations for the $k$- $kl$- $\omega$ Model

The $k$- $kl$- $\omega$ model is considered to be a three-equation eddy-viscosity type, which includes transport equations for turbulent kinetic energy ( $k_T$), laminar kinetic energy ( $k_L$), and the inverse turbulent time scale ( $\omega$)


 \frac{Dk_T}{Dt} = P_{K_T}+R+R_{NAT}-\omega k_T - D_T + \frac... ...a_T}{\alpha_k}\right) \frac{\partial k_T}{\partial x_j}\right] (4.6-1)


 \frac{Dk_L}{Dt} = P_{K_L}-R-R_{NAT}-D_L + \frac{\partial}{\partial x_j}\left[ \nu \frac{\partial k_L}{\partial x_j}\right] (4.6-2)


 \frac{D_{\omega}}{D_t} = C_{\omega 1} \frac{\omega}{k_T}P_{k... ..._{\omega}}\right) \frac{\partial \omega}{\partial x_j} \right] (4.6-3)

The inclusion of the turbulent and laminar fluctuations on the mean flow and energy equations via the eddy viscosity and total thermal diffusivity is as follows:


 \overline{-u_i u_j} = \nu_{TOT}\left(\frac{\partial U_i}{\p... ...artial U_j}{\partial x_i}\right)-\frac{2}{3}k_{TOT}\delta_{ij} (4.6-4)


 \overline{-u_i \theta}=\alpha_{\theta,TOT}\frac{\partial \theta}{\partial x_i} (4.6-5)

The effective length is defined as


 \lambda_{eff}=MIN(C_{\lambda} d,\lambda_T) (4.6-6)

where $\lambda_T$ is the turbulent length scale and is defined by


 \lambda_T = \frac{\sqrt{k}}{\omega} (4.6-7)

and the small scale energy is defined by

 k_{T,s}=f_{ss}f_W k_T (4.6-8)


 f_W = \frac{\lambda_{eff}}{\lambda_T} (4.6-9)


 f_{ss} = exp\left[ -\left(\frac{C_{ss}\nu \Omega}{k_T}\right) ^2\right] (4.6-10)

The large scale energy is given by


 k_{T,l}=k_T - k_{T,s} (4.6-11)

Note that the sum of Equations  4.6-8 and 4.6-11 yields the turbulent kinetic energy $k_T$.

The turbulence production term generated by turbulent fluctuations is given by


 P_{k_T} = \nu_{T,s} S^2 (4.6-12)

where the small-scale turbulent viscosity is $\nu_{T,s}$

 \nu_{T,s} = f_{\nu} f_{INT} C_{\mu}\sqrt{k_{T,s}}\lambda_{eff} (4.6-13)

and


 C_{\mu}=\frac{1}{A_0+A_s(S/\omega)} (4.6-14)


 f_{\nu}=1-exp\left(-\frac{\sqrt{Re_{T,s}}}{A_{\nu}}\right) (4.6-15)

A damping function defining the turbulent production due to intermittency is given by

 f_{INT} = MIN\left(\frac{k_L}{C_{INT}k_{TOT}},1\right) (4.6-16)


 Re_{T,s} = \frac{f^2_W k_T}{\nu \omega} (4.6-17)

In Equation  4.6-2, $P_{k_L}$ is the production of laminar kinetic energy by large scale turbulent fluctuations, such that


 P_{k_L} = \nu_{T,l}S^2 (4.6-18)

The large-scale turbulent viscosity $\nu_{T,1}$ is modeled as


 \nu_{T,1} = MIN\left\lbrace \nu^*_{T,1},\frac{0.5(k_L+k_{T,1})}{S}\right\rbrace (4.6-19)

where


 \nu^*_{T,1}=f_{\tau,1}C_{11}\left(\frac{\Omega \lambda^2_{e... ...sqrt{k_{T,1}}\lambda_{eff}+\beta_{TS}C_{12}\phi_{NAT}d^2\Omega (4.6-20)

The limit in Equation  4.6-19 binds the realizability such that it is not violated in the two-dimensional developing boundary layer. The time-scale-based damping function $f_{\tau,1}$ is


 f_{\tau,1}=1-exp\left[ -C_{\tau,1}\frac{k_{T,1}}{\lambda^2_{eff}\Omega^2}\right] (4.6-21)

where $\beta_{TS}$ from Equation  4.6-20 is


 \beta_{TS}=1-exp\left(-\frac{MAX(\phi_{NAT} - C_{TS,crit},0)^2}{A_{TS}}\right) (4.6-22)


 \phi_{NAT}=\frac{d^2\Omega}{\nu} (4.6-23)

Near-wall dissipation is given by

 D_T=2\nu \frac{\partial \sqrt{k_T}}{\partial x_j}\frac{\partial \sqrt{k_T}}{\partial x_j} (4.6-24)


 D_L=2\nu \frac{\partial \sqrt{k_L}}{\partial x_j}\frac{\partial \sqrt{k_L}}{\partial x_j} (4.6-25)

In Equation  4.6-1 - 4.6-3, $R$ represents the averaged effect of the breakdown of streamwise fluctuations into turbulence during bypass transition:


 R=C_R\beta_{BP}k_L\omega/f_W (4.6-26)

$\beta_{BP}$, which is the threshold function controls the bypass transition process:

 \beta_{BP}=1-exp\left(-\frac{\phi_{BP}}{A_{BP}}\right) (4.6-27)


 \phi_{BP}=MAX\left[ \left(\frac{k_T}{\nu \Omega}-C_{BP,crit}\right),0\right] (4.6-28)

The breakdown to turbulence due to instabilities is considered to be a natural transition production term, given by

 R_{NAT}=C_{R,NAT}\beta_{NAT}k_L\Omega (4.6-29)


 \beta_{NAT}=1-exp\left[ -\frac{MAX(\phi_{NAT}-C_{NAT,crit}/f_{NAT,crit},0)}{A_{NAT}}\right\rbrace (4.6-30)


 f_{NAT,crit}=1-exp\left(C_{NC} \frac{\sqrt{k_L}d}{\nu}\right) (4.6-31)

The use of $\omega$ as the scale-determining variable can lead to a reduced intermittency effect in the outer region of a turbulent boundary layer, and consequently an elimination of the wake region in the velocity profile. From Equation  4.6-3, the following damping is defined as


 f_{\omega} = 1-exp\left[ -0.41 \left(\frac{\lambda_{eff}}{\lambda_T}\right)^4\right] (4.6-32)

The total eddy viscosity and eddy diffusivity included in Equations  4.6-4 and 4.6-5 are given by


 \nu_{TOT} = \nu_{T,s} + \nu_{T,l} (4.6-33)


 \alpha_{\theta,TOT}=f_W\left(\frac{k_T}{k_{TOT}}\right)\fra... ...Pr_\theta}+(1-f_W)C_{\alpha,\theta} \sqrt{k_{T}}\lambda_{eff} (4.6-34)

The turbulent scalar diffusivity in Equations  4.6-1 - 4.6-3 is defined as


 \alpha_T=f_\nu C_{\mu,std} \sqrt{k_{T,s}}\lambda_{eff} (4.6-35)


 k_{TOT}=k_T + k_L (4.6-36)



Model Constants


The model constants for the $k$- $kl$- $\omega$ transition model are listed below [ 364]


A_0 = 4.04, \;\; A_s = 2.12, \;\; A_{\nu} = 6.75, \;\; A_{BP}= 0.6


A_{NAT} = 200, \;\; A_{TS} = 200, \;\; C_{BP,crit} = 1.2, \;\; C_{NC}= 0.1


C_{NAT,crit} = 1250, \;\; C_{INT} = 0.75, \;\; C_{TS,crit} = 1000, \;\; C_{R,NAT}= 0.02


C_{11} = 3.4 \times 10^{-6}, \;\; C_{12} = 1.0 \times 10^{-10}, \;\; C_R = 0.12, \;\; C_{\alpha,\theta}= 0.035


C_{SS} = 1.5, \;\; C_{\tau,1} = 4360, \;\; C_{\omega 1} = 0.44, \;\; C_{\omega 2} = 0.92


C_{\omega 3} = 0.3, \;\; C_{\omega R} = 1.5, \;\; C_{\lambda} = 2.495, \;\; C_{\mu,std} = 0.09


Pr_{\theta} = 0.85, \;\; \sigma_k = 1, \;\; \sigma_{\omega} = 1.17


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