next up previous
Next: Selected validational testcases and Up: Eddy-Viscosity Transport Model Previous: Eddy-Viscosity Transport Model

Production-Term Modification

Amongst the various recent publications on one-equation models, Menters [2] rigorous derivation of a generic one-equation model casted in terms of a transport equation for the eddy-viscosity $ \nu_t$ is, perhaps, the most instructive. Based on the application of local-equilibrium assumptions to a two-equation - e.g. $ k-\varepsilon$ - model, Menters approach provides a keen insight into the one-equation modeling framework, in particular the related coefficients. The procedure reveals that the four most influential production and destruction terms of the two-equation approach collapse into a single production-type term in the one-equation framework, viz.
$\displaystyle P_{\tilde \nu_t}$ $\displaystyle =$ $\displaystyle \tilde \nu_t S^* \quad \left( C_{\varepsilon 2} - C_{\varepsilon ...
...mu \, S^*k/\varepsilon )
\quad \approx \quad \tilde \nu_t \tilde S \quad C_{b1}$ (5)

The coefficient $ C_{b1}$ is thus crucial to the model's predictive performance. As indicated by eq. (5), $ C_{b1}$ is a function of the strain rate and model coefficients. Substituting the employed coefficients of the background $ k-\varepsilon$ turbulence model by $ C_{\varepsilon1}=1.45$ and $ C_{\varepsilon2}=1.9$, additionally employing $ c_\mu S^*k/\varepsilon = \sqrt{c_\mu}$ one obtains $ C_{b1}=\sqrt{c_\mu} (C_{\varepsilon2}-C_{\varepsilon1}) = 0.135$, which is close to the original SA model ( $ C_{b1}=0.1355$). Both expressions, $ \left( C_{\varepsilon 2} - C_{\varepsilon 1} \right)$ and the anisotropy parameter $ c_\mu$, are itself a function of strain and rotation rate invariants. In general, they both tend to decrease with an increase of strain, which motivates the following modification of the standard coefficient $ C_{b1}$:
$\displaystyle C_{b1} = 0.1355 \sqrt{\Gamma} \qquad \Gamma=\min \left(1.25, \max(\gamma,0.75) \right) \; ,
\qquad \gamma = \max\left(\alpha_1,\alpha_2\right)$      


$\displaystyle \alpha_1= \left( 1.01 \frac{ \tilde \nu_t}{ \kappa^2 \: l_n ^2 S^...
..._2= \max \left( 0,1-\tanh \left( \frac{\nu_t^+}{68} \right) \right)^{0.65}
\; .$     (6)

Due to the lack of an individual length-scale the approach relies on some heuristics based on the comparison of a mixing-length related eddy-viscosity with the value obtained from the solution of the transport equation. The modification $ \sqrt{\Gamma}$ primarily causes a reduction of production for excessive strains via $ \alpha_1$. Additionally, undesirable wall-damping is suppressed by the inclusion of $ \alpha_2$. The limitation of $ \Gamma$ are necessary due to the proportionality of $ \tilde \nu_t$ and $ \alpha_1$, i.e. a decreasing $ \tilde \nu_t$ causes a decreasing $ \alpha_1$. Since it is closely related to the destruction parameter $ \Psi$, the modification of $ \tilde C_{b1}$ represents a cross-term between production and destruction.
next up previous
Next: Selected validational testcases and Up: Eddy-Viscosity Transport Model Previous: Eddy-Viscosity Transport Model
Markus Schatz 2004-02-10