CMS-Flow:Subgrid Turbulence Model: Difference between revisions

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== Subgrid Turbulence Model ==
== Subgrid Turbulence Model ==


In CMS-Flow eddy viscosity is calculated as <math> \nu_t = (1-\theta_m)\nu_{tc} + \theta_m \nu_m </math>  where <math>\theta_m</math>  is weighting factor equal to <math>\theta_m = (H_s/h)^3 </math>  in which <math>H_s</math>  is the significant wave height and <math>\nu_{tc}</math>  and <math>\nu_{tw}</math>  are the current- and wave-related eddy viscosity components respectively. The wave contribution is included using the equation of Kraus and Larson (1991)  <math> \nu_tw = \Lambda u_w h </math>, where  <math>\Lambda</math> is an empirical coefficient (default is 0.5), and  <math>u_w</math> is the wave bottom orbital velocity. The current-related eddy viscosity is calculated as a function of the flow gradients, and the bottom shear stress
In CMS-Flow eddy viscosity is calculated as  


       <math> \nu_{tc} = \nu_{t0} + \sqrt{ (c_0 u_* h)^2 + (\sqrt{c_{sm} \Delta x \Delta y}  |S| )^2 } </math>
       <math> \nu_t = \nu_c + \nu_w </math>


where <math>\nu_{t0}</math> is a base value approximately equal to the dynamic viscosity, and <math>c_0</math> is an empirical coefficient and <math>l_h</math> is the subgrid mixing length. The mixing length is calculated here as 
where <math>\nu_c</math> and <math>\nu_w</math> are the current- and wave-related eddy viscosity components respectively. The wave contribution is included using the equation of Kraus and Larson (1991)


       <math>l_h = c_{sm} \Delta x \Delta y </math>  
       <math> \nu_w = \Lambda u_w h </math>
 
where  <math>\Lambda</math> is an empirical coefficient (default is 0.5), and  <math>u_w</math> is the wave bottom orbital velocity and <math>h</math> is the water depth. The current-related eddy viscosity is calculated as a function of the flow gradients, and the bottom shear stress
 
      <math> \nu_{c} = \nu_{0} + \sqrt{ (c_0 u_* h)^2 + (c_{sm}\Delta |S| )^2 } </math>
 
where  <math>\nu_{0}</math> is a base value approximately equal to the kinematic viscosity, <math>c_0</math> is an empirical coefficient, <math>c_{sm}</math>  is an empirical coefficient (Smagorinsky coefficient), <math> \Delta </math> is the local cell area, and <math>|S|</math> is equal to
 
      <math> |S| = \sqrt{ \biggl( \frac{ \partial U}{\partial x} \biggr) ^2 +  \biggl( \frac{ \partial V}{\partial y} \biggr) ^2 + \frac{1}{2} \biggl( \frac{ \partial U}{\partial y} + \frac{ \partial V}{\partial x}  \biggr) ^2 } </math>


where <math>c_{sm}</math>  is an empirical coefficient (Smagorinsky coefficient).


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Revision as of 18:39, 5 May 2010

Subgrid Turbulence Model

In CMS-Flow eddy viscosity is calculated as

     νt=νc+νw  

where νc and νw are the current- and wave-related eddy viscosity components respectively. The wave contribution is included using the equation of Kraus and Larson (1991)

     νw=Λuwh

where Λ is an empirical coefficient (default is 0.5), and uw is the wave bottom orbital velocity and h is the water depth. The current-related eddy viscosity is calculated as a function of the flow gradients, and the bottom shear stress

     νc=ν0+(c0u*h)2+(csmΔ|S|)2

where ν0 is a base value approximately equal to the kinematic viscosity, c0 is an empirical coefficient, csm is an empirical coefficient (Smagorinsky coefficient), Δ is the local cell area, and |S| is equal to

     |S|=(Ux)2+(Vy)2+12(Uy+Vx)2



References

LARSON, M.; HANSON, H., and KRAUS, N. C., 2003. Numerical modeling of beach topography change. Advances in Coastal Modeling, V.C. Lakhan (eds.), Elsevier Oceanography Series, 67, Amsterdam, The Netherlands, 337-365.


CMS-Flow