CMS-Flow:Subgrid Turbulence Model: Difference between revisions

From CIRPwiki
Jump to navigation Jump to search
Deleted (talk | contribs)
No edit summary
Deleted (talk | contribs)
Line 2: Line 2:
== Subgrid Turbulence Model ==
== Subgrid Turbulence Model ==


In CMS-Flow eddy viscosity is calculated as  
In CMS-Flow eddy viscosity is calculated as the sum of the kinematic viscosity <math>\nu_{0}</math>, the current-related eddy viscosity  <math>\nu_c</math> and the wave-related eddy viscosity  <math>\nu_w</math>


       <math> \nu_t = \nu_c + \nu_w </math>   
       <math> \nu_t = \nu_0 + \nu_c + \nu_w </math>   


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)  
The wave contribution is included using the equation of Kraus and Larson (1991)  


       <math> \nu_w = \Lambda u_w h </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
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.


       <math> \nu_{c} = \nu_{0} + \sqrt{ (c_0 u_* h)^2 + (c_{sm}\Delta |S| )^2 } </math>
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_1\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  
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  

Revision as of 18:41, 5 May 2010

Subgrid Turbulence Model

In CMS-Flow eddy viscosity is calculated as the sum of the kinematic viscosity ν0, the current-related eddy viscosity νc and the wave-related eddy viscosity νw

     νt=ν0+νc+νw  

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+(c1Δ|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