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 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>
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_0 + \nu_c + \nu_w </math>   
       <math> \nu_t = \nu_0 + \nu_c + \nu_w </math>   


There are two options to calculate  <math>\nu_c</math>. The first is the Falconer (1980) equation given by
There are three options for calculating the current-related eddy viscosity. The first is the Falconer (1980) equation given by


       <math> \nu_c = 0.575C_f|U|h </math>
       <math> \nu_c = 0.575c_b|U|h </math>


where <math>C_f</math> is the bottom friction coefficient, <math>U</math> is the depth-averaged current velocity, and <math>h</math> is the total water depth.
where <math>c_b</math> is the bottom friction coefficient, <math>U</math> is the depth-averaged current velocity, and <math>h</math> is the total water depth.


The second option is a subgrid turbulence model given by
The second option is the parabolic model given by
 
      <math> \nu_c = c_0u_{*}h </math>
 
where <math>c_0</math> is approximately equal to <math>\kappa/6</math>
 
The third option for calculating <math>\nu_c</math> is the subgrid turbulence model given by


       <math> \nu_{c} = \sqrt{ (c_0 u_{*})^2 h + (c_1 \Delta |S|)^2}  </math>
       <math> \nu_{c} = \sqrt{ (c_0 u_{*})^2 h + (c_1 \Delta |S|)^2}  </math>


where <math>c_0</math> and <math>c_1</math> are empirical coefficients and <math>\Delta</math> is the average grid area.  <math>c_0</math> is approximately equal to 0.0667 (default) but may vary from 0.01-0.2. <math>c_1</math> may vary from 0.1 to 0.5 and is set to a default value of 0.4. <math>|S|</math> is equal to
where <math>c_0</math> and <math>c_1</math> are empirical coefficients, and <math>\Delta</math> is the average grid area.  <math>c_0</math> is approximately equal to 0.0667 (default) but may vary from 0.01-0.2. <math>c_1</math> may vary from 0.1 to 0.5 and is set to a default value of 0.4. <math>|S|</math> is equal to


       <math> |S| = \sqrt{ \biggl( 2\frac{ \partial U}{\partial x} \biggr) ^2 +  2\biggl( \frac{ \partial V}{\partial y} \biggr) ^2 + \biggl( \frac{ \partial U}{\partial y} + \frac{ \partial V}{\partial x}  \biggr) ^2 } </math>
       <math> |S| = \sqrt{ \biggl( 2\frac{ \partial U}{\partial x} \biggr) ^2 +  2\biggl( \frac{ \partial V}{\partial y} \biggr) ^2 + \biggl( \frac{ \partial U}{\partial y} + \frac{ \partial V}{\partial x}  \biggr) ^2 } </math>

Revision as of 18:54, 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  

There are three options for calculating the current-related eddy viscosity. The first is the Falconer (1980) equation given by

     νc=0.575cb|U|h

where cb is the bottom friction coefficient, U is the depth-averaged current velocity, and h is the total water depth.

The second option is the parabolic model given by

     νc=c0u*h

where c0 is approximately equal to κ/6

The third option for calculating νc is the subgrid turbulence model given by

     νc=(c0u*)2h+(c1Δ|S|)2

where c0 and c1 are empirical coefficients, and Δ is the average grid area. c0 is approximately equal to 0.0667 (default) but may vary from 0.01-0.2. c1 may vary from 0.1 to 0.5 and is set to a default value of 0.4. |S| is equal to

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

The wave component of the eddy viscosity is calculated as

     νw=ΛuwHs

where Λ is an empirical coefficient approximately equal to 0.5, Hs is the significant wave height and uw is bottom orbital velocity based on the significant wave height. Outside of the surf zone the bottom orbital velocity is calculated as

     uw=πHsTpsinh(kh)

where Hs is the significant wave height, Tp is the peak wave period, k=2π/L is the wave number. Inside the surf zone, the turbulence due to wave breaking is considered by increasing the bottom orbital velocity as

     uw=Hs2hgh

The default turbulence model is the subgrid model, but may be changed with the advanced card

     TURBULENCE_MODEL                  SUBGRID   !FALCONER | PARABOLIC | SUBGRID | SUBGRID-WU 

The turbulence model parameters may be changed in the advanced cards as

     EDDY_VISCOSITY_CONSTANT           1.0e-6    ![m^2/sec], kinematic viscosity, ~1.0e-6
     EDDY_VISCOSITY_BOTTOM             0.015     ![-], bottom shear coefficient, ~0.1667
     EDDY_VISCOSITY_HORIZONTAL         0.2       ![-], smagorinsky coefficient, ~0.1-0.5
     EDDY_VISCOSITY_WAVE               0.5       ![-], wave coefficient, ~0.25-0.5

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.


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