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Changeset 2132 for branches/devmercator2010_1/DOC/TexFiles/Chapters/Chap_ZDF.tex – NEMO

Ignore:
Timestamp:
2010-09-29T17:31:36+02:00 (14 years ago)
Author:
cbricaud
Message:

add change from DEV_r1784_GLS

File:
1 edited

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  • branches/devmercator2010_1/DOC/TexFiles/Chapters/Chap_ZDF.tex

    r1225 r2132  
    233233 
    234234% ------------------------------------------------------------------------------------------------------------- 
     235%        GLS Generic Length Scale Scheme  
     236% ------------------------------------------------------------------------------------------------------------- 
     237\subsection{GLS Generic Length Scale (\key{zdfgls})} 
     238\label{ZDF_gls} 
     239 
     240%--------------------------------------------namgls--------------------------------------------------------- 
     241\namdisplay{namgls} 
     242%-------------------------------------------------------------------------------------------------------------- 
     243 
     244The model allows to resolve two prognostic equations for turbulent  
     245kinetic energy $\bar {e}$ and a generic length scale \citep{Umlauf_Burchard_2003}. Thanks to the latter, commonly  
     246used closures can be retrieved: $k-kl$ \citep{Mellor_Yamada_1982}, $k-{\epsilon }$ \citep{Rodi_1987} and $k-{\omega }$  
     247\citep{Wilcox_1988}. These equations could be written in a generic form with the incorporation  
     248of a new variable : ${\psi} = (C^{0}_{\mu})^{p} \ {\bar{e}}^{m} \ l^{n}$. 
     249 
     250\begin{equation} \label{Eq_zdfgls_e} 
     251\frac{\partial \bar{e}}{\partial t} =  
     252\frac{A^{vm}}{{\sigma_e} {e_3} }\;\left[ {\left( {\frac{\partial u}{\partial k}} \right)^2 
     253                                                        +\left( {\frac{\partial v}{\partial k}} \right)^2} \right] 
     254-A^{vT}\,N^2 
     255+\frac{1}{e_3}  \;\frac{\partial }{\partial k}\left[ {\frac{A^{vm}}{e_3 } 
     256                                \;\frac{\partial \bar{e}}{\partial k}} \right] 
     257- \epsilon \; 
     258\end{equation} 
     259 
     260\begin{equation} \label{Eq_zdfgls_psi} 
     261\frac{\partial \psi}{\partial t} = \frac{\psi}{\bar{e}}  
     262(\frac{{C_1}A^{vm}}{{\sigma_{\psi}} {e_3} }\;\left[ {\left( {\frac{\partial u}{\partial k}} \right)^2 
     263                                                        +\left( {\frac{\partial v}{\partial k}} \right)^2} \right] 
     264-{C_3}A^{vT}\,N^2- C_2{\epsilon}Fw)  
     265+\frac{1}{e_3}  \;\frac{\partial }{\partial k}\left[ {\frac{A^{vm}}{e_3 } 
     266                                \;\frac{\partial \psi}{\partial k}} \right]\; 
     267\end{equation} 
     268 
     269\begin{equation} \label{Eq_zdfgls_kz} 
     270   \begin{split} 
     271         A^{vm} &= C_{\mu} \ \sqrt {\bar{e}} \ l         \\ 
     272         A^{vT} &= C_{\mu'}\ \sqrt {\bar{e}} \ l 
     273   \end{split} 
     274\end{equation} 
     275 
     276\begin{equation} \label{Eq_zdfgls_eps} 
     277{\epsilon} = (C^{0}_{\mu}) \frac{\bar {e}^{3/2}}{l} \; 
     278\end{equation} 
     279where $N$ is the local Brunt-Vais\"{a}l\"{a} frequency (see \S\ref{TRA_bn2}) and $\epsilon$ the dissipation rate. 
     280In function of the parameters k, m and n, common turbulent closure could be retrieved. 
     281The constants C1, C2, C3, ${\sigma_e}$, ${\sigma_{\psi}}$ and the wall function (Fw) depends of the choice of the turbulence model. 
     282%>>>>>>>>>>>>>>>>>>>>>>>>>>>> 
     283\begin{figure}[!h] 
     284\centering 
     285\includegraphics[scale=0.7]{./TexFiles/Figures/tabgls.png} 
     286\caption {Values of the parameters in function of the model of turbulence.} 
     287\label{tabgls} 
     288\end{figure} 
     289%>>>>>>>>>>>>>>>>>>>>>>>>>>>> 
     290 
     291About the Mellor-Yamada model, the negativity of n allows to use a wall function to force 
     292the convergence of the mixing length towards Kzb (K: Kappa and zb: rugosity length) value 
     293near physical boundaries (logarithmic boundary layer law). $C_{\mu}$ and $C_{\mu'}$ are calculated from stability functions  
     294of \citet{Galperin_1988}, \citet{Kantha_Clayson_1994} or \citet{Canuto_2001}. 
     295$C^{0}_{\mu}$ depends of the choice of the stability function. 
     296 
     297The boundary condition at the surface and the bottom could be calculated thanks to Diriclet or Neumann condition. 
     298The wave effect on the mixing could be also being considered \citep{Craig_Banner_1994}. 
     299 
     300------------------------------------------------------------------------------------------------------------- 
    235301%        K Profile Parametrisation (KPP)  
    236302% ------------------------------------------------------------------------------------------------------------- 
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