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branches/devmercator2010_1/DOC/TexFiles/Chapters/Chap_ZDF.tex
r1225 r2132 233 233 234 234 % ------------------------------------------------------------------------------------------------------------- 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 %-------------------------------------------------------------------------------------------------------------- 243 244 The model allows to resolve two prognostic equations for turbulent 245 kinetic energy $\bar {e}$ and a generic length scale \citep{Umlauf_Burchard_2003}. Thanks to the latter, commonly 246 used 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 248 of 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} 279 where $N$ is the local Brunt-Vais\"{a}l\"{a} frequency (see \S\ref{TRA_bn2}) and $\epsilon$ the dissipation rate. 280 In function of the parameters k, m and n, common turbulent closure could be retrieved. 281 The 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 %>>>>>>>>>>>>>>>>>>>>>>>>>>>> 290 291 About the Mellor-Yamada model, the negativity of n allows to use a wall function to force 292 the convergence of the mixing length towards Kzb (K: Kappa and zb: rugosity length) value 293 near physical boundaries (logarithmic boundary layer law). $C_{\mu}$ and $C_{\mu'}$ are calculated from stability functions 294 of \citet{Galperin_1988}, \citet{Kantha_Clayson_1994} or \citet{Canuto_2001}. 295 $C^{0}_{\mu}$ depends of the choice of the stability function. 296 297 The boundary condition at the surface and the bottom could be calculated thanks to Diriclet or Neumann condition. 298 The wave effect on the mixing could be also being considered \citep{Craig_Banner_1994}. 299 300 ------------------------------------------------------------------------------------------------------------- 235 301 % K Profile Parametrisation (KPP) 236 302 % -------------------------------------------------------------------------------------------------------------
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