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branches/2015/nemo_v3_6_STABLE/DOC/TexFiles/Chapters/Chap_ZDF.tex
r6317 r6322 1313 1313 1314 1314 % ================================================================ 1315 % Internal wave-driven mixing 1316 % ================================================================ 1317 \section{Internal wave-driven mixing (\key{zdftmx\_new})} 1318 \label{ZDF_tmx_new} 1319 1320 %--------------------------------------------namzdf_tmx_new------------------------------------------ 1321 \namdisplay{namzdf_tmx_new} 1322 %-------------------------------------------------------------------------------------------------------------- 1323 1324 The parameterization of mixing induced by breaking internal waves is a generalization 1325 of the approach originally proposed by \citet{St_Laurent_al_GRL02}. 1326 A three-dimensional field of internal wave energy dissipation $\epsilon(x,y,z)$ is first constructed, 1327 and the resulting diffusivity is obtained as 1328 \begin{equation} \label{Eq_Kwave} 1329 A^{vT}_{wave} = R_f \,\frac{ \epsilon }{ \rho \, N^2 } 1330 \end{equation} 1331 where $R_f$ is the mixing efficiency and $\epsilon$ is a specified three dimensional distribution 1332 of the energy available for mixing. If the \np{ln\_mevar} namelist parameter is set to false, 1333 the mixing efficiency is taken as constant and equal to 1/6 \citep{Osborn_JPO80}. 1334 In the opposite (recommended) case, $R_f$ is instead a function of the turbulence intensity parameter 1335 $Re_b = \frac{ \epsilon}{\nu \, N^2}$, with $\nu$ the molecular viscosity of seawater, 1336 following the model of \cite{Bouffard_Boegman_DAO2013} 1337 and the implementation of \cite{de_lavergne_JPO2016_efficiency}. 1338 Note that $A^{vT}_{wave}$ is bounded by $10^{-2}\,m^2/s$, a limit that is often reached when the mixing efficiency is constant. 1339 1340 In addition to the mixing efficiency, the ratio of salt to heat diffusivities can chosen to vary 1341 as a function of $Re_b$ by setting the \np{ln\_tsdiff} parameter to true, a recommended choice). 1342 This parameterization of differential mixing, due to \cite{Jackson_Rehmann_JPO2014}, 1343 is implemented as in \cite{de_lavergne_JPO2016_efficiency}. 1344 1345 The three-dimensional distribution of the energy available for mixing, $\epsilon(i,j,k)$, is constructed 1346 from three static maps of column-integrated internal wave energy dissipation, $E_{cri}(i,j)$, 1347 $E_{pyc}(i,j)$, and $E_{bot}(i,j)$, combined to three corresponding vertical structures 1348 (de Lavergne et al., in prep): 1349 \begin{align*} 1350 F_{cri}(i,j,k) &\propto e^{-h_{ab} / h_{cri} }\\ 1351 F_{pyc}(i,j,k) &\propto N^{n\_p}\\ 1352 F_{bot}(i,j,k) &\propto N^2 \, e^{- h_{wkb} / h_{bot} } 1353 \end{align*} 1354 In the above formula, $h_{ab}$ denotes the height above bottom, 1355 $h_{wkb}$ denotes the WKB-stretched height above bottom, defined by 1356 \begin{equation*} 1357 h_{wkb} = H \, \frac{ \int_{-H}^{z} N \, dz' } { \int_{-H}^{\eta} N \, dz' } \; , 1358 \end{equation*} 1359 The $n_p$ parameter (given by \np{nn\_zpyc} in \ngn{namzdf\_tmx\_new} namelist) controls the stratification-dependence of the pycnocline-intensified dissipation. 1360 It can take values of 1 (recommended) or 2. 1361 Finally, the vertical structures $F_{cri}$ and $F_{bot}$ require the specification of 1362 the decay scales $h_{cri}(i,j)$ and $h_{bot}(i,j)$, which are defined by two additional input maps. 1363 $h_{cri}$ is related to the large-scale topography of the ocean (etopo2) 1364 and $h_{bot}$ is a function of the energy flux $E_{bot}$, the characteristic horizontal scale of 1365 the abyssal hill topography \citep{Goff_JGR2010} and the latitude. 1366 1367 % ================================================================ 1368 1369 1370
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