\documentclass[../main/NEMO_manual]{subfiles} \begin{document} \chapter{A brief guide to the DOMAINcfg tool} \label{apdx:DOMCFG} % {\em 4.0} & {\em Andrew Coward} & {\em Created at v4.0 from materials removed from chap\_DOM that are still relevant to the \forcode{DOMAINcfg} tool and which illustrate and explain the choices to be made by the user when setting up new domains } \\ \thispagestyle{plain} \chaptertoc \paragraph{Changes record} ~\\ {\footnotesize \begin{tabularx}{\textwidth}{l||X|X} Release & Author(s) & Modifications \\ \hline {\em 4.0} & {\em ...} & {\em ...} \\ {\em 3.6} & {\em ...} & {\em ...} \\ {\em 3.4} & {\em ...} & {\em ...} \\ {\em <=3.4} & {\em ...} & {\em ...} \end{tabularx} } \clearpage This appendix briefly describes some of the options available in the \forcode{DOMAINcfg} tool mentioned in \autoref{chap:DOM}. This tool will evolve into an independent utility with its own documentation but its current manifestation is mostly a wrapper for \NEMO\ \forcode{DOM} modules more aligned to those in the previous versions of \NEMO. These versions allowed the user to define some horizontal and vertical grids through additional namelist parameters. Explanations of these parameters are retained here for reference pending better documentation for \forcode{DOMAINcfg}. Please note that the namelist blocks named in this appendix refer to those read by \forcode{DOMAINcfg} via its own \forcode{namelist_ref} and \forcode{namelist_cfg} files. Although, due to their origins, these namelists share names with those used by \NEMO, they are not interchangeable and should be considered independent of those described elsewhere in this manual. %% ================================================================================================= \section{Choice of horizontal grid} \label{sec:DOMCFG_hor} \begin{listing} \nlst{namdom_domcfg} \caption{\forcode{&namdom_domcfg}} \label{lst:namdom_domcfg} \end{listing} The user has three options available in defining a horizontal grid, which involve the namelist variable \np{jphgr_mesh}{jphgr\_mesh} of the \nam{dom}{dom} (\texttt{DOMAINcfg} variant only) namelist. \begin{description} \item [{\np{jphgr_mesh}{jphgr\_mesh}=0}] The most general curvilinear orthogonal grids. The coordinates and their first derivatives with respect to $i$ and $j$ are provided in a input file (\ifile{coordinates}), read in \rou{hgr\_read} subroutine of the domhgr module. This is now the only option available within \NEMO\ itself from v4.0 onwards. \item [{\np{jphgr_mesh}{jphgr\_mesh}=1 to 5}] A few simple analytical grids are provided (see below). For other analytical grids, the \mdl{domhgr} module (\texttt{DOMAINcfg} variant) must be modified by the user. In most cases, modifying the \mdl{usrdef\_hgr} module of \NEMO\ is a better alternative since this is designed to allow simple analytical domains to be configured and used without the need for external data files. \end{description} There are two simple cases of geographical grids on the sphere. With \np{jphgr_mesh}{jphgr\_mesh}=1, the grid (expressed in degrees) is regular in space, with grid sizes specified by parameters \np{ppe1_deg}{ppe1\_deg} and \np{ppe2_deg}{ppe2\_deg}, respectively. Such a geographical grid can be very anisotropic at high latitudes because of the convergence of meridians (the zonal scale factors $e_1$ become much smaller than the meridional scale factors $e_2$). The Mercator grid (\np{jphgr_mesh}{jphgr\_mesh}=4) avoids this anisotropy by refining the meridional scale factors in the same way as the zonal ones. In this case, meridional scale factors and latitudes are calculated analytically using the formulae appropriate for a Mercator projection, based on \np{ppe1_deg}{ppe1\_deg} which is a reference grid spacing at the equator (this applies even when the geographical equator is situated outside the model domain). In these two cases (\np{jphgr_mesh}{jphgr\_mesh}=1 or 4), the grid position is defined by the longitude and latitude of the south-westernmost point (\np{ppglamt0} and \np{ppgphi0}{ppgphi0}). Note that for the Mercator grid the user need only provide an approximate starting latitude: the real latitude will be recalculated analytically, in order to ensure that the equator corresponds to line passing through $t$- and $u$-points. Rectangular grids ignoring the spherical geometry are defined with \np{jphgr_mesh}{jphgr\_mesh} = 2, 3, 5. The domain is either an $f$-plane (\np{jphgr_mesh}{jphgr\_mesh} = 2, Coriolis factor is constant) or a beta-plane (\np{jphgr_mesh}{jphgr\_mesh} = 3, the Coriolis factor is linear in the $j$-direction). The grid size is uniform in meter in each direction, and given by the parameters \np{ppe1_m}{ppe1\_m} and \np{ppe2_m}{ppe2\_m} respectively. The zonal grid coordinate (\textit{glam} arrays) is in kilometers, starting at zero with the first $t$-point. The meridional coordinate (gphi. arrays) is in kilometers, and the second $t$-point corresponds to coordinate $gphit=0$. The input variable \np{ppglam0}{ppglam0} is ignored. \np{ppgphi0}{ppgphi0} is used to set the reference latitude for computation of the Coriolis parameter. In the case of the beta plane, \np{ppgphi0}{ppgphi0} corresponds to the center of the domain. Finally, the special case \np{jphgr_mesh}{jphgr\_mesh}=5 corresponds to a beta plane in a rotated domain for the GYRE configuration, representing a classical mid-latitude double gyre system. The rotation allows us to maximize the jet length relative to the gyre areas (and the number of grid points). %% ================================================================================================= \section{Vertical grid} \label{sec:DOMCFG_vert} %% ================================================================================================= \subsection{Vertical reference coordinate} \label{sec:DOMCFG_zref} \begin{figure}[!tb] \centering \includegraphics[width=0.66\textwidth]{DOMCFG_zgr} \caption[DOMAINcfg: default vertical mesh for ORCA2]{ Default vertical mesh for ORCA2: 30 ocean levels (L30). Vertical level functions for (a) T-point depth and (b) the associated scale factor for the $z$-coordinate case.} \label{fig:DOMCFG_zgr} \end{figure} The reference coordinate transformation $z_0(k)$ defines the arrays $gdept_0$ and $gdepw_0$ for $t$- and $w$-points, respectively. See \autoref{sec:DOMCFG_sco} for the S-coordinate options. As indicated on \autoref{fig:DOM_index_vert} \jp{jpk} is the number of $w$-levels. $gdepw_0(1)$ is the ocean surface. There are at most \jp{jpk}-1 $t$-points inside the ocean, the additional $t$-point at $jk = jpk$ is below the sea floor and is not used. The vertical location of $w$- and $t$-levels is defined from the analytic expression of the depth $z_0(k)$ whose analytical derivative with respect to $k$ provides the vertical scale factors. The user must provide the analytical expression of both $z_0$ and its first derivative with respect to $k$. This is done in routine \mdl{domzgr} through statement functions, using parameters provided in the \nam{dom}{dom} namelist (\texttt{DOMAINcfg} variant). It is possible to define a simple regular vertical grid by giving zero stretching (\np[=0]{ppacr}{ppacr}). In that case, the parameters \jp{jpk} (number of $w$-levels) and \np{pphmax}{pphmax} (total ocean depth in meters) fully define the grid. For climate-related studies it is often desirable to concentrate the vertical resolution near the ocean surface. The following function is proposed as a standard for a $z$-coordinate (with either full or partial steps): \begin{gather} \label{eq:DOMCFG_zgr_ana_1} z_0 (k) = h_{sur} - h_0 \; k - \; h_1 \; \log \big[ \cosh ((k - h_{th}) / h_{cr}) \big] \\ e_3^0(k) = \lt| - h_0 - h_1 \; \tanh \big[ (k - h_{th}) / h_{cr} \big] \rt| \end{gather} where $k = 1$ to \jp{jpk} for $w$-levels and $k = 1$ to $k = 1$ for $t-$levels. Such an expression allows us to define a nearly uniform vertical location of levels at the ocean top and bottom with a smooth hyperbolic tangent transition in between (\autoref{fig:DOMCFG_zgr}). A double hyperbolic tangent version (\np[=.true.]{ldbletanh}{ldbletanh}) is also available which permits finer control and is used, typically, to obtain a well resolved upper ocean without compromising on resolution at depth using a moderate number of levels. \begin{gather} \label{eq:DOMCFG_zgr_ana_1b} \begin{split} z_0 (k) = h_{sur} - h_0 \; k &- \; h_1 \; \log \big[ \cosh ((k - h_{th}) / h_{cr}) \big] \\ \; &- \; h2_1 \; \log \big[ \cosh ((k - h2_{th}) / h2_{cr}) \big] \end{split} \end{gather} \begin{gather} \begin{split} e_3^0(k) = \big| - h_0 &- h_1 \; \tanh \big[ (k - h_{th}) / h_{cr} \big] \\ &- h2_1 \; \tanh \big[ (k - h2_{th}) / h2_{cr} \big] \big| \end{split} \end{gather} If the ice shelf cavities are opened (\np[=.true.]{ln_isfcav}{ln\_isfcav}), the definition of $z_0$ is the same. However, definition of $e_3^0$ at $t$- and $w$-points is respectively changed to: \begin{equation} \label{eq:DOMCFG_zgr_ana_2} \begin{split} e_3^T(k) &= z_W (k + 1) - z_W (k ) \\ e_3^W(k) &= z_T (k ) - z_T (k - 1) \end{split} \end{equation} This formulation decreases the self-generated circulation into the ice shelf cavity (which can, in extreme case, leads to numerical instability). This is now the recommended formulation for all configurations using v4.0 onwards. The analytical derivation of thicknesses is maintained for backwards compatibility. The most used vertical grid for ORCA2 has $10~m$ ($500~m$) resolution in the surface (bottom) layers and a depth which varies from 0 at the sea surface to a minimum of $-5000~m$. This leads to the following conditions: \begin{equation} \label{eq:DOMCFG_zgr_coef} \begin{array}{ll} e_3 (1 + 1/2) = 10. & z(1 ) = 0. \\ e_3 (jpk - 1/2) = 500. & z(jpk) = -5000. \end{array} \end{equation} With the choice of the stretching $h_{cr} = 3$ and the number of levels \jp{jpk}~$= 31$, the four coefficients $h_{sur}$, $h_0$, $h_1$, and $h_{th}$ in \autoref{eq:DOMCFG_zgr_ana_2} have been determined such that \autoref{eq:DOMCFG_zgr_coef} is satisfied, through an optimisation procedure using a bisection method. For the first standard ORCA2 vertical grid this led to the following values: $h_{sur} = 4762.96$, $h_0 = 255.58, h_1 = 245.5813$, and $h_{th} = 21.43336$. The resulting depths and scale factors as a function of the model levels are shown in \autoref{fig:DOMCFG_zgr} and given in \autoref{tab:DOMCFG_orca_zgr}. Those values correspond to the parameters \np{ppsur}{ppsur}, \np{ppa0}{ppa0}, \np{ppa1}{ppa1}, \np{ppkth}{ppkth} in \nam{cfg}{cfg} namelist. Rather than entering parameters $h_{sur}$, $h_0$, and $h_1$ directly, it is possible to recalculate them. In that case the user sets \np{ppsur}{ppsur}~$=$~\np{ppa0}{ppa0}~$=$~\np{ppa1}{ppa1}~$= 999999$., in \nam{cfg}{cfg} namelist, and specifies instead the four following parameters: \begin{itemize} \item \np{ppacr}{ppacr}~$= h_{cr}$: stretching factor (nondimensional). The larger \np{ppacr}{ppacr}, the smaller the stretching. Values from $3$ to $10$ are usual. \item \np{ppkth}{ppkth}~$= h_{th}$: is approximately the model level at which maximum stretching occurs (nondimensional, usually of order 1/2 or 2/3 of \jp{jpk}) \item \np{ppdzmin}{ppdzmin}: minimum thickness for the top layer (in meters). \item \np{pphmax}{pphmax}: total depth of the ocean (meters). \end{itemize} As an example, for the $45$ layers used in the DRAKKAR configuration those parameters are: \jp{jpk}~$= 46$, \np{ppacr}{ppacr}~$= 9$, \np{ppkth}{ppkth}~$= 23.563$, \np{ppdzmin}{ppdzmin}~$= 6~m$, \np{pphmax}{pphmax}~$= 5750~m$. \begin{table} \centering \begin{tabular}{c||r|r|r|r} \hline \textbf{LEVEL} & \textbf{gdept\_1d} & \textbf{gdepw\_1d} & \textbf{e3t\_1d } & \textbf{e3w\_1d} \\ \hline 1 & \textbf{ 5.00} & 0.00 & \textbf{ 10.00} & 10.00 \\ \hline 2 & \textbf{ 15.00} & 10.00 & \textbf{ 10.00} & 10.00 \\ \hline 3 & \textbf{ 25.00} & 20.00 & \textbf{ 10.00} & 10.00 \\ \hline 4 & \textbf{ 35.01} & 30.00 & \textbf{ 10.01} & 10.00 \\ \hline 5 & \textbf{ 45.01} & 40.01 & \textbf{ 10.01} & 10.01 \\ \hline 6 & \textbf{ 55.03} & 50.02 & \textbf{ 10.02} & 10.02 \\ \hline 7 & \textbf{ 65.06} & 60.04 & \textbf{ 10.04} & 10.03 \\ \hline 8 & \textbf{ 75.13} & 70.09 & \textbf{ 10.09} & 10.06 \\ \hline 9 & \textbf{ 85.25} & 80.18 & \textbf{ 10.17} & 10.12 \\ \hline 10 & \textbf{ 95.49} & 90.35 & \textbf{ 10.33} & 10.24 \\ \hline 11 & \textbf{ 105.97} & 100.69 & \textbf{ 10.65} & 10.47 \\ \hline 12 & \textbf{ 116.90} & 111.36 & \textbf{ 11.27} & 10.91 \\ \hline 13 & \textbf{ 128.70} & 122.65 & \textbf{ 12.47} & 11.77 \\ \hline 14 & \textbf{ 142.20} & 135.16 & \textbf{ 14.78} & 13.43 \\ \hline 15 & \textbf{ 158.96} & 150.03 & \textbf{ 19.23} & 16.65 \\ \hline 16 & \textbf{ 181.96} & 169.42 & \textbf{ 27.66} & 22.78 \\ \hline 17 & \textbf{ 216.65} & 197.37 & \textbf{ 43.26} & 34.30 \\ \hline 18 & \textbf{ 272.48} & 241.13 & \textbf{ 70.88} & 55.21 \\ \hline 19 & \textbf{ 364.30} & 312.74 & \textbf{ 116.11} & 90.99 \\ \hline 20 & \textbf{ 511.53} & 429.72 & \textbf{ 181.55} & 146.43 \\ \hline 21 & \textbf{ 732.20} & 611.89 & \textbf{ 261.03} & 220.35 \\ \hline 22 & \textbf{ 1033.22} & 872.87 & \textbf{ 339.39} & 301.42 \\ \hline 23 & \textbf{ 1405.70} & 1211.59 & \textbf{ 402.26} & 373.31 \\ \hline 24 & \textbf{ 1830.89} & 1612.98 & \textbf{ 444.87} & 426.00 \\ \hline 25 & \textbf{ 2289.77} & 2057.13 & \textbf{ 470.55} & 459.47 \\ \hline 26 & \textbf{ 2768.24} & 2527.22 & \textbf{ 484.95} & 478.83 \\ \hline 27 & \textbf{ 3257.48} & 3011.90 & \textbf{ 492.70} & 489.44 \\ \hline 28 & \textbf{ 3752.44} & 3504.46 & \textbf{ 496.78} & 495.07 \\ \hline 29 & \textbf{ 4250.40} & 4001.16 & \textbf{ 498.90} & 498.02 \\ \hline 30 & \textbf{ 4749.91} & 4500.02 & \textbf{ 500.00} & 499.54 \\ \hline 31 & \textbf{ 5250.23} & 5000.00 & \textbf{ 500.56} & 500.33 \\ \hline \end{tabular} \caption[Default vertical mesh in $z$-coordinate for 30 layers ORCA2 configuration]{ Default vertical mesh in $z$-coordinate for 30 layers ORCA2 configuration as computed from \autoref{eq:DOMCFG_zgr_ana_2} using the coefficients given in \autoref{eq:DOMCFG_zgr_coef}} \label{tab:DOMCFG_orca_zgr} \end{table} %%%YY %% % ------------------------------------------------------------------------------------------------------------- %% % Meter Bathymetry %% % ------------------------------------------------------------------------------------------------------------- %% ================================================================================================= \subsection{Model bathymetry} \label{subsec:DOMCFG_bathy} Three options are possible for defining the bathymetry, according to the namelist variable \np{nn_bathy}{nn\_bathy} (found in \nam{dom}{dom} namelist (\texttt{DOMAINCFG} variant) ): \begin{description} \item [{\np[=0]{nn_bathy}{nn\_bathy}}]: a flat-bottom domain is defined. The total depth $z_w (jpk)$ is given by the coordinate transformation. The domain can either be a closed basin or a periodic channel depending on the parameter \np{jperio}{jperio}. \item [{\np[=-1]{nn_bathy}{nn\_bathy}}]: a domain with a bump of topography one third of the domain width at the central latitude. This is meant for the "EEL-R5" configuration, a periodic or open boundary channel with a seamount. \item [{\np[=1]{nn_bathy}{nn\_bathy}}]: read a bathymetry and ice shelf draft (if needed). The \ifile{bathy\_meter} file (Netcdf format) provides the ocean depth (positive, in meters) at each grid point of the model grid. The bathymetry is usually built by interpolating a standard bathymetry product (\eg\ ETOPO2) onto the horizontal ocean mesh. Defining the bathymetry also defines the coastline: where the bathymetry is zero, no wet levels are defined (all levels are masked). \end{description} %% ================================================================================================= \subsection{Choice of vertical grid} \label{sec:DOMCFG_vgrd} After reading the bathymetry, the algorithm for vertical grid definition differs between the different options: \begin{description} \item [\forcode{ln_zco = .true.}] set a reference coordinate transformation $z_0(k)$, and set $z(i,j,k,t) = z_0(k)$ where $z_0(k)$ is the closest match to the depth at $(i,j)$. \item [\forcode{ln_zps = .true.}] set a reference coordinate transformation $z_0(k)$, and calculate the thickness of the deepest level at each $(i,j)$ point using the bathymetry, to obtain the final three-dimensional depth and scale factor arrays. \item [\forcode{ln_sco = .true.}] smooth the bathymetry to fulfill the hydrostatic consistency criteria and set the three-dimensional transformation. \item [\forcode{s-z and s-zps}] smooth the bathymetry to fulfill the hydrostatic consistency criteria and set the three-dimensional transformation $z(i,j,k)$, and possibly introduce masking of extra land points to better fit the original bathymetry file. \end{description} %% ================================================================================================= \subsubsection[$Z$-coordinate with uniform thickness levels (\forcode{ln_zco})]{$Z$-coordinate with uniform thickness levels (\protect\np{ln_zco}{ln\_zco})} \label{subsec:DOMCFG_zco} With this option the model topography can be fully described by the reference vertical coordinate and a 2D integer field giving the number of wet levels at each location (\forcode{bathy_level}). The resulting match to the real topography is likely to be poor though (especially with thick, deep levels) and slopes poorly represented. This option is rarely used in modern simulations but it can be useful for testing purposes. %% ================================================================================================= \subsubsection[$Z$-coordinate with partial step (\forcode{ln_zps})]{$Z$-coordinate with partial step (\protect\np{ln_zps}{ln\_zps})} \label{subsec:DOMCFG_zps} In $z$-coordinate partial step, the depths of the model levels are defined by the reference analytical function $z_0(k)$ as described in \autoref{sec:DOMCFG_zref}, \textit{except} in the bottom layer. The thickness of the bottom layer is allowed to vary as a function of geographical location $(\lambda,\varphi)$ to allow a better representation of the bathymetry, especially in the case of small slopes (where the bathymetry varies by less than one level thickness from one grid point to the next). The reference layer thicknesses $e_{3t}^0$ have been defined in the absence of bathymetry. With partial steps, layers from 1 to \jp{jpk}-2 can have a thickness smaller than $e_{3t}(jk)$. The model deepest layer (\jp{jpk}-1) is allowed to have either a smaller or larger thickness than $e_{3t}(jpk)$: the maximum thickness allowed is $2*e_{3t}(jpk - 1)$. This has to be kept in mind when specifying values in \nam{dom}{dom} namelist (\texttt{DOMAINCFG} variant), such as the maximum depth \np{pphmax}{pphmax} in partial steps. For example, with \np{pphmax}{pphmax}~$= 5750~m$ for the DRAKKAR 45 layer grid, the maximum ocean depth allowed is actually $6000~m$ (the default thickness $e_{3t}(jpk - 1)$ being $250~m$). Two variables in the namdom namelist are used to define the partial step vertical grid. The mimimum water thickness (in meters) allowed for a cell partially filled with bathymetry at level jk is the minimum of \np{rn_e3zps_min}{rn\_e3zps\_min} (thickness in meters, usually $20~m$) or $e_{3t}(jk)*$\np{rn_e3zps_rat}{rn\_e3zps\_rat} (a fraction, usually 10\%, of the default thickness $e_{3t}(jk)$). %% ================================================================================================= \subsubsection[$S$-coordinate (\forcode{ln_sco})]{$S$-coordinate (\protect\np{ln_sco}{ln\_sco})} \label{sec:DOMCFG_sco} \begin{listing} \nlst{namzgr_sco_domcfg} \caption{\forcode{&namzgr_sco_domcfg}} \label{lst:namzgr_sco_domcfg} \end{listing} Options are defined in \nam{zgr_sco}{zgr\_sco} (\texttt{DOMAINcfg} only). In $s$-coordinate (\np[=.true.]{ln_sco}{ln\_sco}), the depth and thickness of the model levels are defined from the product of a depth field and either a stretching function or its derivative, respectively: \begin{align*} % \label{eq:DOMCFG_sco_ana} z(k) &= h(i,j) \; z_0 (k) \\ e_3(k) &= h(i,j) \; z_0'(k) \end{align*} where $h$ is the depth of the last $w$-level ($z_0(k)$) defined at the $t$-point location in the horizontal and $z_0(k)$ is a function which varies from $0$ at the sea surface to $1$ at the ocean bottom. The depth field $h$ is not necessary the ocean depth, since a mixed step-like and bottom-following representation of the topography can be used (\autoref{fig:DOM_z_zps_s_sps}) or an envelop bathymetry can be defined (\autoref{fig:DOM_z_zps_s_sps}). The namelist parameter \np{rn_rmax}{rn\_rmax} determines the slope at which the terrain-following coordinate intersects the sea bed and becomes a pseudo z-coordinate. The coordinate can also be hybridised by specifying \np{rn_sbot_min}{rn\_sbot\_min} and \np{rn_sbot_max}{rn\_sbot\_max} as the minimum and maximum depths at which the terrain-following vertical coordinate is calculated. Options for stretching the coordinate are provided as examples, but care must be taken to ensure that the vertical stretch used is appropriate for the application. The original default \NEMO\ s-coordinate stretching is available if neither of the other options are specified as true (\np[=.false.]{ln_s_SH94}{ln\_s\_SH94} and \np[=.false.]{ln_s_SF12}{ln\_s\_SF12}). This uses a depth independent $\tanh$ function for the stretching \citep{madec.delecluse.ea_JPO96}: \[ z = s_{min} + C (s) (H - s_{min}) % \label{eq:DOMCFG_SH94_1} \] where $s_{min}$ is the depth at which the $s$-coordinate stretching starts and allows a $z$-coordinate to placed on top of the stretched coordinate, and $z$ is the depth (negative down from the asea surface). \begin{gather*} s = - \frac{k}{n - 1} \quad \text{and} \quad 0 \leq k \leq n - 1 % \label{eq:DOMCFG_s} \\ \label{eq:DOMCFG_sco_function} C(s) = \frac{[\tanh(\theta \, (s + b)) - \tanh(\theta \, b)]}{2 \; \sinh(\theta)} \end{gather*} A stretching function, modified from the commonly used \citet{song.haidvogel_JCP94} stretching (\np[=.true.]{ln_s_SH94}{ln\_s\_SH94}), is also available and is more commonly used for shelf seas modelling: \[ C(s) = (1 - b) \frac{\sinh(\theta s)}{\sinh(\theta)} + b \frac{\tanh \lt[ \theta \lt(s + \frac{1}{2} \rt) \rt] - \tanh \lt( \frac{\theta}{2} \rt)} { 2 \tanh \lt( \frac{\theta}{2} \rt)} \label{eq:DOMCFG_SH94_2} \] \begin{figure}[!ht] \centering \includegraphics[width=0.66\textwidth]{DOMCFG_sco_function} \caption[DOMAINcfg: examples of the stretching function applied to a seamount]{ Examples of the stretching function applied to a seamount; from left to right: surface, surface and bottom, and bottom intensified resolutions} \label{fig:DOMCFG_sco_function} \end{figure} where $H_c$ is the critical depth (\np{rn_hc}{rn\_hc}) at which the coordinate transitions from pure $\sigma$ to the stretched coordinate, and $\theta$ (\np{rn_theta}{rn\_theta}) and $b$ (\np{rn_bb}{rn\_bb}) are the surface and bottom control parameters such that $0 \leqslant \theta \leqslant 20$, and $0 \leqslant b \leqslant 1$. $b$ has been designed to allow surface and/or bottom increase of the vertical resolution (\autoref{fig:DOMCFG_sco_function}). Another example has been provided at version 3.5 (\np{ln_s_SF12}{ln\_s\_SF12}) that allows a fixed surface resolution in an analytical terrain-following stretching \citet{siddorn.furner_OM13}. In this case the a stretching function $\gamma$ is defined such that: \begin{equation} z = - \gamma h \quad \text{with} \quad 0 \leq \gamma \leq 1 % \label{eq:DOMCFG_z} \end{equation} The function is defined with respect to $\sigma$, the unstretched terrain-following coordinate: \begin{gather*} % \label{eq:DOMCFG_gamma_deriv} \gamma = A \lt( \sigma - \frac{1}{2} (\sigma^2 + f (\sigma)) \rt) + B \lt( \sigma^3 - f (\sigma) \rt) + f (\sigma) \\ \intertext{Where:} \label{eq:DOMCFG_gamma} f(\sigma) = (\alpha + 2) \sigma^{\alpha + 1} - (\alpha + 1) \sigma^{\alpha + 2} \quad \text{and} \quad \sigma = \frac{k}{n - 1} \end{gather*} This gives an analytical stretching of $\sigma$ that is solvable in $A$ and $B$ as a function of the user prescribed stretching parameter $\alpha$ (\np{rn_alpha}{rn\_alpha}) that stretches towards the surface ($\alpha > 1.0$) or the bottom ($\alpha < 1.0$) and user prescribed surface (\np{rn_zs}{rn\_zs}) and bottom depths. The bottom cell depth in this example is given as a function of water depth: \[ % \label{eq:DOMCFG_zb} Z_b = h a + b \] where the namelist parameters \np{rn_zb_a}{rn\_zb\_a} and \np{rn_zb_b}{rn\_zb\_b} are $a$ and $b$ respectively. \begin{figure}[!ht] \centering \includegraphics[width=0.66\textwidth]{DOMCFG_compare_coordinates_surface} \caption[DOMAINcfg: comparison of $s$- and $z$-coordinate]{ A comparison of the \citet{song.haidvogel_JCP94} $S$-coordinate (solid lines), a 50 level $Z$-coordinate (contoured surfaces) and the \citet{siddorn.furner_OM13} $S$-coordinate (dashed lines) in the surface $100~m$ for a idealised bathymetry that goes from $50~m$ to $5500~m$ depth. For clarity every third coordinate surface is shown.} \label{fig:DOMCFG_fig_compare_coordinates_surface} \end{figure} % >>>>>>>>>>>>>>>>>>>>>>>>>>>> This gives a smooth analytical stretching in computational space that is constrained to given specified surface and bottom grid cell thicknesses in real space. This is not to be confused with the hybrid schemes that superimpose geopotential coordinates on terrain following coordinates thus creating a non-analytical vertical coordinate that therefore may suffer from large gradients in the vertical resolutions. This stretching is less straightforward to implement than the \citet{song.haidvogel_JCP94} stretching, but has the advantage of resolving diurnal processes in deep water and has generally flatter slopes. As with the \citet{song.haidvogel_JCP94} stretching the stretch is only applied at depths greater than the critical depth $h_c$. In this example two options are available in depths shallower than $h_c$, with pure sigma being applied if the \np{ln_sigcrit}{ln\_sigcrit} is true and pure z-coordinates if it is false (the z-coordinate being equal to the depths of the stretched coordinate at $h_c$). Minimising the horizontal slope of the vertical coordinate is important in terrain-following systems as large slopes lead to hydrostatic consistency. A hydrostatic consistency parameter diagnostic following \citet{haney_JPO91} has been implemented, and is output as part of the model mesh file at the start of the run. %% ================================================================================================= \subsubsection[\zstar- or \sstar-coordinate (\forcode{ln_linssh})]{\zstar- or \sstar-coordinate (\protect\np{ln_linssh}{ln\_linssh})} \label{subsec:DOMCFG_zgr_star} This option is described in the Report by Levier \textit{et al.} (2007), available on the \NEMO\ web site. \section{Ice shelf cavity definition} \label{subsec:zgrisf} If the under ice shelf seas are opened (\np{ln_isfcav}{ln\_isfcav}), the depth of the ice shelf/ocean interface has to be include in the \ifile{isfdraft\_meter} file (Netcdf format). This file need to include the \ifile{isf\_draft} variable. A positive value will me an ice shelf/ocean or ice shelf bedrock interface below the reference 0m ssh. The exact shape of the ice shelf cavity (grounding line position and minimum thickness of the water column under an ice shelf, ...) can be specify in \nam{lst:namzgr_isf}. \begin{listing} \nlst{namzgr_isf_domcfg} \caption{\forcode{&namzgr_isf}} \label{lst:namzgr_isf} \end{listing} The options available to define the shape of the under ice shelf cavities are listed in \nam{namzgr_isf}{namzgr\_isf} (\texttt{DOMAINcfg} only, \autoref{lst:namzgr_isf}). \subsection{Model ice shelf draft definition} \label{subsec:zgrisf_isfd} First of all, the tool make sure, the ice shelf draft ($h_{isf}$) is sensible and compatible with the bathymetry. There are 3 compulsory steps to achieve this: \begin{description} \item{\np{rn_isfdep_min}{rn\_isfdep\_min}:} this is the minimum ice shelf draft. This is to make sure there is no ridiculous thin ice shelf. If \np{rn_isfdep_min}{rn\_isfdep\_min} is smaller than the surface level, \np{rn_isfdep_min}{rn\_isfdep\_min} is set to $e3t\_1d(1)$. Where $h_{isf} < MAX(e3t\_1d(1),\np{rn_isfdep_min}{rn\_isfdep\_min}$), $h_{isf}$ is set to \np{rn_isfdep_min}{rn\_isfdep\_min}. \item{\np{rn_glhw_min}{rn\_glhw\_min}:} This parameter is used to define the grounding line position. Where the difference between the bathymetry and the ice shelf draft is smaller than \np{rn_glhw_min}{rn\_glhw\_min}, the cell are grounded (ie masked). This step is needed to take into account possible small mismatch between ice shelf draft value and bathymetry value (sources are coming from different grid, different data processes, rounding error, ...). \item{\np{rn_isfhw_min}{rn\_isfhw\_min}:} This parameter is minimum water column thickness in the cavity. Where the water column thickness is lower than \np{rn_isfhw_min}{rn\_isfhw\_min}, the ice shelf draft is adjusted to match this criterion. If for any reason, this adjustement break the minimum ice shelf draft allowed (\np{rn_isfdep_min}{rn\_isfdep\_min}), the cell is masked. \end{description} Once all these adjustements are made, if the water column thickness contains one cell wide channels, these channels can be closed using \np{ln_isfchannel}{ln\_isfchannel}. \subsection{Model top level definition} After the definition of the ice shelf draft, the tool defines the top level. The compulsory criterion is that the water column needs at least 2 wet cells in the water column at U- and V-points. To do so, if there one cell wide water column, the tools adjust the ice shelf draft to fillful the requierement.\\ The process is the following: \begin{description} \item{step 1:} The top level is defined in the same way as the bottom level is defined. \item{step 2:} The isolated grid point in the bathymetry are filled (as it is done in a domain without ice shelf) \item{step 3:} The tools make sure, the top level is above or equal to the bottom level \item{step 4:} If the water column at a U- or V- point is one wet cell wide, the ice shelf draft is adjusted. So the actual top cell become fully open and the new top cell thickness is set to the minimum cell thickness allowed (following the same logic as for the bottom partial cell). This step is iterated 4 times to ensure the condition is fullfill along the 4 sides of the cell. \end{description} In case of steep slope and shallow water column, it likely that 2 cells are disconnected (bathymetry above its neigbourg ice shelf draft). The option \np{ln_isfconnect}{ln\_isfconnect} allow the tool to force the connection between these 2 cells. Some limiters in meter or levels on the digging allowed by the tool are available (respectively, \np{rn_zisfmax}{rn\_zisfmax} or \np{rn_kisfmax}{rn\_kisfmax}). This will prevent the formation of subglacial lakes at the expense of long vertical pipe to connect cells at very different levels. \subsection{Subglacial lakes} Despite careful setting of your ice shelf draft and bathymetry input file as well as setting described in \autoref{subsec:zgrisf_isfd}, some situation are unavoidable. For exemple if you setup your ice shelf draft and bathymetry to do ocean/ice sheet coupling, you may decide to fill the whole antarctic with a bathymetry and an ice shelf draft value (ice/bedrock interface depth when grounded). If you do so, the subglacial lakes will show up (Vostock for example). An other possibility is with coarse vertical resolution, some ice shelves could be cut in 2 parts: one connected to the main ocean and an other one closed which can be considered as a subglacial sea be the model.\\ The namelist option \np{ln_isfsubgl}{ln\_isfsubgl} allow you to remove theses subglacial lakes. This may be useful for esthetical reason or for stability reasons: \begin{description} \item $\bullet$ In a subglacial lakes, in case of very weak circulation (often the case), the only heat flux is the conductive heat flux through the ice sheet. This will lead to constant freezing until water reaches -20C. This is one of the defitiency of the 3 equation melt formulation (for details on this formulation, see: \autoref{sec:isf}). \item $\bullet$ In case of coupling with an ice sheet model, the ssh in the subglacial lakes and the main ocean could be very different (ssh initial adjustement for example), and so if for any reason both a connected at some point, the model is likely to fall over.\\ \end{description} \section{Closed sea definition} \label{sec:clocfg} \begin{listing} \nlst{namclo_domcfg} \caption{\forcode{&namclo}} \label{lst:namclo} \end{listing} The options available to define the closed seas and how closed sea net fresh water input will be redistributed by NEMO are listed in \nam{clo} (\texttt{DOMAINcfg} only, \autoref{lst:namclo}). The individual definition of each closed sea is managed by \np{sn_lake}{sn\_lake}. In this fields the user needs to defined:\\ \begin{description} \item $\bullet$ the name of the closed sea (print output purposes). \item $\bullet$ the seed location to define the area of the closed sea (if seed on land because not present in this configuration, this closed sea will be ignored).\\ \item $\bullet$ the seed location for the target area. \item $\bullet$ the type of target area ('local','coast' or 'global'). See point 6 for definition of these cases. \item $\bullet$ the type of redistribution scheme for the net fresh water flux over the closed sea (as a runoff in a target area, as emp in a target area, as emp globally). For the runoff case, if the net fwf is negative, it will be redistribut globally. \item $\bullet$ the radius of the target area (not used for the 'global' case). So the target defined by a 'local' target area of a radius of 100km, for example, correspond to all the wet points within this radius. The coastal case will return only the coastal point within the specifid radius. \item $\bullet$ the target id. This target id is used to group multiple lakes into the same river ouflow (Great Lakes for example). \end{description} The closed sea module defines a number of masks in the \ifile{domain\_cfg} output: \begin{description} \item[\textit{mask\_opensea}:] a mask of the main ocean without all the closed seas closed. This mask is defined by a flood filling algorithm with an initial seed (localisation defined by \np{rn_lon_opnsea}{rn\_lon\_opnsea} and \np{rn_lat_opnsea}{rn\_lat\_opnsea}). \item[\textit{mask\_csglo}, \textit{mask\_csrnf}, \textit{mask\_csemp}:] a mask of all the closed seas defined in the namelist by \np{sn_lake}{sn\_lake} for each redistribution scheme. The total number of defined closed seas has to be defined in \np{nn_closea}{nn\_closea}. \item[\textit{mask\_csgrpglo}, \textit{mask\_csgrprnf}, \textit{mask\_csgrpemp}:] a mask of all the closed seas and targets grouped by target id for each type of redistribution scheme. \item[\textit{mask\_csundef}:] a mask of all the closed sea not defined in \np{sn_lake}{sn\_lake}. This will allows NEMO to mask them if needed or to inform the user of potential minor issues in its bathymetry. \end{description} \subinc{\input{../../global/epilogue}} \end{document}