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%\begin{center} |
%\begin{center} |
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%{\Large \bf Using MITgcm to Simulate Global Climatalogical Ocean Circulation |
%{\Large \bf Using MITgcm to Simulate Global Climatological Ocean Circulation |
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%At Four Degree Resolution with Asynchronous Time Stepping} |
%At Four Degree Resolution with Asynchronous Time Stepping} |
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% |
% |
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%\vspace*{4mm} |
%\vspace*{4mm} |
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\subsection{Introduction} |
\subsection{Introduction} |
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This document describes the third example MITgcm experiment. The first |
This document describes the third example MITgcm experiment. The first |
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two examples illustrated how to configure the code for hydrostatic idealised |
two examples illustrated how to configure the code for hydrostatic idealized |
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geophysical fluids simulations. This example iilustrates the use of |
geophysical fluids simulations. This example illustrates the use of |
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the MITgcm for large scale ocean circulation simulation. |
the MITgcm for large scale ocean circulation simulation. |
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\subsection{Overview} |
\subsection{Overview} |
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processor desktop computer. |
processor desktop computer. |
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\\ |
\\ |
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The model is forced with climatalogical wind stress data and surface |
The model is forced with climatological wind stress data and surface |
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flux data from DaSilva \cite{DaSilva94}. Climatalogical data |
flux data from DaSilva \cite{DaSilva94}. Climatological data |
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from Levitus \cite{Levitus94} is used to initialise the model hydrography. |
from Levitus \cite{Levitus94} is used to initialize the model hydrography. |
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Levitus seasonal clmatology data is also used throughout the calculation |
Levitus seasonal climatology data is also used throughout the calculation |
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to provide additional air-sea fluxes. |
to provide additional air-sea fluxes. |
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These fluxes are combined with the DaSilva climatalogical estimates of |
These fluxes are combined with the DaSilva climatological estimates of |
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surface heat flux and fresh water, resulting in a mixed boundary |
surface heat flux and fresh water, resulting in a mixed boundary |
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condition of the style decribed in Haney \cite{Haney}. |
condition of the style described in Haney \cite{Haney}. |
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Altogether, this yields the following forcing applied |
Altogether, this yields the following forcing applied |
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in the model surface layer. |
in the model surface layer. |
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|
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$\Delta \phi=\Delta \lambda=4^{\circ}$, so |
$\Delta \phi=\Delta \lambda=4^{\circ}$, so |
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that there are ninety grid cells in the zonal and forty in the |
that there are ninety grid cells in the zonal and forty in the |
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meridional direction. The internal model coordinate variables |
meridional direction. The internal model coordinate variables |
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$x$ and $y$ are initialised according to |
$x$ and $y$ are initialized according to |
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\begin{eqnarray} |
\begin{eqnarray} |
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x=r\cos(\phi),~\Delta x & = &r\cos(\Delta \phi) \\ |
x=r\cos(\phi),~\Delta x & = &r\cos(\Delta \phi) \\ |
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y=r\lambda,~\Delta x &= &r\Delta \lambda |
y=r\lambda,~\Delta x &= &r\Delta \lambda |
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\Delta z_{20}=815\,{\rm m} |
\Delta z_{20}=815\,{\rm m} |
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$ (here the numeric subscript indicates the model level index number, ${\tt k}$). |
$ (here the numeric subscript indicates the model level index number, ${\tt k}$). |
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The implicit free surface form of the pressure equation described in Marshall et. al |
The implicit free surface form of the pressure equation described in Marshall et. al |
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\cite{Marshall97a} is employed. A laplacian operator, $\nabla^2$, provides viscous |
\cite{Marshall97a} is employed. A Laplacian operator, $\nabla^2$, provides viscous |
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dissipation. Thermal and haline diffusion is also represented by a laplacian operator. |
dissipation. Thermal and haline diffusion is also represented by a Laplacian operator. |
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|
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Wind-stress forcing is added to the momentum equations for both |
Wind-stress forcing is added to the momentum equations for both |
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the zonal flow, $u$ and the merdional flow $v$, according to equations |
the zonal flow, $u$ and the meridional flow $v$, according to equations |
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(\ref{EQ:global_forcing_fu}) and (\ref{EQ:global_forcing_fv}). |
(\ref{EQ:global_forcing_fu}) and (\ref{EQ:global_forcing_fv}). |
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Thermodynamic forcing inputs are added to the equations for |
Thermodynamic forcing inputs are added to the equations for |
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potential temperature, $\theta$, and salinity, $S$, according to equations |
potential temperature, $\theta$, and salinity, $S$, according to equations |
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\subsubsection{Numerical Stability Criteria} |
\subsubsection{Numerical Stability Criteria} |
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The laplacian dissipation coefficient, $A_{h}$, is set to $5 \times 10^5 m s^{-1}$. |
The Laplacian dissipation coefficient, $A_{h}$, is set to $5 \times 10^5 m s^{-1}$. |
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This value is chosen to yield a Munk layer width \cite{Adcroft_thesis}, |
This value is chosen to yield a Munk layer width \cite{Adcroft_thesis}, |
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\begin{eqnarray} |
\begin{eqnarray} |
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\label{EQ:munk_layer} |
\label{EQ:munk_layer} |
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\noindent The model is stepped forward with a |
\noindent The model is stepped forward with a |
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time step $\delta t_{\theta}=30~{\rm hours}$ for thermodynamic variables and |
time step $\delta t_{\theta}=30~{\rm hours}$ for thermodynamic variables and |
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$\delta t_{v}=40~{\rm minutes}$ for momentum terms. With this time step, the stability |
$\delta t_{v}=40~{\rm minutes}$ for momentum terms. With this time step, the stability |
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parameter to the horizontal laplacian friction \cite{Adcroft_thesis} |
parameter to the horizontal Laplacian friction \cite{Adcroft_thesis} |
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\begin{eqnarray} |
\begin{eqnarray} |
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\label{EQ:laplacian_stability} |
\label{EQ:laplacian_stability} |
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S_{l} = 4 \frac{A_{h} \delta t_{v}}{{\Delta x}^2} |
S_{l} = 4 \frac{A_{h} \delta t_{v}}{{\Delta x}^2} |
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\end{eqnarray} |
\end{eqnarray} |
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\noindent evaluates to $0.015$ for the smallest model |
\noindent evaluates to $0.015$ for the smallest model |
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level spcing ($\Delta z_{1}=50{\rm m}$) which is again well below |
level spacing ($\Delta z_{1}=50{\rm m}$) which is again well below |
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the upper stability limit. |
the upper stability limit. |
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\\ |
\\ |
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\label{EQ:laplacian_stability_xtheta} |
\label{EQ:laplacian_stability_xtheta} |
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S_{l} = \frac{4 K_{h} \delta t_{\theta}}{{\Delta x}^2} |
S_{l} = \frac{4 K_{h} \delta t_{\theta}}{{\Delta x}^2} |
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\end{eqnarray} |
\end{eqnarray} |
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evaluates to $0.07$, well below the stabilit limit of $S_{l} \approx 0.5$. The |
evaluates to $0.07$, well below the stability limit of $S_{l} \approx 0.5$. The |
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stability parameter related to $K_{z}$ |
stability parameter related to $K_{z}$ |
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\begin{eqnarray} |
\begin{eqnarray} |
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\label{EQ:laplacian_stability_ztheta} |
\label{EQ:laplacian_stability_ztheta} |
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limit of 0.5. |
limit of 0.5. |
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\\ |
\\ |
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\noindent The stability parameter for internal gravity waves propogating |
\noindent The stability parameter for internal gravity waves propagating |
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with a maximum speed of $c_{g}=10~{\rm ms}^{-1}$ |
with a maximum speed of $c_{g}=10~{\rm ms}^{-1}$ |
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\cite{Adcroft_thesis} |
\cite{Adcroft_thesis} |
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\item {\it code/CPP\_OPTIONS.h}, |
\item {\it code/CPP\_OPTIONS.h}, |
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\item {\it code/SIZE.h}. |
\item {\it code/SIZE.h}. |
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\end{itemize} |
\end{itemize} |
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contain the code customisations and parameter settings for these |
contain the code customizations and parameter settings for these |
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experiements. Below we describe the customisations |
experiments. Below we describe the customizations |
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to these files associated with this experiment. |
to these files associated with this experiment. |
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\subsubsection{File {\it input/data}} |
\subsubsection{File {\it input/data}} |
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\item Line 15, |
\item Line 15, |
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\begin{verbatim} viscAz=1.E-3, \end{verbatim} |
\begin{verbatim} viscAz=1.E-3, \end{verbatim} |
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this line sets the vertical laplacian dissipation coefficient to |
this line sets the vertical Laplacian dissipation coefficient to |
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$1 \times 10^{-3} {\rm m^{2}s^{-1}}$. Boundary conditions |
$1 \times 10^{-3} {\rm m^{2}s^{-1}}$. Boundary conditions |
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for this operator are specified later. This variable is copied into |
for this operator are specified later. This variable is copied into |
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model general vertical coordinate variable {\bf viscAr}. |
model general vertical coordinate variable {\bf viscAr}. |
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\begin{verbatim} |
\begin{verbatim} |
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viscAh=5.E5, |
viscAh=5.E5, |
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\end{verbatim} |
\end{verbatim} |
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this line sets the horizontal laplacian frictional dissipation coefficient to |
this line sets the horizontal Laplacian frictional dissipation coefficient to |
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$5 \times 10^{5} {\rm m^{2}s^{-1}}$. Boundary conditions |
$5 \times 10^{5} {\rm m^{2}s^{-1}}$. Boundary conditions |
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for this operator are specified later. |
for this operator are specified later. |
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no_slip_sides=.FALSE. |
no_slip_sides=.FALSE. |
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\end{verbatim} |
\end{verbatim} |
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this line selects a free-slip lateral boundary condition for |
this line selects a free-slip lateral boundary condition for |
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the horizontal laplacian friction operator |
the horizontal Laplacian friction operator |
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e.g. $\frac{\partial u}{\partial y}$=0 along boundaries in $y$ and |
e.g. $\frac{\partial u}{\partial y}$=0 along boundaries in $y$ and |
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$\frac{\partial v}{\partial x}$=0 along boundaries in $x$. |
$\frac{\partial v}{\partial x}$=0 along boundaries in $x$. |
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|
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no_slip_bottom=.TRUE. |
no_slip_bottom=.TRUE. |
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\end{verbatim} |
\end{verbatim} |
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this line selects a no-slip boundary condition for bottom |
this line selects a no-slip boundary condition for bottom |
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boundary condition in the vertical laplacian friction operator |
boundary condition in the vertical Laplacian friction operator |
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e.g. $u=v=0$ at $z=-H$, where $H$ is the local depth of the domain. |
e.g. $u=v=0$ at $z=-H$, where $H$ is the local depth of the domain. |
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\item Line 19, |
\item Line 19, |
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\begin{verbatim} |
\begin{verbatim} |
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gravity=9.81, |
gravity=9.81, |
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\end{verbatim} |
\end{verbatim} |
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Sets the gravitational acceleration coeeficient to $9.81{\rm m}{\rm s}^{-1}$.\\ |
Sets the gravitational acceleration coefficient to $9.81{\rm m}{\rm s}^{-1}$.\\ |
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\fbox{ |
\fbox{ |
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\begin{minipage}{5.0in} |
\begin{minipage}{5.0in} |
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{\it S/R CALC\_PHI\_HYD}~({\it calc\_phi\_hyd.F})\\ |
{\it S/R CALC\_PHI\_HYD}~({\it calc\_phi\_hyd.F})\\ |
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\item {\it input/windx.sin\_y}, |
\item {\it input/windx.sin\_y}, |
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\end{itemize} |
\end{itemize} |
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contain the code customisations and parameter settings for this |
contain the code customisations and parameter settings for this |
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experiements. Below we describe the customisations |
experiments. Below we describe the customisations |
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to these files associated with this experiment. |
to these files associated with this experiment. |