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1 % $Header: /u/gcmpack/manual/part3/case_studies/rotating_tank/tank.tex,v 1.3 2004/07/26 16:21:15 afe Exp $
2 % $Name: $
3
4 \bodytext{bgcolor="#FFFFFFFF"}
5
6 %\begin{center}
7 %{\Large \bf Using MITgcm to Simulate a Rotating Tank in Cylindrical
8 %Coordinates}
9 %
10 %\vspace*{4mm}
11 %
12 %\vspace*{3mm}
13 %{\large May 2001}
14 %\end{center}
15
16 \section{A Rotating Tank in Cylindrical Coordinates}
17 \label{sect:eg-tank}
18 \label{www:tutorials}
19
20 This section illustrates an example of MITgcm simulating a laboratory
21 experiment on much smaller scales than those common to geophysical
22 fluid dynamics.
23
24 \subsection{Overview}
25 \label{www:tutorials}
26
27
28 This example experiment demonstrates using the MITgcm to simulate
29 a laboratory experiment with a rotating tank of water with an ice
30 bucket in the center. The simulation is configured for a laboratory
31 scale on a
32 $3^{\circ}$ $\times$ 20cm
33 cyclindrical grid with twenty-nine vertical
34 levels.
35 \\
36
37
38
39 This example experiment demonstrates using the MITgcm to simulate
40 a Barotropic, wind-forced, ocean gyre circulation. The experiment
41 is a numerical rendition of the gyre circulation problem similar
42 to the problems described analytically by Stommel in 1966
43 \cite{Stommel66} and numerically in Holland et. al \cite{Holland75}.
44
45 In this experiment the model
46 is configured to represent a rectangular enclosed box of fluid,
47 $1200 \times 1200 $~km in lateral extent. The fluid is $5$~km deep and is forced
48 by a constant in time zonal wind stress, $\tau_x$, that varies sinusoidally
49 in the ``north-south'' direction. Topologically the grid is Cartesian and
50 the coriolis parameter $f$ is defined according to a mid-latitude beta-plane
51 equation
52
53 \begin{equation}
54 \label{EQ:eg-baro-fcori}
55 f(y) = f_{0}+\beta y
56 \end{equation}
57
58 \noindent where $y$ is the distance along the ``north-south'' axis of the
59 simulated domain. For this experiment $f_{0}$ is set to $10^{-4}s^{-1}$ in
60 (\ref{EQ:eg-baro-fcori}) and $\beta = 10^{-11}s^{-1}m^{-1}$.
61 \\
62 \\
63 The sinusoidal wind-stress variations are defined according to
64
65 \begin{equation}
66 \label{EQ:eg-baro-taux}
67 \tau_x(y) = \tau_{0}\sin(\pi \frac{y}{L_y})
68 \end{equation}
69
70 \noindent where $L_{y}$ is the lateral domain extent ($1200$~km) and
71 $\tau_0$ is set to $0.1N m^{-2}$.
72 \\
73 \\
74 Figure \ref{FIG:eg-baro-simulation_config}
75 summarizes the configuration simulated.
76
77 %% === eh3 ===
78 \begin{figure}
79 %% \begin{center}
80 %% \resizebox{7.5in}{5.5in}{
81 %% \includegraphics*[0.2in,0.7in][10.5in,10.5in]
82 %% {part3/case_studies/barotropic_gyre/simulation_config.eps} }
83 %% \end{center}
84 \centerline{
85 \scalefig{.95}
86 \epsfbox{part3/case_studies/barotropic_gyre/simulation_config.eps}
87 }
88 \caption{Schematic of simulation domain and wind-stress forcing function
89 for barotropic gyre numerical experiment. The domain is enclosed bu solid
90 walls at $x=$~0,1200km and at $y=$~0,1200km.}
91 \label{FIG:eg-baro-simulation_config}
92 \end{figure}
93
94 \subsection{Equations Solved}
95 \label{www:tutorials}
96 The model is configured in hydrostatic form. The implicit free surface form of the
97 pressure equation described in Marshall et. al \cite{marshall:97a} is
98 employed.
99 A horizontal Laplacian operator $\nabla_{h}^2$ provides viscous
100 dissipation. The wind-stress momentum input is added to the momentum equation
101 for the ``zonal flow'', $u$. Other terms in the model
102 are explicitly switched off for this experiment configuration (see section
103 \ref{SEC:code_config} ), yielding an active set of equations solved in this
104 configuration as follows
105
106 \begin{eqnarray}
107 \label{EQ:eg-baro-model_equations}
108 \frac{Du}{Dt} - fv +
109 g\frac{\partial \eta}{\partial x} -
110 A_{h}\nabla_{h}^2u
111 & = &
112 \frac{\tau_{x}}{\rho_{0}\Delta z}
113 \\
114 \frac{Dv}{Dt} + fu + g\frac{\partial \eta}{\partial y} -
115 A_{h}\nabla_{h}^2v
116 & = &
117 0
118 \\
119 \frac{\partial \eta}{\partial t} + \nabla_{h}\cdot \vec{u}
120 &=&
121 0
122 \end{eqnarray}
123
124 \noindent where $u$ and $v$ and the $x$ and $y$ components of the
125 flow vector $\vec{u}$.
126 \\
127
128
129 \subsection{Discrete Numerical Configuration}
130 \label{www:tutorials}
131
132 The domain is discretised with
133 a uniform grid spacing in the horizontal set to
134 $\Delta x=\Delta y=20$~km, so
135 that there are sixty grid cells in the $x$ and $y$ directions. Vertically the
136 model is configured with a single layer with depth, $\Delta z$, of $5000$~m.
137
138 \subsubsection{Numerical Stability Criteria}
139 \label{www:tutorials}
140
141 The Laplacian dissipation coefficient, $A_{h}$, is set to $400 m s^{-1}$.
142 This value is chosen to yield a Munk layer width \cite{adcroft:95},
143
144 \begin{eqnarray}
145 \label{EQ:eg-baro-munk_layer}
146 M_{w} = \pi ( \frac { A_{h} }{ \beta } )^{\frac{1}{3}}
147 \end{eqnarray}
148
149 \noindent of $\approx 100$km. This is greater than the model
150 resolution $\Delta x$, ensuring that the frictional boundary
151 layer is well resolved.
152 \\
153
154 \noindent The model is stepped forward with a
155 time step $\delta t=1200$secs. With this time step the stability
156 parameter to the horizontal Laplacian friction \cite{adcroft:95}
157
158
159
160 \begin{eqnarray}
161 \label{EQ:eg-baro-laplacian_stability}
162 S_{l} = 4 \frac{A_{h} \delta t}{{\Delta x}^2}
163 \end{eqnarray}
164
165 \noindent evaluates to 0.012, which is well below the 0.3 upper limit
166 for stability.
167 \\
168
169 \noindent The numerical stability for inertial oscillations
170 \cite{adcroft:95}
171
172 \begin{eqnarray}
173 \label{EQ:eg-baro-inertial_stability}
174 S_{i} = f^{2} {\delta t}^2
175 \end{eqnarray}
176
177 \noindent evaluates to $0.0144$, which is well below the $0.5$ upper
178 limit for stability.
179 \\
180
181 \noindent The advective CFL \cite{adcroft:95} for an extreme maximum
182 horizontal flow speed of $ | \vec{u} | = 2 ms^{-1}$
183
184 \begin{eqnarray}
185 \label{EQ:eg-baro-cfl_stability}
186 S_{a} = \frac{| \vec{u} | \delta t}{ \Delta x}
187 \end{eqnarray}
188
189 \noindent evaluates to 0.12. This is approaching the stability limit
190 of 0.5 and limits $\delta t$ to $1200s$.
191
192 \subsection{Code Configuration}
193 \label{www:tutorials}
194 \label{SEC:eg-baro-code_config}
195
196 The model configuration for this experiment resides under the
197 directory {\it verification/exp0/}. The experiment files
198 \begin{itemize}
199 \item {\it input/data}
200 \item {\it input/data.pkg}
201 \item {\it input/eedata},
202 \item {\it input/windx.sin\_y},
203 \item {\it input/topog.box},
204 \item {\it code/CPP\_EEOPTIONS.h}
205 \item {\it code/CPP\_OPTIONS.h},
206 \item {\it code/SIZE.h}.
207 \end{itemize}
208 contain the code customizations and parameter settings for this
209 experiments. Below we describe the customizations
210 to these files associated with this experiment.
211
212 \subsubsection{File {\it input/data}}
213 \label{www:tutorials}
214
215 This file, reproduced completely below, specifies the main parameters
216 for the experiment. The parameters that are significant for this configuration
217 are
218
219 \begin{itemize}
220
221 \item Line 7, \begin{verbatim} viscAh=4.E2, \end{verbatim} this line sets
222 the Laplacian friction coefficient to $400 m^2s^{-1}$
223 \item Line 10, \begin{verbatim} beta=1.E-11, \end{verbatim} this line sets
224 $\beta$ (the gradient of the coriolis parameter, $f$) to $10^{-11} s^{-1}m^{-1}$
225
226 \item Lines 15 and 16
227 \begin{verbatim}
228 rigidLid=.FALSE.,
229 implicitFreeSurface=.TRUE.,
230 \end{verbatim}
231 these lines suppress the rigid lid formulation of the surface
232 pressure inverter and activate the implicit free surface form
233 of the pressure inverter.
234
235 \item Line 27,
236 \begin{verbatim}
237 startTime=0,
238 \end{verbatim}
239 this line indicates that the experiment should start from $t=0$
240 and implicitly suppresses searching for checkpoint files associated
241 with restarting an numerical integration from a previously saved state.
242
243 \item Line 29,
244 \begin{verbatim}
245 endTime=12000,
246 \end{verbatim}
247 this line indicates that the experiment should start finish at $t=12000s$.
248 A restart file will be written at this time that will enable the
249 simulation to be continued from this point.
250
251 \item Line 30,
252 \begin{verbatim}
253 deltaTmom=1200,
254 \end{verbatim}
255 This line sets the momentum equation timestep to $1200s$.
256
257 \item Line 39,
258 \begin{verbatim}
259 usingCartesianGrid=.TRUE.,
260 \end{verbatim}
261 This line requests that the simulation be performed in a
262 Cartesian coordinate system.
263
264 \item Line 41,
265 \begin{verbatim}
266 delX=60*20E3,
267 \end{verbatim}
268 This line sets the horizontal grid spacing between each x-coordinate line
269 in the discrete grid. The syntax indicates that the discrete grid
270 should be comprise of $60$ grid lines each separated by $20 \times 10^{3}m$
271 ($20$~km).
272
273 \item Line 42,
274 \begin{verbatim}
275 delY=60*20E3,
276 \end{verbatim}
277 This line sets the horizontal grid spacing between each y-coordinate line
278 in the discrete grid to $20 \times 10^{3}m$ ($20$~km).
279
280 \item Line 43,
281 \begin{verbatim}
282 delZ=5000,
283 \end{verbatim}
284 This line sets the vertical grid spacing between each z-coordinate line
285 in the discrete grid to $5000m$ ($5$~km).
286
287 \item Line 46,
288 \begin{verbatim}
289 bathyFile='topog.box'
290 \end{verbatim}
291 This line specifies the name of the file from which the domain
292 bathymetry is read. This file is a two-dimensional ($x,y$) map of
293 depths. This file is assumed to contain 64-bit binary numbers
294 giving the depth of the model at each grid cell, ordered with the x
295 coordinate varying fastest. The points are ordered from low coordinate
296 to high coordinate for both axes. The units and orientation of the
297 depths in this file are the same as used in the MITgcm code. In this
298 experiment, a depth of $0m$ indicates a solid wall and a depth
299 of $-5000m$ indicates open ocean. The matlab program
300 {\it input/gendata.m} shows an example of how to generate a
301 bathymetry file.
302
303
304 \item Line 49,
305 \begin{verbatim}
306 zonalWindFile='windx.sin_y'
307 \end{verbatim}
308 This line specifies the name of the file from which the x-direction
309 surface wind stress is read. This file is also a two-dimensional
310 ($x,y$) map and is enumerated and formatted in the same manner as the
311 bathymetry file. The matlab program {\it input/gendata.m} includes example
312 code to generate a valid {\bf zonalWindFile} file.
313
314 \end{itemize}
315
316 \noindent other lines in the file {\it input/data} are standard values
317 that are described in the MITgcm Getting Started and MITgcm Parameters
318 notes.
319
320 \begin{small}
321 \input{part3/case_studies/barotropic_gyre/input/data}
322 \end{small}
323
324 \subsubsection{File {\it input/data.pkg}}
325 \label{www:tutorials}
326
327 This file uses standard default values and does not contain
328 customizations for this experiment.
329
330 \subsubsection{File {\it input/eedata}}
331 \label{www:tutorials}
332
333 This file uses standard default values and does not contain
334 customizations for this experiment.
335
336 \subsubsection{File {\it input/windx.sin\_y}}
337 \label{www:tutorials}
338
339 The {\it input/windx.sin\_y} file specifies a two-dimensional ($x,y$)
340 map of wind stress ,$\tau_{x}$, values. The units used are $Nm^{-2}$.
341 Although $\tau_{x}$ is only a function of $y$n in this experiment
342 this file must still define a complete two-dimensional map in order
343 to be compatible with the standard code for loading forcing fields
344 in MITgcm. The included matlab program {\it input/gendata.m} gives a complete
345 code for creating the {\it input/windx.sin\_y} file.
346
347 \subsubsection{File {\it input/topog.box}}
348 \label{www:tutorials}
349
350
351 The {\it input/topog.box} file specifies a two-dimensional ($x,y$)
352 map of depth values. For this experiment values are either
353 $0m$ or {\bf -delZ}m, corresponding respectively to a wall or to deep
354 ocean. The file contains a raw binary stream of data that is enumerated
355 in the same way as standard MITgcm two-dimensional, horizontal arrays.
356 The included matlab program {\it input/gendata.m} gives a complete
357 code for creating the {\it input/topog.box} file.
358
359 \subsubsection{File {\it code/SIZE.h}}
360 \label{www:tutorials}
361
362 Two lines are customized in this file for the current experiment
363
364 \begin{itemize}
365
366 \item Line 39,
367 \begin{verbatim} sNx=60, \end{verbatim} this line sets
368 the lateral domain extent in grid points for the
369 axis aligned with the x-coordinate.
370
371 \item Line 40,
372 \begin{verbatim} sNy=60, \end{verbatim} this line sets
373 the lateral domain extent in grid points for the
374 axis aligned with the y-coordinate.
375
376 \end{itemize}
377
378 \begin{small}
379 \input{part3/case_studies/barotropic_gyre/code/SIZE.h}
380 \end{small}
381
382 \subsubsection{File {\it code/CPP\_OPTIONS.h}}
383 \label{www:tutorials}
384
385 This file uses standard default values and does not contain
386 customizations for this experiment.
387
388
389 \subsubsection{File {\it code/CPP\_EEOPTIONS.h}}
390 \label{www:tutorials}
391
392 This file uses standard default values and does not contain
393 customizations for this experiment.
394

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