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1 % $Header: /u/u3/gcmpack/manual/part3/getting_started.tex,v 1.18 2004/01/29 19:22:35 edhill Exp $
2 % $Name: $
3
4 %\section{Getting started}
5
6 In this section, we describe how to use the model. In the first
7 section, we provide enough information to help you get started with
8 the model. We believe the best way to familiarize yourself with the
9 model is to run the case study examples provided with the base
10 version. Information on how to obtain, compile, and run the code is
11 found there as well as a brief description of the model structure
12 directory and the case study examples. The latter and the code
13 structure are described more fully in chapters
14 \ref{chap:discretization} and \ref{chap:sarch}, respectively. Here, in
15 this section, we provide information on how to customize the code when
16 you are ready to try implementing the configuration you have in mind.
17
18 \section{Where to find information}
19 \label{sect:whereToFindInfo}
20
21 A web site is maintained for release 2 (``Pelican'') of MITgcm:
22 \begin{rawhtml} <A href=http://mitgcm.org/pelican/ target="idontexist"> \end{rawhtml}
23 \begin{verbatim}
24 http://mitgcm.org/pelican
25 \end{verbatim}
26 \begin{rawhtml} </A> \end{rawhtml}
27 Here you will find an on-line version of this document, a
28 ``browsable'' copy of the code and a searchable database of the model
29 and site, as well as links for downloading the model and
30 documentation, to data-sources, and other related sites.
31
32 There is also a web-archived support mailing list for the model that
33 you can email at \texttt{MITgcm-support@mitgcm.org} or browse at:
34 \begin{rawhtml} <A href=http://mitgcm.org/mailman/listinfo/mitgcm-support/ target="idontexist"> \end{rawhtml}
35 \begin{verbatim}
36 http://mitgcm.org/mailman/listinfo/mitgcm-support/
37 http://mitgcm.org/pipermail/mitgcm-support/
38 \end{verbatim}
39 \begin{rawhtml} </A> \end{rawhtml}
40 Essentially all of the MITgcm web pages can be searched using a
41 popular web crawler such as Google or through our own search facility:
42 \begin{rawhtml} <A href=http://mitgcm.org/mailman/htdig/ target="idontexist"> \end{rawhtml}
43 \begin{verbatim}
44 http://mitgcm.org/htdig/
45 \end{verbatim}
46 \begin{rawhtml} </A> \end{rawhtml}
47 %%% http://www.google.com/search?q=hydrostatic+site%3Amitgcm.org
48
49
50
51 \section{Obtaining the code}
52 \label{sect:obtainingCode}
53
54 MITgcm can be downloaded from our system by following
55 the instructions below. As a courtesy we ask that you send e-mail to us at
56 \begin{rawhtml} <A href=mailto:MITgcm-support@mitgcm.org> \end{rawhtml}
57 MITgcm-support@mitgcm.org
58 \begin{rawhtml} </A> \end{rawhtml}
59 to enable us to keep track of who's using the model and in what application.
60 You can download the model two ways:
61
62 \begin{enumerate}
63 \item Using CVS software. CVS is a freely available source code management
64 tool. To use CVS you need to have the software installed. Many systems
65 come with CVS pre-installed, otherwise good places to look for
66 the software for a particular platform are
67 \begin{rawhtml} <A href=http://www.cvshome.org/ target="idontexist"> \end{rawhtml}
68 cvshome.org
69 \begin{rawhtml} </A> \end{rawhtml}
70 and
71 \begin{rawhtml} <A href=http://www.wincvs.org/ target="idontexist"> \end{rawhtml}
72 wincvs.org
73 \begin{rawhtml} </A> \end{rawhtml}
74 .
75
76 \item Using a tar file. This method is simple and does not
77 require any special software. However, this method does not
78 provide easy support for maintenance updates.
79
80 \end{enumerate}
81
82 \subsubsection{Checkout from CVS}
83 \label{sect:cvs_checkout}
84
85 If CVS is available on your system, we strongly encourage you to use it. CVS
86 provides an efficient and elegant way of organizing your code and keeping
87 track of your changes. If CVS is not available on your machine, you can also
88 download a tar file.
89
90 Before you can use CVS, the following environment variable(s) should
91 be set within your shell. For a csh or tcsh shell, put the following
92 \begin{verbatim}
93 % setenv CVSROOT :pserver:cvsanon@mitgcm.org:/u/gcmpack
94 \end{verbatim}
95 in your .cshrc or .tcshrc file. For bash or sh shells, put:
96 \begin{verbatim}
97 % export CVSROOT=':pserver:cvsanon@mitgcm.org:/u/gcmpack'
98 \end{verbatim}
99 in your \texttt{.profile} or \texttt{.bashrc} file.
100
101
102 To get MITgcm through CVS, first register with the MITgcm CVS server
103 using command:
104 \begin{verbatim}
105 % cvs login ( CVS password: cvsanon )
106 \end{verbatim}
107 You only need to do a ``cvs login'' once.
108
109 To obtain the latest sources type:
110 \begin{verbatim}
111 % cvs co MITgcm
112 \end{verbatim}
113 or to get a specific release type:
114 \begin{verbatim}
115 % cvs co -P -r checkpoint52i_post MITgcm
116 \end{verbatim}
117 The MITgcm web site contains further directions concerning the source
118 code and CVS. It also contains a web interface to our CVS archive so
119 that one may easily view the state of files, revisions, and other
120 development milestones:
121 \begin{rawhtml} <A href=''http://mitgcm.org/download'' target="idontexist"> \end{rawhtml}
122 \begin{verbatim}
123 http://mitgcm.org/source_code.html
124 \end{verbatim}
125 \begin{rawhtml} </A> \end{rawhtml}
126
127 As a convenience, the MITgcm CVS server contains aliases which are
128 named subsets of the codebase. These aliases can be especially
129 helpful when used over slow internet connections or on machines with
130 restricted storage space. Table \ref{tab:cvsModules} contains a list
131 of CVS aliases
132 \begin{table}[htb]
133 \centering
134 \begin{tabular}[htb]{|lp{3.25in}|}\hline
135 \textbf{Alias Name} & \textbf{Information (directories) Contained} \\\hline
136 \texttt{MITgcm\_code} & Only the source code -- none of the verification examples. \\
137 \texttt{MITgcm\_verif\_basic}
138 & Source code plus a small set of the verification examples
139 (\texttt{global\_ocean.90x40x15}, \texttt{aim.5l\_cs}, \texttt{hs94.128x64x5},
140 \texttt{front\_relax}, and \texttt{plume\_on\_slope}). \\
141 \texttt{MITgcm\_verif\_atmos} & Source code plus all of the atmospheric examples. \\
142 \texttt{MITgcm\_verif\_ocean} & Source code plus all of the oceanic examples. \\
143 \texttt{MITgcm\_verif\_all} & Source code plus all of the
144 verification examples. \\\hline
145 \end{tabular}
146 \caption{MITgcm CVS Modules}
147 \label{tab:cvsModules}
148 \end{table}
149
150 The checkout process creates a directory called \textit{MITgcm}. If
151 the directory \textit{MITgcm} exists this command updates your code
152 based on the repository. Each directory in the source tree contains a
153 directory \textit{CVS}. This information is required by CVS to keep
154 track of your file versions with respect to the repository. Don't edit
155 the files in \textit{CVS}! You can also use CVS to download code
156 updates. More extensive information on using CVS for maintaining
157 MITgcm code can be found
158 \begin{rawhtml} <A href=''http://mitgcm.org/usingcvstoget.html'' target="idontexist"> \end{rawhtml}
159 here
160 \begin{rawhtml} </A> \end{rawhtml}
161 .
162 It is important to note that the CVS aliases in Table
163 \ref{tab:cvsModules} cannot be used in conjunction with the CVS
164 \texttt{-d DIRNAME} option. However, the \texttt{MITgcm} directories
165 they create can be changed to a different name following the check-out:
166 \begin{verbatim}
167 % cvs co MITgcm_verif_basic
168 % mv MITgcm MITgcm_verif_basic
169 \end{verbatim}
170
171
172 \subsubsection{Conventional download method}
173 \label{sect:conventionalDownload}
174
175 If you do not have CVS on your system, you can download the model as a
176 tar file from the web site at:
177 \begin{rawhtml} <A href=http://mitgcm.org/download target="idontexist"> \end{rawhtml}
178 \begin{verbatim}
179 http://mitgcm.org/download/
180 \end{verbatim}
181 \begin{rawhtml} </A> \end{rawhtml}
182 The tar file still contains CVS information which we urge you not to
183 delete; even if you do not use CVS yourself the information can help
184 us if you should need to send us your copy of the code. If a recent
185 tar file does not exist, then please contact the developers through
186 the
187 \begin{rawhtml} <A href=''mailto:MITgcm-support@mitgcm.org"> \end{rawhtml}
188 MITgcm-support@mitgcm.org
189 \begin{rawhtml} </A> \end{rawhtml}
190 mailing list.
191
192 \subsubsection{Upgrading from an earlier version}
193
194 If you already have an earlier version of the code you can ``upgrade''
195 your copy instead of downloading the entire repository again. First,
196 ``cd'' (change directory) to the top of your working copy:
197 \begin{verbatim}
198 % cd MITgcm
199 \end{verbatim}
200 and then issue the cvs update command such as:
201 \begin{verbatim}
202 % cvs -q update -r checkpoint52i_post -d -P
203 \end{verbatim}
204 This will update the ``tag'' to ``checkpoint52i\_post'', add any new
205 directories (-d) and remove any empty directories (-P). The -q option
206 means be quiet which will reduce the number of messages you'll see in
207 the terminal. If you have modified the code prior to upgrading, CVS
208 will try to merge your changes with the upgrades. If there is a
209 conflict between your modifications and the upgrade, it will report
210 that file with a ``C'' in front, e.g.:
211 \begin{verbatim}
212 C model/src/ini_parms.F
213 \end{verbatim}
214 If the list of conflicts scrolled off the screen, you can re-issue the
215 cvs update command and it will report the conflicts. Conflicts are
216 indicated in the code by the delimites ``$<<<<<<<$'', ``======='' and
217 ``$>>>>>>>$''. For example,
218 {\small
219 \begin{verbatim}
220 <<<<<<< ini_parms.F
221 & bottomDragLinear,myOwnBottomDragCoefficient,
222 =======
223 & bottomDragLinear,bottomDragQuadratic,
224 >>>>>>> 1.18
225 \end{verbatim}
226 }
227 means that you added ``myOwnBottomDragCoefficient'' to a namelist at
228 the same time and place that we added ``bottomDragQuadratic''. You
229 need to resolve this conflict and in this case the line should be
230 changed to:
231 {\small
232 \begin{verbatim}
233 & bottomDragLinear,bottomDragQuadratic,myOwnBottomDragCoefficient,
234 \end{verbatim}
235 }
236 and the lines with the delimiters ($<<<<<<$,======,$>>>>>>$) be deleted.
237 Unless you are making modifications which exactly parallel
238 developments we make, these types of conflicts should be rare.
239
240 \paragraph*{Upgrading to the current pre-release version}
241
242 We don't make a ``release'' for every little patch and bug fix in
243 order to keep the frequency of upgrades to a minimum. However, if you
244 have run into a problem for which ``we have already fixed in the
245 latest code'' and we haven't made a ``tag'' or ``release'' since that
246 patch then you'll need to get the latest code:
247 \begin{verbatim}
248 % cvs -q update -A -d -P
249 \end{verbatim}
250 Unlike, the ``check-out'' and ``update'' procedures above, there is no
251 ``tag'' or release name. The -A tells CVS to upgrade to the
252 very latest version. As a rule, we don't recommend this since you
253 might upgrade while we are in the processes of checking in the code so
254 that you may only have part of a patch. Using this method of updating
255 also means we can't tell what version of the code you are working
256 with. So please be sure you understand what you're doing.
257
258 \section{Model and directory structure}
259
260 The ``numerical'' model is contained within a execution environment
261 support wrapper. This wrapper is designed to provide a general
262 framework for grid-point models. MITgcmUV is a specific numerical
263 model that uses the framework. Under this structure the model is split
264 into execution environment support code and conventional numerical
265 model code. The execution environment support code is held under the
266 \textit{eesupp} directory. The grid point model code is held under the
267 \textit{model} directory. Code execution actually starts in the
268 \textit{eesupp} routines and not in the \textit{model} routines. For
269 this reason the top-level \textit{MAIN.F} is in the
270 \textit{eesupp/src} directory. In general, end-users should not need
271 to worry about this level. The top-level routine for the numerical
272 part of the code is in \textit{model/src/THE\_MODEL\_MAIN.F}. Here is
273 a brief description of the directory structure of the model under the
274 root tree (a detailed description is given in section 3: Code
275 structure).
276
277 \begin{itemize}
278
279 \item \textit{bin}: this directory is initially empty. It is the
280 default directory in which to compile the code.
281
282 \item \textit{diags}: contains the code relative to time-averaged
283 diagnostics. It is subdivided into two subdirectories \textit{inc}
284 and \textit{src} that contain include files (*.\textit{h} files) and
285 Fortran subroutines (*.\textit{F} files), respectively.
286
287 \item \textit{doc}: contains brief documentation notes.
288
289 \item \textit{eesupp}: contains the execution environment source code.
290 Also subdivided into two subdirectories \textit{inc} and
291 \textit{src}.
292
293 \item \textit{exe}: this directory is initially empty. It is the
294 default directory in which to execute the code.
295
296 \item \textit{model}: this directory contains the main source code.
297 Also subdivided into two subdirectories \textit{inc} and
298 \textit{src}.
299
300 \item \textit{pkg}: contains the source code for the packages. Each
301 package corresponds to a subdirectory. For example, \textit{gmredi}
302 contains the code related to the Gent-McWilliams/Redi scheme,
303 \textit{aim} the code relative to the atmospheric intermediate
304 physics. The packages are described in detail in section 3.
305
306 \item \textit{tools}: this directory contains various useful tools.
307 For example, \textit{genmake2} is a script written in csh (C-shell)
308 that should be used to generate your makefile. The directory
309 \textit{adjoint} contains the makefile specific to the Tangent
310 linear and Adjoint Compiler (TAMC) that generates the adjoint code.
311 The latter is described in details in part V.
312
313 \item \textit{utils}: this directory contains various utilities. The
314 subdirectory \textit{knudsen2} contains code and a makefile that
315 compute coefficients of the polynomial approximation to the knudsen
316 formula for an ocean nonlinear equation of state. The
317 \textit{matlab} subdirectory contains matlab scripts for reading
318 model output directly into matlab. \textit{scripts} contains C-shell
319 post-processing scripts for joining processor-based and tiled-based
320 model output.
321
322 \item \textit{verification}: this directory contains the model
323 examples. See section \ref{sect:modelExamples}.
324
325 \end{itemize}
326
327 \section{Example experiments}
328 \label{sect:modelExamples}
329
330 %% a set of twenty-four pre-configured numerical experiments
331
332 The MITgcm distribution comes with more than a dozen pre-configured
333 numerical experiments. Some of these example experiments are tests of
334 individual parts of the model code, but many are fully fledged
335 numerical simulations. A few of the examples are used for tutorial
336 documentation in sections \ref{sect:eg-baro} - \ref{sect:eg-global}.
337 The other examples follow the same general structure as the tutorial
338 examples. However, they only include brief instructions in a text file
339 called {\it README}. The examples are located in subdirectories under
340 the directory \textit{verification}. Each example is briefly described
341 below.
342
343 \subsection{Full list of model examples}
344
345 \begin{enumerate}
346
347 \item \textit{exp0} - single layer, ocean double gyre (barotropic with
348 free-surface). This experiment is described in detail in section
349 \ref{sect:eg-baro}.
350
351 \item \textit{exp1} - Four layer, ocean double gyre. This experiment
352 is described in detail in section \ref{sect:eg-baroc}.
353
354 \item \textit{exp2} - 4x4 degree global ocean simulation with steady
355 climatological forcing. This experiment is described in detail in
356 section \ref{sect:eg-global}.
357
358 \item \textit{exp4} - Flow over a Gaussian bump in open-water or
359 channel with open boundaries.
360
361 \item \textit{exp5} - Inhomogenously forced ocean convection in a
362 doubly periodic box.
363
364 \item \textit{front\_relax} - Relaxation of an ocean thermal front (test for
365 Gent/McWilliams scheme). 2D (Y-Z).
366
367 \item \textit{internal wave} - Ocean internal wave forced by open
368 boundary conditions.
369
370 \item \textit{natl\_box} - Eastern subtropical North Atlantic with KPP
371 scheme; 1 month integration
372
373 \item \textit{hs94.1x64x5} - Zonal averaged atmosphere using Held and
374 Suarez '94 forcing.
375
376 \item \textit{hs94.128x64x5} - 3D atmosphere dynamics using Held and
377 Suarez '94 forcing.
378
379 \item \textit{hs94.cs-32x32x5} - 3D atmosphere dynamics using Held and
380 Suarez '94 forcing on the cubed sphere.
381
382 \item \textit{aim.5l\_zon-ave} - Intermediate Atmospheric physics.
383 Global Zonal Mean configuration, 1x64x5 resolution.
384
385 \item \textit{aim.5l\_XZ\_Equatorial\_Slice} - Intermediate
386 Atmospheric physics, equatorial Slice configuration. 2D (X-Z).
387
388 \item \textit{aim.5l\_Equatorial\_Channel} - Intermediate Atmospheric
389 physics. 3D Equatorial Channel configuration.
390
391 \item \textit{aim.5l\_LatLon} - Intermediate Atmospheric physics.
392 Global configuration, on latitude longitude grid with 128x64x5 grid
393 points ($2.8^\circ{\rm degree}$ resolution).
394
395 \item \textit{adjustment.128x64x1} Barotropic adjustment problem on
396 latitude longitude grid with 128x64 grid points ($2.8^\circ{\rm
397 degree}$ resolution).
398
399 \item \textit{adjustment.cs-32x32x1} Barotropic adjustment problem on
400 cube sphere grid with 32x32 points per face ( roughly $2.8^\circ{\rm
401 degree}$ resolution).
402
403 \item \textit{advect\_cs} Two-dimensional passive advection test on
404 cube sphere grid.
405
406 \item \textit{advect\_xy} Two-dimensional (horizontal plane) passive
407 advection test on Cartesian grid.
408
409 \item \textit{advect\_yz} Two-dimensional (vertical plane) passive
410 advection test on Cartesian grid.
411
412 \item \textit{carbon} Simple passive tracer experiment. Includes
413 derivative calculation. Described in detail in section
414 \ref{sect:eg-carbon-ad}.
415
416 \item \textit{flt\_example} Example of using float package.
417
418 \item \textit{global\_ocean.90x40x15} Global circulation with GM, flux
419 boundary conditions and poles.
420
421 \item \textit{global\_ocean\_pressure} Global circulation in pressure
422 coordinate (non-Boussinesq ocean model). Described in detail in
423 section \ref{sect:eg-globalpressure}.
424
425 \item \textit{solid-body.cs-32x32x1} Solid body rotation test for cube
426 sphere grid.
427
428 \end{enumerate}
429
430 \subsection{Directory structure of model examples}
431
432 Each example directory has the following subdirectories:
433
434 \begin{itemize}
435 \item \textit{code}: contains the code particular to the example. At a
436 minimum, this directory includes the following files:
437
438 \begin{itemize}
439 \item \textit{code/CPP\_EEOPTIONS.h}: declares CPP keys relative to
440 the ``execution environment'' part of the code. The default
441 version is located in \textit{eesupp/inc}.
442
443 \item \textit{code/CPP\_OPTIONS.h}: declares CPP keys relative to
444 the ``numerical model'' part of the code. The default version is
445 located in \textit{model/inc}.
446
447 \item \textit{code/SIZE.h}: declares size of underlying
448 computational grid. The default version is located in
449 \textit{model/inc}.
450 \end{itemize}
451
452 In addition, other include files and subroutines might be present in
453 \textit{code} depending on the particular experiment. See Section 2
454 for more details.
455
456 \item \textit{input}: contains the input data files required to run
457 the example. At a minimum, the \textit{input} directory contains the
458 following files:
459
460 \begin{itemize}
461 \item \textit{input/data}: this file, written as a namelist,
462 specifies the main parameters for the experiment.
463
464 \item \textit{input/data.pkg}: contains parameters relative to the
465 packages used in the experiment.
466
467 \item \textit{input/eedata}: this file contains ``execution
468 environment'' data. At present, this consists of a specification
469 of the number of threads to use in $X$ and $Y$ under multithreaded
470 execution.
471 \end{itemize}
472
473 In addition, you will also find in this directory the forcing and
474 topography files as well as the files describing the initial state
475 of the experiment. This varies from experiment to experiment. See
476 section 2 for more details.
477
478 \item \textit{results}: this directory contains the output file
479 \textit{output.txt} produced by the simulation example. This file is
480 useful for comparison with your own output when you run the
481 experiment.
482 \end{itemize}
483
484 Once you have chosen the example you want to run, you are ready to
485 compile the code.
486
487 \section{Building the code}
488 \label{sect:buildingCode}
489
490 To compile the code, we use the {\em make} program. This uses a file
491 ({\em Makefile}) that allows us to pre-process source files, specify
492 compiler and optimization options and also figures out any file
493 dependencies. We supply a script ({\em genmake2}), described in
494 section \ref{sect:genmake}, that automatically creates the {\em
495 Makefile} for you. You then need to build the dependencies and
496 compile the code.
497
498 As an example, let's assume that you want to build and run experiment
499 \textit{verification/exp2}. The are multiple ways and places to
500 actually do this but here let's build the code in
501 \textit{verification/exp2/input}:
502 \begin{verbatim}
503 % cd verification/exp2/input
504 \end{verbatim}
505 First, build the {\em Makefile}:
506 \begin{verbatim}
507 % ../../../tools/genmake2 -mods=../code
508 \end{verbatim}
509 The command line option tells {\em genmake} to override model source
510 code with any files in the directory {\em ./code/}.
511
512 On many systems, the {\em genmake2} program will be able to
513 automatically recognize the hardware, find compilers and other tools
514 within the user's path (``echo \$PATH''), and then choose an
515 appropriate set of options from the files contained in the {\em
516 tools/build\_options} directory. Under some circumstances, a user
517 may have to create a new ``optfile'' in order to specify the exact
518 combination of compiler, compiler flags, libraries, and other options
519 necessary to build a particular configuration of MITgcm. In such
520 cases, it is generally helpful to read the existing ``optfiles'' and
521 mimic their syntax.
522
523 Through the MITgcm-support list, the MITgcm developers are willing to
524 provide help writing or modifing ``optfiles''. And we encourage users
525 to post new ``optfiles'' (particularly ones for new machines or
526 architectures) to the
527 \begin{rawhtml} <A href=''mailto:MITgcm-support@mitgcm.org"> \end{rawhtml}
528 MITgcm-support@mitgcm.org
529 \begin{rawhtml} </A> \end{rawhtml}
530 list.
531
532 To specify an optfile to {\em genmake2}, the syntax is:
533 \begin{verbatim}
534 % ../../../tools/genmake2 -mods=../code -of /path/to/optfile
535 \end{verbatim}
536
537 Once a {\em Makefile} has been generated, we create the dependencies:
538 \begin{verbatim}
539 % make depend
540 \end{verbatim}
541 This modifies the {\em Makefile} by attaching a [long] list of files
542 upon which other files depend. The purpose of this is to reduce
543 re-compilation if and when you start to modify the code. The {\tt make
544 depend} command also creates links from the model source to this
545 directory.
546
547 Next compile the code:
548 \begin{verbatim}
549 % make
550 \end{verbatim}
551 The {\tt make} command creates an executable called \textit{mitgcmuv}.
552 Additional make ``targets'' are defined within the makefile to aid in
553 the production of adjoint and other versions of MITgcm.
554
555 Now you are ready to run the model. General instructions for doing so are
556 given in section \ref{sect:runModel}. Here, we can run the model with:
557 \begin{verbatim}
558 ./mitgcmuv > output.txt
559 \end{verbatim}
560 where we are re-directing the stream of text output to the file {\em
561 output.txt}.
562
563
564 \subsection{Building/compiling the code elsewhere}
565
566 In the example above (section \ref{sect:buildingCode}) we built the
567 executable in the {\em input} directory of the experiment for
568 convenience. You can also configure and compile the code in other
569 locations, for example on a scratch disk with out having to copy the
570 entire source tree. The only requirement to do so is you have {\tt
571 genmake2} in your path or you know the absolute path to {\tt
572 genmake2}.
573
574 The following sections outline some possible methods of organizing
575 your source and data.
576
577 \subsubsection{Building from the {\em ../code directory}}
578
579 This is just as simple as building in the {\em input/} directory:
580 \begin{verbatim}
581 % cd verification/exp2/code
582 % ../../../tools/genmake2
583 % make depend
584 % make
585 \end{verbatim}
586 However, to run the model the executable ({\em mitgcmuv}) and input
587 files must be in the same place. If you only have one calculation to make:
588 \begin{verbatim}
589 % cd ../input
590 % cp ../code/mitgcmuv ./
591 % ./mitgcmuv > output.txt
592 \end{verbatim}
593 or if you will be making multiple runs with the same executable:
594 \begin{verbatim}
595 % cd ../
596 % cp -r input run1
597 % cp code/mitgcmuv run1
598 % cd run1
599 % ./mitgcmuv > output.txt
600 \end{verbatim}
601
602 \subsubsection{Building from a new directory}
603
604 Since the {\em input} directory contains input files it is often more
605 useful to keep {\em input} pristine and build in a new directory
606 within {\em verification/exp2/}:
607 \begin{verbatim}
608 % cd verification/exp2
609 % mkdir build
610 % cd build
611 % ../../../tools/genmake2 -mods=../code
612 % make depend
613 % make
614 \end{verbatim}
615 This builds the code exactly as before but this time you need to copy
616 either the executable or the input files or both in order to run the
617 model. For example,
618 \begin{verbatim}
619 % cp ../input/* ./
620 % ./mitgcmuv > output.txt
621 \end{verbatim}
622 or if you tend to make multiple runs with the same executable then
623 running in a new directory each time might be more appropriate:
624 \begin{verbatim}
625 % cd ../
626 % mkdir run1
627 % cp build/mitgcmuv run1/
628 % cp input/* run1/
629 % cd run1
630 % ./mitgcmuv > output.txt
631 \end{verbatim}
632
633 \subsubsection{Building on a scratch disk}
634
635 Model object files and output data can use up large amounts of disk
636 space so it is often the case that you will be operating on a large
637 scratch disk. Assuming the model source is in {\em ~/MITgcm} then the
638 following commands will build the model in {\em /scratch/exp2-run1}:
639 \begin{verbatim}
640 % cd /scratch/exp2-run1
641 % ~/MITgcm/tools/genmake2 -rootdir=~/MITgcm \
642 -mods=~/MITgcm/verification/exp2/code
643 % make depend
644 % make
645 \end{verbatim}
646 To run the model here, you'll need the input files:
647 \begin{verbatim}
648 % cp ~/MITgcm/verification/exp2/input/* ./
649 % ./mitgcmuv > output.txt
650 \end{verbatim}
651
652 As before, you could build in one directory and make multiple runs of
653 the one experiment:
654 \begin{verbatim}
655 % cd /scratch/exp2
656 % mkdir build
657 % cd build
658 % ~/MITgcm/tools/genmake2 -rootdir=~/MITgcm \
659 -mods=~/MITgcm/verification/exp2/code
660 % make depend
661 % make
662 % cd ../
663 % cp -r ~/MITgcm/verification/exp2/input run2
664 % cd run2
665 % ./mitgcmuv > output.txt
666 \end{verbatim}
667
668
669
670 \subsection{Using \textit{genmake2}}
671 \label{sect:genmake}
672
673 To compile the code, first use the program \texttt{genmake2} (located
674 in the \textit{tools} directory) to generate a Makefile.
675 \texttt{genmake2} is a shell script written to work with all
676 ``sh''--compatible shells including bash v1, bash v2, and Bourne.
677 Internally, \texttt{genmake2} determines the locations of needed
678 files, the compiler, compiler options, libraries, and Unix tools. It
679 relies upon a number of ``optfiles'' located in the {\em
680 tools/build\_options} directory.
681
682 The purpose of the optfiles is to provide all the compilation options
683 for particular ``platforms'' (where ``platform'' roughly means the
684 combination of the hardware and the compiler) and code configurations.
685 Given the combinations of possible compilers and library dependencies
686 ({\it eg.} MPI and NetCDF) there may be numerous optfiles available
687 for a single machine. The naming scheme for the majority of the
688 optfiles shipped with the code is
689 \begin{center}
690 {\bf OS\_HARDWARE\_COMPILER }
691 \end{center}
692 where
693 \begin{description}
694 \item[OS] is the name of the operating system (generally the
695 lower-case output of the {\tt 'uname'} command)
696 \item[HARDWARE] is a string that describes the CPU type and
697 corresponds to output from the {\tt 'uname -m'} command:
698 \begin{description}
699 \item[ia32] is for ``x86'' machines such as i386, i486, i586, i686,
700 and athlon
701 \item[ia64] is for Intel IA64 systems (eg. Itanium, Itanium2)
702 \item[amd64] is AMD x86\_64 systems
703 \item[ppc] is for Mac PowerPC systems
704 \end{description}
705 \item[COMPILER] is the compiler name (generally, the name of the
706 FORTRAN executable)
707 \end{description}
708
709 In many cases, the default optfiles are sufficient and will result in
710 usable Makefiles. However, for some machines or code configurations,
711 new ``optfiles'' must be written. To create a new optfile, it is
712 generally best to start with one of the defaults and modify it to suit
713 your needs. Like \texttt{genmake2}, the optfiles are all written
714 using a simple ``sh''--compatible syntax. While nearly all variables
715 used within \texttt{genmake2} may be specified in the optfiles, the
716 critical ones that should be defined are:
717
718 \begin{description}
719 \item[FC] the FORTRAN compiler (executable) to use
720 \item[DEFINES] the command-line DEFINE options passed to the compiler
721 \item[CPP] the C pre-processor to use
722 \item[NOOPTFLAGS] options flags for special files that should not be
723 optimized
724 \end{description}
725
726 For example, the optfile for a typical Red Hat Linux machine (``ia32''
727 architecture) using the GCC (g77) compiler is
728 \begin{verbatim}
729 FC=g77
730 DEFINES='-D_BYTESWAPIO -DWORDLENGTH=4'
731 CPP='cpp -traditional -P'
732 NOOPTFLAGS='-O0'
733 # For IEEE, use the "-ffloat-store" option
734 if test "x$IEEE" = x ; then
735 FFLAGS='-Wimplicit -Wunused -Wuninitialized'
736 FOPTIM='-O3 -malign-double -funroll-loops'
737 else
738 FFLAGS='-Wimplicit -Wunused -ffloat-store'
739 FOPTIM='-O0 -malign-double'
740 fi
741 \end{verbatim}
742
743 If you write an optfile for an unrepresented machine or compiler, you
744 are strongly encouraged to submit the optfile to the MITgcm project
745 for inclusion. Please send the file to the
746 \begin{rawhtml} <A href="mail-to:MITgcm-support@mitgcm.org"> \end{rawhtml}
747 \begin{center}
748 MITgcm-support@mitgcm.org
749 \end{center}
750 \begin{rawhtml} </A> \end{rawhtml}
751 mailing list.
752
753 In addition to the optfiles, \texttt{genmake2} supports a number of
754 helpful command-line options. A complete list of these options can be
755 obtained from:
756 \begin{verbatim}
757 % genmake2 -h
758 \end{verbatim}
759
760 The most important command-line options are:
761 \begin{description}
762
763 \item[\texttt{--optfile=/PATH/FILENAME}] specifies the optfile that
764 should be used for a particular build.
765
766 If no "optfile" is specified (either through the command line or the
767 MITGCM\_OPTFILE environment variable), genmake2 will try to make a
768 reasonable guess from the list provided in {\em
769 tools/build\_options}. The method used for making this guess is
770 to first determine the combination of operating system and hardware
771 (eg. "linux\_ia32") and then find a working FORTRAN compiler within
772 the user's path. When these three items have been identified,
773 genmake2 will try to find an optfile that has a matching name.
774
775 \item[\texttt{--pdepend=/PATH/FILENAME}] specifies the dependency file
776 used for packages.
777
778 If not specified, the default dependency file {\em pkg/pkg\_depend}
779 is used. The syntax for this file is parsed on a line-by-line basis
780 where each line containes either a comment ("\#") or a simple
781 "PKGNAME1 (+|-)PKGNAME2" pairwise rule where the "+" or "-" symbol
782 specifies a "must be used with" or a "must not be used with"
783 relationship, respectively. If no rule is specified, then it is
784 assumed that the two packages are compatible and will function
785 either with or without each other.
786
787 \item[\texttt{--pdefault='PKG1 PKG2 PKG3 ...'}] specifies the default
788 set of packages to be used.
789
790 If not set, the default package list will be read from {\em
791 pkg/pkg\_default}
792
793 \item[\texttt{--adof=/path/to/file}] specifies the "adjoint" or
794 automatic differentiation options file to be used. The file is
795 analogous to the ``optfile'' defined above but it specifies
796 information for the AD build process.
797
798 The default file is located in {\em
799 tools/adjoint\_options/adjoint\_default} and it defines the "TAF"
800 and "TAMC" compilers. An alternate version is also available at
801 {\em tools/adjoint\_options/adjoint\_staf} that selects the newer
802 "STAF" compiler. As with any compilers, it is helpful to have their
803 directories listed in your {\tt \$PATH} environment variable.
804
805 \item[\texttt{--mods='DIR1 DIR2 DIR3 ...'}] specifies a list of
806 directories containing ``modifications''. These directories contain
807 files with names that may (or may not) exist in the main MITgcm
808 source tree but will be overridden by any identically-named sources
809 within the ``MODS'' directories.
810
811 The order of precedence for this "name-hiding" is as follows:
812 \begin{itemize}
813 \item ``MODS'' directories (in the order given)
814 \item Packages either explicitly specified or provided by default
815 (in the order given)
816 \item Packages included due to package dependencies (in the order
817 that that package dependencies are parsed)
818 \item The "standard dirs" (which may have been specified by the
819 ``-standarddirs'' option)
820 \end{itemize}
821
822 \item[\texttt{--make=/path/to/gmake}] Due to the poor handling of
823 soft-links and other bugs common with the \texttt{make} versions
824 provided by commercial Unix vendors, GNU \texttt{make} (sometimes
825 called \texttt{gmake}) should be preferred. This option provides a
826 means for specifying the make executable to be used.
827
828 \end{description}
829
830
831
832 \section{Running the model}
833 \label{sect:runModel}
834
835 If compilation finished succesfuully (section \ref{sect:buildModel})
836 then an executable called {\em mitgcmuv} will now exist in the local
837 directory.
838
839 To run the model as a single process (ie. not in parallel) simply
840 type:
841 \begin{verbatim}
842 % ./mitgcmuv
843 \end{verbatim}
844 The ``./'' is a safe-guard to make sure you use the local executable
845 in case you have others that exist in your path (surely odd if you
846 do!). The above command will spew out many lines of text output to
847 your screen. This output contains details such as parameter values as
848 well as diagnostics such as mean Kinetic energy, largest CFL number,
849 etc. It is worth keeping this text output with the binary output so we
850 normally re-direct the {\em stdout} stream as follows:
851 \begin{verbatim}
852 % ./mitgcmuv > output.txt
853 \end{verbatim}
854
855 For the example experiments in {\em verification}, an example of the
856 output is kept in {\em results/output.txt} for comparison. You can compare
857 your {\em output.txt} with this one to check that the set-up works.
858
859
860
861 \subsection{Output files}
862
863 The model produces various output files. At a minimum, the instantaneous
864 ``state'' of the model is written out, which is made of the following files:
865
866 \begin{itemize}
867 \item \textit{U.00000nIter} - zonal component of velocity field (m/s and $>
868 0 $ eastward).
869
870 \item \textit{V.00000nIter} - meridional component of velocity field (m/s
871 and $> 0$ northward).
872
873 \item \textit{W.00000nIter} - vertical component of velocity field (ocean:
874 m/s and $> 0$ upward, atmosphere: Pa/s and $> 0$ towards increasing pressure
875 i.e. downward).
876
877 \item \textit{T.00000nIter} - potential temperature (ocean: $^{0}$C,
878 atmosphere: $^{0}$K).
879
880 \item \textit{S.00000nIter} - ocean: salinity (psu), atmosphere: water vapor
881 (g/kg).
882
883 \item \textit{Eta.00000nIter} - ocean: surface elevation (m), atmosphere:
884 surface pressure anomaly (Pa).
885 \end{itemize}
886
887 The chain \textit{00000nIter} consists of ten figures that specify the
888 iteration number at which the output is written out. For example, \textit{%
889 U.0000000300} is the zonal velocity at iteration 300.
890
891 In addition, a ``pickup'' or ``checkpoint'' file called:
892
893 \begin{itemize}
894 \item \textit{pickup.00000nIter}
895 \end{itemize}
896
897 is written out. This file represents the state of the model in a condensed
898 form and is used for restarting the integration. If the C-D scheme is used,
899 there is an additional ``pickup'' file:
900
901 \begin{itemize}
902 \item \textit{pickup\_cd.00000nIter}
903 \end{itemize}
904
905 containing the D-grid velocity data and that has to be written out as well
906 in order to restart the integration. Rolling checkpoint files are the same
907 as the pickup files but are named differently. Their name contain the chain
908 \textit{ckptA} or \textit{ckptB} instead of \textit{00000nIter}. They can be
909 used to restart the model but are overwritten every other time they are
910 output to save disk space during long integrations.
911
912 \subsection{Looking at the output}
913
914 All the model data are written according to a ``meta/data'' file format.
915 Each variable is associated with two files with suffix names \textit{.data}
916 and \textit{.meta}. The \textit{.data} file contains the data written in
917 binary form (big\_endian by default). The \textit{.meta} file is a
918 ``header'' file that contains information about the size and the structure
919 of the \textit{.data} file. This way of organizing the output is
920 particularly useful when running multi-processors calculations. The base
921 version of the model includes a few matlab utilities to read output files
922 written in this format. The matlab scripts are located in the directory
923 \textit{utils/matlab} under the root tree. The script \textit{rdmds.m} reads
924 the data. Look at the comments inside the script to see how to use it.
925
926 Some examples of reading and visualizing some output in {\em Matlab}:
927 \begin{verbatim}
928 % matlab
929 >> H=rdmds('Depth');
930 >> contourf(H');colorbar;
931 >> title('Depth of fluid as used by model');
932
933 >> eta=rdmds('Eta',10);
934 >> imagesc(eta');axis ij;colorbar;
935 >> title('Surface height at iter=10');
936
937 >> eta=rdmds('Eta',[0:10:100]);
938 >> for n=1:11; imagesc(eta(:,:,n)');axis ij;colorbar;pause(.5);end
939 \end{verbatim}
940
941 \section{Doing it yourself: customizing the code}
942
943 When you are ready to run the model in the configuration you want, the
944 easiest thing is to use and adapt the setup of the case studies
945 experiment (described previously) that is the closest to your
946 configuration. Then, the amount of setup will be minimized. In this
947 section, we focus on the setup relative to the ``numerical model''
948 part of the code (the setup relative to the ``execution environment''
949 part is covered in the parallel implementation section) and on the
950 variables and parameters that you are likely to change.
951
952 \subsection{Configuration and setup}
953
954 The CPP keys relative to the ``numerical model'' part of the code are
955 all defined and set in the file \textit{CPP\_OPTIONS.h }in the
956 directory \textit{ model/inc }or in one of the \textit{code
957 }directories of the case study experiments under
958 \textit{verification.} The model parameters are defined and declared
959 in the file \textit{model/inc/PARAMS.h }and their default values are
960 set in the routine \textit{model/src/set\_defaults.F. }The default
961 values can be modified in the namelist file \textit{data }which needs
962 to be located in the directory where you will run the model. The
963 parameters are initialized in the routine
964 \textit{model/src/ini\_parms.F}. Look at this routine to see in what
965 part of the namelist the parameters are located.
966
967 In what follows the parameters are grouped into categories related to
968 the computational domain, the equations solved in the model, and the
969 simulation controls.
970
971 \subsection{Computational domain, geometry and time-discretization}
972
973 \begin{description}
974 \item[dimensions] \
975
976 The number of points in the x, y, and r directions are represented
977 by the variables \textbf{sNx}, \textbf{sNy} and \textbf{Nr}
978 respectively which are declared and set in the file
979 \textit{model/inc/SIZE.h}. (Again, this assumes a mono-processor
980 calculation. For multiprocessor calculations see the section on
981 parallel implementation.)
982
983 \item[grid] \
984
985 Three different grids are available: cartesian, spherical polar, and
986 curvilinear (which includes the cubed sphere). The grid is set
987 through the logical variables \textbf{usingCartesianGrid},
988 \textbf{usingSphericalPolarGrid}, and \textbf{usingCurvilinearGrid}.
989 In the case of spherical and curvilinear grids, the southern
990 boundary is defined through the variable \textbf{phiMin} which
991 corresponds to the latitude of the southern most cell face (in
992 degrees). The resolution along the x and y directions is controlled
993 by the 1D arrays \textbf{delx} and \textbf{dely} (in meters in the
994 case of a cartesian grid, in degrees otherwise). The vertical grid
995 spacing is set through the 1D array \textbf{delz} for the ocean (in
996 meters) or \textbf{delp} for the atmosphere (in Pa). The variable
997 \textbf{Ro\_SeaLevel} represents the standard position of Sea-Level
998 in ``R'' coordinate. This is typically set to 0m for the ocean
999 (default value) and 10$^{5}$Pa for the atmosphere. For the
1000 atmosphere, also set the logical variable \textbf{groundAtK1} to
1001 \texttt{'.TRUE.'} which puts the first level (k=1) at the lower
1002 boundary (ground).
1003
1004 For the cartesian grid case, the Coriolis parameter $f$ is set
1005 through the variables \textbf{f0} and \textbf{beta} which correspond
1006 to the reference Coriolis parameter (in s$^{-1}$) and
1007 $\frac{\partial f}{ \partial y}$(in m$^{-1}$s$^{-1}$) respectively.
1008 If \textbf{beta } is set to a nonzero value, \textbf{f0} is the
1009 value of $f$ at the southern edge of the domain.
1010
1011 \item[topography - full and partial cells] \
1012
1013 The domain bathymetry is read from a file that contains a 2D (x,y)
1014 map of depths (in m) for the ocean or pressures (in Pa) for the
1015 atmosphere. The file name is represented by the variable
1016 \textbf{bathyFile}. The file is assumed to contain binary numbers
1017 giving the depth (pressure) of the model at each grid cell, ordered
1018 with the x coordinate varying fastest. The points are ordered from
1019 low coordinate to high coordinate for both axes. The model code
1020 applies without modification to enclosed, periodic, and double
1021 periodic domains. Periodicity is assumed by default and is
1022 suppressed by setting the depths to 0m for the cells at the limits
1023 of the computational domain (note: not sure this is the case for the
1024 atmosphere). The precision with which to read the binary data is
1025 controlled by the integer variable \textbf{readBinaryPrec} which can
1026 take the value \texttt{32} (single precision) or \texttt{64} (double
1027 precision). See the matlab program \textit{gendata.m} in the
1028 \textit{input} directories under \textit{verification} to see how
1029 the bathymetry files are generated for the case study experiments.
1030
1031 To use the partial cell capability, the variable \textbf{hFacMin}
1032 needs to be set to a value between 0 and 1 (it is set to 1 by
1033 default) corresponding to the minimum fractional size of the cell.
1034 For example if the bottom cell is 500m thick and \textbf{hFacMin} is
1035 set to 0.1, the actual thickness of the cell (i.e. used in the code)
1036 can cover a range of discrete values 50m apart from 50m to 500m
1037 depending on the value of the bottom depth (in \textbf{bathyFile})
1038 at this point.
1039
1040 Note that the bottom depths (or pressures) need not coincide with
1041 the models levels as deduced from \textbf{delz} or \textbf{delp}.
1042 The model will interpolate the numbers in \textbf{bathyFile} so that
1043 they match the levels obtained from \textbf{delz} or \textbf{delp}
1044 and \textbf{hFacMin}.
1045
1046 (Note: the atmospheric case is a bit more complicated than what is
1047 written here I think. To come soon...)
1048
1049 \item[time-discretization] \
1050
1051 The time steps are set through the real variables \textbf{deltaTMom}
1052 and \textbf{deltaTtracer} (in s) which represent the time step for
1053 the momentum and tracer equations, respectively. For synchronous
1054 integrations, simply set the two variables to the same value (or you
1055 can prescribe one time step only through the variable
1056 \textbf{deltaT}). The Adams-Bashforth stabilizing parameter is set
1057 through the variable \textbf{abEps} (dimensionless). The stagger
1058 baroclinic time stepping can be activated by setting the logical
1059 variable \textbf{staggerTimeStep} to \texttt{'.TRUE.'}.
1060
1061 \end{description}
1062
1063
1064 \subsection{Equation of state}
1065
1066 First, because the model equations are written in terms of
1067 perturbations, a reference thermodynamic state needs to be specified.
1068 This is done through the 1D arrays \textbf{tRef} and \textbf{sRef}.
1069 \textbf{tRef} specifies the reference potential temperature profile
1070 (in $^{o}$C for the ocean and $^{o}$K for the atmosphere) starting
1071 from the level k=1. Similarly, \textbf{sRef} specifies the reference
1072 salinity profile (in ppt) for the ocean or the reference specific
1073 humidity profile (in g/kg) for the atmosphere.
1074
1075 The form of the equation of state is controlled by the character
1076 variables \textbf{buoyancyRelation} and \textbf{eosType}.
1077 \textbf{buoyancyRelation} is set to \texttt{'OCEANIC'} by default and
1078 needs to be set to \texttt{'ATMOSPHERIC'} for atmosphere simulations.
1079 In this case, \textbf{eosType} must be set to \texttt{'IDEALGAS'}.
1080 For the ocean, two forms of the equation of state are available:
1081 linear (set \textbf{eosType} to \texttt{'LINEAR'}) and a polynomial
1082 approximation to the full nonlinear equation ( set \textbf{eosType} to
1083 \texttt{'POLYNOMIAL'}). In the linear case, you need to specify the
1084 thermal and haline expansion coefficients represented by the variables
1085 \textbf{tAlpha} (in K$^{-1}$) and \textbf{sBeta} (in ppt$^{-1}$). For
1086 the nonlinear case, you need to generate a file of polynomial
1087 coefficients called \textit{POLY3.COEFFS}. To do this, use the program
1088 \textit{utils/knudsen2/knudsen2.f} under the model tree (a Makefile is
1089 available in the same directory and you will need to edit the number
1090 and the values of the vertical levels in \textit{knudsen2.f} so that
1091 they match those of your configuration).
1092
1093 There there are also higher polynomials for the equation of state:
1094 \begin{description}
1095 \item[\texttt{'UNESCO'}:] The UNESCO equation of state formula of
1096 Fofonoff and Millard \cite{fofonoff83}. This equation of state
1097 assumes in-situ temperature, which is not a model variable; {\em its
1098 use is therefore discouraged, and it is only listed for
1099 completeness}.
1100 \item[\texttt{'JMD95Z'}:] A modified UNESCO formula by Jackett and
1101 McDougall \cite{jackett95}, which uses the model variable potential
1102 temperature as input. The \texttt{'Z'} indicates that this equation
1103 of state uses a horizontally and temporally constant pressure
1104 $p_{0}=-g\rho_{0}z$.
1105 \item[\texttt{'JMD95P'}:] A modified UNESCO formula by Jackett and
1106 McDougall \cite{jackett95}, which uses the model variable potential
1107 temperature as input. The \texttt{'P'} indicates that this equation
1108 of state uses the actual hydrostatic pressure of the last time
1109 step. Lagging the pressure in this way requires an additional pickup
1110 file for restarts.
1111 \item[\texttt{'MDJWF'}:] The new, more accurate and less expensive
1112 equation of state by McDougall et~al. \cite{mcdougall03}. It also
1113 requires lagging the pressure and therefore an additional pickup
1114 file for restarts.
1115 \end{description}
1116 For none of these options an reference profile of temperature or
1117 salinity is required.
1118
1119 \subsection{Momentum equations}
1120
1121 In this section, we only focus for now on the parameters that you are
1122 likely to change, i.e. the ones relative to forcing and dissipation
1123 for example. The details relevant to the vector-invariant form of the
1124 equations and the various advection schemes are not covered for the
1125 moment. We assume that you use the standard form of the momentum
1126 equations (i.e. the flux-form) with the default advection scheme.
1127 Also, there are a few logical variables that allow you to turn on/off
1128 various terms in the momentum equation. These variables are called
1129 \textbf{momViscosity, momAdvection, momForcing, useCoriolis,
1130 momPressureForcing, momStepping} and \textbf{metricTerms }and are
1131 assumed to be set to \texttt{'.TRUE.'} here. Look at the file
1132 \textit{model/inc/PARAMS.h }for a precise definition of these
1133 variables.
1134
1135 \begin{description}
1136 \item[initialization] \
1137
1138 The velocity components are initialized to 0 unless the simulation
1139 is starting from a pickup file (see section on simulation control
1140 parameters).
1141
1142 \item[forcing] \
1143
1144 This section only applies to the ocean. You need to generate
1145 wind-stress data into two files \textbf{zonalWindFile} and
1146 \textbf{meridWindFile} corresponding to the zonal and meridional
1147 components of the wind stress, respectively (if you want the stress
1148 to be along the direction of only one of the model horizontal axes,
1149 you only need to generate one file). The format of the files is
1150 similar to the bathymetry file. The zonal (meridional) stress data
1151 are assumed to be in Pa and located at U-points (V-points). As for
1152 the bathymetry, the precision with which to read the binary data is
1153 controlled by the variable \textbf{readBinaryPrec}. See the matlab
1154 program \textit{gendata.m} in the \textit{input} directories under
1155 \textit{verification} to see how simple analytical wind forcing data
1156 are generated for the case study experiments.
1157
1158 There is also the possibility of prescribing time-dependent periodic
1159 forcing. To do this, concatenate the successive time records into a
1160 single file (for each stress component) ordered in a (x,y,t) fashion
1161 and set the following variables: \textbf{periodicExternalForcing }to
1162 \texttt{'.TRUE.'}, \textbf{externForcingPeriod }to the period (in s)
1163 of which the forcing varies (typically 1 month), and
1164 \textbf{externForcingCycle} to the repeat time (in s) of the forcing
1165 (typically 1 year -- note: \textbf{ externForcingCycle} must be a
1166 multiple of \textbf{externForcingPeriod}). With these variables set
1167 up, the model will interpolate the forcing linearly at each
1168 iteration.
1169
1170 \item[dissipation] \
1171
1172 The lateral eddy viscosity coefficient is specified through the
1173 variable \textbf{viscAh} (in m$^{2}$s$^{-1}$). The vertical eddy
1174 viscosity coefficient is specified through the variable
1175 \textbf{viscAz} (in m$^{2}$s$^{-1}$) for the ocean and
1176 \textbf{viscAp} (in Pa$^{2}$s$^{-1}$) for the atmosphere. The
1177 vertical diffusive fluxes can be computed implicitly by setting the
1178 logical variable \textbf{implicitViscosity }to \texttt{'.TRUE.'}.
1179 In addition, biharmonic mixing can be added as well through the
1180 variable \textbf{viscA4} (in m$^{4}$s$^{-1}$). On a spherical polar
1181 grid, you might also need to set the variable \textbf{cosPower}
1182 which is set to 0 by default and which represents the power of
1183 cosine of latitude to multiply viscosity. Slip or no-slip conditions
1184 at lateral and bottom boundaries are specified through the logical
1185 variables \textbf{no\_slip\_sides} and \textbf{no\_slip\_bottom}. If
1186 set to \texttt{'.FALSE.'}, free-slip boundary conditions are
1187 applied. If no-slip boundary conditions are applied at the bottom, a
1188 bottom drag can be applied as well. Two forms are available: linear
1189 (set the variable \textbf{bottomDragLinear} in s$ ^{-1}$) and
1190 quadratic (set the variable \textbf{bottomDragQuadratic} in
1191 m$^{-1}$).
1192
1193 The Fourier and Shapiro filters are described elsewhere.
1194
1195 \item[C-D scheme] \
1196
1197 If you run at a sufficiently coarse resolution, you will need the
1198 C-D scheme for the computation of the Coriolis terms. The
1199 variable\textbf{\ tauCD}, which represents the C-D scheme coupling
1200 timescale (in s) needs to be set.
1201
1202 \item[calculation of pressure/geopotential] \
1203
1204 First, to run a non-hydrostatic ocean simulation, set the logical
1205 variable \textbf{nonHydrostatic} to \texttt{'.TRUE.'}. The pressure
1206 field is then inverted through a 3D elliptic equation. (Note: this
1207 capability is not available for the atmosphere yet.) By default, a
1208 hydrostatic simulation is assumed and a 2D elliptic equation is used
1209 to invert the pressure field. The parameters controlling the
1210 behaviour of the elliptic solvers are the variables
1211 \textbf{cg2dMaxIters} and \textbf{cg2dTargetResidual } for
1212 the 2D case and \textbf{cg3dMaxIters} and
1213 \textbf{cg3dTargetResidual} for the 3D case. You probably won't need to
1214 alter the default values (are we sure of this?).
1215
1216 For the calculation of the surface pressure (for the ocean) or
1217 surface geopotential (for the atmosphere) you need to set the
1218 logical variables \textbf{rigidLid} and \textbf{implicitFreeSurface}
1219 (set one to \texttt{'.TRUE.'} and the other to \texttt{'.FALSE.'}
1220 depending on how you want to deal with the ocean upper or atmosphere
1221 lower boundary).
1222
1223 \end{description}
1224
1225 \subsection{Tracer equations}
1226
1227 This section covers the tracer equations i.e. the potential
1228 temperature equation and the salinity (for the ocean) or specific
1229 humidity (for the atmosphere) equation. As for the momentum equations,
1230 we only describe for now the parameters that you are likely to change.
1231 The logical variables \textbf{tempDiffusion} \textbf{tempAdvection}
1232 \textbf{tempForcing}, and \textbf{tempStepping} allow you to turn
1233 on/off terms in the temperature equation (same thing for salinity or
1234 specific humidity with variables \textbf{saltDiffusion},
1235 \textbf{saltAdvection} etc.). These variables are all assumed here to
1236 be set to \texttt{'.TRUE.'}. Look at file \textit{model/inc/PARAMS.h}
1237 for a precise definition.
1238
1239 \begin{description}
1240 \item[initialization] \
1241
1242 The initial tracer data can be contained in the binary files
1243 \textbf{hydrogThetaFile} and \textbf{hydrogSaltFile}. These files
1244 should contain 3D data ordered in an (x,y,r) fashion with k=1 as the
1245 first vertical level. If no file names are provided, the tracers
1246 are then initialized with the values of \textbf{tRef} and
1247 \textbf{sRef} mentioned above (in the equation of state section). In
1248 this case, the initial tracer data are uniform in x and y for each
1249 depth level.
1250
1251 \item[forcing] \
1252
1253 This part is more relevant for the ocean, the procedure for the
1254 atmosphere not being completely stabilized at the moment.
1255
1256 A combination of fluxes data and relaxation terms can be used for
1257 driving the tracer equations. For potential temperature, heat flux
1258 data (in W/m$ ^{2}$) can be stored in the 2D binary file
1259 \textbf{surfQfile}. Alternatively or in addition, the forcing can
1260 be specified through a relaxation term. The SST data to which the
1261 model surface temperatures are restored to are supposed to be stored
1262 in the 2D binary file \textbf{thetaClimFile}. The corresponding
1263 relaxation time scale coefficient is set through the variable
1264 \textbf{tauThetaClimRelax} (in s). The same procedure applies for
1265 salinity with the variable names \textbf{EmPmRfile},
1266 \textbf{saltClimFile}, and \textbf{tauSaltClimRelax} for freshwater
1267 flux (in m/s) and surface salinity (in ppt) data files and
1268 relaxation time scale coefficient (in s), respectively. Also for
1269 salinity, if the CPP key \textbf{USE\_NATURAL\_BCS} is turned on,
1270 natural boundary conditions are applied i.e. when computing the
1271 surface salinity tendency, the freshwater flux is multiplied by the
1272 model surface salinity instead of a constant salinity value.
1273
1274 As for the other input files, the precision with which to read the
1275 data is controlled by the variable \textbf{readBinaryPrec}.
1276 Time-dependent, periodic forcing can be applied as well following
1277 the same procedure used for the wind forcing data (see above).
1278
1279 \item[dissipation] \
1280
1281 Lateral eddy diffusivities for temperature and salinity/specific
1282 humidity are specified through the variables \textbf{diffKhT} and
1283 \textbf{diffKhS} (in m$^{2}$/s). Vertical eddy diffusivities are
1284 specified through the variables \textbf{diffKzT} and
1285 \textbf{diffKzS} (in m$^{2}$/s) for the ocean and \textbf{diffKpT
1286 }and \textbf{diffKpS} (in Pa$^{2}$/s) for the atmosphere. The
1287 vertical diffusive fluxes can be computed implicitly by setting the
1288 logical variable \textbf{implicitDiffusion} to \texttt{'.TRUE.'}.
1289 In addition, biharmonic diffusivities can be specified as well
1290 through the coefficients \textbf{diffK4T} and \textbf{diffK4S} (in
1291 m$^{4}$/s). Note that the cosine power scaling (specified through
1292 \textbf{cosPower}---see the momentum equations section) is applied to
1293 the tracer diffusivities (Laplacian and biharmonic) as well. The
1294 Gent and McWilliams parameterization for oceanic tracers is
1295 described in the package section. Finally, note that tracers can be
1296 also subject to Fourier and Shapiro filtering (see the corresponding
1297 section on these filters).
1298
1299 \item[ocean convection] \
1300
1301 Two options are available to parameterize ocean convection: one is
1302 to use the convective adjustment scheme. In this case, you need to
1303 set the variable \textbf{cadjFreq}, which represents the frequency
1304 (in s) with which the adjustment algorithm is called, to a non-zero
1305 value (if set to a negative value by the user, the model will set it
1306 to the tracer time step). The other option is to parameterize
1307 convection with implicit vertical diffusion. To do this, set the
1308 logical variable \textbf{implicitDiffusion} to \texttt{'.TRUE.'}
1309 and the real variable \textbf{ivdc\_kappa} to a value (in m$^{2}$/s)
1310 you wish the tracer vertical diffusivities to have when mixing
1311 tracers vertically due to static instabilities. Note that
1312 \textbf{cadjFreq} and \textbf{ivdc\_kappa}can not both have non-zero
1313 value.
1314
1315 \end{description}
1316
1317 \subsection{Simulation controls}
1318
1319 The model ''clock'' is defined by the variable \textbf{deltaTClock}
1320 (in s) which determines the IO frequencies and is used in tagging
1321 output. Typically, you will set it to the tracer time step for
1322 accelerated runs (otherwise it is simply set to the default time step
1323 \textbf{deltaT}). Frequency of checkpointing and dumping of the model
1324 state are referenced to this clock (see below).
1325
1326 \begin{description}
1327 \item[run duration] \
1328
1329 The beginning of a simulation is set by specifying a start time (in
1330 s) through the real variable \textbf{startTime} or by specifying an
1331 initial iteration number through the integer variable
1332 \textbf{nIter0}. If these variables are set to nonzero values, the
1333 model will look for a ''pickup'' file \textit{pickup.0000nIter0} to
1334 restart the integration. The end of a simulation is set through the
1335 real variable \textbf{endTime} (in s). Alternatively, you can
1336 specify instead the number of time steps to execute through the
1337 integer variable \textbf{nTimeSteps}.
1338
1339 \item[frequency of output] \
1340
1341 Real variables defining frequencies (in s) with which output files
1342 are written on disk need to be set up. \textbf{dumpFreq} controls
1343 the frequency with which the instantaneous state of the model is
1344 saved. \textbf{chkPtFreq} and \textbf{pchkPtFreq} control the output
1345 frequency of rolling and permanent checkpoint files, respectively.
1346 See section 1.5.1 Output files for the definition of model state and
1347 checkpoint files. In addition, time-averaged fields can be written
1348 out by setting the variable \textbf{taveFreq} (in s). The precision
1349 with which to write the binary data is controlled by the integer
1350 variable w\textbf{riteBinaryPrec} (set it to \texttt{32} or
1351 \texttt{64}).
1352
1353 \end{description}
1354
1355
1356 %%% Local Variables:
1357 %%% mode: latex
1358 %%% TeX-master: t
1359 %%% End:

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