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1 % $Header: /u/u3/gcmpack/manual/part3/getting_started.tex,v 1.15 2004/01/28 20:50:14 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 If CVS is available on your system, we strongly encourage you to use it. CVS
83 provides an efficient and elegant way of organizing your code and keeping
84 track of your changes. If CVS is not available on your machine, you can also
85 download a tar file.
86
87 Before you can use CVS, the following environment variable(s) should
88 be set within your shell. For a csh or tcsh shell, put the following
89 \begin{verbatim}
90 % setenv CVSROOT :pserver:cvsanon@mitgcm.org:/u/gcmpack
91 \end{verbatim}
92 in your .cshrc or .tcshrc file. For bash or sh shells, put:
93 \begin{verbatim}
94 % export CVSROOT=':pserver:cvsanon@mitgcm.org:/u/gcmpack'
95 \end{verbatim}
96 in your .profile or .bashrc file.
97
98
99 To get MITgcm through CVS, first register with the MITgcm CVS server
100 using command:
101 \begin{verbatim}
102 % cvs login ( CVS password: cvsanon )
103 \end{verbatim}
104 You only need to do a ``cvs login'' once.
105
106 To obtain the latest sources type:
107 \begin{verbatim}
108 % cvs co MITgcm
109 \end{verbatim}
110 or to get a specific release type:
111 \begin{verbatim}
112 % cvs co -P -r checkpoint52i_post MITgcm
113 \end{verbatim}
114 The MITgcm web site contains further directions concerning the source
115 code and CVS. It also contains a web interface to our CVS archive so
116 that one may easily view the state of files, revisions, and other
117 development milestones:
118 \begin{rawhtml} <A href=http://mitgcm.org/download target="idontexist"> \end{rawhtml}
119 \begin{verbatim}
120 http://mitgcm.org/source\_code.html
121 \end{verbatim}
122 \begin{rawhtml} </A> \end{rawhtml}
123
124
125 The checkout process creates a directory called \textit{MITgcm}. If
126 the directory \textit{MITgcm} exists this command updates your code
127 based on the repository. Each directory in the source tree contains a
128 directory \textit{CVS}. This information is required by CVS to keep
129 track of your file versions with respect to the repository. Don't edit
130 the files in \textit{CVS}! You can also use CVS to download code
131 updates. More extensive information on using CVS for maintaining
132 MITgcm code can be found
133 \begin{rawhtml} <A href=http://mitgcm.org/usingcvstoget.html target="idontexist"> \end{rawhtml}
134 here
135 \begin{rawhtml} </A> \end{rawhtml}
136 .
137
138
139 \paragraph*{Conventional download method}
140 \label{sect:conventionalDownload}
141
142 If you do not have CVS on your system, you can download the model as a
143 tar file from the web site at:
144 \begin{rawhtml} <A href=http://mitgcm.org/download target="idontexist"> \end{rawhtml}
145 \begin{verbatim}
146 http://mitgcm.org/download/
147 \end{verbatim}
148 \begin{rawhtml} </A> \end{rawhtml}
149 The tar file still contains CVS information which we urge you not to
150 delete; even if you do not use CVS yourself the information can help
151 us if you should need to send us your copy of the code. If a recent
152 tar file does not exist, then please contact the developers through
153 the MITgcm-support list.
154
155 \paragraph*{Upgrading from an earlier version}
156
157 If you already have an earlier version of the code you can ``upgrade''
158 your copy instead of downloading the entire repository again. First,
159 ``cd'' (change directory) to the top of your working copy:
160 \begin{verbatim}
161 % cd MITgcm
162 \end{verbatim}
163 and then issue the cvs update command such as:
164 \begin{verbatim}
165 % cvs -q update -r checkpoint52i_post -d -P
166 \end{verbatim}
167 This will update the ``tag'' to ``checkpoint52i\_post'', add any new
168 directories (-d) and remove any empty directories (-P). The -q option
169 means be quiet which will reduce the number of messages you'll see in
170 the terminal. If you have modified the code prior to upgrading, CVS
171 will try to merge your changes with the upgrades. If there is a
172 conflict between your modifications and the upgrade, it will report
173 that file with a ``C'' in front, e.g.:
174 \begin{verbatim}
175 C model/src/ini_parms.F
176 \end{verbatim}
177 If the list of conflicts scrolled off the screen, you can re-issue the
178 cvs update command and it will report the conflicts. Conflicts are
179 indicated in the code by the delimites ``$<<<<<<<$'', ``======='' and
180 ``$>>>>>>>$''. For example,
181 \begin{verbatim}
182 <<<<<<< ini_parms.F
183 & bottomDragLinear,myOwnBottomDragCoefficient,
184 =======
185 & bottomDragLinear,bottomDragQuadratic,
186 >>>>>>> 1.18
187 \end{verbatim}
188 means that you added ``myOwnBottomDragCoefficient'' to a namelist at
189 the same time and place that we added ``bottomDragQuadratic''. You
190 need to resolve this conflict and in this case the line should be
191 changed to:
192 \begin{verbatim}
193 & bottomDragLinear,bottomDragQuadratic,myOwnBottomDragCoefficient,
194 \end{verbatim}
195 and the lines with the delimiters ($<<<<<<$,======,$>>>>>>$) be deleted.
196 Unless you are making modifications which exactly parallel
197 developments we make, these types of conflicts should be rare.
198
199 \paragraph*{Upgrading to the current pre-release version}
200
201 We don't make a ``release'' for every little patch and bug fix in
202 order to keep the frequency of upgrades to a minimum. However, if you
203 have run into a problem for which ``we have already fixed in the
204 latest code'' and we haven't made a ``tag'' or ``release'' since that
205 patch then you'll need to get the latest code:
206 \begin{verbatim}
207 % cvs -q update -A -d -P
208 \end{verbatim}
209 Unlike, the ``check-out'' and ``update'' procedures above, there is no
210 ``tag'' or release name. The -A tells CVS to upgrade to the
211 very latest version. As a rule, we don't recommend this since you
212 might upgrade while we are in the processes of checking in the code so
213 that you may only have part of a patch. Using this method of updating
214 also means we can't tell what version of the code you are working
215 with. So please be sure you understand what you're doing.
216
217 \section{Model and directory structure}
218
219 The ``numerical'' model is contained within a execution environment
220 support wrapper. This wrapper is designed to provide a general
221 framework for grid-point models. MITgcmUV is a specific numerical
222 model that uses the framework. Under this structure the model is split
223 into execution environment support code and conventional numerical
224 model code. The execution environment support code is held under the
225 \textit{eesupp} directory. The grid point model code is held under the
226 \textit{model} directory. Code execution actually starts in the
227 \textit{eesupp} routines and not in the \textit{model} routines. For
228 this reason the top-level
229 \textit{MAIN.F} is in the \textit{eesupp/src} directory. In general,
230 end-users should not need to worry about this level. The top-level routine
231 for the numerical part of the code is in \textit{model/src/THE\_MODEL\_MAIN.F%
232 }. Here is a brief description of the directory structure of the model under
233 the root tree (a detailed description is given in section 3: Code structure).
234
235 \begin{itemize}
236 \item \textit{bin}: this directory is initially empty. It is the default
237 directory in which to compile the code.
238
239 \item \textit{diags}: contains the code relative to time-averaged
240 diagnostics. It is subdivided into two subdirectories \textit{inc} and
241 \textit{src} that contain include files (*.\textit{h} files) and Fortran
242 subroutines (*.\textit{F} files), respectively.
243
244 \item \textit{doc}: contains brief documentation notes.
245
246 \item \textit{eesupp}: contains the execution environment source code. Also
247 subdivided into two subdirectories \textit{inc} and \textit{src}.
248
249 \item \textit{exe}: this directory is initially empty. It is the default
250 directory in which to execute the code.
251
252 \item \textit{model}: this directory contains the main source code. Also
253 subdivided into two subdirectories \textit{inc} and \textit{src}.
254
255 \item \textit{pkg}: contains the source code for the packages. Each package
256 corresponds to a subdirectory. For example, \textit{gmredi} contains the
257 code related to the Gent-McWilliams/Redi scheme, \textit{aim} the code
258 relative to the atmospheric intermediate physics. The packages are described
259 in detail in section 3.
260
261 \item \textit{tools}: this directory contains various useful tools. For
262 example, \textit{genmake2} is a script written in csh (C-shell) that should
263 be used to generate your makefile. The directory \textit{adjoint} contains
264 the makefile specific to the Tangent linear and Adjoint Compiler (TAMC) that
265 generates the adjoint code. The latter is described in details in part V.
266
267 \item \textit{utils}: this directory contains various utilities. The
268 subdirectory \textit{knudsen2} contains code and a makefile that
269 compute coefficients of the polynomial approximation to the knudsen
270 formula for an ocean nonlinear equation of state. The \textit{matlab}
271 subdirectory contains matlab scripts for reading model output directly
272 into matlab. \textit{scripts} contains C-shell post-processing
273 scripts for joining processor-based and tiled-based model output.
274
275 \item \textit{verification}: this directory contains the model examples. See
276 section \ref{sect:modelExamples}.
277 \end{itemize}
278
279 \section{Example experiments}
280 \label{sect:modelExamples}
281
282 %% a set of twenty-four pre-configured numerical experiments
283
284 The MITgcm distribution comes with more than a dozen pre-configured
285 numerical experiments. Some of these example experiments are tests of
286 individual parts of the model code, but many are fully fledged
287 numerical simulations. A few of the examples are used for tutorial
288 documentation in sections \ref{sect:eg-baro} - \ref{sect:eg-global}.
289 The other examples follow the same general structure as the tutorial
290 examples. However, they only include brief instructions in a text file
291 called {\it README}. The examples are located in subdirectories under
292 the directory \textit{verification}. Each example is briefly described
293 below.
294
295 \subsection{Full list of model examples}
296
297 \begin{enumerate}
298 \item \textit{exp0} - single layer, ocean double gyre (barotropic with
299 free-surface). This experiment is described in detail in section
300 \ref{sect:eg-baro}.
301
302 \item \textit{exp1} - Four layer, ocean double gyre. This experiment
303 is described in detail in section \ref{sect:eg-baroc}.
304
305 \item \textit{exp2} - 4x4 degree global ocean simulation with steady
306 climatological forcing. This experiment is described in detail in
307 section \ref{sect:eg-global}.
308
309 \item \textit{exp4} - Flow over a Gaussian bump in open-water or
310 channel with open boundaries.
311
312 \item \textit{exp5} - Inhomogenously forced ocean convection in a
313 doubly periodic box.
314
315 \item \textit{front\_relax} - Relaxation of an ocean thermal front (test for
316 Gent/McWilliams scheme). 2D (Y-Z).
317
318 \item \textit{internal wave} - Ocean internal wave forced by open
319 boundary conditions.
320
321 \item \textit{natl\_box} - Eastern subtropical North Atlantic with KPP
322 scheme; 1 month integration
323
324 \item \textit{hs94.1x64x5} - Zonal averaged atmosphere using Held and
325 Suarez '94 forcing.
326
327 \item \textit{hs94.128x64x5} - 3D atmosphere dynamics using Held and
328 Suarez '94 forcing.
329
330 \item \textit{hs94.cs-32x32x5} - 3D atmosphere dynamics using Held and
331 Suarez '94 forcing on the cubed sphere.
332
333 \item \textit{aim.5l\_zon-ave} - Intermediate Atmospheric physics.
334 Global Zonal Mean configuration, 1x64x5 resolution.
335
336 \item \textit{aim.5l\_XZ\_Equatorial\_Slice} - Intermediate
337 Atmospheric physics, equatorial Slice configuration. 2D (X-Z).
338
339 \item \textit{aim.5l\_Equatorial\_Channel} - Intermediate Atmospheric
340 physics. 3D Equatorial Channel configuration.
341
342 \item \textit{aim.5l\_LatLon} - Intermediate Atmospheric physics.
343 Global configuration, on latitude longitude grid with 128x64x5 grid
344 points ($2.8^\circ{\rm degree}$ resolution).
345
346 \item \textit{adjustment.128x64x1} Barotropic adjustment problem on
347 latitude longitude grid with 128x64 grid points ($2.8^\circ{\rm
348 degree}$ resolution).
349
350 \item \textit{adjustment.cs-32x32x1} Barotropic adjustment problem on
351 cube sphere grid with 32x32 points per face ( roughly $2.8^\circ{\rm
352 degree}$ resolution).
353
354 \item \textit{advect\_cs} Two-dimensional passive advection test on
355 cube sphere grid.
356
357 \item \textit{advect\_xy} Two-dimensional (horizontal plane) passive
358 advection test on Cartesian grid.
359
360 \item \textit{advect\_yz} Two-dimensional (vertical plane) passive
361 advection test on Cartesian grid.
362
363 \item \textit{carbon} Simple passive tracer experiment. Includes
364 derivative calculation. Described in detail in section
365 \ref{sect:eg-carbon-ad}.
366
367 \item \textit{flt\_example} Example of using float package.
368
369 \item \textit{global\_ocean.90x40x15} Global circulation with GM, flux
370 boundary conditions and poles.
371
372 \item \textit{global\_ocean\_pressure} Global circulation in pressure
373 coordinate (non-Boussinesq ocean model). Described in detail in
374 section \ref{sect:eg-globalpressure}.
375
376 \item \textit{solid-body.cs-32x32x1} Solid body rotation test for cube
377 sphere grid.
378
379 \end{enumerate}
380
381 \subsection{Directory structure of model examples}
382
383 Each example directory has the following subdirectories:
384
385 \begin{itemize}
386 \item \textit{code}: contains the code particular to the example. At a
387 minimum, this directory includes the following files:
388
389 \begin{itemize}
390 \item \textit{code/CPP\_EEOPTIONS.h}: declares CPP keys relative to
391 the ``execution environment'' part of the code. The default
392 version is located in \textit{eesupp/inc}.
393
394 \item \textit{code/CPP\_OPTIONS.h}: declares CPP keys relative to
395 the ``numerical model'' part of the code. The default version is
396 located in \textit{model/inc}.
397
398 \item \textit{code/SIZE.h}: declares size of underlying
399 computational grid. The default version is located in
400 \textit{model/inc}.
401 \end{itemize}
402
403 In addition, other include files and subroutines might be present in
404 \textit{code} depending on the particular experiment. See Section 2
405 for more details.
406
407 \item \textit{input}: contains the input data files required to run
408 the example. At a minimum, the \textit{input} directory contains the
409 following files:
410
411 \begin{itemize}
412 \item \textit{input/data}: this file, written as a namelist,
413 specifies the main parameters for the experiment.
414
415 \item \textit{input/data.pkg}: contains parameters relative to the
416 packages used in the experiment.
417
418 \item \textit{input/eedata}: this file contains ``execution
419 environment'' data. At present, this consists of a specification
420 of the number of threads to use in $X$ and $Y$ under multithreaded
421 execution.
422 \end{itemize}
423
424 In addition, you will also find in this directory the forcing and
425 topography files as well as the files describing the initial state of
426 the experiment. This varies from experiment to experiment. See
427 section 2 for more details.
428
429 \item \textit{results}: this directory contains the output file
430 \textit{output.txt} produced by the simulation example. This file is
431 useful for comparison with your own output when you run the
432 experiment.
433 \end{itemize}
434
435 Once you have chosen the example you want to run, you are ready to compile
436 the code.
437
438 \section{Building the code}
439 \label{sect:buildingCode}
440
441 To compile the code, we use the {\em make} program. This uses a file
442 ({\em Makefile}) that allows us to pre-process source files, specify
443 compiler and optimization options and also figures out any file
444 dependencies. We supply a script ({\em genmake2}), described in
445 section \ref{sect:genmake}, that automatically creates the {\em
446 Makefile} for you. You then need to build the dependencies and
447 compile the code.
448
449 As an example, let's assume that you want to build and run experiment
450 \textit{verification/exp2}. The are multiple ways and places to
451 actually do this but here let's build the code in
452 \textit{verification/exp2/input}:
453 \begin{verbatim}
454 % cd verification/exp2/input
455 \end{verbatim}
456 First, build the {\em Makefile}:
457 \begin{verbatim}
458 % ../../../tools/genmake2 -mods=../code
459 \end{verbatim}
460 The command line option tells {\em genmake} to override model source
461 code with any files in the directory {\em ./code/}.
462
463 On many systems, the {\em genmake2} program will be able to
464 automatically recognize the hardware, find compilers and other tools
465 within the user's path (``echo \$PATH''), and then choose an
466 appropriate set of options from the files contained in the {\em
467 tools/build\_options} directory. Under some circumstances, a user
468 may have to create a new ``optfile'' in order to specify the exact
469 combination of compiler, compiler flags, libraries, and other options
470 necessary to build a particular configuration of MITgcm. In such
471 cases, it is generally helpful to read the existing ``optfiles'' and
472 mimic their syntax.
473
474 Through the MITgcm-support list, the MITgcm developers are willing to
475 provide help writing or modifing ``optfiles''. And we encourage users
476 to post new ``optfiles'' (particularly ones for new machines or
477 architectures) to the MITgcm-support list.
478
479 To specify an optfile to {\em genmake2}, the syntax is:
480 \begin{verbatim}
481 % ../../../tools/genmake2 -mods=../code -of /path/to/optfile
482 \end{verbatim}
483
484 Once a {\em Makefile} has been generated, we create the dependencies:
485 \begin{verbatim}
486 % make depend
487 \end{verbatim}
488 This modifies the {\em Makefile} by attaching a [long] list of files
489 upon which other files depend. The purpose of this is to reduce
490 re-compilation if and when you start to modify the code. The {\tt make
491 depend} command also creates links from the model source to this
492 directory.
493
494 Next compile the code:
495 \begin{verbatim}
496 % make
497 \end{verbatim}
498 The {\tt make} command creates an executable called \textit{mitgcmuv}.
499 Additional make ``targets'' are defined within the makefile to aid in
500 the production of adjoint and other versions of MITgcm.
501
502 Now you are ready to run the model. General instructions for doing so are
503 given in section \ref{sect:runModel}. Here, we can run the model with:
504 \begin{verbatim}
505 ./mitgcmuv > output.txt
506 \end{verbatim}
507 where we are re-directing the stream of text output to the file {\em
508 output.txt}.
509
510
511 \subsection{Building/compiling the code elsewhere}
512
513 In the example above (section \ref{sect:buildingCode}) we built the
514 executable in the {\em input} directory of the experiment for
515 convenience. You can also configure and compile the code in other
516 locations, for example on a scratch disk with out having to copy the
517 entire source tree. The only requirement to do so is you have {\tt
518 genmake2} in your path or you know the absolute path to {\tt
519 genmake2}.
520
521 The following sections outline some possible methods of organizing
522 your source and data.
523
524 \subsubsection{Building from the {\em ../code directory}}
525
526 This is just as simple as building in the {\em input/} directory:
527 \begin{verbatim}
528 % cd verification/exp2/code
529 % ../../../tools/genmake2
530 % make depend
531 % make
532 \end{verbatim}
533 However, to run the model the executable ({\em mitgcmuv}) and input
534 files must be in the same place. If you only have one calculation to make:
535 \begin{verbatim}
536 % cd ../input
537 % cp ../code/mitgcmuv ./
538 % ./mitgcmuv > output.txt
539 \end{verbatim}
540 or if you will be making multiple runs with the same executable:
541 \begin{verbatim}
542 % cd ../
543 % cp -r input run1
544 % cp code/mitgcmuv run1
545 % cd run1
546 % ./mitgcmuv > output.txt
547 \end{verbatim}
548
549 \subsubsection{Building from a new directory}
550
551 Since the {\em input} directory contains input files it is often more
552 useful to keep {\em input} pristine and build in a new directory
553 within {\em verification/exp2/}:
554 \begin{verbatim}
555 % cd verification/exp2
556 % mkdir build
557 % cd build
558 % ../../../tools/genmake2 -mods=../code
559 % make depend
560 % make
561 \end{verbatim}
562 This builds the code exactly as before but this time you need to copy
563 either the executable or the input files or both in order to run the
564 model. For example,
565 \begin{verbatim}
566 % cp ../input/* ./
567 % ./mitgcmuv > output.txt
568 \end{verbatim}
569 or if you tend to make multiple runs with the same executable then
570 running in a new directory each time might be more appropriate:
571 \begin{verbatim}
572 % cd ../
573 % mkdir run1
574 % cp build/mitgcmuv run1/
575 % cp input/* run1/
576 % cd run1
577 % ./mitgcmuv > output.txt
578 \end{verbatim}
579
580 \subsubsection{Building on a scratch disk}
581
582 Model object files and output data can use up large amounts of disk
583 space so it is often the case that you will be operating on a large
584 scratch disk. Assuming the model source is in {\em ~/MITgcm} then the
585 following commands will build the model in {\em /scratch/exp2-run1}:
586 \begin{verbatim}
587 % cd /scratch/exp2-run1
588 % ~/MITgcm/tools/genmake2 -rootdir=~/MITgcm \
589 -mods=~/MITgcm/verification/exp2/code
590 % make depend
591 % make
592 \end{verbatim}
593 To run the model here, you'll need the input files:
594 \begin{verbatim}
595 % cp ~/MITgcm/verification/exp2/input/* ./
596 % ./mitgcmuv > output.txt
597 \end{verbatim}
598
599 As before, you could build in one directory and make multiple runs of
600 the one experiment:
601 \begin{verbatim}
602 % cd /scratch/exp2
603 % mkdir build
604 % cd build
605 % ~/MITgcm/tools/genmake2 -rootdir=~/MITgcm \
606 -mods=~/MITgcm/verification/exp2/code
607 % make depend
608 % make
609 % cd ../
610 % cp -r ~/MITgcm/verification/exp2/input run2
611 % cd run2
612 % ./mitgcmuv > output.txt
613 \end{verbatim}
614
615
616
617 \subsection{Using \textit{genmake2}}
618 \label{sect:genmake}
619
620 To compile the code, first use the program \texttt{genmake2} (located
621 in the \textit{tools} directory) to generate a Makefile.
622 \texttt{genmake2} is a shell script written to work with all
623 ``sh''--compatible shells including bash v1, bash v2, and Bourne.
624 Internally, \texttt{genmake2} determines the locations of needed
625 files, the compiler, compiler options, libraries, and Unix tools. It
626 relies upon a number of ``optfiles'' located in the {\em
627 tools/build\_options} directory.
628
629 The purpose of the optfiles is to provide all the compilation options
630 for particular ``platforms'' (where ``platform'' roughly means the
631 combination of the hardware and the compiler) and code configurations.
632 Given the combinations of possible compilers and library dependencies
633 ({\it eg.} MPI and NetCDF) there may be numerous optfiles available
634 for a single machine. The naming scheme for the majority of the
635 optfiles shipped with the code is
636 \begin{center}
637 {\bf OS\_HARDWARE\_COMPILER }
638 \end{center}
639 where
640 \begin{description}
641 \item[OS] is the name of the operating system (generally the
642 lower-case output of the {\tt 'uname'} command)
643 \item[HARDWARE] is a string that describes the CPU type and
644 corresponds to output from the {\tt 'uname -m'} command:
645 \begin{description}
646 \item[ia32] is for ``x86'' machines such as i386, i486, i586, i686,
647 and athlon
648 \item[ia64] is for Intel IA64 systems (eg. Itanium, Itanium2)
649 \item[amd64] is AMD x86\_64 systems
650 \item[ppc] is for Mac PowerPC systems
651 \end{description}
652 \item[COMPILER] is the compiler name (generally, the name of the
653 FORTRAN executable)
654 \end{description}
655
656 In many cases, the default optfiles are sufficient and will result in
657 usable Makefiles. However, for some machines or code configurations,
658 new ``optfiles'' must be written. To create a new optfile, it is
659 generally best to start with one of the defaults and modify it to suit
660 your needs. Like \texttt{genmake2}, the optfiles are all written
661 using a simple ``sh''--compatible syntax. While nearly all variables
662 used within \texttt{genmake2} may be specified in the optfiles, the
663 critical ones that should be defined are:
664
665 \begin{description}
666 \item[FC] the FORTRAN compiler (executable) to use
667 \item[DEFINES] the command-line DEFINE options passed to the compiler
668 \item[CPP] the C pre-processor to use
669 \item[NOOPTFLAGS] options flags for special files that should not be
670 optimized
671 \end{description}
672
673 For example, the optfile for a typical Red Hat Linux machine (``ia32''
674 architecture) using the GCC (g77) compiler is
675 \begin{verbatim}
676 FC=g77
677 DEFINES='-D_BYTESWAPIO -DWORDLENGTH=4'
678 CPP='cpp -traditional -P'
679 NOOPTFLAGS='-O0'
680 # For IEEE, use the "-ffloat-store" option
681 if test "x$IEEE" = x ; then
682 FFLAGS='-Wimplicit -Wunused -Wuninitialized'
683 FOPTIM='-O3 -malign-double -funroll-loops'
684 else
685 FFLAGS='-Wimplicit -Wunused -ffloat-store'
686 FOPTIM='-O0 -malign-double'
687 fi
688 \end{verbatim}
689
690 If you write an optfile for an unrepresented machine or compiler, you
691 are strongly encouraged to submit the optfile to the MITgcm project
692 for inclusion. Please send the file to the
693 \begin{rawhtml} <A href="mail-to:MITgcm-support@mitgcm.org"> \end{rawhtml}
694 \begin{center}
695 MITgcm-support@mitgcm.org
696 \end{center}
697 \begin{rawhtml} </A> \end{rawhtml}
698 mailing list.
699
700 In addition to the optfiles, \texttt{genmake2} supports a number of
701 helpful command-line options. A complete list of these options can be
702 obtained from:
703 \begin{verbatim}
704 % genmake2 -h
705 \end{verbatim}
706
707 The most important command-line options are:
708 \begin{description}
709
710 \item[--optfile=/PATH/FILENAME] specifies the optfile that should be
711 used for a particular build.
712
713 If no "optfile" is specified (either through the command line or the
714 MITGCM\_OPTFILE environment variable), genmake2 will try to make a
715 reasonable guess from the list provided in {\em
716 tools/build\_options}. The method used for making this guess is
717 to first determine the combination of operating system and hardware
718 (eg. "linux\_ia32") and then find a working FORTRAN compiler within
719 the user's path. When these three items have been identified,
720 genmake2 will try to find an optfile that has a matching name.
721
722 \item[--pdepend=/PATH/FILENAME] specifies the dependency file used for
723 packages.
724
725 If not specified, the default dependency file {\em pkg/pkg\_depend}
726 is used. The syntax for this file is parsed on a line-by-line basis
727 where each line containes either a comment ("\#") or a simple
728 "PKGNAME1 (+|-)PKGNAME2" pairwise rule where the "+" or "-" symbol
729 specifies a "must be used with" or a "must not be used with"
730 relationship, respectively. If no rule is specified, then it is
731 assumed that the two packages are compatible and will function
732 either with or without each other.
733
734 \item[--pdefault='PKG1 PKG2 PKG3 ...'] specifies the default set of
735 packages to be used.
736
737 If not set, the default package list will be read from {\em
738 pkg/pkg\_default}
739
740 \item[--adof=/path/to/file] specifies the "adjoint" or automatic
741 differentiation options file to be used. The file is analogous to
742 the ``optfile'' defined above but it specifies information for the
743 AD build process.
744
745 The default file is located in {\em
746 tools/adjoint\_options/adjoint\_default} and it defines the "TAF"
747 and "TAMC" compilers. An alternate version is also available at
748 {\em tools/adjoint\_options/adjoint\_staf} that selects the newer
749 "STAF" compiler. As with any compilers, it is helpful to have their
750 directories listed in your {\tt \$PATH} environment variable.
751
752 \item[--mods='DIR1 DIR2 DIR3 ...'] specifies a list of directories
753 containing ``modifications''. These directories contain files with
754 names that may (or may not) exist in the main MITgcm source tree but
755 will be overridden by any identically-named sources within the
756 ``MODS'' directories.
757
758 The order of precedence for this "name-hiding" is as follows:
759 \begin{itemize}
760 \item ``MODS'' directories (in the order given)
761 \item Packages either explicitly specified or provided by default
762 (in the order given)
763 \item Packages included due to package dependencies (in the order
764 that that package dependencies are parsed)
765 \item The "standard dirs" (which may have been specified by the
766 ``-standarddirs'' option)
767 \end{itemize}
768
769 \item[--make=/path/to/gmake] Due to the poor handling of soft-links and
770 other bugs common with the \texttt{make} versions provided by
771 commercial Unix vendors, GNU \texttt{make} (sometimes called
772 \texttt{gmake}) should be preferred. This option provides a means
773 for specifying the make executable to be used.
774
775 \end{description}
776
777
778
779 \section{Running the model}
780 \label{sect:runModel}
781
782 If compilation finished succesfuully (section \ref{sect:buildModel})
783 then an executable called {\em mitgcmuv} will now exist in the local
784 directory.
785
786 To run the model as a single process (ie. not in parallel) simply
787 type:
788 \begin{verbatim}
789 % ./mitgcmuv
790 \end{verbatim}
791 The ``./'' is a safe-guard to make sure you use the local executable
792 in case you have others that exist in your path (surely odd if you
793 do!). The above command will spew out many lines of text output to
794 your screen. This output contains details such as parameter values as
795 well as diagnostics such as mean Kinetic energy, largest CFL number,
796 etc. It is worth keeping this text output with the binary output so we
797 normally re-direct the {\em stdout} stream as follows:
798 \begin{verbatim}
799 % ./mitgcmuv > output.txt
800 \end{verbatim}
801
802 For the example experiments in {\em vericication}, an example of the
803 output is kept in {\em results/output.txt} for comparison. You can compare
804 your {\em output.txt} with this one to check that the set-up works.
805
806
807
808 \subsection{Output files}
809
810 The model produces various output files. At a minimum, the instantaneous
811 ``state'' of the model is written out, which is made of the following files:
812
813 \begin{itemize}
814 \item \textit{U.00000nIter} - zonal component of velocity field (m/s and $>
815 0 $ eastward).
816
817 \item \textit{V.00000nIter} - meridional component of velocity field (m/s
818 and $> 0$ northward).
819
820 \item \textit{W.00000nIter} - vertical component of velocity field (ocean:
821 m/s and $> 0$ upward, atmosphere: Pa/s and $> 0$ towards increasing pressure
822 i.e. downward).
823
824 \item \textit{T.00000nIter} - potential temperature (ocean: $^{0}$C,
825 atmosphere: $^{0}$K).
826
827 \item \textit{S.00000nIter} - ocean: salinity (psu), atmosphere: water vapor
828 (g/kg).
829
830 \item \textit{Eta.00000nIter} - ocean: surface elevation (m), atmosphere:
831 surface pressure anomaly (Pa).
832 \end{itemize}
833
834 The chain \textit{00000nIter} consists of ten figures that specify the
835 iteration number at which the output is written out. For example, \textit{%
836 U.0000000300} is the zonal velocity at iteration 300.
837
838 In addition, a ``pickup'' or ``checkpoint'' file called:
839
840 \begin{itemize}
841 \item \textit{pickup.00000nIter}
842 \end{itemize}
843
844 is written out. This file represents the state of the model in a condensed
845 form and is used for restarting the integration. If the C-D scheme is used,
846 there is an additional ``pickup'' file:
847
848 \begin{itemize}
849 \item \textit{pickup\_cd.00000nIter}
850 \end{itemize}
851
852 containing the D-grid velocity data and that has to be written out as well
853 in order to restart the integration. Rolling checkpoint files are the same
854 as the pickup files but are named differently. Their name contain the chain
855 \textit{ckptA} or \textit{ckptB} instead of \textit{00000nIter}. They can be
856 used to restart the model but are overwritten every other time they are
857 output to save disk space during long integrations.
858
859 \subsection{Looking at the output}
860
861 All the model data are written according to a ``meta/data'' file format.
862 Each variable is associated with two files with suffix names \textit{.data}
863 and \textit{.meta}. The \textit{.data} file contains the data written in
864 binary form (big\_endian by default). The \textit{.meta} file is a
865 ``header'' file that contains information about the size and the structure
866 of the \textit{.data} file. This way of organizing the output is
867 particularly useful when running multi-processors calculations. The base
868 version of the model includes a few matlab utilities to read output files
869 written in this format. The matlab scripts are located in the directory
870 \textit{utils/matlab} under the root tree. The script \textit{rdmds.m} reads
871 the data. Look at the comments inside the script to see how to use it.
872
873 Some examples of reading and visualizing some output in {\em Matlab}:
874 \begin{verbatim}
875 % matlab
876 >> H=rdmds('Depth');
877 >> contourf(H');colorbar;
878 >> title('Depth of fluid as used by model');
879
880 >> eta=rdmds('Eta',10);
881 >> imagesc(eta');axis ij;colorbar;
882 >> title('Surface height at iter=10');
883
884 >> eta=rdmds('Eta',[0:10:100]);
885 >> for n=1:11; imagesc(eta(:,:,n)');axis ij;colorbar;pause(.5);end
886 \end{verbatim}
887
888 \section{Doing it yourself: customizing the code}
889
890 When you are ready to run the model in the configuration you want, the
891 easiest thing is to use and adapt the setup of the case studies experiment
892 (described previously) that is the closest to your configuration. Then, the
893 amount of setup will be minimized. In this section, we focus on the setup
894 relative to the ''numerical model'' part of the code (the setup relative to
895 the ''execution environment'' part is covered in the parallel implementation
896 section) and on the variables and parameters that you are likely to change.
897
898 \subsection{Configuration and setup}
899
900 The CPP keys relative to the ''numerical model'' part of the code are all
901 defined and set in the file \textit{CPP\_OPTIONS.h }in the directory \textit{%
902 model/inc }or in one of the \textit{code }directories of the case study
903 experiments under \textit{verification.} The model parameters are defined
904 and declared in the file \textit{model/inc/PARAMS.h }and their default
905 values are set in the routine \textit{model/src/set\_defaults.F. }The
906 default values can be modified in the namelist file \textit{data }which
907 needs to be located in the directory where you will run the model. The
908 parameters are initialized in the routine \textit{model/src/ini\_parms.F}.
909 Look at this routine to see in what part of the namelist the parameters are
910 located.
911
912 In what follows the parameters are grouped into categories related to the
913 computational domain, the equations solved in the model, and the simulation
914 controls.
915
916 \subsection{Computational domain, geometry and time-discretization}
917
918 \begin{itemize}
919 \item dimensions
920 \end{itemize}
921
922 The number of points in the x, y,\textit{\ }and r\textit{\ }directions are
923 represented by the variables \textbf{sNx}\textit{, }\textbf{sNy}\textit{, }%
924 and \textbf{Nr}\textit{\ }respectively which are declared and set in the
925 file \textit{model/inc/SIZE.h. }(Again, this assumes a mono-processor
926 calculation. For multiprocessor calculations see section on parallel
927 implementation.)
928
929 \begin{itemize}
930 \item grid
931 \end{itemize}
932
933 Three different grids are available: cartesian, spherical polar, and
934 curvilinear (including the cubed sphere). The grid is set through the
935 logical variables \textbf{usingCartesianGrid}\textit{, }\textbf{%
936 usingSphericalPolarGrid}\textit{, }and \textit{\ }\textbf{%
937 usingCurvilinearGrid}\textit{. }In the case of spherical and curvilinear
938 grids, the southern boundary is defined through the variable \textbf{phiMin}%
939 \textit{\ }which corresponds to the latitude of the southern most cell face
940 (in degrees). The resolution along the x and y directions is controlled by
941 the 1D arrays \textbf{delx}\textit{\ }and \textbf{dely}\textit{\ }(in meters
942 in the case of a cartesian grid, in degrees otherwise). The vertical grid
943 spacing is set through the 1D array \textbf{delz }for the ocean (in meters)
944 or \textbf{delp}\textit{\ }for the atmosphere (in Pa). The variable \textbf{%
945 Ro\_SeaLevel} represents the standard position of Sea-Level in ''R''
946 coordinate. This is typically set to 0m for the ocean (default value) and 10$%
947 ^{5}$Pa for the atmosphere. For the atmosphere, also set the logical
948 variable \textbf{groundAtK1} to '.\texttt{TRUE}.'. which put the first level
949 (k=1) at the lower boundary (ground).
950
951 For the cartesian grid case, the Coriolis parameter $f$ is set through the
952 variables \textbf{f0}\textit{\ }and \textbf{beta}\textit{\ }which correspond
953 to the reference Coriolis parameter (in s$^{-1}$) and $\frac{\partial f}{%
954 \partial y}$(in m$^{-1}$s$^{-1}$) respectively. If \textbf{beta }\textit{\ }%
955 is set to a nonzero value, \textbf{f0}\textit{\ }is the value of $f$ at the
956 southern edge of the domain.
957
958 \begin{itemize}
959 \item topography - full and partial cells
960 \end{itemize}
961
962 The domain bathymetry is read from a file that contains a 2D (x,y) map of
963 depths (in m) for the ocean or pressures (in Pa) for the atmosphere. The
964 file name is represented by the variable \textbf{bathyFile}\textit{. }The
965 file is assumed to contain binary numbers giving the depth (pressure) of the
966 model at each grid cell, ordered with the x coordinate varying fastest. The
967 points are ordered from low coordinate to high coordinate for both axes. The
968 model code applies without modification to enclosed, periodic, and double
969 periodic domains. Periodicity is assumed by default and is suppressed by
970 setting the depths to 0m for the cells at the limits of the computational
971 domain (note: not sure this is the case for the atmosphere). The precision
972 with which to read the binary data is controlled by the integer variable
973 \textbf{readBinaryPrec }which can take the value \texttt{32} (single
974 precision) or \texttt{64} (double precision). See the matlab program \textit{%
975 gendata.m }in the \textit{input }directories under \textit{verification }to
976 see how the bathymetry files are generated for the case study experiments.
977
978 To use the partial cell capability, the variable \textbf{hFacMin}\textit{\ }%
979 needs to be set to a value between 0 and 1 (it is set to 1 by default)
980 corresponding to the minimum fractional size of the cell. For example if the
981 bottom cell is 500m thick and \textbf{hFacMin}\textit{\ }is set to 0.1, the
982 actual thickness of the cell (i.e. used in the code) can cover a range of
983 discrete values 50m apart from 50m to 500m depending on the value of the
984 bottom depth (in \textbf{bathyFile}) at this point.
985
986 Note that the bottom depths (or pressures) need not coincide with the models
987 levels as deduced from \textbf{delz}\textit{\ }or\textit{\ }\textbf{delp}%
988 \textit{. }The model will interpolate the numbers in \textbf{bathyFile}%
989 \textit{\ }so that they match the levels obtained from \textbf{delz}\textit{%
990 \ }or\textit{\ }\textbf{delp}\textit{\ }and \textbf{hFacMin}\textit{. }
991
992 (Note: the atmospheric case is a bit more complicated than what is written
993 here I think. To come soon...)
994
995 \begin{itemize}
996 \item time-discretization
997 \end{itemize}
998
999 The time steps are set through the real variables \textbf{deltaTMom}
1000 and \textbf{deltaTtracer} (in s) which represent the time step for the
1001 momentum and tracer equations, respectively. For synchronous
1002 integrations, simply set the two variables to the same value (or you
1003 can prescribe one time step only through the variable
1004 \textbf{deltaT}). The Adams-Bashforth stabilizing parameter is set
1005 through the variable \textbf{abEps} (dimensionless). The stagger
1006 baroclinic time stepping can be activated by setting the logical
1007 variable \textbf{staggerTimeStep} to '.\texttt{TRUE}.'.
1008
1009 \subsection{Equation of state}
1010
1011 First, because the model equations are written in terms of
1012 perturbations, a reference thermodynamic state needs to be specified.
1013 This is done through the 1D arrays \textbf{tRef} and \textbf{sRef}.
1014 \textbf{tRef} specifies the reference potential temperature profile
1015 (in $^{o}$C for the ocean and $^{o}$K for the atmosphere) starting
1016 from the level k=1. Similarly, \textbf{sRef} specifies the reference
1017 salinity profile (in ppt) for the ocean or the reference specific
1018 humidity profile (in g/kg) for the atmosphere.
1019
1020 The form of the equation of state is controlled by the character
1021 variables \textbf{buoyancyRelation} and \textbf{eosType}.
1022 \textbf{buoyancyRelation} is set to '\texttt{OCEANIC}' by default and
1023 needs to be set to '\texttt{ATMOSPHERIC}' for atmosphere simulations.
1024 In this case, \textbf{eosType} must be set to '\texttt{IDEALGAS}'.
1025 For the ocean, two forms of the equation of state are available:
1026 linear (set \textbf{eosType} to '\texttt{LINEAR}') and a polynomial
1027 approximation to the full nonlinear equation ( set
1028 \textbf{eosType}\textit{\ }to '\texttt{POLYNOMIAL}'). In the linear
1029 case, you need to specify the thermal and haline expansion
1030 coefficients represented by the variables \textbf{tAlpha}\textit{\
1031 }(in K$^{-1}$) and \textbf{sBeta} (in ppt$^{-1}$). For the nonlinear
1032 case, you need to generate a file of polynomial coefficients called
1033 \textit{POLY3.COEFFS}. To do this, use the program
1034 \textit{utils/knudsen2/knudsen2.f} under the model tree (a Makefile is
1035 available in the same directory and you will need to edit the number
1036 and the values of the vertical levels in \textit{knudsen2.f} so that
1037 they match those of your configuration).
1038
1039 There there are also higher polynomials for the equation of state:
1040 \begin{description}
1041 \item['\texttt{UNESCO}':] The UNESCO equation of state formula of
1042 Fofonoff and Millard \cite{fofonoff83}. This equation of state
1043 assumes in-situ temperature, which is not a model variable; \emph{its use
1044 is therefore discouraged, and it is only listed for completeness}.
1045 \item['\texttt{JMD95Z}':] A modified UNESCO formula by Jackett and
1046 McDougall \cite{jackett95}, which uses the model variable potential
1047 temperature as input. The '\texttt{Z}' indicates that this equation
1048 of state uses a horizontally and temporally constant pressure
1049 $p_{0}=-g\rho_{0}z$.
1050 \item['\texttt{JMD95P}':] A modified UNESCO formula by Jackett and
1051 McDougall \cite{jackett95}, which uses the model variable potential
1052 temperature as input. The '\texttt{P}' indicates that this equation
1053 of state uses the actual hydrostatic pressure of the last time
1054 step. Lagging the pressure in this way requires an additional pickup
1055 file for restarts.
1056 \item['\texttt{MDJWF}':] The new, more accurate and less expensive
1057 equation of state by McDougall et~al. \cite{mcdougall03}. It also
1058 requires lagging the pressure and therefore an additional pickup
1059 file for restarts.
1060 \end{description}
1061 For none of these options an reference profile of temperature or
1062 salinity is required.
1063
1064 \subsection{Momentum equations}
1065
1066 In this section, we only focus for now on the parameters that you are likely
1067 to change, i.e. the ones relative to forcing and dissipation for example.
1068 The details relevant to the vector-invariant form of the equations and the
1069 various advection schemes are not covered for the moment. We assume that you
1070 use the standard form of the momentum equations (i.e. the flux-form) with
1071 the default advection scheme. Also, there are a few logical variables that
1072 allow you to turn on/off various terms in the momentum equation. These
1073 variables are called \textbf{momViscosity, momAdvection, momForcing,
1074 useCoriolis, momPressureForcing, momStepping}\textit{, }and \textit{\ }%
1075 \textbf{metricTerms }and are assumed to be set to '.\texttt{TRUE}.' here.
1076 Look at the file \textit{model/inc/PARAMS.h }for a precise definition of
1077 these variables.
1078
1079 \begin{itemize}
1080 \item initialization
1081 \end{itemize}
1082
1083 The velocity components are initialized to 0 unless the simulation is
1084 starting from a pickup file (see section on simulation control parameters).
1085
1086 \begin{itemize}
1087 \item forcing
1088 \end{itemize}
1089
1090 This section only applies to the ocean. You need to generate wind-stress
1091 data into two files \textbf{zonalWindFile}\textit{\ }and \textbf{%
1092 meridWindFile }corresponding to the zonal and meridional components of the
1093 wind stress, respectively (if you want the stress to be along the direction
1094 of only one of the model horizontal axes, you only need to generate one
1095 file). The format of the files is similar to the bathymetry file. The zonal
1096 (meridional) stress data are assumed to be in Pa and located at U-points
1097 (V-points). As for the bathymetry, the precision with which to read the
1098 binary data is controlled by the variable \textbf{readBinaryPrec}.\textbf{\ }
1099 See the matlab program \textit{gendata.m }in the \textit{input }directories
1100 under \textit{verification }to see how simple analytical wind forcing data
1101 are generated for the case study experiments.
1102
1103 There is also the possibility of prescribing time-dependent periodic
1104 forcing. To do this, concatenate the successive time records into a single
1105 file (for each stress component) ordered in a (x, y, t) fashion and set the
1106 following variables: \textbf{periodicExternalForcing }to '.\texttt{TRUE}.',
1107 \textbf{externForcingPeriod }to the period (in s) of which the forcing
1108 varies (typically 1 month), and \textbf{externForcingCycle }to the repeat
1109 time (in s) of the forcing (typically 1 year -- note: \textbf{%
1110 externForcingCycle }must be a multiple of \textbf{externForcingPeriod}).
1111 With these variables set up, the model will interpolate the forcing linearly
1112 at each iteration.
1113
1114 \begin{itemize}
1115 \item dissipation
1116 \end{itemize}
1117
1118 The lateral eddy viscosity coefficient is specified through the variable
1119 \textbf{viscAh}\textit{\ }(in m$^{2}$s$^{-1}$). The vertical eddy viscosity
1120 coefficient is specified through the variable \textbf{viscAz }(in m$^{2}$s$%
1121 ^{-1}$) for the ocean and \textbf{viscAp}\textit{\ }(in Pa$^{2}$s$^{-1}$)
1122 for the atmosphere. The vertical diffusive fluxes can be computed implicitly
1123 by setting the logical variable \textbf{implicitViscosity }to '.\texttt{TRUE}%
1124 .'. In addition, biharmonic mixing can be added as well through the variable
1125 \textbf{viscA4}\textit{\ }(in m$^{4}$s$^{-1}$). On a spherical polar grid,
1126 you might also need to set the variable \textbf{cosPower} which is set to 0
1127 by default and which represents the power of cosine of latitude to multiply
1128 viscosity. Slip or no-slip conditions at lateral and bottom boundaries are
1129 specified through the logical variables \textbf{no\_slip\_sides}\textit{\ }%
1130 and \textbf{no\_slip\_bottom}. If set to '\texttt{.FALSE.}', free-slip
1131 boundary conditions are applied. If no-slip boundary conditions are applied
1132 at the bottom, a bottom drag can be applied as well. Two forms are
1133 available: linear (set the variable \textbf{bottomDragLinear}\textit{\ }in s$%
1134 ^{-1}$) and quadratic (set the variable \textbf{bottomDragQuadratic}\textit{%
1135 \ }in m$^{-1}$).
1136
1137 The Fourier and Shapiro filters are described elsewhere.
1138
1139 \begin{itemize}
1140 \item C-D scheme
1141 \end{itemize}
1142
1143 If you run at a sufficiently coarse resolution, you will need the C-D scheme
1144 for the computation of the Coriolis terms. The variable\textbf{\ tauCD},
1145 which represents the C-D scheme coupling timescale (in s) needs to be set.
1146
1147 \begin{itemize}
1148 \item calculation of pressure/geopotential
1149 \end{itemize}
1150
1151 First, to run a non-hydrostatic ocean simulation, set the logical variable
1152 \textbf{nonHydrostatic} to '.\texttt{TRUE}.'. The pressure field is then
1153 inverted through a 3D elliptic equation. (Note: this capability is not
1154 available for the atmosphere yet.) By default, a hydrostatic simulation is
1155 assumed and a 2D elliptic equation is used to invert the pressure field. The
1156 parameters controlling the behaviour of the elliptic solvers are the
1157 variables \textbf{cg2dMaxIters}\textit{\ }and \textbf{cg2dTargetResidual }%
1158 for the 2D case and \textbf{cg3dMaxIters}\textit{\ }and \textbf{%
1159 cg3dTargetResidual }for the 3D case. You probably won't need to alter the
1160 default values (are we sure of this?).
1161
1162 For the calculation of the surface pressure (for the ocean) or surface
1163 geopotential (for the atmosphere) you need to set the logical variables
1164 \textbf{rigidLid} and \textbf{implicitFreeSurface}\textit{\ }(set one to '.%
1165 \texttt{TRUE}.' and the other to '.\texttt{FALSE}.' depending on how you
1166 want to deal with the ocean upper or atmosphere lower boundary).
1167
1168 \subsection{Tracer equations}
1169
1170 This section covers the tracer equations i.e. the potential temperature
1171 equation and the salinity (for the ocean) or specific humidity (for the
1172 atmosphere) equation. As for the momentum equations, we only describe for
1173 now the parameters that you are likely to change. The logical variables
1174 \textbf{tempDiffusion}\textit{, }\textbf{tempAdvection}\textit{, }\textbf{%
1175 tempForcing}\textit{,} and \textbf{tempStepping} allow you to turn on/off
1176 terms in the temperature equation (same thing for salinity or specific
1177 humidity with variables \textbf{saltDiffusion}\textit{, }\textbf{%
1178 saltAdvection}\textit{\ }etc). These variables are all assumed here to be
1179 set to '.\texttt{TRUE}.'. Look at file \textit{model/inc/PARAMS.h }for a
1180 precise definition.
1181
1182 \begin{itemize}
1183 \item initialization
1184 \end{itemize}
1185
1186 The initial tracer data can be contained in the binary files \textbf{%
1187 hydrogThetaFile }and \textbf{hydrogSaltFile}. These files should contain 3D
1188 data ordered in an (x, y, r) fashion with k=1 as the first vertical level.
1189 If no file names are provided, the tracers are then initialized with the
1190 values of \textbf{tRef }and \textbf{sRef }mentioned above (in the equation
1191 of state section). In this case, the initial tracer data are uniform in x
1192 and y for each depth level.
1193
1194 \begin{itemize}
1195 \item forcing
1196 \end{itemize}
1197
1198 This part is more relevant for the ocean, the procedure for the atmosphere
1199 not being completely stabilized at the moment.
1200
1201 A combination of fluxes data and relaxation terms can be used for driving
1202 the tracer equations. \ For potential temperature, heat flux data (in W/m$%
1203 ^{2}$) can be stored in the 2D binary file \textbf{surfQfile}\textit{. }%
1204 Alternatively or in addition, the forcing can be specified through a
1205 relaxation term. The SST data to which the model surface temperatures are
1206 restored to are supposed to be stored in the 2D binary file \textbf{%
1207 thetaClimFile}\textit{. }The corresponding relaxation time scale coefficient
1208 is set through the variable \textbf{tauThetaClimRelax}\textit{\ }(in s). The
1209 same procedure applies for salinity with the variable names \textbf{EmPmRfile%
1210 }\textit{, }\textbf{saltClimFile}\textit{, }and \textbf{tauSaltClimRelax}%
1211 \textit{\ }for freshwater flux (in m/s) and surface salinity (in ppt) data
1212 files and relaxation time scale coefficient (in s), respectively. Also for
1213 salinity, if the CPP key \textbf{USE\_NATURAL\_BCS} is turned on, natural
1214 boundary conditions are applied i.e. when computing the surface salinity
1215 tendency, the freshwater flux is multiplied by the model surface salinity
1216 instead of a constant salinity value.
1217
1218 As for the other input files, the precision with which to read the data is
1219 controlled by the variable \textbf{readBinaryPrec}. Time-dependent, periodic
1220 forcing can be applied as well following the same procedure used for the
1221 wind forcing data (see above).
1222
1223 \begin{itemize}
1224 \item dissipation
1225 \end{itemize}
1226
1227 Lateral eddy diffusivities for temperature and salinity/specific humidity
1228 are specified through the variables \textbf{diffKhT }and \textbf{diffKhS }%
1229 (in m$^{2}$/s). Vertical eddy diffusivities are specified through the
1230 variables \textbf{diffKzT }and \textbf{diffKzS }(in m$^{2}$/s) for the ocean
1231 and \textbf{diffKpT }and \textbf{diffKpS }(in Pa$^{2}$/s) for the
1232 atmosphere. The vertical diffusive fluxes can be computed implicitly by
1233 setting the logical variable \textbf{implicitDiffusion }to '.\texttt{TRUE}%
1234 .'. In addition, biharmonic diffusivities can be specified as well through
1235 the coefficients \textbf{diffK4T }and \textbf{diffK4S }(in m$^{4}$/s). Note
1236 that the cosine power scaling (specified through \textbf{cosPower }- see the
1237 momentum equations section) is applied to the tracer diffusivities
1238 (Laplacian and biharmonic) as well. The Gent and McWilliams parameterization
1239 for oceanic tracers is described in the package section. Finally, note that
1240 tracers can be also subject to Fourier and Shapiro filtering (see the
1241 corresponding section on these filters).
1242
1243 \begin{itemize}
1244 \item ocean convection
1245 \end{itemize}
1246
1247 Two options are available to parameterize ocean convection: one is to use
1248 the convective adjustment scheme. In this case, you need to set the variable
1249 \textbf{cadjFreq}, which represents the frequency (in s) with which the
1250 adjustment algorithm is called, to a non-zero value (if set to a negative
1251 value by the user, the model will set it to the tracer time step). The other
1252 option is to parameterize convection with implicit vertical diffusion. To do
1253 this, set the logical variable \textbf{implicitDiffusion }to '.\texttt{TRUE}%
1254 .' and the real variable \textbf{ivdc\_kappa }to a value (in m$^{2}$/s) you
1255 wish the tracer vertical diffusivities to have when mixing tracers
1256 vertically due to static instabilities. Note that \textbf{cadjFreq }and
1257 \textbf{ivdc\_kappa }can not both have non-zero value.
1258
1259 \subsection{Simulation controls}
1260
1261 The model ''clock'' is defined by the variable \textbf{deltaTClock }(in s)
1262 which determines the IO frequencies and is used in tagging output.
1263 Typically, you will set it to the tracer time step for accelerated runs
1264 (otherwise it is simply set to the default time step \textbf{deltaT}).
1265 Frequency of checkpointing and dumping of the model state are referenced to
1266 this clock (see below).
1267
1268 \begin{itemize}
1269 \item run duration
1270 \end{itemize}
1271
1272 The beginning of a simulation is set by specifying a start time (in s)
1273 through the real variable \textbf{startTime }or by specifying an initial
1274 iteration number through the integer variable \textbf{nIter0}. If these
1275 variables are set to nonzero values, the model will look for a ''pickup''
1276 file \textit{pickup.0000nIter0 }to restart the integration\textit{. }The end
1277 of a simulation is set through the real variable \textbf{endTime }(in s).
1278 Alternatively, you can specify instead the number of time steps to execute
1279 through the integer variable \textbf{nTimeSteps}.
1280
1281 \begin{itemize}
1282 \item frequency of output
1283 \end{itemize}
1284
1285 Real variables defining frequencies (in s) with which output files are
1286 written on disk need to be set up. \textbf{dumpFreq }controls the frequency
1287 with which the instantaneous state of the model is saved. \textbf{chkPtFreq }%
1288 and \textbf{pchkPtFreq }control the output frequency of rolling and
1289 permanent checkpoint files, respectively. See section 1.5.1 Output files for the
1290 definition of model state and checkpoint files. In addition, time-averaged
1291 fields can be written out by setting the variable \textbf{taveFreq} (in s).
1292 The precision with which to write the binary data is controlled by the
1293 integer variable w\textbf{riteBinaryPrec }(set it to \texttt{32} or \texttt{%
1294 64}).
1295
1296 %%% Local Variables:
1297 %%% mode: latex
1298 %%% TeX-master: t
1299 %%% End:

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