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1 edhill 1.22 % $Header: /u/gcmpack/manual/part3/getting_started.tex,v 1.21 2004/03/11 16:11:56 edhill Exp $
2 adcroft 1.2 % $Name: $
3 adcroft 1.1
4 adcroft 1.4 %\section{Getting started}
5 adcroft 1.1
6 adcroft 1.4 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 edhill 1.15 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 adcroft 1.4 \begin{verbatim}
24 edhill 1.15 http://mitgcm.org/pelican
25 adcroft 1.4 \end{verbatim}
26 edhill 1.15 \begin{rawhtml} </A> \end{rawhtml}
27 adcroft 1.4 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 edhill 1.15 documentation, to data-sources, and other related sites.
31 adcroft 1.4
32 edhill 1.15 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 edhill 1.16 \begin{rawhtml} <A href=http://mitgcm.org/mailman/htdig/ target="idontexist"> \end{rawhtml}
43 adcroft 1.1 \begin{verbatim}
44 edhill 1.15 http://mitgcm.org/htdig/
45 adcroft 1.1 \end{verbatim}
46 edhill 1.15 \begin{rawhtml} </A> \end{rawhtml}
47     %%% http://www.google.com/search?q=hydrostatic+site%3Amitgcm.org
48    
49    
50 adcroft 1.4
51     \section{Obtaining the code}
52     \label{sect:obtainingCode}
53 adcroft 1.1
54 cnh 1.7 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 edhill 1.14 \begin{rawhtml} <A href=mailto:MITgcm-support@mitgcm.org> \end{rawhtml}
57     MITgcm-support@mitgcm.org
58 cnh 1.7 \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 cnh 1.9 \item Using CVS software. CVS is a freely available source code management
64 cnh 1.7 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 edhill 1.19 \subsubsection{Checkout from CVS}
83     \label{sect:cvs_checkout}
84    
85 adcroft 1.1 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 edhill 1.15 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 adcroft 1.1 \begin{verbatim}
97 edhill 1.15 % export CVSROOT=':pserver:cvsanon@mitgcm.org:/u/gcmpack'
98 adcroft 1.6 \end{verbatim}
99 edhill 1.20 in your \texttt{.profile} or \texttt{.bashrc} file.
100 adcroft 1.6
101 edhill 1.15
102     To get MITgcm through CVS, first register with the MITgcm CVS server
103     using command:
104 adcroft 1.6 \begin{verbatim}
105 adcroft 1.1 % cvs login ( CVS password: cvsanon )
106     \end{verbatim}
107 edhill 1.15 You only need to do a ``cvs login'' once.
108 adcroft 1.1
109 edhill 1.15 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 adcroft 1.1 \begin{verbatim}
115 edhill 1.16 % cvs co -P -r checkpoint52i_post MITgcm
116 adcroft 1.1 \end{verbatim}
117 edhill 1.15 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 edhill 1.17 \begin{rawhtml} <A href=''http://mitgcm.org/download'' target="idontexist"> \end{rawhtml}
122 edhill 1.15 \begin{verbatim}
123 edhill 1.17 http://mitgcm.org/source_code.html
124 edhill 1.15 \end{verbatim}
125     \begin{rawhtml} </A> \end{rawhtml}
126 adcroft 1.1
127 edhill 1.19 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 edhill 1.15
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 edhill 1.17 \begin{rawhtml} <A href=''http://mitgcm.org/usingcvstoget.html'' target="idontexist"> \end{rawhtml}
159 cnh 1.7 here
160     \begin{rawhtml} </A> \end{rawhtml}
161     .
162 edhill 1.19 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 cnh 1.7
171 adcroft 1.1
172 edhill 1.19 \subsubsection{Conventional download method}
173 adcroft 1.4 \label{sect:conventionalDownload}
174 adcroft 1.1
175 adcroft 1.4 If you do not have CVS on your system, you can download the model as a
176 edhill 1.15 tar file from the web site at:
177 cnh 1.7 \begin{rawhtml} <A href=http://mitgcm.org/download target="idontexist"> \end{rawhtml}
178 adcroft 1.1 \begin{verbatim}
179     http://mitgcm.org/download/
180     \end{verbatim}
181 cnh 1.7 \begin{rawhtml} </A> \end{rawhtml}
182 adcroft 1.4 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 edhill 1.15 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 edhill 1.17 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 adcroft 1.1
192 edhill 1.19 \subsubsection{Upgrading from an earlier version}
193 adcroft 1.12
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 edhill 1.15 and then issue the cvs update command such as:
201 adcroft 1.12 \begin{verbatim}
202 edhill 1.16 % cvs -q update -r checkpoint52i_post -d -P
203 adcroft 1.12 \end{verbatim}
204 edhill 1.16 This will update the ``tag'' to ``checkpoint52i\_post'', add any new
205 adcroft 1.12 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 edhill 1.15 indicated in the code by the delimites ``$<<<<<<<$'', ``======='' and
217     ``$>>>>>>>$''. For example,
218 edhill 1.17 {\small
219 adcroft 1.12 \begin{verbatim}
220     <<<<<<< ini_parms.F
221     & bottomDragLinear,myOwnBottomDragCoefficient,
222     =======
223     & bottomDragLinear,bottomDragQuadratic,
224     >>>>>>> 1.18
225     \end{verbatim}
226 edhill 1.17 }
227 adcroft 1.12 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 edhill 1.17 {\small
232 adcroft 1.12 \begin{verbatim}
233     & bottomDragLinear,bottomDragQuadratic,myOwnBottomDragCoefficient,
234     \end{verbatim}
235 edhill 1.17 }
236 edhill 1.15 and the lines with the delimiters ($<<<<<<$,======,$>>>>>>$) be deleted.
237 adcroft 1.12 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 adcroft 1.4 \section{Model and directory structure}
259 adcroft 1.1
260 adcroft 1.12 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 edhill 1.17 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 adcroft 1.1
277     \begin{itemize}
278    
279 edhill 1.17 \item \textit{bin}: this directory is initially empty. It is the
280     default directory in which to compile the code.
281    
282 adcroft 1.1 \item \textit{diags}: contains the code relative to time-averaged
283 edhill 1.17 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 adcroft 1.1
287     \item \textit{doc}: contains brief documentation notes.
288 edhill 1.17
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 adcroft 1.1 \item \textit{utils}: this directory contains various utilities. The
314 edhill 1.17 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 adcroft 1.1
325     \end{itemize}
326    
327 adcroft 1.4 \section{Example experiments}
328     \label{sect:modelExamples}
329 adcroft 1.1
330 edhill 1.15 %% 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 adcroft 1.1
343 cnh 1.8 \subsection{Full list of model examples}
344 adcroft 1.1
345 cnh 1.8 \begin{enumerate}
346 edhill 1.17
347 adcroft 1.1 \item \textit{exp0} - single layer, ocean double gyre (barotropic with
348 edhill 1.15 free-surface). This experiment is described in detail in section
349     \ref{sect:eg-baro}.
350 adcroft 1.1
351 edhill 1.15 \item \textit{exp1} - Four layer, ocean double gyre. This experiment
352     is described in detail in section \ref{sect:eg-baroc}.
353    
354 adcroft 1.1 \item \textit{exp2} - 4x4 degree global ocean simulation with steady
355 edhill 1.15 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 adcroft 1.1
364 cnh 1.8 \item \textit{front\_relax} - Relaxation of an ocean thermal front (test for
365 adcroft 1.1 Gent/McWilliams scheme). 2D (Y-Z).
366    
367 edhill 1.15 \item \textit{internal wave} - Ocean internal wave forced by open
368     boundary conditions.
369    
370 cnh 1.8 \item \textit{natl\_box} - Eastern subtropical North Atlantic with KPP
371 edhill 1.15 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 adcroft 1.1 \item \textit{hs94.cs-32x32x5} - 3D atmosphere dynamics using Held and
380 edhill 1.15 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 adcroft 1.1 \item \textit{aim.5l\_Equatorial\_Channel} - Intermediate Atmospheric
389 edhill 1.15 physics. 3D Equatorial Channel configuration.
390    
391 cnh 1.8 \item \textit{aim.5l\_LatLon} - Intermediate Atmospheric physics.
392 edhill 1.15 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 cnh 1.8 \item \textit{advect\_cs} Two-dimensional passive advection test on
404 edhill 1.15 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 cnh 1.8
416     \item \textit{flt\_example} Example of using float package.
417 edhill 1.15
418     \item \textit{global\_ocean.90x40x15} Global circulation with GM, flux
419     boundary conditions and poles.
420 cnh 1.8
421 mlosch 1.13 \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 edhill 1.15
425     \item \textit{solid-body.cs-32x32x1} Solid body rotation test for cube
426     sphere grid.
427 cnh 1.8
428     \end{enumerate}
429 adcroft 1.1
430 adcroft 1.4 \subsection{Directory structure of model examples}
431 adcroft 1.1
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 edhill 1.16 minimum, this directory includes the following files:
437 adcroft 1.1
438 edhill 1.16 \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 edhill 1.15
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 adcroft 1.1
460 edhill 1.16 \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 edhill 1.17
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 edhill 1.16
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 adcroft 1.1 \end{itemize}
483    
484 edhill 1.17 Once you have chosen the example you want to run, you are ready to
485     compile the code.
486 adcroft 1.1
487 adcroft 1.4 \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 edhill 1.16 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 adcroft 1.4
498     As an example, let's assume that you want to build and run experiment
499 edhill 1.16 \textit{verification/exp2}. The are multiple ways and places to
500     actually do this but here let's build the code in
501 adcroft 1.4 \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 edhill 1.16 % ../../../tools/genmake2 -mods=../code
508 adcroft 1.4 \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 edhill 1.16 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 edhill 1.17 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 edhill 1.16
532     To specify an optfile to {\em genmake2}, the syntax is:
533 adcroft 1.4 \begin{verbatim}
534 edhill 1.16 % ../../../tools/genmake2 -mods=../code -of /path/to/optfile
535 adcroft 1.4 \end{verbatim}
536    
537 edhill 1.16 Once a {\em Makefile} has been generated, we create the dependencies:
538 adcroft 1.4 \begin{verbatim}
539     % make depend
540     \end{verbatim}
541 edhill 1.16 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 adcroft 1.1
547 edhill 1.16 Next compile the code:
548 adcroft 1.4 \begin{verbatim}
549     % make
550     \end{verbatim}
551     The {\tt make} command creates an executable called \textit{mitgcmuv}.
552 edhill 1.16 Additional make ``targets'' are defined within the makefile to aid in
553     the production of adjoint and other versions of MITgcm.
554 adcroft 1.4
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 edhill 1.16 genmake2} in your path or you know the absolute path to {\tt
572     genmake2}.
573 adcroft 1.4
574 edhill 1.16 The following sections outline some possible methods of organizing
575     your source and data.
576 adcroft 1.4
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 edhill 1.16 % ../../../tools/genmake2
583 adcroft 1.4 % 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 cnh 1.9 or if you will be making multiple runs with the same executable:
594 adcroft 1.4 \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 cnh 1.9 useful to keep {\em input} pristine and build in a new directory
606 adcroft 1.4 within {\em verification/exp2/}:
607     \begin{verbatim}
608     % cd verification/exp2
609     % mkdir build
610     % cd build
611 edhill 1.16 % ../../../tools/genmake2 -mods=../code
612 adcroft 1.4 % 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 edhill 1.16 \subsubsection{Building on a scratch disk}
634 adcroft 1.4
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 edhill 1.16 % ~/MITgcm/tools/genmake2 -rootdir=~/MITgcm \
642     -mods=~/MITgcm/verification/exp2/code
643 adcroft 1.4 % 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 edhill 1.16 % ~/MITgcm/tools/genmake2 -rootdir=~/MITgcm \
659     -mods=~/MITgcm/verification/exp2/code
660 adcroft 1.4 % 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 edhill 1.16 \subsection{Using \textit{genmake2}}
671 adcroft 1.4 \label{sect:genmake}
672 adcroft 1.1
673 edhill 1.16 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 adcroft 1.1
753 edhill 1.16 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 edhill 1.17 \item[\texttt{--optfile=/PATH/FILENAME}] specifies the optfile that
764     should be used for a particular build.
765 edhill 1.16
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 edhill 1.22 \item[\texttt{--pdefault='PKG1 PKG2 PKG3 ...'}] specifies the default
776     set of packages to be used. The normal order of precedence for
777     packages is as follows:
778     \begin{enumerate}
779     \item If available, the command line (\texttt{--pdefault}) settings
780     over-rule any others.
781    
782     \item Next, \texttt{genmake2} will look for a file named
783     ``\texttt{packages.conf}'' in the local directory or in any of the
784     directories specified with the \texttt{--mods} option.
785    
786     \item Finally, if neither of the above are available,
787     \texttt{genmake2} will use the \texttt{/pkg/pkg\_default} file.
788     \end{enumerate}
789    
790 edhill 1.17 \item[\texttt{--pdepend=/PATH/FILENAME}] specifies the dependency file
791     used for packages.
792 edhill 1.16
793     If not specified, the default dependency file {\em pkg/pkg\_depend}
794     is used. The syntax for this file is parsed on a line-by-line basis
795     where each line containes either a comment ("\#") or a simple
796     "PKGNAME1 (+|-)PKGNAME2" pairwise rule where the "+" or "-" symbol
797     specifies a "must be used with" or a "must not be used with"
798     relationship, respectively. If no rule is specified, then it is
799     assumed that the two packages are compatible and will function
800     either with or without each other.
801    
802 edhill 1.17 \item[\texttt{--adof=/path/to/file}] specifies the "adjoint" or
803     automatic differentiation options file to be used. The file is
804     analogous to the ``optfile'' defined above but it specifies
805     information for the AD build process.
806 edhill 1.16
807     The default file is located in {\em
808     tools/adjoint\_options/adjoint\_default} and it defines the "TAF"
809     and "TAMC" compilers. An alternate version is also available at
810     {\em tools/adjoint\_options/adjoint\_staf} that selects the newer
811     "STAF" compiler. As with any compilers, it is helpful to have their
812     directories listed in your {\tt \$PATH} environment variable.
813    
814 edhill 1.17 \item[\texttt{--mods='DIR1 DIR2 DIR3 ...'}] specifies a list of
815     directories containing ``modifications''. These directories contain
816     files with names that may (or may not) exist in the main MITgcm
817     source tree but will be overridden by any identically-named sources
818     within the ``MODS'' directories.
819 edhill 1.16
820     The order of precedence for this "name-hiding" is as follows:
821     \begin{itemize}
822     \item ``MODS'' directories (in the order given)
823     \item Packages either explicitly specified or provided by default
824     (in the order given)
825     \item Packages included due to package dependencies (in the order
826     that that package dependencies are parsed)
827     \item The "standard dirs" (which may have been specified by the
828     ``-standarddirs'' option)
829     \end{itemize}
830    
831 edhill 1.17 \item[\texttt{--make=/path/to/gmake}] Due to the poor handling of
832     soft-links and other bugs common with the \texttt{make} versions
833     provided by commercial Unix vendors, GNU \texttt{make} (sometimes
834     called \texttt{gmake}) should be preferred. This option provides a
835     means for specifying the make executable to be used.
836 edhill 1.21
837     \item[\texttt{--bash=/path/to/sh}] On some (usually older UNIX)
838     machines, the ``bash'' shell is unavailable. To run on these
839     systems, \texttt{genmake2} can be invoked using an ``sh'' (that is,
840     a Bourne, POSIX, or compatible) shell. The syntax in these
841     circumstances is:
842     \begin{center}
843     \texttt{/bin/sh genmake2 -bash=/bin/sh [...options...]}
844     \end{center}
845     where \texttt{/bin/sh} can be replaced with the full path and name
846     of the desired shell.
847 adcroft 1.1
848 edhill 1.16 \end{description}
849 adcroft 1.1
850    
851    
852 adcroft 1.4 \section{Running the model}
853     \label{sect:runModel}
854    
855     If compilation finished succesfuully (section \ref{sect:buildModel})
856     then an executable called {\em mitgcmuv} will now exist in the local
857     directory.
858 adcroft 1.1
859 adcroft 1.4 To run the model as a single process (ie. not in parallel) simply
860     type:
861 adcroft 1.1 \begin{verbatim}
862 adcroft 1.4 % ./mitgcmuv
863 adcroft 1.1 \end{verbatim}
864 adcroft 1.4 The ``./'' is a safe-guard to make sure you use the local executable
865     in case you have others that exist in your path (surely odd if you
866     do!). The above command will spew out many lines of text output to
867     your screen. This output contains details such as parameter values as
868     well as diagnostics such as mean Kinetic energy, largest CFL number,
869     etc. It is worth keeping this text output with the binary output so we
870     normally re-direct the {\em stdout} stream as follows:
871 adcroft 1.1 \begin{verbatim}
872 adcroft 1.4 % ./mitgcmuv > output.txt
873 adcroft 1.1 \end{verbatim}
874    
875 edhill 1.17 For the example experiments in {\em verification}, an example of the
876 adcroft 1.4 output is kept in {\em results/output.txt} for comparison. You can compare
877     your {\em output.txt} with this one to check that the set-up works.
878 adcroft 1.1
879    
880    
881 adcroft 1.4 \subsection{Output files}
882 adcroft 1.1
883     The model produces various output files. At a minimum, the instantaneous
884     ``state'' of the model is written out, which is made of the following files:
885    
886     \begin{itemize}
887     \item \textit{U.00000nIter} - zonal component of velocity field (m/s and $>
888     0 $ eastward).
889    
890     \item \textit{V.00000nIter} - meridional component of velocity field (m/s
891     and $> 0$ northward).
892    
893     \item \textit{W.00000nIter} - vertical component of velocity field (ocean:
894     m/s and $> 0$ upward, atmosphere: Pa/s and $> 0$ towards increasing pressure
895     i.e. downward).
896    
897     \item \textit{T.00000nIter} - potential temperature (ocean: $^{0}$C,
898     atmosphere: $^{0}$K).
899    
900     \item \textit{S.00000nIter} - ocean: salinity (psu), atmosphere: water vapor
901     (g/kg).
902    
903     \item \textit{Eta.00000nIter} - ocean: surface elevation (m), atmosphere:
904     surface pressure anomaly (Pa).
905     \end{itemize}
906    
907     The chain \textit{00000nIter} consists of ten figures that specify the
908     iteration number at which the output is written out. For example, \textit{%
909     U.0000000300} is the zonal velocity at iteration 300.
910    
911     In addition, a ``pickup'' or ``checkpoint'' file called:
912    
913     \begin{itemize}
914     \item \textit{pickup.00000nIter}
915     \end{itemize}
916    
917     is written out. This file represents the state of the model in a condensed
918     form and is used for restarting the integration. If the C-D scheme is used,
919     there is an additional ``pickup'' file:
920    
921     \begin{itemize}
922     \item \textit{pickup\_cd.00000nIter}
923     \end{itemize}
924    
925     containing the D-grid velocity data and that has to be written out as well
926     in order to restart the integration. Rolling checkpoint files are the same
927     as the pickup files but are named differently. Their name contain the chain
928     \textit{ckptA} or \textit{ckptB} instead of \textit{00000nIter}. They can be
929     used to restart the model but are overwritten every other time they are
930     output to save disk space during long integrations.
931    
932 adcroft 1.4 \subsection{Looking at the output}
933 adcroft 1.1
934     All the model data are written according to a ``meta/data'' file format.
935     Each variable is associated with two files with suffix names \textit{.data}
936     and \textit{.meta}. The \textit{.data} file contains the data written in
937     binary form (big\_endian by default). The \textit{.meta} file is a
938     ``header'' file that contains information about the size and the structure
939     of the \textit{.data} file. This way of organizing the output is
940     particularly useful when running multi-processors calculations. The base
941     version of the model includes a few matlab utilities to read output files
942     written in this format. The matlab scripts are located in the directory
943     \textit{utils/matlab} under the root tree. The script \textit{rdmds.m} reads
944     the data. Look at the comments inside the script to see how to use it.
945    
946 adcroft 1.4 Some examples of reading and visualizing some output in {\em Matlab}:
947     \begin{verbatim}
948     % matlab
949     >> H=rdmds('Depth');
950     >> contourf(H');colorbar;
951     >> title('Depth of fluid as used by model');
952    
953     >> eta=rdmds('Eta',10);
954     >> imagesc(eta');axis ij;colorbar;
955     >> title('Surface height at iter=10');
956    
957     >> eta=rdmds('Eta',[0:10:100]);
958     >> for n=1:11; imagesc(eta(:,:,n)');axis ij;colorbar;pause(.5);end
959     \end{verbatim}
960 adcroft 1.1
961     \section{Doing it yourself: customizing the code}
962    
963     When you are ready to run the model in the configuration you want, the
964 edhill 1.17 easiest thing is to use and adapt the setup of the case studies
965     experiment (described previously) that is the closest to your
966     configuration. Then, the amount of setup will be minimized. In this
967     section, we focus on the setup relative to the ``numerical model''
968     part of the code (the setup relative to the ``execution environment''
969     part is covered in the parallel implementation section) and on the
970     variables and parameters that you are likely to change.
971 adcroft 1.1
972 adcroft 1.5 \subsection{Configuration and setup}
973 adcroft 1.4
974 edhill 1.17 The CPP keys relative to the ``numerical model'' part of the code are
975     all defined and set in the file \textit{CPP\_OPTIONS.h }in the
976     directory \textit{ model/inc }or in one of the \textit{code
977     }directories of the case study experiments under
978     \textit{verification.} The model parameters are defined and declared
979     in the file \textit{model/inc/PARAMS.h }and their default values are
980     set in the routine \textit{model/src/set\_defaults.F. }The default
981     values can be modified in the namelist file \textit{data }which needs
982     to be located in the directory where you will run the model. The
983     parameters are initialized in the routine
984     \textit{model/src/ini\_parms.F}. Look at this routine to see in what
985     part of the namelist the parameters are located.
986    
987     In what follows the parameters are grouped into categories related to
988     the computational domain, the equations solved in the model, and the
989     simulation controls.
990 adcroft 1.1
991 adcroft 1.4 \subsection{Computational domain, geometry and time-discretization}
992 adcroft 1.1
993 edhill 1.17 \begin{description}
994     \item[dimensions] \
995    
996 edhill 1.18 The number of points in the x, y, and r directions are represented
997     by the variables \textbf{sNx}, \textbf{sNy} and \textbf{Nr}
998     respectively which are declared and set in the file
999     \textit{model/inc/SIZE.h}. (Again, this assumes a mono-processor
1000     calculation. For multiprocessor calculations see the section on
1001     parallel implementation.)
1002 edhill 1.17
1003     \item[grid] \
1004    
1005     Three different grids are available: cartesian, spherical polar, and
1006 edhill 1.18 curvilinear (which includes the cubed sphere). The grid is set
1007     through the logical variables \textbf{usingCartesianGrid},
1008     \textbf{usingSphericalPolarGrid}, and \textbf{usingCurvilinearGrid}.
1009     In the case of spherical and curvilinear grids, the southern
1010     boundary is defined through the variable \textbf{phiMin} which
1011     corresponds to the latitude of the southern most cell face (in
1012     degrees). The resolution along the x and y directions is controlled
1013     by the 1D arrays \textbf{delx} and \textbf{dely} (in meters in the
1014     case of a cartesian grid, in degrees otherwise). The vertical grid
1015     spacing is set through the 1D array \textbf{delz} for the ocean (in
1016     meters) or \textbf{delp} for the atmosphere (in Pa). The variable
1017     \textbf{Ro\_SeaLevel} represents the standard position of Sea-Level
1018     in ``R'' coordinate. This is typically set to 0m for the ocean
1019     (default value) and 10$^{5}$Pa for the atmosphere. For the
1020     atmosphere, also set the logical variable \textbf{groundAtK1} to
1021     \texttt{'.TRUE.'} which puts the first level (k=1) at the lower
1022 edhill 1.17 boundary (ground).
1023    
1024     For the cartesian grid case, the Coriolis parameter $f$ is set
1025 edhill 1.18 through the variables \textbf{f0} and \textbf{beta} which correspond
1026     to the reference Coriolis parameter (in s$^{-1}$) and
1027     $\frac{\partial f}{ \partial y}$(in m$^{-1}$s$^{-1}$) respectively.
1028     If \textbf{beta } is set to a nonzero value, \textbf{f0} is the
1029     value of $f$ at the southern edge of the domain.
1030 edhill 1.17
1031     \item[topography - full and partial cells] \
1032    
1033     The domain bathymetry is read from a file that contains a 2D (x,y)
1034     map of depths (in m) for the ocean or pressures (in Pa) for the
1035     atmosphere. The file name is represented by the variable
1036 edhill 1.18 \textbf{bathyFile}. The file is assumed to contain binary numbers
1037     giving the depth (pressure) of the model at each grid cell, ordered
1038     with the x coordinate varying fastest. The points are ordered from
1039     low coordinate to high coordinate for both axes. The model code
1040     applies without modification to enclosed, periodic, and double
1041     periodic domains. Periodicity is assumed by default and is
1042 edhill 1.17 suppressed by setting the depths to 0m for the cells at the limits
1043     of the computational domain (note: not sure this is the case for the
1044     atmosphere). The precision with which to read the binary data is
1045 edhill 1.18 controlled by the integer variable \textbf{readBinaryPrec} which can
1046 edhill 1.17 take the value \texttt{32} (single precision) or \texttt{64} (double
1047 edhill 1.18 precision). See the matlab program \textit{gendata.m} in the
1048     \textit{input} directories under \textit{verification} to see how
1049 edhill 1.17 the bathymetry files are generated for the case study experiments.
1050    
1051 edhill 1.18 To use the partial cell capability, the variable \textbf{hFacMin}
1052     needs to be set to a value between 0 and 1 (it is set to 1 by
1053     default) corresponding to the minimum fractional size of the cell.
1054     For example if the bottom cell is 500m thick and \textbf{hFacMin} is
1055     set to 0.1, the actual thickness of the cell (i.e. used in the code)
1056     can cover a range of discrete values 50m apart from 50m to 500m
1057     depending on the value of the bottom depth (in \textbf{bathyFile})
1058     at this point.
1059 edhill 1.17
1060     Note that the bottom depths (or pressures) need not coincide with
1061 edhill 1.18 the models levels as deduced from \textbf{delz} or \textbf{delp}.
1062     The model will interpolate the numbers in \textbf{bathyFile} so that
1063     they match the levels obtained from \textbf{delz} or \textbf{delp}
1064     and \textbf{hFacMin}.
1065 edhill 1.17
1066     (Note: the atmospheric case is a bit more complicated than what is
1067     written here I think. To come soon...)
1068    
1069     \item[time-discretization] \
1070    
1071     The time steps are set through the real variables \textbf{deltaTMom}
1072     and \textbf{deltaTtracer} (in s) which represent the time step for
1073     the momentum and tracer equations, respectively. For synchronous
1074     integrations, simply set the two variables to the same value (or you
1075     can prescribe one time step only through the variable
1076     \textbf{deltaT}). The Adams-Bashforth stabilizing parameter is set
1077     through the variable \textbf{abEps} (dimensionless). The stagger
1078     baroclinic time stepping can be activated by setting the logical
1079 edhill 1.18 variable \textbf{staggerTimeStep} to \texttt{'.TRUE.'}.
1080 adcroft 1.1
1081 edhill 1.17 \end{description}
1082 adcroft 1.1
1083    
1084 adcroft 1.4 \subsection{Equation of state}
1085 adcroft 1.1
1086 mlosch 1.13 First, because the model equations are written in terms of
1087     perturbations, a reference thermodynamic state needs to be specified.
1088     This is done through the 1D arrays \textbf{tRef} and \textbf{sRef}.
1089     \textbf{tRef} specifies the reference potential temperature profile
1090     (in $^{o}$C for the ocean and $^{o}$K for the atmosphere) starting
1091     from the level k=1. Similarly, \textbf{sRef} specifies the reference
1092     salinity profile (in ppt) for the ocean or the reference specific
1093     humidity profile (in g/kg) for the atmosphere.
1094    
1095     The form of the equation of state is controlled by the character
1096     variables \textbf{buoyancyRelation} and \textbf{eosType}.
1097 edhill 1.18 \textbf{buoyancyRelation} is set to \texttt{'OCEANIC'} by default and
1098     needs to be set to \texttt{'ATMOSPHERIC'} for atmosphere simulations.
1099     In this case, \textbf{eosType} must be set to \texttt{'IDEALGAS'}.
1100 mlosch 1.13 For the ocean, two forms of the equation of state are available:
1101 edhill 1.18 linear (set \textbf{eosType} to \texttt{'LINEAR'}) and a polynomial
1102     approximation to the full nonlinear equation ( set \textbf{eosType} to
1103     \texttt{'POLYNOMIAL'}). In the linear case, you need to specify the
1104     thermal and haline expansion coefficients represented by the variables
1105     \textbf{tAlpha} (in K$^{-1}$) and \textbf{sBeta} (in ppt$^{-1}$). For
1106     the nonlinear case, you need to generate a file of polynomial
1107     coefficients called \textit{POLY3.COEFFS}. To do this, use the program
1108 mlosch 1.13 \textit{utils/knudsen2/knudsen2.f} under the model tree (a Makefile is
1109     available in the same directory and you will need to edit the number
1110     and the values of the vertical levels in \textit{knudsen2.f} so that
1111     they match those of your configuration).
1112    
1113     There there are also higher polynomials for the equation of state:
1114     \begin{description}
1115 edhill 1.18 \item[\texttt{'UNESCO'}:] The UNESCO equation of state formula of
1116 mlosch 1.13 Fofonoff and Millard \cite{fofonoff83}. This equation of state
1117 edhill 1.18 assumes in-situ temperature, which is not a model variable; {\em its
1118     use is therefore discouraged, and it is only listed for
1119     completeness}.
1120     \item[\texttt{'JMD95Z'}:] A modified UNESCO formula by Jackett and
1121 mlosch 1.13 McDougall \cite{jackett95}, which uses the model variable potential
1122 edhill 1.18 temperature as input. The \texttt{'Z'} indicates that this equation
1123 mlosch 1.13 of state uses a horizontally and temporally constant pressure
1124     $p_{0}=-g\rho_{0}z$.
1125 edhill 1.18 \item[\texttt{'JMD95P'}:] A modified UNESCO formula by Jackett and
1126 mlosch 1.13 McDougall \cite{jackett95}, which uses the model variable potential
1127 edhill 1.18 temperature as input. The \texttt{'P'} indicates that this equation
1128 mlosch 1.13 of state uses the actual hydrostatic pressure of the last time
1129     step. Lagging the pressure in this way requires an additional pickup
1130     file for restarts.
1131 edhill 1.18 \item[\texttt{'MDJWF'}:] The new, more accurate and less expensive
1132 mlosch 1.13 equation of state by McDougall et~al. \cite{mcdougall03}. It also
1133     requires lagging the pressure and therefore an additional pickup
1134     file for restarts.
1135     \end{description}
1136     For none of these options an reference profile of temperature or
1137     salinity is required.
1138 adcroft 1.1
1139 adcroft 1.4 \subsection{Momentum equations}
1140 adcroft 1.1
1141 edhill 1.18 In this section, we only focus for now on the parameters that you are
1142     likely to change, i.e. the ones relative to forcing and dissipation
1143     for example. The details relevant to the vector-invariant form of the
1144     equations and the various advection schemes are not covered for the
1145     moment. We assume that you use the standard form of the momentum
1146     equations (i.e. the flux-form) with the default advection scheme.
1147     Also, there are a few logical variables that allow you to turn on/off
1148     various terms in the momentum equation. These variables are called
1149     \textbf{momViscosity, momAdvection, momForcing, useCoriolis,
1150     momPressureForcing, momStepping} and \textbf{metricTerms }and are
1151     assumed to be set to \texttt{'.TRUE.'} here. Look at the file
1152     \textit{model/inc/PARAMS.h }for a precise definition of these
1153     variables.
1154 adcroft 1.1
1155 edhill 1.17 \begin{description}
1156     \item[initialization] \
1157    
1158     The velocity components are initialized to 0 unless the simulation
1159     is starting from a pickup file (see section on simulation control
1160     parameters).
1161    
1162     \item[forcing] \
1163    
1164     This section only applies to the ocean. You need to generate
1165 edhill 1.18 wind-stress data into two files \textbf{zonalWindFile} and
1166     \textbf{meridWindFile} corresponding to the zonal and meridional
1167 edhill 1.17 components of the wind stress, respectively (if you want the stress
1168     to be along the direction of only one of the model horizontal axes,
1169     you only need to generate one file). The format of the files is
1170     similar to the bathymetry file. The zonal (meridional) stress data
1171     are assumed to be in Pa and located at U-points (V-points). As for
1172     the bathymetry, the precision with which to read the binary data is
1173 edhill 1.18 controlled by the variable \textbf{readBinaryPrec}. See the matlab
1174     program \textit{gendata.m} in the \textit{input} directories under
1175     \textit{verification} to see how simple analytical wind forcing data
1176     are generated for the case study experiments.
1177 edhill 1.17
1178     There is also the possibility of prescribing time-dependent periodic
1179     forcing. To do this, concatenate the successive time records into a
1180 edhill 1.18 single file (for each stress component) ordered in a (x,y,t) fashion
1181     and set the following variables: \textbf{periodicExternalForcing }to
1182     \texttt{'.TRUE.'}, \textbf{externForcingPeriod }to the period (in s)
1183     of which the forcing varies (typically 1 month), and
1184     \textbf{externForcingCycle} to the repeat time (in s) of the forcing
1185     (typically 1 year -- note: \textbf{ externForcingCycle} must be a
1186     multiple of \textbf{externForcingPeriod}). With these variables set
1187     up, the model will interpolate the forcing linearly at each
1188     iteration.
1189 edhill 1.17
1190     \item[dissipation] \
1191    
1192     The lateral eddy viscosity coefficient is specified through the
1193 edhill 1.18 variable \textbf{viscAh} (in m$^{2}$s$^{-1}$). The vertical eddy
1194     viscosity coefficient is specified through the variable
1195     \textbf{viscAz} (in m$^{2}$s$^{-1}$) for the ocean and
1196     \textbf{viscAp} (in Pa$^{2}$s$^{-1}$) for the atmosphere. The
1197     vertical diffusive fluxes can be computed implicitly by setting the
1198     logical variable \textbf{implicitViscosity }to \texttt{'.TRUE.'}.
1199     In addition, biharmonic mixing can be added as well through the
1200     variable \textbf{viscA4} (in m$^{4}$s$^{-1}$). On a spherical polar
1201     grid, you might also need to set the variable \textbf{cosPower}
1202     which is set to 0 by default and which represents the power of
1203     cosine of latitude to multiply viscosity. Slip or no-slip conditions
1204     at lateral and bottom boundaries are specified through the logical
1205     variables \textbf{no\_slip\_sides} and \textbf{no\_slip\_bottom}. If
1206     set to \texttt{'.FALSE.'}, free-slip boundary conditions are
1207     applied. If no-slip boundary conditions are applied at the bottom, a
1208     bottom drag can be applied as well. Two forms are available: linear
1209     (set the variable \textbf{bottomDragLinear} in s$ ^{-1}$) and
1210     quadratic (set the variable \textbf{bottomDragQuadratic} in
1211     m$^{-1}$).
1212 edhill 1.17
1213     The Fourier and Shapiro filters are described elsewhere.
1214    
1215     \item[C-D scheme] \
1216    
1217     If you run at a sufficiently coarse resolution, you will need the
1218     C-D scheme for the computation of the Coriolis terms. The
1219     variable\textbf{\ tauCD}, which represents the C-D scheme coupling
1220     timescale (in s) needs to be set.
1221    
1222     \item[calculation of pressure/geopotential] \
1223    
1224     First, to run a non-hydrostatic ocean simulation, set the logical
1225 edhill 1.18 variable \textbf{nonHydrostatic} to \texttt{'.TRUE.'}. The pressure
1226 edhill 1.17 field is then inverted through a 3D elliptic equation. (Note: this
1227     capability is not available for the atmosphere yet.) By default, a
1228     hydrostatic simulation is assumed and a 2D elliptic equation is used
1229     to invert the pressure field. The parameters controlling the
1230     behaviour of the elliptic solvers are the variables
1231 edhill 1.18 \textbf{cg2dMaxIters} and \textbf{cg2dTargetResidual } for
1232     the 2D case and \textbf{cg3dMaxIters} and
1233     \textbf{cg3dTargetResidual} for the 3D case. You probably won't need to
1234 edhill 1.17 alter the default values (are we sure of this?).
1235    
1236     For the calculation of the surface pressure (for the ocean) or
1237     surface geopotential (for the atmosphere) you need to set the
1238 edhill 1.18 logical variables \textbf{rigidLid} and \textbf{implicitFreeSurface}
1239     (set one to \texttt{'.TRUE.'} and the other to \texttt{'.FALSE.'}
1240     depending on how you want to deal with the ocean upper or atmosphere
1241     lower boundary).
1242 adcroft 1.1
1243 edhill 1.17 \end{description}
1244 adcroft 1.1
1245 adcroft 1.4 \subsection{Tracer equations}
1246 adcroft 1.1
1247 edhill 1.18 This section covers the tracer equations i.e. the potential
1248     temperature equation and the salinity (for the ocean) or specific
1249     humidity (for the atmosphere) equation. As for the momentum equations,
1250     we only describe for now the parameters that you are likely to change.
1251     The logical variables \textbf{tempDiffusion} \textbf{tempAdvection}
1252     \textbf{tempForcing}, and \textbf{tempStepping} allow you to turn
1253     on/off terms in the temperature equation (same thing for salinity or
1254     specific humidity with variables \textbf{saltDiffusion},
1255     \textbf{saltAdvection} etc.). These variables are all assumed here to
1256     be set to \texttt{'.TRUE.'}. Look at file \textit{model/inc/PARAMS.h}
1257     for a precise definition.
1258 adcroft 1.1
1259 edhill 1.17 \begin{description}
1260     \item[initialization] \
1261    
1262     The initial tracer data can be contained in the binary files
1263 edhill 1.18 \textbf{hydrogThetaFile} and \textbf{hydrogSaltFile}. These files
1264     should contain 3D data ordered in an (x,y,r) fashion with k=1 as the
1265     first vertical level. If no file names are provided, the tracers
1266     are then initialized with the values of \textbf{tRef} and
1267     \textbf{sRef} mentioned above (in the equation of state section). In
1268 edhill 1.17 this case, the initial tracer data are uniform in x and y for each
1269     depth level.
1270    
1271     \item[forcing] \
1272    
1273     This part is more relevant for the ocean, the procedure for the
1274     atmosphere not being completely stabilized at the moment.
1275    
1276     A combination of fluxes data and relaxation terms can be used for
1277 edhill 1.18 driving the tracer equations. For potential temperature, heat flux
1278 edhill 1.17 data (in W/m$ ^{2}$) can be stored in the 2D binary file
1279 edhill 1.18 \textbf{surfQfile}. Alternatively or in addition, the forcing can
1280     be specified through a relaxation term. The SST data to which the
1281     model surface temperatures are restored to are supposed to be stored
1282     in the 2D binary file \textbf{thetaClimFile}. The corresponding
1283     relaxation time scale coefficient is set through the variable
1284     \textbf{tauThetaClimRelax} (in s). The same procedure applies for
1285     salinity with the variable names \textbf{EmPmRfile},
1286     \textbf{saltClimFile}, and \textbf{tauSaltClimRelax} for freshwater
1287     flux (in m/s) and surface salinity (in ppt) data files and
1288     relaxation time scale coefficient (in s), respectively. Also for
1289     salinity, if the CPP key \textbf{USE\_NATURAL\_BCS} is turned on,
1290     natural boundary conditions are applied i.e. when computing the
1291     surface salinity tendency, the freshwater flux is multiplied by the
1292     model surface salinity instead of a constant salinity value.
1293 edhill 1.17
1294     As for the other input files, the precision with which to read the
1295     data is controlled by the variable \textbf{readBinaryPrec}.
1296     Time-dependent, periodic forcing can be applied as well following
1297     the same procedure used for the wind forcing data (see above).
1298    
1299     \item[dissipation] \
1300    
1301     Lateral eddy diffusivities for temperature and salinity/specific
1302 edhill 1.18 humidity are specified through the variables \textbf{diffKhT} and
1303     \textbf{diffKhS} (in m$^{2}$/s). Vertical eddy diffusivities are
1304     specified through the variables \textbf{diffKzT} and
1305     \textbf{diffKzS} (in m$^{2}$/s) for the ocean and \textbf{diffKpT
1306     }and \textbf{diffKpS} (in Pa$^{2}$/s) for the atmosphere. The
1307     vertical diffusive fluxes can be computed implicitly by setting the
1308     logical variable \textbf{implicitDiffusion} to \texttt{'.TRUE.'}.
1309     In addition, biharmonic diffusivities can be specified as well
1310     through the coefficients \textbf{diffK4T} and \textbf{diffK4S} (in
1311 edhill 1.17 m$^{4}$/s). Note that the cosine power scaling (specified through
1312 edhill 1.18 \textbf{cosPower}---see the momentum equations section) is applied to
1313     the tracer diffusivities (Laplacian and biharmonic) as well. The
1314 edhill 1.17 Gent and McWilliams parameterization for oceanic tracers is
1315     described in the package section. Finally, note that tracers can be
1316     also subject to Fourier and Shapiro filtering (see the corresponding
1317     section on these filters).
1318    
1319     \item[ocean convection] \
1320    
1321     Two options are available to parameterize ocean convection: one is
1322     to use the convective adjustment scheme. In this case, you need to
1323     set the variable \textbf{cadjFreq}, which represents the frequency
1324     (in s) with which the adjustment algorithm is called, to a non-zero
1325     value (if set to a negative value by the user, the model will set it
1326     to the tracer time step). The other option is to parameterize
1327     convection with implicit vertical diffusion. To do this, set the
1328 edhill 1.18 logical variable \textbf{implicitDiffusion} to \texttt{'.TRUE.'}
1329     and the real variable \textbf{ivdc\_kappa} to a value (in m$^{2}$/s)
1330 edhill 1.17 you wish the tracer vertical diffusivities to have when mixing
1331     tracers vertically due to static instabilities. Note that
1332 edhill 1.18 \textbf{cadjFreq} and \textbf{ivdc\_kappa}can not both have non-zero
1333     value.
1334 adcroft 1.1
1335 edhill 1.17 \end{description}
1336 adcroft 1.1
1337 adcroft 1.4 \subsection{Simulation controls}
1338 adcroft 1.1
1339 edhill 1.18 The model ''clock'' is defined by the variable \textbf{deltaTClock}
1340     (in s) which determines the IO frequencies and is used in tagging
1341     output. Typically, you will set it to the tracer time step for
1342     accelerated runs (otherwise it is simply set to the default time step
1343     \textbf{deltaT}). Frequency of checkpointing and dumping of the model
1344     state are referenced to this clock (see below).
1345 adcroft 1.1
1346 edhill 1.17 \begin{description}
1347     \item[run duration] \
1348    
1349     The beginning of a simulation is set by specifying a start time (in
1350 edhill 1.18 s) through the real variable \textbf{startTime} or by specifying an
1351 edhill 1.17 initial iteration number through the integer variable
1352     \textbf{nIter0}. If these variables are set to nonzero values, the
1353 edhill 1.18 model will look for a ''pickup'' file \textit{pickup.0000nIter0} to
1354     restart the integration. The end of a simulation is set through the
1355     real variable \textbf{endTime} (in s). Alternatively, you can
1356     specify instead the number of time steps to execute through the
1357     integer variable \textbf{nTimeSteps}.
1358 edhill 1.17
1359     \item[frequency of output] \
1360    
1361     Real variables defining frequencies (in s) with which output files
1362 edhill 1.18 are written on disk need to be set up. \textbf{dumpFreq} controls
1363 edhill 1.17 the frequency with which the instantaneous state of the model is
1364 edhill 1.18 saved. \textbf{chkPtFreq} and \textbf{pchkPtFreq} control the output
1365     frequency of rolling and permanent checkpoint files, respectively.
1366     See section 1.5.1 Output files for the definition of model state and
1367     checkpoint files. In addition, time-averaged fields can be written
1368     out by setting the variable \textbf{taveFreq} (in s). The precision
1369     with which to write the binary data is controlled by the integer
1370     variable w\textbf{riteBinaryPrec} (set it to \texttt{32} or
1371     \texttt{64}).
1372 adcroft 1.1
1373 edhill 1.17 \end{description}
1374 adcroft 1.1
1375 mlosch 1.13
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