Stephen Griffies Stephen.Griffies@noaa.gov Niki Zadeh Niki.Zadeh@noaa.gov

The purpose of this section is to provide an overview of MOM and the contents of this web page.

The Modular Ocean Model (MOM) is a numerical representation of the ocean's hydrostatic primitive equations. It is designed primarily as a tool for studying the global ocean climate system, as well as capabilities for regional and coastal applications. The latest release of MOM occurred in 2012, and is named MOM. This code has origins that date back to the pioneering work of Kirk Bryan and Mike Cox in the 1960s-1980s. It is developed and supported by researchers at NOAA's Geophysical Fluid Dynamics Laboratory (GFDL), with critical contributions also provided by researchers worldwide who comprise the MOM community. The purpose of this web guide is to provide general information about MOM, and particular information for how to download and run the code. Here is a table summarizing the algorithmic history of MOM.

MOM has had the following releases (note that MOM4p1 releases are distinguished by release dates). MOM4p0a: January 2004 MOM4p0b: March 2004 MOM4p0c: August 2004 MOM4p0d: May 2005 MOM4p1: 28 September 2007 MOM4p1: 28 December 2007 MOM4p1: Dec 2009 MOM5: 2012 For each release, we aim to update MOM by enhancing features and documentation, and correcting bugs. Each version is generally compatible with the previous versions. However, as updates are made, we cannot guarantee that all features will bitwise agree across releases. Nonetheless, we do maintain a small selection of ``bitwise-legacy'' code to allow for certain modules to bitwise agreement across versions. As the maintenance of bitwise-legacy features represents an onerous task (e.g., bits change when A+B is altered to B+A), we recommend that researchers beginning new projects start with the most recent version, and that researchers with mature projects carefully test the new code prior to moving forward.

We maintain the MOM source code and associated datasets at GForge. MOM users are required to register at the GFDL GForge location. Users need to register only once to get both the source code and datasets of MOM. Registered users then need to request access to the relevant project.

Email concerning MOM should be directed to the MOM-email. All questions, comments, and suggestions are to be referred to this list. Note that by registering at GForge to access the code, you are automatically subscribed to the email list.

There is a sizable user community for MOM. This community has proven to be a great resource, especially for new users, and those with portability questions, some of which are beyond the abilities of GFDL scientists to answer.

The MOM team aims to provide code that is efficient, flexible, and transparent for use across a broad range of computer platforms. Balancing these aims is not always simple. For example, some of the most efficient code is also the least transparent. The MOM developers are scientists whose main concern is to support MOM as a tool for science research. This focus then leads us to weight transparency and portability over efficiency. However, we readily make efficiency modifications that are of a general nature, so please do feel free to volunteer any such changes. Given the above aims, we have continued to support one avenue for code efficiency involving the allocation of arrays. MOM can be compiled in two ways: with static allocation of arrays or dynamic allocation. Static allocation is enabled at compile time via the cpp-preprocessor option MOM\_STATIC\_ARRAYS. At GFDL, we have generally found that static allocation executables are faster than dynamic, since compilers like to know before-hand the size of the model arrays. Work on the SGI machines at GFDL has reduced the difference in efficiency between these two compilations. However, details of the model configuration strongly impact the differences in model speed. Additionally, we understand that on some platforms, the dynamic allocation results in faster code than static. Consequently, we have decided to maintain both the static and dynamic options, given the ambiguous results across platforms, compilers, model configurations, ect.

The purpose of this section is to outline certain features of MOM.

In addition to this online user guide, documentation for MOM is provided by the following LaTeX generated postscript documents: A Technical Guide to MOM4 by Stephen.Griffies@noaa.gov, Matthew.Harrison@noaa.gov, Ronald.Pacanowski@noaa.gov, and Tony.Rosati@noaa.gov. This is the primary reference for MOM4p0. It contains details about some of the numerical algorithms and diagnostics. Reference to MOM4p0 in the literature should refer to this document: A Technical Guide to MOM4 GFDL Ocean Group Technical Report No. 5 S.M. Griffies, M.J. Harrison, R.C. Pacanowski, and A. Rosati NOAA/Geophysical Fluid Dynamics Laboratory August 2004 Available on-line at . Elements of MOM by Stephen.Griffies@noaa.gov is the primary reference for MOM4p1 and MOM5. It contains details about some of the numerical algorithms and diagnostics. Reference to MOM in the literature should refer to this document: Elements of the Modular Ocean Model (MOM) GFDL Ocean Group Technical Report No. 7 Stephen M. Griffies NOAA/Geophysical Fluid Dynamics Laboratory June 2012 620 + xiii pages Available on-line at . A theoretical rationalization of ocean climate models is provided by Fundamentals of Ocean Climate Models. This book by Stephen.Griffies@noaa.gov was published by Princeton University Press in August 2004.

The documentation of most Fortran modules in FMS is inserted right in the source code to enable consistency between the code and documentation. A Perl software tool is used to extract documentation from the source code to create a corresponding html module. For example, documentation for shared/diag_manager/diag_manager.F90 module is shared/diag_manager/diag_manager.html. In general, the embedded documentation is a good starting point to understand the Fortran module, though ultimately the Fortran code is the final source for information.

Although MOM shares much in common with earlier versions of MOM, it possesses a number of computational, numerical, and physical characteristics that are noteworthy. The main characteristics of MOM can be found in the introduction to Elements of MOM).

MOM has been coded within GFDL's Flexible Modeling System (FMS). Doing so allows for MOM developers to use numerous FMS infrastructure and superstructure modules that are shared amongst various atmospheric, ocean, sea ice, land, vegetative, etc. models. Common standards and shared software tools facilitate the development of high-end earth system models, which necessarily involves a wide variety of researchers working on different computational platforms. Such standards also foster efficient input from computational scientists and engineers as they can more readily focus on common computational issues. The following list represents a sample of the FMS shared modules used by MOM. time manager: keeps model time and sets time dependent flags coupler: used to couple MOM to other component models I/O : to read and write data in either NetCDF, ASCII, or native formats parallelization tools: for passing messages across parallel processors diagnostic manager: to register and send fields to be written to a file for later analysis field manager: for integrating multiple tracers and organizing their names, boundary conditions, and advection schemes The FMS infrastructure (the "Siena version") forms the basis for the 2012 release of MOM. The Flexible Modeling System ( FMS), including MOM, is free software; you can redistribute it and/or modify it and are expected to follow the terms of the GNU General Public License as published by the Free Software Foundation; either version 2 of the License, or (at your option) any later version. FMS is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with MOM; if not, write to: Free Software Foundation, Inc. 59 Temple Place, Suite 330 Boston, MA 02111-1307 USA or see:

MOM is distributed with a suite of test cases, with these tests detailed in Elements of MOM. Many of the test cases are NOT sanctioned for their physical relevance. They are instead provided for the user to learn how to run MOM, and to verify the numerical and/or computational integrity of the code. PLEASE do not assume that the experiments will run for more than the short time selected in the sample runscripts.

MOM developers aim to provide the international climate research community with a repository for robust and well documented methods to simulate the ocean climate system. Consequently, we encourage interested researchers to contribute to MOM by commenting on code features, and providing new modules that enhance simulation integrity (e.g., a new physical parameterization or new advection scheme) or increase the model's functionality.

The purpose of this section is to outline methods required to obtain the source code and associated datasets.

The FMS development team uses a local implementation of GForge to serve FMS software, located at . In order to obtain the source code and data sets, you must register as an FMS user on our software server. After submitting the registration form on the software server, you should receive an automatically generated confirmation email within a few minutes. Clicking on the link in the email confirms the creation of your account. After your account has been created, you should log in and request access to the MOM project. Once the project administrator grants you access, you will receive a second email notification. This email requires action on the part of the project administrator and thus may take longer to arrive. The email will contain a software access password along with instructions for obtaining the release package (a tar file). You may download the MOM tar file from . The data set and outputs for selected MOM test experiments are available via ftp More details can be found in the quickstart_guide.html.

There are many datasets provided with the various MOM test cases. All datasets released with MOM are in NetCDF format, since this format is widely used in the community. A number of useful tools are available here that allow the user to perform some necessary operations (editting attributes, merging, etc.) on a NetCDF file.

MOM is distributed with code used to generate model grids, initial conditions, and boundary conditions. Each step must be performed prior to running the ocean model. The steps used during this experimental setup stage are generally termed "preprocessing", and the code used for these purposes is under the /preprocessing directory in the MOM distribution. The purpose of this section of the User Guide is to outline this code and its usage. Further details of usage and algorithms can be found in the internal documentation within the various preprocessing code modules.

We start this section with some general comments regarding the setup of a model experiment. --Setting up an experiment is critical part to the success of a research or development project with MOM. It is important that the user take some time to understand each of the many steps, and scrutinize the output from this code. We have endeavored over the years to provide tools facilitating the ready setup of a new experiment. However, we remain unable to provide code that does everything possible under the sun. Additionally, all features that are provided here may not be fully tested. For these reasons, the preprocessing code continues to evolve as use and functionality evolve. We sincerely appreciate ALL comments about code and documentation, especially comments regarding clarity, completeness, and correctness. Your input is essential for the improvement of the code and documentation. --Many steps in idealized experiments that were formerly performed while running earlier MOM versions have been extracted from MOM and placed into preprocessing. Hence, even if you are running an idealized experiment, it is likely that you will need to perform some if not all of the preprocessing steps discussed here. --If you have a problem that is not addressed here, then please feel free to query the MOM email list. No question is too silly, so please ask! --All code used to setup an experiment with MOM is written in Fortran 90/95 except make_xgrids, which is written in C. Most code is dependent on FMS shared code for the purpose of parallization and interpolation. In addition to the documentation provided here, there are comments within the code to help users debug and to make modifications to suit their purpose. --Some users make nontrivial changes of general use. With your support, assistance, and maintenance, we will endeavour to include your changes in future releases.

Mosaics is the name given to a general framework to define structured grids at GFDL. The details of this scheme are being incorporated by others outside of GFDL as well. Most of the recent global models developed at GFDL employ the conventions of Mosaic. However, MOM is backwards compatible, so that it still supports grids generated with older software (discussed here) For a description of how to create grids using the newer Mosaic tools, which are more general than the older approaches, then please access this link

Within GFDL FMS, ocean and ice are assumed to share the same grid. This means that the two models read in the same grid specification file. Even so, the domain decomposition on parallel systems may be different, and indeed they generally are due to different load balance issues between the two models. Even though the ocean and ice models read the same grid specification file, they use the information from the grid file in a slightly different manner when setting up the respective model's tracer grid. In particular, the ocean model reads the tracer location directly from the arrays (x_T/geolon_t, y_T/geolat_t) written in the grid specification file. In contrast, the GFDL ice model reads (x_vert_T/geolon_vert_t, y_vert_T/geolat_vert_t) from the grid specification file and then averages these four vertex locations to get the tracer location used in the ice model. The result is that diagnostics output from the two models have ocean and ice fields at slightly different locations for cases such as the tripolar grid when the grid is not spherical. The ocean/ice grid specification file is generated by executing the ocean_grid_generator utility. The ocean_grid_generator utility generates the horizontal grid, vertical grid, and topography. A C-shell script is provided to compile relevant code to generate and run the executable to produce the grid file. To create the desired grid and topography, setting namelist options within the runscript is needed. The horizontal grid can be conventional lon-lat spherical grid or a reprojected rotated tripolar grid (R. Murray, "Explicit generation of orthogonal grids for ocean models", 1996, J.Comp.Phys., v. 126, p. 251-273.). The choice is controlled by the namelist option "tripolar grid" (true for tripolar grid and false for lon-lat spherical grid). Note that Cartesian beta-plane and f-plane geometries are set up within MOM, not within the grid generation preprocessing steps discussed here (see ocean_core/ocean_grids.F90 for beta-plane and f-plane namelist options). The grid_spec file contains the following horizontal grid information: geographic location of T,E,C and N-cell (Tracer, East, Corner, and North cells), half and full cell lengths (in meters), rotation information between logical (i.e., grid oriented) and geographic east of cell. The complete description of the horizontal grid and namelist option is available in hgrid The vertical grid information includes depth of tracer points and tracer_boundaries. The complete description of namelist option is available in vgrid The topography can be idealized (various examples are provided and others can be easily added through emulating those provided) or remapped from a source topography dataset. The type of topography is specified by the namelist variable "topography". Namelist "topog_depend_on_vgrid" specifies if the topography will depend on the vertical grid or not. To generate a grid for MOM, "topog_depend_on_vgrid" should always be true. A useful option for those upgrading older models to MOM is "adjust_topo". If this option is set to false, there will be no adjustments made to the topography. See topog for further details about topography namelist options.

"Exchange grid" information is required for coupled models (i.e., ocean/ice coupled to land and/or atmosphere) that employ the GFDL coupler technology. The exchange grid is defined by taking the union of the ocean/ice grid with the atmosphere and land grids. This union is then used to compute area integrals to allow for conservative mapping of fluxes between the component models. The Sutherland-Hodgeman polygon clipping algorithm for model cell interaction calculation The exchange grid information is generated by executing the make_xgrids utility. The execution of the make_xgrids utility will generate a netcdf file with the name grid_spec.nc. The grid_spec.nc contains the component model grids as well as the exchange grid information. In particular, the utility make_xgrids generates two exchange grids used by the FMS coupler: one grid for surface fluxes and another for runoff. make_xgrids is created by compiling its C source: cc -O -o make_xgrids make_xgrids.c -I/usr/local/include -L/usr/local/lib -lnetcdf -lm creates the make_xgrids executable from C-source and the netCDF and standard math libraries. It is executed with the command make_xgrids -o ocean_grid.nc -a atmos_grid.nc -l land_grid.nc This execution produces a grid_spec.nc file (input files containing grid information for the ocean/sea-ice, atmosphere and land component models are indicated by the -o, -a and -l flags, respectively). The grid files ocean_grid.nc, atmosphere_grid.nc, and land_grid.nc all can be generated separately through the ocean_grid_generator utility. Normally at GFDL we select the same atmosphere and land model grid, but such is not necessary. When the land and atmosphere grids are the same, then we can reduce the execute command to make_xgrids -o ocean_grid.nc -a atmos_grid.nc If you further decide to choose same ocean, atmosphere and land grid, the execute command will be make_xgrids -o ocean_grid.nc -a ocean_grid.nc make_xgrids expects a netCDF format input specification for each of the component model grid files. For the ice/ocean grid (ocean_grid.nc), the following three fields are required: 1. wet - a 2D array of double precision numbers set to 1.0 where the ice and ocean models are active and 0.0 elsewhere. wet has im indices in the i-direction (pseudo east-west) and jm indices in the j-direction (pseudo north-south). These correspond to the size of the global arrays of temperature, salinity and ice thickness in the coupled climate model. 2. x_vert_T and y_vert_T - 3D double precision arrays (dimensioned im * jm * 4) that contain the longitudes and latitudes (respectively) of the four corners of T- cells. The numbers are in degrees. For the netCDF format input specification for the atmosphere and land grid (atmos_grid.nc and/or land_grid.nc), x_vert_T and y_vert_t are required. make_xgrids copies all fields of the ice/ocean grid specification file to its output file, grid_spec.nc, and then appends fields that specify the atmosphere and land model grids and then the surface and runoff exchange grids. Using the Sutherland-Hodgeman polygon clipping algorithm (reference in next paragraph) for model cell interaction calculation, make_xgrids takes care that the land and ocean grids perfectly tile the sphere. The land model's domain is defined as that part of the sphere not covered by ocean (where wet=0 on the ocean grid). To accomplish this, the land cells must be modified to remove the ocean parts. This is done in make_xgrids by first taking the intersections of atmosphere and land cells. The overlap area between these cells and active ocean cells are then subtracted. Finally, the modified atmosphere/land intersections are aggregated into land cell areas and atmosphere/land exchange cell areas. Model cell intersections are calculated using the Sutherland-Hodgeman polygon clipping algorithm (Sutherland, I. E. and G. W. Hodgeman, 1974: Reentrant polygon clipping, CACM, 17(1), 32-42.). This algorithm finds the intersection of a convex and arbitrary polygon by successively removing the portion of the latter that is "outside" each boundary of the former. It can be found in many computer graphics text books (e.g., Foley, J. D., A. van Dam, S. K. Feiner, and J. F. Hughes, 1990: Computer graphics: principles and practice, second edition. Addison Wesley, 1174 pp.). The implementation in make_xgrids is particularly simple because the clipping polygon is always a rectangle in longitude/latitude space. For the purpose of finding the line intersections in the clipping operations, the cell boundaries are assumed to be straight lines in longitude/latitude space. This treatment is only perfectly accurate for cells bounded by lines of longitude and latitude. Spherical areas are calculated by taking the integral of the negative sine of latitude around the boundary of a polygon (Jones, P. W., 1999: First- and second-order conservative remapping schemes for grids in spherical coordinates. Monthly Weather Review, 127, 2204-2210.). The integration pathways are again straight lines in longitude/latitude space. make_xgrids checks that the sphere and the individual cells of the atmosphere and ocean grids are tiled by the surface exchange cells. The fractional tiling errors are reported.

After generating the model grid, it is time to generate the initial and boundary conditions (ICs and BCs). These conditions are specific to the details of the model grid, so it is necessary to have the grid specificiation file in hand before moving to the IC and BC generation. There are two options for ICs and BCs. --Idealized Conditions. These conditions are based on subroutines that design idealized setups for either initial conditions (e.g., exponential temperature profile) or boundary conditions (e.g., cosine zonal wind stress). Code for these purposes is found in the idealized_ic and idealized_bc directories in the MOM distribution. Details of available namelist choices are in the documentation file idealized_ic.html as well as the comments within the source code itself. Users can readily incorporate their favorite idealized IC or BC into the MOM idealized preprocessing step by emulating the code provided. --Realistic Conditions. These ICs and BCs generally result from a regridding routine to bring, say, the Levitus analysis onto the model grid for initializing a model, or for mapping surface fluxes onto the grid for boundary conditions. Code enabling the regridding functions is found in the preprocessing/regrid_2d, preprocessing/regrid_3d and preprocessing/regrid directories in the MOM distribution. In the remainder of this section, we detail code to generate the ICs and BCs of use for MOM.

It is typical for air-sea fluxes of momentum, heat, and mosture to live on a grid distinct from the ocean model grid. In particular, most analysis are placed on a spherical latitude-longitude grid, whereas most global ocean models configured from MOM are run with tripolar grids. When running an ocean or ocean-ice model, it is useful to map the boundary fluxes onto the ocean model grid prior to the experiment. This preprocessing step saves computational time that would otherwise be needed if the fluxes were mapped each time step of a running experiment. To enable this regridding, one should access code in the preprocessing/regrid_2d directory. The original data must be on a latitude-longitude grid to use regrid_2d. The target/destination grid can be either latitude-longitude with arbitrary resolution, or tripolar with arbitrary resolution.

In some cases, one may wish to take a set of forcing fields from one tripolar MOM experiment and regrid them onto another tripolar MOM experiment with different grid resolution. In this case, it is necessary to regrid before running the experiment. As of the MOM4p0d distribution, there is a regridding tool within the preprocessing/regrid directory that enables one to regrid fields on one tripolar grid to another tripolar grid. Indeed, one can regrid source data from any logically rectangular grid (e.g., latitude-longitude grid or tripolar grid) to a target/destination grid that is any logically rectangular grid. Note that this is new code, and so has been tested only for particular cases. So the user should be extra careful to scrutinize the results.

The "on_grid" logical in the data_table indicates whether an input file is on the grid of the model or not. on_grid=.true. means that the input file is on the same grid as the ocean model. This is the recommended setting for models running with specified atmospheric forcing from data or an analysis product. on_grid=.false. means the input file has data on a grid differing from the ocean model. This feature is allowed ONLY if the input data lives on a spherical grid. This is a relevant setting if one wishes to keep the input data on their native spherical grid. If the input data is non-spherical, then on_grid=.false. is NOT supported. Instead, it is necessary to preprocess the data onto the ocean model grid.

The tool preprocessing/runoff_regrid is of use to grid river runoff data onto the ocean model grid. In this case, runoff is moved to a nearest ocean/land boundary point on the new grid. Note that the source runoff dataset must be on a spherical latitude-longitude grid, whereas the target/destination grid can be spherical or tripolar. The regridding algorithm is conservative. The conservative regridding scheme used in runoff_regrid is an area average scheme, which is similiar to the algorithm used in coupler flux exchange. If any land point has runoff data, after remapping runoff data onto destination grid, the runoff value of that land point will be moved to the nearest ocean point. Before using this tool, you must use make_xgrids to generate exchange grid information between the source grid and destination grid. The complete description can be found in runoff_regrid.html.

There are two ways to specify surface boundary fluxes when using the coupler feature of FMS. One is through flux exchange, and this employs a conservative algorithm as appropriate for running a coupled ocean-atmosphere model. It is assumed that the atmospheric model grid is spherical with arbitrary resolution. The other method is through data override, and this uses a non-conservative scheme. Data override is of use to selectively remove, say, one of the fluxes coming from an atmospheric model and replace this flux with that from data. GFDL modelers have found this feature to be very useful in diagnosing problems with a coupled model.

When generating realistic initial conditions for an ocean experiment, one generally requires the gridding of temperature and salinity, such as from the Levitus analysis product, onto the model's grid. For this purpose, we are in need of vertical grid information in addition to horizontal 2d information required for the surface boundary conditions. Hence, we use the preprocessing/regrid_3d. A similar procedure is required to develop sponge data. The original data must be on a spherical grid in order to use regrid_3d. If the original data is on a tripolar grid, we should use preprocessing/regrid, which can map data from any logical rectangular grid onto any logical rectangular grid.

For preprocessing/regrid_3d, preprocessing/regrid_2d and preprocessing/regrid, regridding is accomplished non-conservatively using a nearest neighbor distance weighting algorithm, or bilinear interpolation. The interpolation algorithm is controlled through the namelist option "interp_method". Bilinear interpolation is recommanded for most cases since it provides a smooth interpolation when regridding from coarse grid to fine grid (the usual situation with model destination grids typically having resolution more refined than source data products), and it is more efficient. Efficiency can become a particularly important issue when developing initial and boundary conditions for a refined resolution model. If the original data is on a tripolar grid, nearest neighbor distance weighting interpolation found in preprocessing/regrid must be used, since bilinear interpolation assumes the original data is on a latitude-longitude grid. For preprocessing/regrid_2d, preprocessing/regrid_3d and preprocessing/regrid using the nearest neighbor distance weighting algorithm, a maximum distance (in radians) can be selected using the namelist value max_dist. Namelist option "num_nbrs" can be adjusted for speed, although for most applications this refinement is not necessary. The complete namelist description for these algorithms can be found in regrid_2d.html, regrid_3d.html and regrid.html.

When the input data is on a latitude-longitude grid, preprocessing/regrid_2d and preprocessing/regrid_3d can be used. When the input data is on a tripolar grid or a latitude-longitude grid, postprocessing/regrid can be used. For sponge generation, acceptable input data sets must have NetCDF format with COARDS-compliance.

There are many ways that data can be formatted in time. The FMS tools used to read in time information, and to time interpolate, are quite sophisticated and flexible. Nonetheless, these tools cannot do everything, nor can they know a priori what the modeler intends. It is therefore necessary to maintain certain conventions when preparing the time information for datasets. This section aims to outline some of the common issues involved with time, and to provide a guide for resolving possible problems.

Previous versions of MOM used IEEE binary formats and MOM-specific headers to process forcing data. As of MOM4, data are stored in portable formats (NetCDF currently), and contain standardized metadata per the CF1.0 convention. Understading the functions of Fortran modules that handle metadata and time-related problems will be very helpful in identifying some user's problems. Some of the most frequently used modules are listed below: mpp_io_mod Low level I/O (open, close file, write, read,...) axis_utils_mod process metadata: identify cartesian axis information (X/Y/Z/T) time_manager_mod basic time operations, calendar, increment/decrement time time_interp_mod Computes a weight for linearly interpolating between two dates time_interp_external_mod top level routines for requesting data data_override_mod top level routines for requesting data

It is likely that you will encounter an error using "off-the-shelf" NetCDF files to force your ocean model. This could be due to inadequate metadata in the forcing files, mis-specification of the DataTable, or errors in the parsing of the axis information by axis_utils or get_cal_time. You'll need some tools to help you diagnose problems and apply the required fix. The first thing you should do to setup a new forcing file is use the test program: time_interp_external_mod:test_time_interp_external. This test program calls time_interp_external at user-specified model times and returns information on how the times were decoded and the resulting interpolation indices and weights. It is STRONGLY suggested that you pass your forcing files through this program before including them in your model configuration. As you gain familiarity with the metadata requirements, you will more easily be able to identify errors and save a lot of time debugging. The forcing test program is located in src/preprocessing/test_time_interp_ext. There is a csh version and a Perl version. Compilation mkmf -m Makefile -p test_time_interp_ext.exe -t $TEMPLATE -c -Dtest_time_interp_external -x shared/{time_manager,fms,mpp,clocks,time_interp,axis_utils,platform,horiz_interp,constants,memutils} running csh version namelist options: filename='foo.nc' ! name of forcing file fieldname='foo' ! name of variable in file year0=[integer] ! initial year to start model calendar month0=[integer] ! initial month to start model calendar day0=[integer] ! initial day to start model calendar days_inc=[integer] ! increment interval for model calendar ntime=[integer] ! number of model "timesteps" cal_type=['julian','noleap','360day'] ! model calendar running perl version test_time_interp_ext.pl -f 'foo.nc' -v 'foo' [--nt [int] --year0 [int] --month0 [int] --day0 [int] --inc_days [int] --cal_type [char]] Modifying the file metadata should hopefully prove straightforward. The NCO operators need to be installed on your platform. The utility "ncatted" is most useful for modifying or adding metadata. If for some reason, you are unable to install the NCO operators, you can use the NetCDF utilities "ncgen" and "ncdump" which come with the NetCDF package.

Can't identify cartesian axis information axis_utils_mod:get_axis_cart should return the cartesian information. If this fails, you will get a somewhat cryptic error message: "file/fieldname could not recognize axis atts in time_interp_external". The best solution is to add the "cartesian_axis" attribute to the axes, e.g. "ncatted -a cartesian_axis,axis_name,c,c,"X" foo.nc". Calendar attribute does not exist This is a required attribute. time_manager_mod:get_cal_time converts time units appropriate to the specified calendar to the model time representation. If the "calendar" attribute does not exist, an error message appears "get_cal_time: calendar attribute required. Check your dataset to make sure calendar attribute exists " Use a ncatted command such as: "ncatted -a calendar,time_axis_name,c,c,"julian" foo.nc" Currently, the FMS time_manager does not support the Gregorian calendar. So, for instance if you have forcing data that are encoded using the Gregorian calendar which has an average year length of 365.2425 days compared with the Julian calendar with an average year length of 365.25 days, assuming Julian calendar encoding will result in a drift of 0.75 days/100 years. If your forcing times are referenced to an early date such as "0001-01-01" your times will drift by 15 days by the year 2000. Until the Gregorian calendar is implemented in the FMS code, the recommended solution is to change the reference date in the forcing dataset using an application such as Ferret

Scalability of a complex model like MOM is the correlation between the number of processing elements (PE) and the run time. One would expect that run time decreases as the number of PEs increases. It is important, however, to note that there are a number of important factors that can affect scalability considerably: MOM test cases are designed for testing the code integrity, they are not set for scalability study or "production" purpose. Changes should be made if one wants to study scalability of the code. diag_step set the time steps at which numerical diagnostics (e.g., energy, tracer budgets) are computed. The user needs to set this value to be equal to the time step at the end of the experiment, so that only a single instance of the diagnostics is evaluated. For example, if time step is 1 hour and run length is 4 days, diag_step (or diag_freq in MOM4p0) should be set to 96. diag_table contains all fields that will be saved in history files. The frequency of saving and number of fields can afect the total run time greatly. So when testing performance, it is recommended that the researcher reduce the output of history files. Scalability is also dependent on the configuration of the computing platform: Ethernet card, interconnect between PEs, implementation of MPI, memory hierarchy, version of compiler, ... In examining the total run time the overheads due to initialization and termination should be extracted from total runtime for scalability study since they contain a lot of I/O activities.

When running an ocean-ice model with atmospheric data forcing, it may happen that some ocean-ice tasks contain only land points, in which case these processors stand idle. FMS provides a feature to mask land-only tasks and to thus run the model without allocating a processor for these land-only domains. For example, if a processor domain layout 30x50 is specified, but say 500 subdomains are land only, you may run the model with 1500-500=1000 MPI tasks only. Note that you do not get your results faster when eliminating land-only processors, but compute costs may be reduced. In the following example, an "x" represents a land-only subdomain, whereas a dot indicates a domain with a nonzero number of "wet" ocean points: x . x x . . . . . In this example, three idle processors could be left out (two in the northern-most row, and one in the second row) since there are no wet ocean points on these "x" domains. The ocean-ice model may thus be run with only 6 MPI tasks rather than nine. To enable this feature of FMS, the following variables in the namelist coupler_nml must be specified. coupler_nml ... do_atmos = .false. .... n_mask = 3 layout_mask = 3, 3 mask_list = 1,2, 1,3, 3,3 If a mask list is specified, the domain layout of the ocean and the ice model is automatically the same, as specified with layout_mask. Running the model, only 6 MPI tasks need to be started. For large and complex model topography, it is very tedious to specify the mask list by hand. To simplify this task, the preprocessing tool "check_mask" can be used after the model grid and topography are specified, i.e., when grid_spec.nc is generated. To do so requires adding the following to topog_nml during the preprocessing stage topog_nml check_mask=.true. The preprocessing code prints out a number of proposals for possible domain layouts, number of land-only subdomains, and templates for setting the mask_list. You may copy these layouts to coupler_nml, but note that you must replace spaces by a comma in "mask_list". You may configure "check_mask" from the namelist check_mask_nml. There are two variables "max_pe" and "halo" required to perform the mask checking. The default settings are max_pe = 128 halo = 1 If you intend to employ more processors, then increase max_pe. If you want to use higher order advection schemes, then increase halo to halo=2 or even halo=3. Otherwise, the halo information of masked domains may leak into ocean domains, in which case the model will fail, with errors reporting land values at ocean points. In the postprocessing step, the single netCDF-output files from the MPI tasks can be combined into one file using the tool mppnccombine. The latest version adds "missing" values at the location of land-only domains. Hence, the only remaining trace of masking out land-only processors is in your account files, where some compute time is saved.

For many analysis applications, it is sufficient, and often preferable, to have output on the model's native grid (i.e., the grid used to run the simulation). Accurate computation of budgets, for example, must be done on the model's native grid, preferably online during integration. MOM provides numerous online diagnostics for this purpose. Many applications, such as model comparison projects, require results on a common latitude-longitude spherical grid. Such facilitates the development of difference maps. For this purpose, we have developed a tool to regrid scalar and vector fields from a tripolar grid to a spherical grid. In principle, this tool can be used to regrid any logically rectangular gridded field onto a spherical grid. However, applications at GFDL have been limited to the tripolar to spherical regrid case. In general, regridding is a difficult task to perform accurately and without producing noise or spurious results. The user should carefully examine regridding results for their physical integrity. Problems occur, in particular, with fields near MOM's partial bottom step topography in the presence of realistic topography and land/sea geometry. Indeed, we were unable to find a simple algorithm to handle regridding in the vertical that did not produce egregious levels of noise. Hence, the regridding tool provided with MOM only handles horizontal regridding. The regridded data will thus be on the source vertical grid. Model comparisons should ideally be performed only after regridding output using the same regridding algorithm. Unfortunately, such is not generally the case since there is no standard regridding algorithm used in the modeling community.

The regridding algorithm provided with the MOM distribution is located in the directory postprocessing/regrid The algorithm accepts data from any logically rectangular grid (e.g., tripolar or latitude-longitude) and regrids to a spherical latitude-longitude grid. When the data is on the tracer cell (T-cell), the regridding interpolation is conservative. Thus, total heat, salt, and passive tracer remain the same on the two grids. However, when data is located at another position: corner or C-cell as for a B-grid horizontal velocity component east or E-cell as for an eastward tracer flux north or N-cell as for a northward tracer flux then regridding is accomplished non-conservatively using a nearest neighbor distance weighting algorithm. It is for this reason that computationally accurate results are only available when working on the model's native grids. The regridding tool reads grids information from a netcdf file, specified by the namelist "grid_spec_file". "grid_spec_file" contains source grid, destination grid and exchange grid information. source grid: src_grid.nc. This is the model's native grid. It results from running preprocessing grid generation code. destination grid: dst_grid.nc. This is the spherical latitude-lontitude grid. This grid can also be obtained from running preprocessing grid generation code. Be sure that the tripolar option is set to false to ensure that dst_grid.nc is spherical. exchange grid: grid_spec.nc. This is the union of the source grid and destination grid. The exchange grid is needed for conservative regridding. The same conservative regridding algorithm is used for coupled models with FMS. The tool to construct the exchange grid is know as "make_xgrids". It is located in the preprocessing directory. After grid_spec.nc is generated, it should be passed to the regrid tool through namelist "grid_spec_file"(No need to pass src_grid.nc and dst_grid.nc to the regrid tool). To create the exchange grid, execute the command make_xgrids -o src_grid.nc -a dst_grid.nc The exchange grid creates a file grid_spec.nc. It has new fields with names: AREA_ATMxOCN, DI_ATMxOCN, DJ_ATMxOCN, I_ATM_ATMxOCN, J_ATM_ATMxOCN, I_OCN_ATMxOCN, J_OCN_ATMxOCN, AREA_ATMxLND, DI_ATMxLND, DJ_ATMxLND, I_ATM_ATMxLND, J_ATM_ATMxLND, I_LND_ATMxLND, J_LND_ATMxLND, AREA_LNDxOCN, DI_LNDxOCN, DJ_LNDxOCN, I_LND_LNDxOCN, J_LND_LNDxOCN, I_OCN_LNDxOCN, J_OCN_LNDxOCN, xba, yba, xta, yta, AREA_ATM, xbl, ybl, xtl, ytl, AREA_LND, AREA_LND_CELL, xto, yto, AREA_OCN It is critical that src_grid.nc DO NOT already have any of the above new exchange grid fields. If they do, then these fields should be removed using netcdf tools such as ncks. After the grid_spec.nc file is generated, it is passed into the regrid program through the nml option "grid_spec_file". The regrid program reads model data from a netcdf file, which is specfied by the namelist variable "src_data". Again, src_data fields are gridded according to src_grid.nc. The number of fields to be regridded is specified by num_flds. The name of the fields (e.g., temp, salt) to be regridded is specified by the namelist variable "fld_name". Each field can be a scalar or vector. If a vector, then specify by vector_fld. Vector fields should always be paired together (e.g., u,v components to the horizontal current). The output file is a netcdf file specified by the namelist variable "dst_data". The complete namelist option description is available in regrid.html or the code itself.

A runscript is provided in each test case directory (exp/$test_case ) for each test case. Details can be found in quickstart_guide.html. Incorporated in the FMS infrastructure is MPP (Massively Parallel Processing), which provides a uniform message-passing API interface to the different message-passing libraries. If MPICH is installed, the user can compile the MOM source code with MPI. If the user does not have MPICH or the communications library, the MOM source code can be compiled without MPI by omitting the CPPFLAGS value -Duse_libMPI in the example runscript.

The diagnostics table allows users to specify the sampling rates and choose the output fields prior to executing the MOM source code. It is included in the input directory for each test case (exp/$test_case/input). A portion of a sample MOM diagnostic table is displayed below. Reference diag_manager.html for detailed information on the use of diag_manager. "Diagnostics for MOM test case" 1980 1 1 0 0 0 #output files "ocean_month",1,"months",1,"hours","Time" "ocean_snap",1,"days",1,"hours","Time" #####diagnostic field entries#### #=============================================================== # ocean model grid quantities (static fields and so not time averaged)) "ocean_model","geolon_t","geolon_t","ocean_month" "all",.false.,"none",2 "ocean_model","geolat_t","geolat_t","ocean_month","all",.false.,"none",2 #================================================================ # prognostic fields "ocean_model","temp","temp","ocean_month","all", "max", "none",2 "ocean_model","age_global","age_global","ocean_month","all","min","none",2 #================================================================ # diagnosing tracer transport "ocean_model","temp_xflux_sigma","temp_xflux_sigma","ocean_month","all",.true.,"none",2 "ocean_model","temp_yflux_sigma","temp_yflux_sigma","ocean_month","all",.true.,"none",2 #================================================================ # surface forcing "ocean_model","sfc_hflux","sfc_hflux","ocean_month","all",.true.,"none",2 "ocean_model","sfc_hflux_adj","sfc_hflux_adj","ocean_month","all",.true.,"none",2 #================================================================ # ice model fields "ice_model", "FRAZIL", "FRAZIL", "ice_month", "all", .true., "none", 2, "ice_model", "HI", "HI", "ice_month", "all", .true., "none", 2 #----------------------------------------------------------------- The diagnostics manager module, diag_manager_mod, is a set of simple calls for parallel diagnostics on distributed systems. It provides a convenient set of interfaces for writing data to disk in NetCDF format. The diagnostics manager is packaged with the MOM source code. The FMS diagnostic manager can handle scalar fields as well as arrays. For more information on the diagnostics manager, reference diag_manager.html.

The MOM field table is used to specify tracers and their advection schemes, cross-land tracer mixing, cross-land insertion, and other options. The field table is included in the runscript as a namelist and is written to an output file upon execution of the runscript. "prog_tracers","ocean_mod","temp" horizontal-advection-scheme = quicker vertical-advection-scheme = quicker restart_file = ocean_temp_salt.res.nc / "prog_tracers","ocean_mod","salt" horizontal-advection-scheme = mdfl_sweby vertical-advection-scheme = mdfl_sweby restart_file = ocean_temp_salt.res.nc / "tracer_packages","ocean_mod","ocean_age_tracer" names = global horizontal-advection-scheme = mdfl_sweby vertical-advection-scheme = mdfl_sweby restart_file = ocean_age.res.nc min_tracer_limit=0.0 / "namelists","ocean_mod","ocean_age_tracer/global" slat = -90.0 nlat = 90.0 wlon = 0.0 elon = 360.0 / "xland_mix","ocean_mod","xland_mix" "xland","Gibraltar","ixland_1=274,ixland_2=276,jxland_1=146,jxland_2=146,kxland_1=1,kxland_2=28,vxland=0.55e6" "xland","Gibraltar","ixland_1=274,ixland_2=276,jxland_1=147,jxland_2=147,kxland_1=1,kxland_2=28,vxland=0.55e6" "xland","Black-Med","ixland_1=305,ixland_2=309,jxland_1=151,jxland_2=152,kxland_1=1,kxland_2=6,vxland=0.01e6" "xland","Black-Med","ixland_1=306,ixland_2=309,jxland_1=151,jxland_2=153,kxland_1=1,kxland_2=6,vxland=0.01e6"/ "xland_insert","ocean_mod","xland_insert" "xland","Gibraltar","ixland_1=274,ixland_2=276,jxland_1=146,jxland_2=146,kxland_1=1,kxland_2=18,tauxland=86400.0" "xland","Gibraltar","ixland_1=274,ixland_2=276,jxland_1=147,jxland_2=147,kxland_1=1,kxland_2=18,tauxland=86400.0" "xland","Black-Med","ixland_1=305,ixland_2=309,jxland_1=151,jxland_2=152,kxland_1=1,kxland_2=6,tauxland=86400.0" "xland","Black-Med","ixland_1=306,ixland_2=309,jxland_1=151,jxland_2=153,kxland_1=1,kxland_2=6,tauxland=86400.0"/ "diff_cbt_enhance","ocean_mod","diff_cbt_enhance" "diffcbt","Gibraltar","itable=274,jtable=146,ktable_1=1,ktable_2=18,diff_cbt_table=0.01" "diffcbt","Gibraltar","itable=276,jtable=146,ktable_1=1,ktable_2=18,diff_cbt_table=0.01" "diffcbt","Gibraltar","itable=274,jtable=147,ktable_1=1,ktable_2=18,diff_cbt_table=0.01" "diffcbt","Gibraltar","itable=276,jtable=147,ktable_1=1,ktable_2=18,diff_cbt_table=0.01" "diffcbt","Black-Med","itable=305,jtable=151,ktable_1=1,ktable_2=6,diff_cbt_table=0.01" "diffcbt","Black-Med","itable=309,jtable=152,ktable_1=1,ktable_2=6,diff_cbt_table=0.01" "diffcbt","Black-Med","itable=306,jtable=151,ktable_1=1,ktable_2=6,diff_cbt_table=0.01" "diffcbt","Black-Med","itable=309,jtable=153,ktable_1=1,ktable_2=6,diff_cbt_table=0.01"/ In the first section of the field table, the user can specify tracers to be used in the simulation. Although there is no limit to the number of tracers specified, temperature (temp) and salinity (salt) must be included. The user may also define the horizontal and vertical tracer advection schemes. For more information on the field manager, reference field_manager.html. In climate modeling, it is often necessary to allow water masses that are separated by land to exchange tracer and surface height properties. This situation arises in models when the grid mesh is too coarse to resolve narrow passageways that in reality provide crucial connections between water masses. The cross-land mixing and cross-land insertion establishes communication between bodies of water separated by land. The communication consists of mixing tracers and volume between non-adjacent water columns. Momentum is not mixed. The scheme conserves total tracer content, total volume, and maintains compatibility between the tracer and volume budgets. The grid points where this exchange takes place, and the rates of the exchange, are specified in the field table. For some cases, it is necessary to set a large vertical tracer diffusivity at a specified point in the model, say next to a river mouth to ensure fresh water is mixed vertically. These diffusivities are specified in the field table. For a technical description of cross-land tracer mixing and insertion, please reference A Technical Guide to MOM4.

Running the MOM source code in a parallel processing environment will produce one output NetCDF diagnostic file per processor. mppnccombine joins together an arbitrary number of data files containing chunks of a decomposed domain into a unified NetCDF file. If the user is running the source code on one processor, the domain is not decomposed and there is only one data file. mppnccombine will still copy the full contents of the data file, but this is inefficient and mppnccombine should not be used in this case. Executing mppnccombine is automated through the runscripts. The data files are NetCDF format for now, but IEEE binary may be supported in the future. mppnccombine requires decomposed dimensions in each file to have a domain_decomposition attribute. This attribute contains four integer values: starting value of the entire non-decomposed dimension range (usually 1), ending value of the entire non-decomposed dimension range, starting value of the current chunk's dimension range and ending value of the current chunk's dimension range. mppnccombine also requires that each file have a NumFilesInSet global attribute which contains a single integer value representing the total number of chunks (i.e., files) to combine. The syntax of mppnccombine is: mppnccombine [-v] [-a] [-r] output.nc [input ...] -v print some progress information -a append to an existing NetCDF file -r remove the '.####' decomposed files after a successful\ run An output file must be specified and it is assumed to be the first filename argument. If the output file already exists, then it will not be modified unless the option is chosen to append to it. If no input files are specified, their names will be based on the name of the output file plus the extensions '.0000', '.0001', etc. If input files are specified, they are assumed to be absolute filenames. A value of 0 is returned if execution is completed successfully and a value of 1 indicates otherwise. The source of mppnccombine is packaged with the MOM module in the postprocessing directory. mppnccombine.c should be compiled on the platform where the user intends to run the FMS MOM source code so the runscript can call it. A C compiler and NetCDF library are required for compiling mppnccombine.c: cc -O -o mppnccombine -I/usr/local/include -L/usr/local/lib mppnccombine.c -lnetcdf

Sample MOM model output data files are available at GFDL ftp site. Output files are classified into three subdirectories: ascii: the description of the setup of the run and verbose comments printed out during the run. restart: the model fields necessary to initialize future runs of the model. history: output of the model, both averaged over specified time intervals and snapshots. Note that these output files are compressed using tar. All .tar files should be decompressed for viewing. The decompress command is: tar -xvf filename.tar

There are several graphical packages available to display the model output. These packages vary widely depending on factors, such as the number of dimensions, the amount and complexity of options available and the output data format. The data will first have to be put into a common format that all the packages can read. FMS requires the data to be stored in NetCDF format since it is so widely supported for scientific visualization. The graphical package is also dependent upon the computing environment. For ocean modeling, ncview, Ferret and GrADS are most commonly used.