MITgcm tips: Difference between revisions

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The equation of state is specified by the namelist entry <code>eosType</code> in the <code>PARM01</code> namelist of the <code>data</code> file. To choose the JMD95Z equation of state, you would include the following in your <code>data</code> file
The equation of state is specified by the namelist entry <code>eosType</code> in the <code>PARM01</code> namelist of the <code>data</code> file. To choose the JMD95Z equation of state, you would include the following in your <code>data</code> file


    &PARM01
<syntaxhighlight lang="bash">
    ...
&PARM01
    eosType='JMD95Z',
...
    ....
eosType='JMD95Z',
....
</syntaxhighlight>


=== Using checkpoint files ===
=== Using checkpoint files ===
Line 36: Line 38:
See the example <code>SIZE.h</code> file below. You can copy this file from <code>MITgcm/model/inc/SIZE.h</code>. You will need to comment out the first few lines, and change the values to match your configuration.
See the example <code>SIZE.h</code> file below. You can copy this file from <code>MITgcm/model/inc/SIZE.h</code>. You will need to comment out the first few lines, and change the values to match your configuration.


<syntaxhighlight lang="bash">
     CBOP
     CBOP
     C    !ROUTINE: SIZE.h
     C    !ROUTINE: SIZE.h
Line 99: Line 102:
           PARAMETER ( MAX_OLX = OLx,
           PARAMETER ( MAX_OLX = OLx,
         &            MAX_OLY = OLy )
         &            MAX_OLY = OLy )
 
</syntaxhighlight>
==== Run-time options ====
==== Run-time options ====


The resolution is specified at run time in namelist <code>PARM04</code> in the <code>data</code> file. The grids are specified as <code>(int: number of points) * (float: distance between points)</code> or by specifying a list of distances between neighbouring points. See example namelist below
The resolution is specified at run time in namelist <code>PARM04</code> in the <code>data</code> file. The grids are specified as <code>(int: number of points) * (float: distance between points)</code> or by specifying a list of distances between neighbouring points. See example namelist below


    &PARM04
<syntaxhighlight lang="bash">
    usingCartesianGrid =.TRUE.,
&PARM04
    usingSphericalPolarGrid=.FALSE.,
usingCartesianGrid =.TRUE.,
    delX =400∗12.50,
usingSphericalPolarGrid=.FALSE.,
    delY =400∗12.50,
delX =400∗12.50,
    delR =50∗0.2 ,
delY =400∗12.50,
delR =50∗0.2 ,
</syntaxhighlight>


== Available Packages ==
== Available Packages ==
Line 350: Line 355:
The starting date for the forcing file is specified in the entry <code>[fieldname]startdate1</code> (YYYYMMDD format), and the time is <code>startdate2</code> (hhmmss format).
The starting date for the forcing file is specified in the entry <code>[fieldname]startdate1</code> (YYYYMMDD format), and the time is <code>startdate2</code> (hhmmss format).


    &EXF_NML_01
<syntaxhighlight lang="bash">
    repeatPeriod = 86400.0,
&EXF_NML_01
    &
repeatPeriod = 86400.0,
   
&
    &EXF_NML_02
 
    uwindstartdate1 = 20050401,
&EXF_NML_02
    uwindstartdate2 = 000000,
uwindstartdate1 = 20050401,
    uwindperiod = 3600.0,
uwindstartdate2 = 000000,
    uwindfile = 'u_wind.bin',
uwindperiod = 3600.0,
    &
uwindfile = 'u_wind.bin',
&
</syntaxhighlight>


You will also have to specify the same start dates in the <code>data.cal</code> file,
You will also have to specify the same start dates in the <code>data.cal</code> file,


    &CAL_NML
<syntaxhighlight lang="bash">
    TheCalendar='gregorian',
&CAL_NML
    startDate_1 = 20050401,
TheCalendar='gregorian',
    startDate_2 = 000000,
startDate_1 = 20050401,
    &
startDate_2 = 000000,
&
</syntaxhighlight>
 
== Visualization tools ==
 
Some of the available tools for visualizing MITgcm data are:
 
* The [https://git.uwaterloo.ca/tghill/gcmpy gcmpy] python postprocessing routines exist for making quick animations of model output
* 3D visualization with Visit. See [[Visualization]], [[Visit]], and [[Visit scripting]]

Revision as of 14:42, 16 August 2018

This page is intended to supplement the MITgcm documentation in a way that is more focused on how to use the model, rather than the the inner workings of the model. Recommended parameters and flags are listed, and the EXF and SEAICE packages are described.

The first section is relevant to the core model. It covers choosing an equation of state, using checkpoint files, and specifying the model grid. The following sections cover the EXF, SEAICE, and DIAGNOSTICS packages that supplement the core model.

Maybe the most important section here (at the time of writing) is the SEAICE default settings. There is currently an active pull request to fix the defaults, but there are some strongly recommended settings to use with this package.

Core model parameters and recommendations

Choosing an equation of state

The equation of state relates temperature, density, and salinity of water. The MITgcm has several choices available. The default choice is a linear equation of state. This is generally a poor choice when using SEAICE. Freshwater is most dense at 4 C, so if temperatures are near 4 C the linear equation of state will not represent the true densities. A much better choice is to use a nonlinear equation of state that includes the density maximum. In MITgcm, a good choice is the JMD95Z equation of state. More detail about this EOS is given in the EOS documentation page.

Setting the equation of state

The equation of state is specified by the namelist entry eosType in the PARM01 namelist of the data file. To choose the JMD95Z equation of state, you would include the following in your data file

&PARM01
...
eosType='JMD95Z',
....

Using checkpoint files

At some point you will be running the model, and it will fail. This can happen on Graham if the node fails, the power flicks or goes out, or any number of other reasons. This can cost you a lot of time when you're running big jobs. Therefore, it's best practice to use checkpoint files. MITgcm has built-in rolling and permanent checkpoint files. As the names suggest, rolling checkpoint files save the model current state with one of two file names (pickup.ckptA.data and pickup.ckptB.data), overwriting the oldest of the two to save each new checkpoint file. Permanent checkpoint files are saved with the model iteration number in their name and don't get overwritten. The frequencies are controlled separately by the keywords chkptFreq for rolling checkpoints and pchkptFreq for permanent checkpoint files. These keywords belong in the time namelist PARM03 (with other time-stepping parameters) in the data file.

Specifying a model grid

The size of the model grid needs to be specified at compile time and at run time. Each compiled executable must always be run with the same number of grid points and processors, but can be run for different resolutions on the same grid.

Compile-time options

The model grid is first specified in the SIZE.h file. The full domain (size Nx x Ny) is split into tiles in X and Y. Each tile is split into a number of grid points in X and Y (variables sNx and sNy). A group of tiles (size nSx x nSy) is sent to each processor, and the number of processors in the X and Y directions are specified by nPx and nPy. Therefore, we need Nx = sNx * nSx * nPx and Ny = sNy * nSy * nPy.

Each tile must overlap so each tile sharing the edge agrees on the field values on the edge. The overlap extent is specified by OLx and OLy. The required values depend on the advection scheme and packages used.

See the example SIZE.h file below. You can copy this file from MITgcm/model/inc/SIZE.h. You will need to comment out the first few lines, and change the values to match your configuration.

    CBOP
    C    !ROUTINE: SIZE.h
    C    !INTERFACE:
    C    include SIZE.h
    C    !DESCRIPTION: \bv
    C     *==========================================================*
    C     | SIZE.h Declare size of underlying computational grid.
    C     *==========================================================*
    C     | The design here supports a three-dimensional model grid
    C     | with indices I,J and K. The three-dimensional domain
    C     | is comprised of nPx*nSx blocks (or tiles) of size sNx
    C     | along the first (left-most index) axis, nPy*nSy blocks
    C     | of size sNy along the second axis and one block of size
    C     | Nr along the vertical (third) axis.
    C     | Blocks/tiles have overlap regions of size OLx and OLy
    C     | along the dimensions that are subdivided.
    C     *==========================================================*
    C     \ev
    C
    C     Voodoo numbers controlling data layout:
    C     sNx :: Number of X points in tile.
    C     sNy :: Number of Y points in tile.
    C     OLx :: Tile overlap extent in X.
    C     OLy :: Tile overlap extent in Y.
    C     nSx :: Number of tiles per process in X.
    C     nSy :: Number of tiles per process in Y.
    C     nPx :: Number of processes to use in X.
    C     nPy :: Number of processes to use in Y.
    C     Nx  :: Number of points in X for the full domain.
    C     Ny  :: Number of points in Y for the full domain.
    C     Nr  :: Number of points in vertical direction.
    CEOP
          INTEGER sNx
          INTEGER sNy
          INTEGER OLx
          INTEGER OLy
          INTEGER nSx
          INTEGER nSy
          INTEGER nPx
          INTEGER nPy
          INTEGER Nx
          INTEGER Ny
          INTEGER Nr
          PARAMETER (
         &           sNx =  30,
         &           sNy =  15,
         &           OLx =   2,
         &           OLy =   2,
         &           nSx =   2,
         &           nSy =   4,
         &           nPx =   1,
         &           nPy =   1,
         &           Nx  = sNx*nSx*nPx,
         &           Ny  = sNy*nSy*nPy,
         &           Nr  =   4)
    
    C     MAX_OLX :: Set to the maximum overlap region size of any array
    C     MAX_OLY    that will be exchanged. Controls the sizing of exch
    C                routine buffers.
          INTEGER MAX_OLX
          INTEGER MAX_OLY
          PARAMETER ( MAX_OLX = OLx,
         &            MAX_OLY = OLy )

Run-time options

The resolution is specified at run time in namelist PARM04 in the data file. The grids are specified as (int: number of points) * (float: distance between points) or by specifying a list of distances between neighbouring points. See example namelist below

&PARM04
usingCartesianGrid =.TRUE.,
usingSphericalPolarGrid=.FALSE.,
delX =400∗12.50,
delY =400∗12.50,
delR =50∗0.2 ,

Available Packages

The sections discusses the diagnostics, seaice, and exf packages. All packages required some compile time and some run time options. At minimum, packages must be enabled at compile time by adding the package name to the packages.conf file. At run time, the package must be enabled in data.pkg

   packages.conf:
   
   oceanic
   diagnostics
   exf
   cal
   seaice
   data.pkg:
   
   &PACKAGES
   useEXF        =.TRUE.,
   useCAL        =.TRUE.,
   useSEAICE.    =.TRUE.,
   useDIAGNOSTICS=.TRUE.,
   &

DIAGNOSTICS

The diagnostics package exists to make it easier to control the output files generated by the model. It makes it easy to choose which output fields are written and how frequently output files are generated.

Compile time options

At compile time you should have the file DIAGNOSTICS_SIZE.h. This can be copied from the package code pkg/diagnostics/DIAGNOSTICS_SIZE.h. The following is an example:

   C     Diagnostics Array Dimension
   C     ---------------------------
   C     ndiagMax   :: maximum total number of available diagnostics
   C     numlists   :: maximum number of diagnostics list (in data.diagnostics)
   C     numperlist :: maximum number of active diagnostics per list (data.diagnostics)
   C     numLevels  :: maximum number of levels to write    (data.diagnostics)
   C     numdiags   :: maximum size of the storage array for active 2D/3D diagnostics
   C     nRegions   :: maximum number of regions (statistics-diagnostics)
   C     sizRegMsk  :: maximum size of the regional-mask (statistics-diagnostics)
   C     nStats     :: maximum number of statistics (e.g.: aver,min,max ...)
   C     diagSt_size:: maximum size of the storage array for statistics-diagnostics
   C Note : may need to increase "numdiags" when using several 2D/3D diagnostics,
   C  and "diagSt_size" (statistics-diags) since values here are deliberately small.
         INTEGER    ndiagMax
         INTEGER    numlists, numperlist, numLevels
         INTEGER    numdiags
         INTEGER    nRegions, sizRegMsk, nStats
         INTEGER    diagSt_size
         PARAMETER( ndiagMax = 500 )
         PARAMETER( numlists = 10, numperlist = 50, numLevels=2*Nr )
         PARAMETER( numdiags = 10*Nr )
         PARAMETER( nRegions = 0 , sizRegMsk = 1 , nStats = 4 )
         PARAMETER( diagSt_size = 10*Nr )
   
   
   CEH3 ;;; Local Variables: ***
   CEH3 ;;; mode:fortran ***
   CEH3 ;;; End: ***

In this example, you can only output up to 10 diagnostics. By increasing the maximum sizes to numlists = 25 and numdiags = 25*Nr you could output up to 25 diagnostics.

Run time options

The diagnostics and frequency are specified in the file data.diagnostics. Specify the field names in the field and filename lines, and set the frequency. The file needs to have namelists &DIAGNOSTICS_LIST (for writing en entire field to file) and DIAG_STATISPARMS (for writing per-level statistics), even if one of them is empty. Example:

   # Diagnostic Package Choices
   #-----------------
   # for each output-stream:
   #  filename(n) : prefix of the output file name (only 8.c long) for outp.stream n
   #  frequency(n):< 0 : write snap-shot output every |frequency| seconds
   #               > 0 : write time-average output every frequency seconds
   #  timePhase(n)     : write at time = timePhase + multiple of |frequency|
   #  averagingFreq(n) : frequency (in s) for periodic averaging interval
   #  averagingPhase(n): phase     (in s) for periodic averaging interval
   #  repeatCycle(n)   : number of averaging intervals in 1 cycle
   #  levels(:,n) : list of levels to write to file (Notes: declared as REAL)
   #                 when this entry is missing, select all common levels of this list
   #  fields(:,n) : list of diagnostics fields (8.c) (see "available_diagnostics.log"
   #                 file for the list of all available diag. in this particular config)
   #−−−−−−−−−−−−−−−−−
   &DIAGNOSTICS_LIST
   # diag_mnc = .FALSE. ,
   # dumpAtLast = .TRUE. ,
   #==============================
   frequency(1) = −3600.0 ,
   timePhase(1) =0,
   fields(1, 1) = ’THETA’ ,
   filename( 1) =’T’,
   #−−−−−−−−−−−−−−−−−
   frequency(2) = −3600.0,
   timePhase(2) = 0 ,
   fields(1, 2) = ’UVEL’,
   filename( 2) = ’U’,
   #−−−−−−−−−−−−−−−−− 
   # ...
   &
   
   &DIAG_STATIS_PARMS
   &
         

In this example, only the temperature and U velocity will be written to file. Their instantaneous value is written to file once per hour of model time. We could add more diagnostics by continuing the namelist in the same way.

All available diagnostics are written to the file available_diagnostics.log when the model runs.

SEAICE

The SEAICE package includes physical parameterizations for ice dynamics and simple thermodynamics. The dynamical model is described in the documentation.

Compile time options

The SEAICE packages requires the files SEAICE_OPTIONS.h and SEAICE_SIZE.h to be present at compile time. You can copy the files from the SEAICE tutorial or the package code pkg/seaice/SEAICE_OPTIONS.h and modify as desired.

Run time options

Run time options are specified in the file data.seaice. The SEAICE package defaults are some questionable. See this GitHub issue and corresponding Pull Request. In short, you should at minimum have the following in your data.seaice file

   # SEAICE parameters
   
   &SEAICE_PARM01
   SEAICEuseDYNAMICS      =.TRUE.,
   SEAICEscaleSurfStress  =.TRUE.,
   SEAICE_useMultiDimSnow = .TRUE.,
   SEAICEetaZmethod       = 3
   SEAICE_drag            = 0.001,
   SEAICEadvHEFF          = .TRUE.,
   SEAICEadvAREA          = .TRUE.,
   
   # Always use either 33 or 77
   SEAICEadvScheme        = 33,
   
   # These help thin ice behave better
   SEAICE_area_reg        = 1.0E-5,
   SEAICE_hice_reg        = 1.0E-5,
   &
   
   &SEAICEPARM03
   &

EXF

The external forcing (EXF) package allows the model to be forced with real (or simulated) observations of meteorological data. This package has temporal interpolation abilities which will be convenient when working with real observations.

Compile time options

The compile time options are specified in file EXF_OPTIONS.h. This file can be copied from the EXF package code pkg/exf/EXF_OPTIONS.h. Some CPP options are also required in CPP_OPTIONS.h (see table below).

The package has 6 different combinations of forcing fields that can be specified to force the model. The headers relate to CPP options:

ALLOW_ATM_TEMP TEMP
ALLOW_DOWNWARD_RADIATION DOWN
ALLOW_BULKFORMULAE BULK
EXF_READ_EVAP EVAP
ALLOW_READ_TURBFLUXES TURB


Possible EXF forcing combinations
# Temp DOWN BULK EVAP TURB Actions
(1) - - - - - Read in hflux, swflux, and sflux
(2) - def - - - Read in hflux, swdown, and sflux. Compute swflux.
(3) def def def - - Read in atemp, aqh, swdown, lwdown, precip, and runoff. Compute hflux, swflux, and sflux.
(4) def - def - - Read in atemp, aqh, swflux, lwflux, precip, and runoff. Compute hflux and sflux.
(5) def def - def def Read in hs, hl, swdown, lwdown, evap, precip, and runoff. Compute flux, swflux, and flux.
(6) def - - def def Read in hs, hl, swflux, lwflux, evap, precip, and runoff. Compute hflux and flux.

Configurations (3)-(6) are compatible with SEAICE. I have usually run with configuration (3).


Run time options

The run time options are specified in file data.exf. Forcing files are specified in EXF_NML_02 with the keywords [fieldname]file.

This package is intended to handle time-dependent forcing. You must specify the time between consecutive entries in the forcing files, as well as a global repeat time for the period of the forcing.

The time between consecutive entries is specified for each field as [fieldname]period (EXF_NML_02), and the global repeat period is repeatPeriod (EXF_NML_01). The snippet below is part of the data.exf file for forcing that repeats daily, with 1 hour increments in the forcing fields.

The starting date for the forcing file is specified in the entry [fieldname]startdate1 (YYYYMMDD format), and the time is startdate2 (hhmmss format).

&EXF_NML_01
repeatPeriod = 86400.0,
&

&EXF_NML_02
uwindstartdate1 = 20050401,
uwindstartdate2 = 000000,
uwindperiod = 3600.0,
uwindfile = 'u_wind.bin',
&

You will also have to specify the same start dates in the data.cal file,

&CAL_NML
TheCalendar='gregorian',
startDate_1 = 20050401,
startDate_2 = 000000,
&

Visualization tools

Some of the available tools for visualizing MITgcm data are: