Difference between revisions of "Tool Box"

Revision as of 10:46, 11 May 2022

Pre-processing Tools

newstart

start2archive

visualization tools

other third party scripts and tools

TO BE COMPLETED

Post-processing tools

zrecast

TO BE COMPLETED

mass stream function

The mass stream function (and the total angular momentum) can be computed from a diagfi.nc or a stats.nc, using the streamfunction.F90 script. The script is located at

trunk/LMDZ.GENERIC/utilities

To compile the script, open the compile file in the same directory and do the following:

• Replace "pgf90" with your favorite fortran compiler
• replace "/distrib/local/netcdf/pgi_7.1-6_32/lib" with the lib address and directory that contains your NetCDF library (file libnetcdf.a).
• Replace "/distrib/local/netcdf/pgi_7.1-6_32/include" with the address of the directory that contains the NetCDF include file (netcdf.inc).
• You can mess with the compiling options but it is not mandatory.

Once the script is compiled, copy it in the same directory as your .nc file and run

./streamfunction.e

The script will ask you for the name of your .nc file, and will run and produce a new nameofyourfile_stream.nc file.

Be careful : In this new file, all fields are temporally and zonally averaged.

If you want to use python instead of fortran, you can take a look at this repo. It hosts a tool to perform dynamical analysis of GCM simulations (and therefore, it computes the mass stream function and a lot of other stuff), but it is tailored for Dynamico only. This repo also takes care of recasting (it does the job of both zrecast.F90 and streamfunction.F90)

Continuing Simulations

manually

At the end of a simulation, the model generates restart files (files 'restart.nc' and 'restartfi.nc') which contain the final state of the model. The 'restart.nc' and 'restartfi.nc' files have the same format as the 'start.nc' and 'startfi.nc' files, respectively.

These files can in fact be used as initial states to continue the simulation, using the following renaming command lines:

mv restart.nc start.nc
mv restartfi.nc startfi.nc

Running a simulation with these start files will in fact resume the simulation from where the previous run ended.

with bash scripts

We have set up very simple bash scripts to automatize the launching of chain simulations. Here is an example of bash script that does the job:

#!/bin/bash
###########################################################################
# Script to perform several chained LMD Mars GCM simulations
# SET HERE the maximum total number of simulations

nummax=100

###########################################################################


echo "---------------------------------------------------------"
echo "STARTING LOOP RUN"
echo "---------------------------------------------------------"

dir=`pwd`
machine=`hostname`
address=`whoami`

# Look for file "num_run" which should contain 
# the value of the previously computed season
# (defaults to 0 if file "num_run" does not exist)
if [[ -r num_run ]] ; then
  echo "found file num_run"
  numold=`cat num_run`
else
  numold=0
fi
echo "numold is set to" ${numold}


# Set value of current season 
(( numnew = ${numold} + 1 ))
echo "numnew is set to" ${numnew}

# Look for initialization data files (exit if none found)
if [[ ( -r start${numold}.nc  &&  -r startfi${numold}.nc ) ]] ; then
   \cp -f start${numold}.nc start.nc
   \cp -f startfi${numold}.nc startfi.nc
else
   if (( ${numold} == 99999 )) ; then
    echo "No run because previous run crashed ! (99999 in num_run)"
    exit
   else
   echo "Where is file start"${numold}".nc??"
   exit
   fi
fi

# Run GCM -- THIS LINE NEEDS TO BE MODIFIED WITH THE CORRECT GCM EXECUTION COMMAND
mpirun -np 8 gcm_64x48x26_phystd_para.e < diagfi.def > lrun${numnew}


# Check if run ended normaly and copy datafiles
if [[ ( -r restartfi.nc  &&  -r restart.nc ) ]] ; then
  echo "Run seems to have ended normaly"


  \mv -f restart.nc start${numnew}.nc
  \mv -f restartfi.nc startfi${numnew}.nc  
    
else
  if [[ -r num_run ]] ; then
    \mv -f num_run num_run.crash
  else
    echo "No file num_run to build num_run.crash from !!"
    # Impose a default value of 0 for num_run
    echo 0 > num_run.crash
  fi
 echo 99999 > num_run
 exit
fi

# Copy other datafiles that may have been generated
if [[ -r diagfi.nc ]] ; then
  \mv -f diagfi.nc diagfi${numnew}.nc
fi
if [[ -r diagsoil.nc ]] ; then
  \mv -f diagsoil.nc diagsoil${numnew}.nc
fi
if [[ -r stats.nc ]] ; then
  \mv -f stats.nc stats${numnew}.nc
fi
if [[ -f profiles.dat ]] ; then
  \mv -f profiles.dat profiles${numnew}.dat
  \mv -f profiles.hdr profiles${numnew}.hdr
fi

# Prepare things for upcoming runs by writing
# value of computed season in file num_run
echo ${numnew} > num_run

# If we are over nummax : stop
if (( $numnew + 1 > $nummax )) ; then
   exit
else
   \cp -f run_gnome exe_mars
   ./exe_mars
fi

Summary of what this bash script does:

• It reads the file 'num_run' which contains the step of the simulation.

If num_run is

5

then the script expects to read start5.nc and startfi5.nc.

• It modifies start5.nc and startfi5.nc into start.nc and startfi.nc, respectively.
• It runs the GCM.
• It modifies restart.nc and restartfi.nc into start6.nc and startfi6.nc
• It rewrite num_run as follows:

6

• It restarts the loop until num_run reaches the value (defined in nummax):

100

Visualization software

Panoply

Panoply is a user-friendly tool for viewing raw NetCDF data, available here: https://www.giss.nasa.gov/tools/panoply/

Screenshot of panoply showing here LMD Generic results for the exoplanet TRAPPIST-1e

Planetoplot

Planetoplot is a in-house, python based library developped to vizualize LMDG data.

The code and documentation can be found at: https://nbviewer.org/github/aymeric-spiga/planetoplot/blob/master/tutorial/planetoplot_tutorial.ipynb

ncview

Command line tool to visualize NetCDF data.

• Installation on Linux:

sudo apt install ncview

• Installation on Mac:

...

paraview

planetoplot

python scripts

The xarray python library is a very good tool to easily load and plot netcdf data.

TBD