Fstpy is a high level interface to rpn's rpnpy python library that produces pandas dataframes from CMC standard files. In order to promote decoupling, modularization and collaboration, fstpy only reads and writes. All other operations and algorithms can be independent.
The idea of using a dataframe is to have a pythonic way of working with standard files without having to know the mechanics of rmnlib. Since many people come here with numpy and pandas knowledge, the learning curve is much less steep.
They are good for organizing information. eg: select all the tt's, sort them by grid then by level and produce 3d matrices for each tt of each grid. Dataframes will help to integrate new model changes and new data types. Thanks to the dataframes we can also export our results more easily to different types of formats.
Dask is the type of array that is used by fstpy to wrap numpy arrays for parallelisation purposes. You can use most of numpy's API directly on these types of arrays. The only difference is that until array.compute() is done, the dask array stores tasks instead of actually doing the computations.
- pandas>=1.2.4
- numpy>=1.19.5
- dask>=2021.8.0
- ci_fstcomp>=1.0.6
- pandas>=1.2.4
- numpy>=1.19.5
- dask>=2021.8.0
- pytest>=5.3.5
- Sphinx>=3.4.3
- sphinx-autodoc-typehints>=1.12.0
- sphinx-gallery>=0.9.0
- sphinx-rtd-theme>=1.0.0
- nbsphinx>=0.8.7
- ipython>=7.12.0
- jupyterlab>=3.1.13
- myst-parser>=0.15.2
This is an ssm package that we use at CMC on the science network and that contains a wide variety of packages
. ssmuse-sh -p /fs/ssm/eccc/cmd/cmds/env/python/py39_2022.09.29_all
Use the ssm package
. ssmuse-sh -d /fs/ssm/eccc/cmd/cmds/fstpy/202206/
Use the git repository package: at your own risk ;)
python3 -m pip install git+http://gitlab.science.gc.ca/CMDS/fstpy.git
# use CMDS Py39
. ssmuse-sh -p /fs/ssm/eccc/cmd/cmds/env/python/py39_2022.09.29_all
# get rmn python library
. r.load.dot eccc/mrd/rpn/MIG/ENV/migdep/5.1.1 eccc/mrd/rpn/MIG/ENV/rpnpy/2.1-u2.4
# get fstpy ssm package
. ssmuse-sh -d /fs/ssm/eccc/cmd/cmds/fstpy/202206/
# inside your script
import fstpy
df = fstpy.StandardFileReader('path to my fst file').to_pandas()
data_path = prefix + '/data/'
import fstpy
# setup your file to read
records=fstpy.StandardFileReader(data_path + 'ttuvre.std').to_pandas()
# display selected records in a rpn voir format
fstpy.voir(records)
# get statistics on the selected records
df = fstpy.fststat(records)
# get a subset of records containing only UU and VV momvar
just_tt_and_uv = records.query('nomvar in ["TT","UV"]')
# display selected records in a rpn voir format
fstpy.voir(just_tt_and_uv)
dest_path = '/tmp/out.std'
# write the selected records to the output file
fstpy.StandardFileWriter(dest_path,just_tt_and_uv).to_fst()
git clone [email protected]:cmds/fstpy.git
# create a new branch
git checkout -b my_change
# modify the code
# commit your changes
# fetch changes
git fetch
# merge recent master
git merge origin/master
# push your changes
git push my_change
Then create a merge request on science's gitlab https://gitlab.science.gc.ca/CMDS/fstpy/merge_requests
# From the $project_root directory of the project
source setup.sh
# Use CMDS Py39
. ssmuse-sh -p /fs/ssm/eccc/cmd/cmds/env/python/py39_2022.09.29_all
# get rmn python library
. r.load.dot eccc/mrd/rpn/MIG/ENV/migdep/5.1.1 eccc/mrd/rpn/MIG/ENV/rpnpy/2.1-u2.4
# From the $project_root/test directory of the project
python -m pytest -vrf
# This will build documentation in docs/build and there you will find index.html
cd doc
make clean
make doc
From $PROJECTROOT
cd ssm
./make_ssm_package.ssh
Great thanks to:
- Phillipe Carphin for inspiring the use of pandas.
- Dominik Jacques for the awsome domUtils project, a great structure of what should be a python project.
- Micheal Neish for the awsome fstd2nc project, great insights on how to develop xarray structure from CMC standard files and great functions to work on fst files. He played a pivotal role in the integration of dask into fstpy.