SCOPE Documentation

SCOPE: A Script Based Coupler for Simulations of the Earth System

https://img.shields.io/pypi/v/scope-coupler.svg Documentation Status

scope is a offline, script-based coupler for various simulations of the Earth System. It is written in Python and configured with YAML files.

Features

  • TODO

Credits

This package was created with Cookiecutter and the audreyr/cookiecutter-pypackage project template.

Installation

Stable release

To install scope, run this command in your terminal:

$ pip install scope-coupler

This is the preferred method to install scope, as it will always install the most recent stable release.

Warning

Since scope is still under active development, there is no “stable release” yet.

If you don’t have pip installed, this Python installation guide can guide you through the process.

From sources

The sources for scope can be downloaded from AWI’s Gitlab repo.

You can either clone the public repository:

$ git clone git://gitlab.awi.de/pgierz/scope

Or download the tarball:

$ curl  -OL https://gitlab.awi.de/pgierz/scope/tarball/master

Once you have a copy of the source, you can install it with:

$ python setup.py install

Usage

An example configuration file is provided under examples/scope_config.yaml:

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template_replacements:
    EXP_ID: "PI_1x10"
    DATE_PATTERN: "[0-9]{6}"

scope:
    couple_dir: "/work/ollie/pgierz/scope_tests/couple/"
    number openMP processes: 8

echam:
    type: atmosphere
    griddes: T63
    outdata_dir: "/work/ollie/pgierz/scope_tests/outdata/echam/"
    code table: "echam6"
    pre_preprocess:
        program: "echo \"hello from pre_preprocess. Do you know: $(( 7 * 6 )) is the answer!\""
    send:
        ice:
            temp2:
                files:
                    pattern: "{{ EXP_ID }}_echam6_echam_{{ DATE_PATTERN }}.grb"
                    take:
                        newest: 12
                code table: "echam6"
            aprl:
                files:
                    dir: "/work/ollie/pgierz/scope_tests/outdata/echam/"
                    pattern: "{{ EXP_ID }}_echam6_echam_{{ DATE_PATTERN }}.grb"
                    take:
                        newest: 12
                code table: "/work/ollie/pgierz/scope_tests/outdata/echam/PI_1x10_185001.01_echam.codes"
            aprc:
                files:
                    dir: "/work/ollie/pgierz/scope_tests/outdata/echam/"
                    pattern: "{{ EXP_ID }}_echam6_echam_{{ DATE_PATTERN }}.grb"
                    take:
                        newest: 12

pism:
    type: ice
    griddes: ice.griddes
    recieve:
        atmosphere:
            temp2:
                interp: bil
                transformation:
                    - expr: "air_temp=temp2-273.15"
        ocean:
    send:
        atmosphere:
        ocean:

To use scope in a project:

import scope

scope

scope package

Submodules

scope.cli module

Console script for scope.

scope.cli.yaml_file_to_dict(filepath)[source]

Given a yaml file, returns a corresponding dictionary.

If you do not give an extension, tries again after appending one.

Parameters:filepath (str) – Where to get the YAML file from
Returns:A dictionary representation of the yaml file.
Return type:dict

scope.models module

Not sure what to do with this stuff yet…

class scope.models.Component[source]

Bases: scope.models.SimObj

NAME = 'Generic Component Object'
class scope.models.Model[source]

Bases: scope.models.SimObj

NAME = 'Generic Model Object'
class scope.models.SimObj[source]

Bases: object

after_run()[source]
before_recieve()[source]
before_send()[source]
recieve()[source]
send()[source]
NAME = 'Generic Sim Object'

scope.scope module

Here, the scope library is described. This allows you to use specific parts of scope from other programs.

scope consists of several main classes. Note that most of them provide Python access to cdo calls via Python’s built-in subprocess module. Without a correctly installed cdo, many of these functions/classes will not work.

Here, we provide a quick summary, but please look at the documentation for each function and class for more complete information. The following functions are defined:

  • determine_cdo_openMP – using cdo --version, determines if you have openMP support.

The following classes are defined here:

  • Scope – an abstract base class useful for starting other classes from. This provides a way to determine if cdo has openMP support or not by parsing cdo --version. Additionally, it has a nested class which gives you decorators to put around methods for enabling arbitrary shell calls before and after the method is executed, which can be configured via the Scope.config dictionary.
  • Preprocess – a class to extract and combine various NetCDF files for further processing.
  • Regrid – a class to easily regrid from one model to another, depending on the specifications in the scope_config.yaml
class scope.scope.Preprocess(config, whos_turn)[source]

Bases: scope.scope.Scope

Subclass of Scope which enables preprocessing of models via cdo. Use the preprocess method after building a Precprocess object.

Base class for various Scope objects. Other classes should extend this one.

Parameters:
  • config (dict) – A dictionary (normally recieved from a YAML file) describing the scope configuration. An example dictionary is included in the root directory under examples/scope_config.yaml
  • whos_turn (str) – An explicit model name telling you which model is currently interfacing with scope e.g. echam or pism.

Warning

This function has a filesystem side-effect: it generates the couple folder defined in config["scope"]["couple_dir"]. If you don’t have permissions to create this folder, the object initialization will fail…

Some design features are listed below:

  • ``pre`` and ``post`` hooks

Any appropriately decorated method of a scope object has a hook to call a script with specific arguments and flags before and after the main scope method call. Best explained by an example. Assume your Scope subclass has a method “preprocess”. Here is the order the program will execute in, given the following configuration:

pre_preprocess:
    program: /some/path/to/an/executable
    args:
        - list
        - of
        - arguments
    flags:
        - "--flag value1"
        - "--different_flag value2"

post_preprocess:
    program: /some/other/path
    args:
        - A
        - B
        - C
    flags:
        - "--different_flag value3"

Given this configuration, an idealized system call would look like the example shown below. Note however that the Python program calls the shell and immediately destroys it again, so any variables exported to the environment (probably) don’t survive:

$ ./pre_preprocess['program'] list of arguments --flag value1 --different_flag value2
$ <... python call to preprocess method ...>
$ ./post_preprocess['program'] A B C --different_flag value 3
_all_senders()[source]

A generator giving tuples of the reciever_type (e.g. ice, atmosphere, ocean, solid earth), and the configuration for the reciever type, including variables and corresponding specifications for which files to use and how to process them.

Example

Here is an example for the reciever specification dictionary. See the documentation regarding scope configuration for further information:

temp2:
    files:
        pattern: "{{ EXP_ID }}_echam6_echam_{{ DATE_PATTERN }}.grb"
        take:
            newest: 12
    code table: "echam6"
aprl:
    files:
        dir: "/work/ollie/pgierz/scope_tests/outdata/echam/"
        pattern: "{{ EXP_ID }}_echam6_echam_{{ DATE_PATTERN }}.grb"
        take:
            newest: 12
    code table: "/work/ollie/pgierz/scope_tests/outdata/echam/PI_1x10_185001.01_echam.codes"
Yields:

tuple of (str, dict) – The first element of the tuple, reciever_type, is a string describing what sort of model should get this data; e.g. “ice”, “atmosphere”

The second element, reciever_spec, is a dictionary describing which files should be used.

_combine_tmp_variable_files(reciever_type)[source]

Combines all files in the couple directory for a particular reciever type.

Depending on the configuration, this method combines all files found in the couple_dir which may have been further processed by scope to a file <sender_type>_file_for_<reciever_type>.nc

Parameters:reciever_type (str) – Which reciever the model is sending to, e.g. ice, ocean, atmosphere
Returns:
Return type:None

Notes

This executes a cdo mergetime command to concatenate all files found which should be sent to particular model.

_construct_filelist(var_dict)[source]

Example

The variable configuration dictionary can have the following top-level keys:

  • files may contain:
    • a filepattern in regex to look for
    • take which files to take, either specific, or newest/latest followed by an integer.
    • dir a directory where to look for the files. Note that if this is not provided, the default is to fall back to the top level outdata_dir for the currently sending model.
_make_tmp_files_for_variable(varname, var_dict)[source]

Generates temporary files for further processing with scope.

Given a variable name and a description dictionary of how it should be extracted and processed, this method makes a temporary file, <sender_name>_<varname>_file_for_scope.nc, e.g. echam_temp2_file_for_scope.nc in the couple_dir.

Parameters:
  • varname (str) – Variable name as that should be selected from the files
  • var_dict (dict) – A configuration dictionary describing how the variable should be extracted. An example is given in _construct_filelist.

Notes

In addition to the dictionary description of files, further information may be added with the following top-level keys:

  • code table describing which GRIB code numbers correspond to which variables. If not given, the fallback value is the value of code table in the sender configuration.

Converts any input file to nc via cdo. Runs both select and settable.

Returns:
Return type:None
preprocess()[source]
class scope.scope.Regrid(config, whos_turn)[source]

Bases: scope.scope.Scope

Base class for various Scope objects. Other classes should extend this one.

Parameters:
  • config (dict) – A dictionary (normally recieved from a YAML file) describing the scope configuration. An example dictionary is included in the root directory under examples/scope_config.yaml
  • whos_turn (str) – An explicit model name telling you which model is currently interfacing with scope e.g. echam or pism.

Warning

This function has a filesystem side-effect: it generates the couple folder defined in config["scope"]["couple_dir"]. If you don’t have permissions to create this folder, the object initialization will fail…

Some design features are listed below:

  • ``pre`` and ``post`` hooks

Any appropriately decorated method of a scope object has a hook to call a script with specific arguments and flags before and after the main scope method call. Best explained by an example. Assume your Scope subclass has a method “preprocess”. Here is the order the program will execute in, given the following configuration:

pre_preprocess:
    program: /some/path/to/an/executable
    args:
        - list
        - of
        - arguments
    flags:
        - "--flag value1"
        - "--different_flag value2"

post_preprocess:
    program: /some/other/path
    args:
        - A
        - B
        - C
    flags:
        - "--different_flag value3"

Given this configuration, an idealized system call would look like the example shown below. Note however that the Python program calls the shell and immediately destroys it again, so any variables exported to the environment (probably) don’t survive:

$ ./pre_preprocess['program'] list of arguments --flag value1 --different_flag value2
$ <... python call to preprocess method ...>
$ ./post_preprocess['program'] A B C --different_flag value 3
_calculate_weights(Model, Type, Interp)[source]
regrid()[source]
regrid_one_var(Model, Type, Interp, Variable)[source]
class scope.scope.Scope(config, whos_turn)[source]

Bases: object

Base class for various Scope objects. Other classes should extend this one.

Parameters:
  • config (dict) – A dictionary (normally recieved from a YAML file) describing the scope configuration. An example dictionary is included in the root directory under examples/scope_config.yaml
  • whos_turn (str) – An explicit model name telling you which model is currently interfacing with scope e.g. echam or pism.

Warning

This function has a filesystem side-effect: it generates the couple folder defined in config["scope"]["couple_dir"]. If you don’t have permissions to create this folder, the object initialization will fail…

Some design features are listed below:

  • ``pre`` and ``post`` hooks

Any appropriately decorated method of a scope object has a hook to call a script with specific arguments and flags before and after the main scope method call. Best explained by an example. Assume your Scope subclass has a method “preprocess”. Here is the order the program will execute in, given the following configuration:

pre_preprocess:
    program: /some/path/to/an/executable
    args:
        - list
        - of
        - arguments
    flags:
        - "--flag value1"
        - "--different_flag value2"

post_preprocess:
    program: /some/other/path
    args:
        - A
        - B
        - C
    flags:
        - "--different_flag value3"

Given this configuration, an idealized system call would look like the example shown below. Note however that the Python program calls the shell and immediately destroys it again, so any variables exported to the environment (probably) don’t survive:

$ ./pre_preprocess['program'] list of arguments --flag value1 --different_flag value2
$ <... python call to preprocess method ...>
$ ./post_preprocess['program'] A B C --different_flag value 3
class ScopeDecorators[source]

Bases: object

Contains decorators you can use on class methods

static _wrap_hook(self, meth)[source]
classmethod post_hook(meth)[source]
classmethod pre_hook(meth)[source]

Based upon the self.config, runs a specific system command

Using the method name, you can define

get_cdo_prefix(has_openMP=None)[source]

Return a string with an appropriate cdo prefix for using OpenMP with the -P flag.

Parameters:has_openMP (bool) – Default is None. You can explicitly override the ability of cdo to use the -P flag. If set to True, the config must have an entry under config[scope][number openMP processes] defining how many openMP processes to use (should be an int)
Returns:A string which should be used for the cdo call, either with or without -P X, where X is the number of openMP processes to use.
Return type:str
scope.scope.determine_cdo_openMP()[source]

Checks if the cdo version being used supports OpenMP; useful to check if you need a -P flag or not.

Parameters:None
Returns:True if OpenMP is listed in the Features of cdo, otherwise False
Return type:bool

Module contents

Top-level package for SCOPE.

Contributing

Contributions are welcome, and they are greatly appreciated! Every little bit helps, and credit will always be given.

You can contribute in many ways:

Types of Contributions

Report Bugs

Report bugs at https://github.com/pgierz/scope/issues.

If you are reporting a bug, please include:

  • Your operating system name and version.
  • Any details about your local setup that might be helpful in troubleshooting.
  • Detailed steps to reproduce the bug.

Fix Bugs

Look through the GitHub issues for bugs. Anything tagged with “bug” and “help wanted” is open to whoever wants to implement it.

Implement Features

Look through the GitHub issues for features. Anything tagged with “enhancement” and “help wanted” is open to whoever wants to implement it.

Write Documentation

SCOPE: A Script Based Coupler for Simulations of the Earth System could always use more documentation, whether as part of the official SCOPE: A Script Based Coupler for Simulations of the Earth System docs, in docstrings, or even on the web in blog posts, articles, and such.

Submit Feedback

The best way to send feedback is to file an issue at https://github.com/pgierz/scope/issues.

If you are proposing a feature:

  • Explain in detail how it would work.
  • Keep the scope as narrow as possible, to make it easier to implement.
  • Remember that this is a volunteer-driven project, and that contributions are welcome :)

Get Started!

Ready to contribute? Here’s how to set up scope for local development.

  1. Fork the scope repo on GitHub.

  2. Clone your fork locally:

    $ git clone git@github.com:your_name_here/scope.git
    
  3. Install your local copy into a virtualenv. Assuming you have virtualenvwrapper installed, this is how you set up your fork for local development:

    $ mkvirtualenv scope
    $ cd scope/
    $ python setup.py develop
    
  4. Create a branch for local development:

    $ git checkout -b name-of-your-bugfix-or-feature
    

    Now you can make your changes locally.

  5. When you’re done making changes, check that your changes pass flake8 and the tests, including testing other Python versions with tox:

    $ flake8 scope tests
    $ python setup.py test or py.test
    $ tox
    

    To get flake8 and tox, just pip install them into your virtualenv.

  6. Commit your changes and push your branch to GitHub:

    $ git add .
    $ git commit -m "Your detailed description of your changes."
    $ git push origin name-of-your-bugfix-or-feature
    
  7. Submit a pull request through the GitHub website.

Pull Request Guidelines

Before you submit a pull request, check that it meets these guidelines:

  1. The pull request should include tests.
  2. If the pull request adds functionality, the docs should be updated. Put your new functionality into a function with a docstring, and add the feature to the list in README.rst.
  3. The pull request should work for Python 2.7, 3.4, 3.5 and 3.6, and for PyPy. Check https://travis-ci.org/pgierz/scope/pull_requests and make sure that the tests pass for all supported Python versions.

Tips

To run a subset of tests:

$ python -m unittest tests.test_scope

Deploying

A reminder for the maintainers on how to deploy. Make sure all your changes are committed (including an entry in HISTORY.rst). Then run:

$ bumpversion patch # possible: major / minor / patch
$ git push
$ git push --tags

Travis will then deploy to PyPI if tests pass.

Credits

History

0.1.3 (2019-12-4)

  • Automatically builds documentation from docstrings
  • Most of scope send works

0.1.0 (2019-11-13)

  • First release on PyPI.

Indices and tables