# Coding Guide

## Introduction

This guide describes common conventions, guidelines, and strategies for contributing code to PlasmaPy. The purpose of this guide is not to provide a set of rigid guidelines that must be adhered to, but rather to provide a common framework that helps us develop PlasmaPy together as a community.

Having a shared coding style makes it easier to understand code written by multiple contributors. The particulars of the coding style are not as important as consistency, readability, and maintainability.

This guide can (and should!) be regularly refined by the PlasmaPy community as we collectively learn new practices and our shared coding style changes. Please feel free to propose revisions to this guide by submitting a pull request or by bringing up an idea at a community meeting.

PlasmaPy generally follows the PEP 8 style guide for Python code, using auto-formatters such as black and isort that are executed using pre-commit.

## Coding guidelines

• Write short functions that do exactly one thing with no side effects.

• Use NumPy array options instead of for loops to make code more compact, readable, and performant.

• Instead of defining variables like a0, a1, & a2, define these values in a collection such as an ndarray or a list.

• Use the property decorator instead of getters and setters.

• Some plasma parameters depend on more than one Quantity of the same physical type. For example, when reading the following line of code, we cannot immediately tell which is the electron temperature and which is the ion temperature.

f(1e6 * u.K, 2e6 * u.K)


Spell out the parameter names to improve readability and reduce the likelihood of errors.

f(T_i=1e6 * u.K, T_e=2e6 * u.K)


Similarly, when a function has parameters named T_e and T_i, these parameters should be made keyword-only to avoid ambiguity and reduce the chance of errors.

def f(*, T_i, T_e):
...

• The __eq__ and __ne__ methods of a class should not raise exceptions. If the comparison for equality is being made between objects of different types, these methods should return False instead. This behavior is for consistency with operations like 1 == "1" which will return False.

• Limit usage of lambda functions to one-liners, such as when defining the default factory of a defaultdict). For anything longer than one line, use def instead.

• List and dictionary comprehensions can be used for simple for loops, like:

>>> [x**2 for x in range(17) if x % 2 == 0]
[0, 4, 16, 36, 64, 100, 144, 196, 256]

• Avoid putting any significant implementation code in __init__.py files. Implementation details should be contained in a different file, and then imported into __init__.py.

• Avoid defining global variables when possible.

• Use assert statements only in tests.

• Use formatted string literals (f-strings) instead of legacy formatting for strings.

>>> package_name = "PlasmaPy"
>>> print(f"The name of the package is {package_name}.")
The name of the package is PlasmaPy.
>>> print(f"{package_name=}")
package_name='PlasmaPy'
>>> print(f"{package_name!r}")  # shortcut for f"{repr(package_name)}"
'PlasmaPy'

• Functions that accept array_like or Quantity inputs should accept and return nan (not a number) values. This guideline applies when nan is the input as well as when nan values are included in an array.

Tip

Normally, numpy.nan == numpy.nan evaluates to False, which complicates testing nan behavior. The equal_nan keyword of functions like numpy.allclose and numpy.testing.assert_allclose makes it so that nan is considered equal to itself.

• Do not use mutable objects as default values in the function or method declaration. This can lead to unexpected behavior.

>>> def function(l=[]):
...     l.append("x")
...     print(l)
...
>>> function()
['x']
>>> function()
['x', 'x']

• Use pathlib when working with paths to data files.

### Names

Names are our most fundamental means of communicating the intent and purpose of code. Wisely chosen names can greatly improve the understandability of code, while inadequate names can obfuscate what the code is supposed to be doing.

• PlasmaPy generally uses the PEP 8 conventions for variable names.

• Use lowercase words separated by underscores for function and variable names (e.g., function_name and variable_name).

• Use capitalized words without separators when naming a class (e.g., ClassName), but keep acronyms capitalized (e.g., MHDEquations).

• Use capital letters words separated by underscores when naming constants (e.g., CONSTANT or CONSTANT_NAME).

There are some situations in PlasmaPy which justify a departure from the PEP 8 conventions.

• Functions based on plasma parameters that are named after people may be capitalized (e.g., Alfven_speed).

• Capital letters may be used for a variable when it matches the standard usage in plasma science (e.g., B for magnetic field and T for temperature).

• Choose names that are pronounceable to make them more memorable and compatible with text-to-speech technology.

• Choose names will produce more relevant results when searching the internet.

• Avoid unnecessary abbreviations, as these make code harder to read. Prefer clarity over brevity, except for code that is used frequently and interactively (e.g., cd or ls).

Tip

Measure the length of a variable not by the number of characters, but rather by the time needed to understand its meaning.

By this measure, cggglm is significantly longer than solve_gauss_markov_linear_model.

• Avoid ambiguity. Does temp mean “temperature”, “temporary”, or “template”?

• Append _e to a variable name to indicate that it refers to electrons, _i for ions, and _p for protons (e.g., T_e, T_i, and T_p).

• Only ASCII characters should be used in code that is part of the public API.

• Python allows alphanumeric Unicode characters to be used in object names (e.g., πλάσμα or φυσική). These characters may be used for internal code when doing so improves readability (i.e., to match a commonly used symbol) and in Jupyter notebooks.

• If a plasma parameter has multiple names, then use the name that provides the most physical insight. For example, gyrofrequency indicates gyration but Larmor_frequency does not.

• It is usually preferable to name a variable after its name rather than its symbol. An object named Debye_length is more broadly understandable and searchable than lambda_D. However, there are some exceptions to this guideline.

• Symbols used widely across plasma science can be used with low risk of confusion, such as $$T$$ for temperature or $$β$$ for plasma beta.

• Symbols that are defined in docstrings can be used with decreased likelihood of confusion.

• Sometimes code that represents an equation will be more readable if the Unicode characters for the symbols are used, especially for complex equations. For someone who is familiar with the symbols, λ = c / ν will be more readable than lambda = c / nu or wavelength = speed_of_light / frequency.

• If an implementation is based on a journal article, then variable names may be based on the symbols used in that article. The article should be cited in the appropriate docstring so that it appears in the Bibliography.

• To mark that an object is not part of PlasmaPy’s public API, begin its name with a leading underscore (e.g., _private_variable). Private variables should not be included in __all__.

• Avoid single character variable names except for standard plasma physics symbols (e.g., B) or as indices in for loops.

• Avoid encoding type information in a variable name.

• Intermediate variable names can provide additional context and meaning. For example, suppose we have a conditional operating on a complicated expression:

if u[0] < x < u[1] and v[0] < y < v[1] and w[0] < z < w[1]:
...


Defining an intermediate variable allows us to communicate the meaning and intent of the expression.

point_is_in_grid_cell = u[0] < x < u[1] and v[0] < y < v[1] and w[0] < z < w[1]

if point_is_in_grid_cell:
...


In for loops, this may take the form of assignment expressions with the walrus operator (:=).

Tip

It is common for an integrated development environment (IDE) to have a built-in tool for simultaneously renaming a variable throughout a project. For example, a rename refactoring in PyCharm can be done with Shift+F6 on Windows or Linux, and ⇧F6 or ⌥⌘R on macOS.

A well-placed and well-written comment can prevent future frustrations. However, comments are not inherently good. As code evolves, an unmaintained comment may become outdated, or get separated from the section of code that it was meant to describe. Cryptic and obsolete comments may end up confusing contributors. In the worst case, an unmaintained comment may contain inaccurate or misleading information (hence the saying that “a comment is a lie waiting to happen”).

Important

The code we write should read like a book. The full meaning of code’s functionality should be attainable by reading the code. Comments should only be used when the code itself cannot communicate its full meaning.

• Refactor code to make it more readable, rather than explaining how it works .

• Instead of using a comment to define a variable, rename the variable to encode its meaning and intent. For example, code like:

# collision frequency
nu = 1e6 * u.s**-1


could be achieved with no comment by doing:

collision_frequency = 1e6 * u.s**-1

• Use comments to communicate information that you wish you knew before starting to work on a particular section of code, including information that took some time to learn.

• Use comments to communicate information that the code cannot, such as why an alternative approach was not taken.

• Use comments to include references to books or articles that describe the equation, algorithm, or software design pattern that is being implemented. Even better, include these references in docstrings.

• Provide enough contextual information in the comment for a new user to be able to understand it.

• Remove commented out code before merging a pull request.

• When updating code, be sure to review and update, if necessary, associated comments too!

• When a comment is used as the header for a section of code, consider extracting that section of code into its own function. For example, we might start out with a function that includes multiple lines of code for each step.

def analyze_experiment(data):
# Step 1: calibrate the data
...
# Step 2: normalize the data
...


We can apply the extract function refactoring pattern by creating a separate function for each of these steps. The name of each function can often be extracted directly from the comment.

def calibrate_data(data):
...
return calibrated_data

def normalize_data(data):
...
return normalized_data

def analyze_experiment(data):
calibrated_data = calibrate_data(data)
normalized_data = normalize_data(calibrated_data)


This refactoring pattern is appropriate for long functions where the different steps can be cleanly separated from each other. This pattern leads to functions that are shorter, more reusable, and easier to test. The original function contains fewer low-level implementation details and thus gives a higher level view of what the function is doing. This pattern reduces cognitive complexity.

The extract function refactoring pattern should be used judiciously, as taking it to an extreme and applying it at too fine of a scale can reduce readability and maintainability by producing overly fragmented code.

Hint

The extract function refactoring pattern might not be appropriate if the different sections of code are intertwined with each other (e.g., if both sections require the same intermediate variables). An alternative in such cases would be to create a class instead.

### Error messages

Error messages are a vital but underappreciated form of documentation. A good error message can help someone pinpoint the source of a problem in seconds, while a cryptic or missing error message can lead to hours of frustration.

• Use error messages to indicate the source of the problem while providing enough information for the user to troubleshoot it. When possible, make it clear what the user should do next.

• Include diagnostic information when appropriate. For example, if an error occurred at a single index in an array operation, then including the index where the error happened can help the user better understand the cause of the error.

• Write error messages that are concise when possible, as users often skim or skip long error messages.

• Avoid including information that is irrelevant to the source of the problem.

• Write error messages in language that is plain enough to be understandable to someone who is undertaking their first research project.

• If necessary, technical information may be placed after a plain language summary statement.

• Alternatively, an error message may reference a docstring or a page in the narrative documentation.

• Write error messages that are friendly, supportive, and helpful. Error message should never be condescending or blame the user.

## Project infrastructure

### Imports

• Use standard abbreviations for imported packages:

import astropy.constants as const
import astropy.units as u
import matplotlib.pyplot as plt
import numpy as np
import pandas as pd

• PlasmaPy uses isort to organize import statements via a pre-commit hook.

• For infrequently used objects, import the package, subpackage, or module rather than the individual code object. Including more of the namespace provides contextual information that can make code easier to read. For example, json.loads is more readable than using only loads.

• For frequently used objects (e.g., Particle) and type hint annotations (e.g., Optional and Real), import the object directly instead of importing the package, subpackage, or module. Including more of the namespace would increase clutter and decrease readability without providing commensurately more information.

• Use absolute imports (e.g., from plasmapy.particles import Particle) rather than relative imports (e.g., from ..particles import Particle).

• Do not use star imports (e.g., from package.subpackage import *), except in very limited situations.

### Requirements

• Package requirements are specified in pyproject.toml. tox.ini also contains a testing environment for the minimal dependencies.

• Each release of PlasmaPy should support all minor versions of Python that have been released in the prior 42 months, and all minor versions of NumPy that have been released in the last 24 months. This schedule was proposed in NumPy Enhancement Proposal 29 for the scientific Python ecosystem, and has been adopted by upstream packages such as NumPy, matplotlib, and Astropy.

Tip

Tools like pyupgrade help automatically upgrade the code base to the minimum supported version of Python for the next release.

• In general, it is preferable to support minor releases of dependencies from the last ≲ 24 months, unless there is a new feature in a dependency that would be greatly beneficial for plasmapy development.

• Do not set maximum requirements (e.g., numpy <= 1.22.3) unless absolutely necessary. Maximum requirements can lead to version conflicts when installed alongside other packages. Instead, update PlasmaPy to become compatible with the latest versions of its dependencies. Similarly, do not require exact versions of packages (e.g., scipy == 1.5.3).

• Minor versions of Python are generally released in October of each year. However, it may take a few months before packages like NumPy and Numba become compatible with the newest minor version of Python.

## Special function categories

### Aliases

An alias is an abbreviated version of a commonly used function. For example, va_ is an alias to Alfven_speed.

Aliases are intended to give users the option for shortening their code while maintaining some readability and explicit meaning. As such, aliases are given to functionality that already has a widely-used symbol in plasma literature.

Here is a minimal example of an alias f_ to function as would be defined in plasmapy/subpackage/module.py.

__all__ = ["function"]
__aliases__ = ["f_"]

__all__ += __aliases__

def function():
...

f_ = function
"""Alias to ~plasmapy.subpackage.module.function."""

• Aliases should only be defined for functionality that already has a symbol that is widely used in the community’s literature. This is to ensure that the abbreviated function name is still widely understandable. For example, cwp_ is a shortcut for $$c/ω_p$$.

• The name of an alias should end with a trailing underscore.

• An alias should be defined immediately after the original function.

• Each alias should have a one-line docstring that refers users to the original function.

• The name of the original function should be included in __all__ near the top of each module, and the name of the alias should be included in __aliases__, which will then get appended to __all__. This is done so both the alias and the original function get properly documented.

• Aliases are intended for end users, and should not be used in PlasmaPy or other collaborative software development efforts because of reduced readability and searchability for someone new to plasma science.

### Lite Functions

Most functions in plasmapy.formulary accept Quantity instances as arguments and use validate_quantities() to verify that Quantity arguments are valid. The use of Quantity operations and validations do not noticeably impact performance during typical interactive use, but the performance penalty can become significant for numerically intensive applications.

A lite-function is an optimized version of another plasmapy function that accepts numbers and NumPy arrays in assumed SI units. Lite-functions skip all validations and instead prioritize performance. Most lite-functions are defined in plasmapy.formulary.

Caution

Unlike most formulary functions, no validations are performed on the arguments provided to a lite-function for the sake of computational efficiency. When using lite-functions, it is vital to double-check your implementation!

Here is a minimal example of a lite-function function_lite that corresponds to function as would be defined in plasmapy/subpackage/module.py.

__all__ = ["function"]
__lite_funcs__ = ["function_lite"]

from numbers import Real

from numba import njit
from plasmapy.utils.decorators import bind_lite_func, preserve_signature

__all__ += __lite_funcs__

@preserve_signature
@njit
def function_lite(v: Real) -> Real:
"""
The lite-function which accepts and returns real numbers in
assumed SI units.
"""
...

@bind_lite_func(function_lite)
def function(v):
"""A function that accepts and returns Quantity arguments."""
...

• The name of each lite-function should be the name of the original function with _lite appended at the end. For example, thermal_speed_lite is the lite-function associated with thermal_speed.

• Lite-functions assume SI units for all arguments that represent physical quantities.

• Lite-functions should be defined immediately before the normal version of the function.

• Lite-functions should be used by their associate non-lite counterpart, except for well reasoned exceptions. This is done to reduce code duplication.

• Lite-functions are bound to their normal version as the lite attribute using the bind_lite_func decorator. This allows the lite-function to also be accessed like thermal_speed.lite().

• If a lite-function is decorated with something like @njit, then it should also be decorated with preserve_signature. This preserves the function signature so interpreters can still give hints about function arguments.

• When possible, a lite-function should incorporate numba’s just-in-time compilation or utilize Cython. At a minimum any “extra” code beyond the raw calculation should be removed.

• The name of the original function should be included in __all__ near the top of each module, and the name of the lite-function should be included in __lite_funcs__, which will then get appended to __all__. This is done so both the lite-function and the original function get properly documented.

## Physics

### Units

PlasmaPy uses astropy.units to assign physical units to values in the form of a Quantity.

>>> import astropy.units as u
>>> 5 * u.m / u.s
<Quantity 5. m / s>


Using astropy.units improves compatibility with Python packages in adjacent fields such as astronomy and heliophysics. To get started with astropy.units, check out this example notebook on units.

Caution

Some scipy functions silently drop units when used on Quantity instances.

### Particles

The Particle class provides an object-oriented interface for accessing basic particle data. Particle accepts particle-like inputs.

>>> from plasmapy.particles import Particle
>>> alpha = Particle("He-4 2+")
>>> alpha.mass
<Quantity 6.6446...e-27 kg>
>>> alpha.charge
<Quantity 3.20435...e-19 C>


To get started with plasmapy.particles, check out this example notebook on particles.

### Equations and Physical Formulae

• Physical formulae should be inputted without first evaluating all of the physical constants. For example, the following line of code obscures information about the physics being represented:

>>> omega_ce = 1.76e7*(B/u.G)*u.rad/u.s


In contrast, the following line of code shows the exact formula which makes the code much more readable.

>>> omega_ce = (e * B) / (m_e * c)


The origins of numerical coefficients in formulae should be documented.

• Docstrings should describe the physics associated with these quantities in ways that are understandable to students who are taking their first course in plasma physics while still being useful to experienced plasma physicists.

### Angular Frequencies

Unit conversions involving angles must be treated with care. Angles are dimensionless but do have units. Angular velocity is often given in units of radians per second, though dimensionally this is equivalent to inverse seconds. Astropy will treat radians dimensionlessly when using the dimensionless_angles equivalency, but dimensionless_angles does not account for the multiplicative factor of 2*pi that is used when converting between frequency (1 / s) and angular frequency (rad / s). An explicit way to do this conversion is to set up an equivalency between cycles/s and Hz:

>>> from astropy import units as u
>>> f_ce = omega_ce.to(u.Hz, equivalencies=[(u.cy/u.s, u.Hz)])


However, dimensionless_angles does work when dividing a velocity by an angular frequency to get a length scale:

>>> d_i = (c/omega_pi).to(u.m, equivalencies=u.dimensionless_angles())


## Example notebooks

Examples in PlasmaPy are written as Jupyter notebooks, taking advantage of their mature ecosystems. They are located in docs/notebooks. nbsphinx takes care of executing them at documentation build time and including them in the documentation.

Please note that it is necessary to store notebooks with their outputs stripped (use the “Edit -> Clear all” option in JupyterLab and the “Cell -> All Output -> Clear” option in the “classic” Jupyter Notebook). This accomplishes two goals:

1. helps with versioning the notebooks, as binary image data is not stored in the notebook

2. signals nbsphinx that it should execute the notebook.

Note

In the future, verifying and running this step may be automated via a GitHub bot. Currently, reviewers should ensure that submitted notebooks have outputs stripped.

If you have an example notebook that includes packages unavailable in the documentation building environment (e.g., bokeh) or runs some heavy computation that should not be executed on every commit, keep the outputs in the notebook but store it in the repository with a preexecuted_ prefix, e.g., preexecuted_full_3d_mhd_chaotic_turbulence_simulation.ipynb.

## Compatibility with Prior Versions of Python, NumPy, and Astropy

PlasmaPy releases will generally abide by the following standards, which are adapted from NEP 29 for the support of old versions of Python, NumPy, and Astropy.

• PlasmaPy should support at least the minor versions of Python initially released 42 months prior to a planned project release date.

• PlasmaPy should support at least the 3 latest minor versions of Python.

• PlasmaPy should support minor versions of NumPy initially released in the 24 months prior to a planned project release date or the oldest version that supports the minimum Python version (whichever is higher).

• PlasmaPy should support at least the 3 latest minor versions of NumPy and Astropy.

The required major and minor version numbers of upstream packages may only change during major or minor releases of PlasmaPy, and never during patch releases.

Exceptions to these guidelines should only be made when there are major improvements or fixes to upstream functionality or when other required packages have stricter requirements.

## Benchmarks

PlasmaPy has a set of asv benchmarks that monitor performance of its functionalities. This is meant to protect the package from performance regressions. The benchmarks can be viewed at benchmarks. They’re generated from results located in benchmarks-repo. Detailed instructions on writing such benchmarks can be found at asv-docs. Up-to-date instructions on running the benchmark suite will be located in the README file of benchmarks-repo.