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Published in Journal of Open Source Software
Keywords
Repository
A data analysis Python package for the PLUTO code
Basic Info
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Metadata Files
README.md
PyPLUTO: a data analysis Python package for the PLUTO code
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PyPLUTO is a Python library which loads and plots the data obtain from the PLUTO code simulations. The aim of this package is to simplify some non-trivial python routines in order to quickly recover effective plots that are suited for scientific publications.
The package is designed to be used in both an interactive environment like ipython shell or Jupyter notebook and standard Python scripts.
The package is structured as follow:
- the Load class is used to load the data from the PLUTO simulation fluid files.
- the LoadPart class is used to load the data from the PLUTO simulation particle files.
- the Image class is used to visualize the loaded data.
- additional functions (e.g., to save the images) are included in the package.
The package includes a set of examples in the Examples directory.
The package is tested on Python 3.10 (and newer versions) and with the following dependencies:
numpymatplotlibscipypandash5pyPyQt6
The package is provided with a LICENSE file which contains the license terms.
The package is provided with an extensive documentation in the Docs directory.
Installation Instructions
To install the PyPLUTO package, you can use the following methods:
Installation with pip
The easiest way to install PyPLUTO is through pip. Open your terminal and run the following command:
bash
pip install ./
Ensure that you are using Python 3.10 or newer, as the package is compatible from this version onwards. Installation through pipenv or uv is also possible (see the documentation).
This method allows installation in a non-editable mode, and it is recommended to use a virtual environment to avoid conflicts with other packages.
Quick Start
python
import pyPLUTO as pp
Simulations can be loaded by just providing the path to the simulation directory. The last output (if not specific file is selected) is automatically found, as well as the available PLUTO file in the selected folder.
python
D = pp.Load()
print(D)
Relevant simulations attributes (such as the computational grid, the geometry and the variables to load) are found automatically. The data can be plotted through the Image class, which acts as a simplified maptlotlib wrapper. An example of 1D plot of the density can be:
python
D = pp.Load()
pp.Image().plot(D.x1, D.rho)
pp.show()
while 2D plots can be created with
python
D = pp.Load()
pp.Image().display(D.rho, x1=D.x1, x2=D.x2, cpos="right")
pp.show()
Examples
In order to test PyPLUTO capabilities, even without the PLUTO code, we provide
an extensive tests suite with all the necessary data.
In this way, PyPLUTO can be explored without any knowledge of the PLUTO code.
All the tests are located in the Examples directory and are aimed at showing
how to exploit the package capabilities.
The GUI
A Graphical User Interface has been implemented in order to simplify and enhance the visualization and analysis of simulation data. The GUI is built with PyQt6 and allows users to load and visualize 1D and 2D fluid data (or slices) from PLUTO simulations. To run the GUI after the package installation, one should simply run the command
bash
pypluto-gui
from the terminal. More details on how to use the GUI can be found in the documentation.
Documentation
For more detailed instructions and additional installation options, please refer to the PyPLUTO documentation where you can find comprehensive guides and examples.
Cite This Repository
If you use this repository in your research or projects, please consider citing the arxiv paper.
@ARTICLE{PyPLUTO2025,
author = {{Mattia}, Giancarlo and {Crocco}, Daniele and {Melon Fuksman}, David and {Bugli}, Matteo and {Berta}, Vittoria and {Puzzoni}, Eleonora and {Mignone}, Andrea and {Vaidya}, Bhargav},
title = "{PyPLUTO: a data analysis Python package for the PLUTO code}",
journal = {arXiv e-prints},
keywords = {Astrophysics - Instrumentation and Methods for Astrophysics},
year = 2025,
month = jan,
eid = {arXiv:2501.09748},
pages = {arXiv:2501.09748},
doi = {10.48550/arXiv.2501.09748},
}
We recommend to put one the following expressions in your manuscript:
"The figures presented in this paper were generated using the PyPLUTO package (citation to the paper)"
"This research has benefited from the PyPLUTO package for data visualization (citation to the paper)"
Contributing
If you have any questions, suggestions or find a bug, feel free to open an issue or fork the repository and create a pull request. Any contribution aimed at helping the PLUTO code community to have better plots with less efforts will be greatly appreciated. If you want to contribute to PyPLUTO please be sure to install it in the developer mode, through the command:
bash
pip install -r requirements_dev.txt
Rules for Contributing
We use pre-commit to ensure that the code is consistent with the code guidelines, including the "black" format and several "ruff" checks. You can either link the pre-commit to the repository through the command
bash
pre-commit install
or by enforcing the guide styles manually through the command
bash
pre-commit run --all-files
Before opening a pull request,there is the possibility to run a deeper series of checks, including tests with coverage, pylint check, docstring coverage and so through the command
bash
pre-commit run --all-files --hook-stage manual
If one or more tests do not pass the automatic code checks anforced through github actions will not allow the pull request to pass, so is higly recommended to run the full pre-commit before every pull request. For any question or enquiry, please contact one of the administrators.
Owner
- Login: GiMattia
- Kind: user
- Repositories: 1
- Profile: https://github.com/GiMattia
JOSS Publication
PyPLUTO: a data analysis Python package for the PLUTO code
Authors
Max-Planck-Institut für Astronomie, Königstuhl 17, Heidelberg, 69117, Germany, INFN, Sezione di Firenze, Via G. Sansone 1, Sesto Fiorentino (FI), 50019, Italy
Dipartimento di Fisica, Università di Torino, Via P. Giuria 1, Torino, 10125, Italy, Institut d’Astrophysique de Paris, UMR 7095, CNRS & Sorbonne Université, 98 bis boulevard Arago, 75014 Paris, France, Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, 91191, France, INFN, Sezione di Torino, Via P. Giuria 1, Torino, 10125, Italy
Dipartimento di Fisica, Università di Torino, Via P. Giuria 1, Torino, 10125, Italy, INFN, Sezione di Torino, Via P. Giuria 1, Torino, 10125, Italy
Observatoire de la Côte d’Azur, Laboratoire Lagrange, Bd de l’Observatoire, CS 34229, 06304 Nice cedex 4, France
Tags
astronomy magnetohydrodynamics computational astrophysics data visualizationGitHub Events
Total
- Create event: 8
- Commit comment event: 46
- Release event: 3
- Watch event: 13
- Delete event: 11
- Issue comment event: 7
- Public event: 1
- Push event: 248
- Pull request event: 96
Last Year
- Create event: 8
- Commit comment event: 46
- Release event: 3
- Watch event: 13
- Delete event: 11
- Issue comment event: 7
- Public event: 1
- Push event: 248
- Pull request event: 96
Issues and Pull Requests
Last synced: 6 months ago
All Time
- Total issues: 0
- Total pull requests: 43
- Average time to close issues: N/A
- Average time to close pull requests: about 4 hours
- Total issue authors: 0
- Total pull request authors: 2
- Average comments per issue: 0
- Average comments per pull request: 0.14
- Merged pull requests: 26
- Bot issues: 0
- Bot pull requests: 0
Past Year
- Issues: 0
- Pull requests: 43
- Average time to close issues: N/A
- Average time to close pull requests: about 4 hours
- Issue authors: 0
- Pull request authors: 2
- Average comments per issue: 0
- Average comments per pull request: 0.14
- Merged pull requests: 26
- Bot issues: 0
- Bot pull requests: 0
Top Authors
Issue Authors
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- GiMattia (31)
- BabbiBear (7)