paircars 3.0.2

A package to calibrate and image MWA solar observation

P-AIRCARS

An automated spectropolarimetric calibration and imaging pipeline designed for solar radio observations using the Murchision Widefield Array (MWA) radio telescope. It performs end-to-end calibration, flagging, and imaging with a focus on dynamic solar data, supporting both spectral and temporal flexibility in imaging products.

Background

Solar radio data presents unique challenges due to the high variability and brightness of the Sun, as well as the need for high time-frequency resolution. The P-AIRCARS pipeline addresses these challenges by:

• Automating the calibration of interferometric data, including flux, phase, and polarization calibrations
• Supporting time-sliced and frequency-sliced imaging workflows
• Leveraging Dask for scalable parallel processing
• Providing hooks for integration with contextual data from other wavelegths for enhanced solar analysis

Documentation

P-AIRCARS documentation is available at: p-aircars.readthedocs.io

Software environment

P-AIRCARS is tested on Ubuntu22, Ubuntu 24, and CentOS 7 with Python 3.10. P-AIRCARS may not work in other operating system and python versions. If user wants to use P-AIRCARS in other environments, limited support is available in debugging or solving the issues. User may look at Containersed Use section in the docuement for these scenarios.

Quickstart

P-AIRCARS is distributed on PyPI. To use it:

1. Create conda environment with python 3.10 with compaitable C/C++ libraries

   conda create -n paircars_env --override-channels -c conda-forge python=3.10 gcc_linux-64=14 gxx_linux-64=14 gfortran_linux-64=14 cmake pkg-config pip
   
   conda activate paircars_env
   

   We suggest using Mamba for fast conda installtion and environment creation.

2. Install P-AIRCARS in conda environment

   pip install paircars
   

3. Initiate necessary metadata

   init-paircars-setup --init
   

   By default, the necessary data will be saved in home directory and requires about 20 GB of disk space. We suggest using any other location with larger disk space and specify that by --datadir </full/path/to/paircars_datadir> in the above command.

4. Before running the pipeline, setup your data as following:

   -- Create a <target_datadir> and put all coarse channel measurement sets of solar scan of a single observation ID (OBSID) inside it.

   -- Create a <cal_datadir> and put all coarse channel measurement sets for calibrator observation of a single OBSID inside it.

5. Run P-AIRCARS pipeline

   run-mwa-paircars <full path of target measurement set directory> <full path of target metafits file> --cal_datadir <full path of calibrator measurement set directory> --cal_metafits <full path of calibrator metafits> --workdir <full path of work directory> --outdir <full path of output products directory>
   

   N.B.: Always provide the entire direcotry path. Short path or only directory name may cause errors. Keep target measurement sets for a single OBSID and calibrator measurement sets for a single OBSID must be kept in seperate directories. If calibrator is not present, do not provide these information.

That's all. You started P-AIRCARS pipeline for analysing your MWA solar observation 🎉.

6. To see all running P-AIRCARS jobs

   show-paircars-status --show
   

7. If P-AIRCARS is running in a local machine, see local log of any job using the

   run-mwa-mwalogger --jobid <jobid>
   

   N.B.: If you are running P-AIRCARS is cluster environment, first checkout HPC Settings in the document for viewing P-AIRCARS log remotely using prefect dashboard.

8. Output products will be saved in : <path of output products directory>

Sample dataset

User can download and test entire P-AIRCARS pipeline using the sample dataset available in Zenodo: https://doi.org/10.5281/zenodo.18641232. Do not use this sample dataset for any publication without permission from the developer.

Acknowledgements

P-AIRCARS is developed by Devojyoti Kansabanik (NCRA-TIFR, Pune, India and CPAESS-UCAR, Boulder, USA) and an incarnation of AIRCARS. Other contributors are, Surajt Mondal (NCRA-TIFR, Pune, India) and and Puja Majee (NCRA-TIFR, Pune, India). If you use P-AIRCARS for analysing your MWA solar observations, include the following statement in your paper, and cite the following papers:

This MWA solar observations are analysed using P-AIRCARS pipeline. 

1. Cite P-AIRCARS software in zenodo: [https://doi.org/10.5281/zenodo.18625477][kansbanikzenodo]

2. Kansabanik et al., 2025, ApJS, v278:26

3. Kansabanik et al., 2023, ApJS, v264:47

4. Kansabanik et al., 2022, ApJ, v932:110

5. Kansbanik 2022, Solar Physics, v297:122

6. Mondal et al., 2019, ApJ, v875:97

If you use observations before 2015, include this additonal statement and citation:

Flux calibration of the observations are done using the menthod described in the following paper.

7. Kansabanik et al., 2022, ApJ, v927:17

P-AIRCARS name is given by Dr. Barnali Das (NCRA-TIFR, Pune, India)

License

This project is licensed under the MIT License.