RATANSunPy

RATANSunPy

RATANSunPy is a Python package developed for accessing, visualizing, and analyzing multi-band radio observations of the Sun from the RATAN-600 complex. These data are valuable for diagnosing solar plasma conditions and predicting solar activity. However, working with these data requires extensive processing and a thorough understanding of the RATAN-600 system. The package offers comprehensive data processing functionalities, including direct access to raw data, essential processing steps such as calibration and quiet Sun normalization, and tools for analyzing solar activity. This includes automatic detection of local sources, identifying them with NOAA active regions, and further determining parameters for local sources and active regions.

Installation

To install RATANSunPy, run the following command:

pip install ratansunpy

Usage

For more detailed information about the package and its functionalities, please refer to the official documentation. The best place to start is the in example gallery
also includes a collection of shorter and more specific examples of using ratansunpy, or you can look at example usages in colab notebook if you want to try it yourself.

Related works

Articles:

• RatanSunPy: A robust preprocessing pipeline for RATAN-600 solar radio observations data: https://arxiv.org/abs/2412.08230
• The Ratan Active Region Patches (RARPs) Database: A New Database of Solar Active Region Radio Signatures from the RATAN-600 Telescope: https://arxiv.org/abs/2512.05702

Conference paper:

• https://link.springer.com/chapter/10.1007/978-3-032-07690-8_7

Contributing

Contributions are welcome! If you have suggestions for improvements or bug fixes, please feel free to open an issue or submit a pull request.