Reconstructing the XUV Spectra of Active Sun-like Stars Using Solar Scaling Relations with Magnetic Flux

bibcode: 2023ApJ...945..147N

Authors: Namekata, Kosuke, Toriumi, Shin, Airapetian, Vladimir S., Shoda, Munehito, Watanabe, Kyoko, Notsu, Yuta

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About

This repository contains files initially drafted using AI, which are then manually validated for quality assurance. These files are designed to aid in the understanding and analysis of academic papers, with a download script specifically tailored for retrieving data from the Virtual Solar Observatory (VSO).

Sources and Instruments Used

Sources

• SDO: Solar Dynamics Observatory
• SOHO: Solar and Heliospheric Observatory

Instruments

• EVE: Extreme Ultraviolet Variability Experiment
• HMI: Helioseismic and Magnetic Imager
• MDI: Michelson Doppler Imager

Usage

1. Python Data Download Script: Run the download_script.py to fetch data related to the paper. Ensure you have all the necessary dependencies, including SunPy, installed. This script is designed to retrieve data specifically from the VSO. Please note that this script represents a starting point and may not be 100% perfect. Users are encouraged to review and modify it as needed.
2. Instrument Information: Check INSTRUMENT_DETAILS.md for comprehensive information on the instruments used. This can provide context and help in understanding the data fetched by the script.

Contributions and Contact

For any further details or contributions, please refer to our Contributing Guide.

If you encounter any problems or have suggestions for improvements, please submit an issue on GitHub or make a pull request to correct anything you think is wrong.