Transverse Coronal-Loop Oscillations Induced by the Non-radial Eruption of a Magnetic Flux Rope

bibcode: 2022SoPh..297...18Z

Authors: Zhang, Q. M., Chen, J. L., Li, S. T., Lu, L., Li, D.

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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
• BBSO: Big Bear Solar Observatory
• SOHO: Solar and Heliospheric Observatory
• GOES16: Geostationary Operational Environmental Satellite (GOES-R) Series 16
• STEREO_A: Solar TErrestrial RElations Observatory - Ahead

Instruments

• AIA: Atmospheric Imaging Assembly
• HMI: Helioseismic and Magnetic Imager
• LASCO: Large Angle and Spectrometric Coronagraph
• SECCHI: Sun Earth Connection Coronal and Heliospheric Investigation
• BIG BEAR: Big Bear Solar Observatory, California TON and GONG+ sites

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.