Description
The attached data files underpin the doctoral thesis "Three-Dimensional Magnetic Field Extrapolation Using Analytical Magnetohydrostatic Equilibrium Solutions". The following file types and formats are included:
- Python code files: .py (requires at least a text editor to be opened, but a code editor is recommended)
- Jupyter notebook files: .ipynb (requires a program capable to read Jupyter notebooks, e.g. VSCode)
- Magnetogram and continuum observations by SDO and Solar Orbiter: .fits (require specialised reading routines, e.g. Sunpy in Python, an example is given in one of the Jupyter notebooks)
- X-Ray time series by GOES: .nc (same requirements as .fits files)
- Additional figures: .png (no special requirements)
More details on the underpinning data are provided in the REAME.md file.
- Python code files: .py (requires at least a text editor to be opened, but a code editor is recommended)
- Jupyter notebook files: .ipynb (requires a program capable to read Jupyter notebooks, e.g. VSCode)
- Magnetogram and continuum observations by SDO and Solar Orbiter: .fits (require specialised reading routines, e.g. Sunpy in Python, an example is given in one of the Jupyter notebooks)
- X-Ray time series by GOES: .nc (same requirements as .fits files)
- Additional figures: .png (no special requirements)
More details on the underpinning data are provided in the REAME.md file.
| Date made available | 14 Apr 2025 |
|---|---|
| Publisher | University of St Andrews |
| Date of data production | 2024 |
Student theses
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Three-dimensional solar magnetic field extrapolation using analytical magnetohydrostatic equilibrium solutions
Nadol, L. M. (Author), Neukirch, T. (Supervisor), 3 Jul 2025Student thesis: Doctoral Thesis (PhD)