Title: Nowcasting Solar EUV Irradiance with Photospheric Magnetic Fields and the MgII Index
Authors: Kara L. Kniezewski, Samuel J. Schonfeld, Carl J. Henney

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Description of contents: Contains all input data and Python scripts used to generate the models and figures in this paper.

Data Description:
- MgII_composite is a .dat file containing the observed MgII core-to-wing ratio; this file was compiled by Mark Weber (University of Bremen)

Script Description:
- MgII_magsum_modelling_KLK is a Python Jupyter Notebook used to generate the MgII nowcast model using the plage and active region magnetic sums
- EUV_magsum_modelling_KLK is a Python Jupyter Notebook used to generate the EUV nowcast model using the plage and active region magnetic sums and apply the MgII correction term to improve the models

Figure Description:
- fig2 is a .tar file containing plots comparing the plage and active region sums, the MgII observed core-to-wing ratio and model, and the EUV observed index and model for all 37 bands
- fig3 is a .tar file containing plots for all 37 EUV bands which compares the EUV and MgII difference between model and observed values
- fig4 is a .tar file containing plots which compare the EUV model difference and the MgII correction term for each of the 37 bands
- fig6 is a .tar file containing the Box and Whisker plots of the original and corrected EUV observed to model difference for all 37 EUV bands

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System requirements: Read .txt and .dat files, display .png files, and run .ipynb scripts.

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Additional comments: For further assistance, please contact me at karakniezewski@gmail.com