Uranus's Highly Nonaxisymmetric Magnetopause and its Impact on Magnetic Reconnection Data

Simulation and calculated data used for making figures in Uranus’s Highly Nonaxisymmetric Magnetopause and its Impact on Magnetic Reconnection by Jack H. Crump, Ali H. Sulaiman, Xianzhe Jia, Sophia Zomerdijk-Russell, Adam Masters. All files can be found in a .zip folder. With the exception of the full simulation files (which are .dat files), all files are .csv with the first row labeling the contents of the columns. Within this folder there are several subfolders. conditions: Includes all of the magnetosphere and magnetosheath plasma, magnetic field, and reconnection conditions in Figures 2-4, 6-7, 9-10. This folder is divided by the simulation file with Equinox being the equinox case and Voyager2_By being the solstice case. Each simulation is then labeled by its time snapshot (0, 4, 8, or 12). Additionally, there is a folder (analytical) that contains the data needed to plot the analytical comparisons on the aforementioned figures. dirunal: Contains the values of r used in creating Figure 8 for both reconnection conditions and the combined conditions divided by season. field_lines: Contains all of the field lines that appear on Figure 1. each field line is a different file named by its starting location and whether it is in the magnetosphere or magnetosheath. full_simulations: Contains the 8 snapshots of the two simulations that were run (the two seasonal cases). These files were used to calculate all other simulation derived outputs. streamlines: Contains the streamlines plotted on Figure 5. Files are labeled by the initial angle the stremline makes in the yz plane.