Supporting materials and data from: Hypotheses concerning global magnetospheric convection, magnetosphere-Ionosphere coupling, and auroral activity at Uranus

Summary: The data and figures contained in this dataset are supporting materials for the paper referenced in the title and abstract below.  This study involved an analytical and numerical assessment of the Uranian magnetosphere and its interaction with the solar wind and interplanetary magnetic field (IMF). The data and figures contained in this dataset include supplementary results for a greater number of IMF orientations and Uranian seasons than the examples presented in the corresponding paper.
Abstract from corresponding paper: doi:10.1029/2023JA031791 with Journal of Geophysical Research Space Physics:We investigate the unique magnetosphere of Uranus and its interaction with the solar wind. Following previous work, we developed and validated a simple yet valuable and illustrative model of Uranus’ offset, tilted, and rapidly-spinning magnetic field and magnetopause (nominal and fit to the Voyager-2 inbound crossing point) in three-dimensional space. With this model, we investigated ..., See the corresponding paper for description of the model that was used to generate these results. These movies and graphics and table all correspond to simulations of Uranus' interaction with the solar wind and estimates of reconnection along the dayside and flank magnetopause of the Uranian magnetosphere system. Also included are movies and graphics estimating auroral activity in the ionosphere at Uranus. All results are dependent on Uranian season (soltices, equinoxes, and mid-seasons), solar wind magnetic field vector (IMF), and diurnal (spin) phase. Also included are results supporting the validation of the model tested on Earth's magnetosphere. General descriptions of the various files are included in the README file., The files and data contained here are in a series of figures (.pdf format), movies (.mp4 format), and excel spreadsheets.