Simulations of Coronal Mass Ejections on the star ε Eridani

These files include simulated Titov- Démoulin CME events on the star epsilon Eridani due to be published in Ó Fionnagáin et al. (2021). These simulations are conducted using the BATS-R-US AWSOM model, defined by van der Holst et al. (2014) and Gombosi et al. (2018). Provided in this dataset are the CME events at the 10 minute post-eruption mark. The datasets are provided in binary format (.plt), readable by the Tecplot software. The columns included in this data are given below and consist of position [x,y,z], velocity [x,y,z], magnetic field [x,y,z], Alfvén wave energy densities, Pressure [electron, ion_parallel, ion_perpendicular, current [x, y, z]. variables = X [R], Y [R], Z [R], rho [g/cm^3], U_x [km/s], U_y [km/s], U_z [km/s], B_x [Gauss], B_y [Gauss], B_z [Gauss], Ehot [erg/cm^3], I01 [erg/cm^3], I02 [erg/cm^3], Pe [dyne/cm^2], P_par [dyne/cm^2], P_perp [dyne/cm^2], P [dyne/cm^2], J_x [`mA/m^2], J_y [`mA/m^2], J_z [`mA/m^2] Providing the entire dataset was unfeasible due to the large size of the data. However, the entire dataset can be made available upon reasonable request from the authors. This research was funded by the Irish Research Council (IRC).