Simulations of Coronal Mass Ejections on the star ε Eridani

<p>These files include simulated Titov- D&eacute;moulin CME events on the star epsilon Eridani due to be published in &Oacute; Fionnag&aacute;in et al. (2021).</p> <p>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.</p> <p>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], Alfv&eacute;n wave energy densities, Pressure [electron, ion_parallel, ion_perpendicular, current [x, y, z].</p> <p>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]</p> <p>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.</p> <p>This research was funded by the Irish Research Council (IRC).</p>