Simulation data from "Dynamic modeling of coronal abundances during flares on M-dwarf stars"

Simulation data and code used to create the plots from the paper by Brooks et al., entitled "Dynamic modeling of coronal abundances during flares on M-dwarf stars". The code has been modified in the enhanced high-FIP case to change the abundances of elements with FIP > 10 eV. The naming convention is to first denote whether the high-FIP species have been enhanced or the low-FIP species depleted, followed by the loop length (e.g. L50 means a 50 Mm loop), and the cases with asymmetric heating have "_AsymmHeat" appended. In those cases, the right leg of the loop receives exactly half the total heat as the left leg.