Data based on the study of "What controls the dawn-dusk asymmetry of dayside Alfvénic power: Interplanetary magnetic field or ionospheric conductance?"

This dataset includes drawing codes and simulation data based on the Grid Agnostic MHD for Extended Research Applications (GAMERA) model and the Magnetosphere-Ionosphere Coupler/Solver (MIX) and is used to investigate whether the cause of this dayside asymmetric Alfvénic energy fluxes distribution is the IMF By or the ionospheric conductance gradient.