Simulated Cusp Boundary Data Derived from Global MHD Modeling

This dataset contains the simulation results of the three-dimensional cusp boundaries derived from global magnetohydrodynamic (MHD) modeling of the near-Earth space environment. The simulations were performed using the PPMLR-MHD global code developed at the National Space Science Center (NSSC), Chinese Academy of Sciences, under various solar wind conditions. The dataset provides plasma parameters including thermal pressure, magnetic field, and related quantities that are used to determine the locations and shapes of the cusp boundaries.