Self-consistent inner-magnetosphere model is driven by inputs from the Lyon-Fedder- Mobarry global magnetohydrodynamic model. The expanded inner magnotospheric modeling region captures high-resolution bursty bulk flows in the plasma sheet. Realistic bursty bulk flows induced aurora patterns are simulated. This includes data and visualization methods that reproduce the figures in the manuscript. Please refer to README for details. Submitted to JGR for review.