Comparing Simulated and Observed Particle Energy Distributions through Magnetic Reconnection in Earth's Magnetotail
This study demonstrates that data-driven 2D fully kinetic simulations initialized with MMS mission parameters successfully reproduce the overall shape of ion and electron energy distributions during magnetotail magnetic reconnection, though they tend to underestimate the high-energy electron tail, highlighting the critical influence of initial upstream temperatures and the need for 3D models to fully capture observed particle energization.