I am a theoretical and computational plasma physicist specializing in magnetohydrodynamics (MHD) and magnetic reconnection, with applications to both astrophysical and laboratory plasmas. My primary focus is understanding the fundamental physics driving solar flares, coronal mass ejections, and coronal heating, using advanced numerical methods and high-performance computing. I also contribute to magnetic confinement fusion research by developing computational tools for simulating complex plasma behavior. My work aims to improve our predictive capabilities for space weather and advance fusion energy research.