George Cherry

George Cherry is a Doctoral Research Fellow at the Rosseland Centre for Solar Physics, University of Oslo. His work focuses on magnetic flux emergence, MHD simulations, and applying Fortran and machine learning to astrophysical problems. He holds an MMath in Mathematics from the University of St Andrews (2022), with a thesis on volcanic plume dynamics and magnetic flux transport simulations.

Research Interests:

• Magnetic flux emergence mechanisms in the solar atmosphere
• Development of numerical models for thermal conduction in MHD codes like Bifrost
• Application of machine learning to astrophysical simulations
• Plume dynamics in solar chromosphere and corona

His recent publications address thermal conduction models in solar atmosphere simulations, contributing to both computational methods and analytical solutions for nonlinear phenomena. These studies advance understanding of energy transfer processes in magnetohydrodynamic environments.

Awards:

• University of St Andrews Principals Medal (2022)

Cherry's research is supported through participation in collaborative projects at UiO's Institute of Theoretical Astrophysics. He is actively involved in code development for solar physics simulations and has presented at international astrophysics conferences.