J. J. González-Avilés

Numerical schemes and dissipative processes in three-dimensional modeling of post-flare loops and their EUV signatures

Solar flares release magnetic energy into the solar corona and drive the formation of hot post-flare loops, but their thermodynamic evolution depends on both the physical processes included in the model and the numerical scheme used to solve the magnetohydrodynamic (MHD) equations. We investigate the formation and evol...