Zoran Mikic

TL;DR: In this paper, a global magnetohydrodynamics (MHD) solution for Carrington rotation (CR) 2068 was developed, which includes energy-transport processes, such as coronal heating, conduction of heat parallel to the magnetic field, radiative losses, and the effects of Alfven waves, producing significantly better estimates of the plasma temperature and density in the corona than have been possible in the past.

TL;DR: In this article, the three-dimensional dynamical evolution of twisted magnetic flux tubes using a time-dependent magnetohydrodynamic (MHD) model was studied using a photospheric line tying model.

TL;DR: In this article, the effects of geometrical assumptions in one-dimensional (1D) models of coronal loops were investigated, and it was shown that loops with nonuniform cross-sectional area are more likely to experience thermal nonequilibrium and that they produce significantly enhanced coronal emission, compared with their uniform-area counterparts.

TL;DR: In this paper, the authors present results on the coupling of coronal and heliospheric numerical magnetohydrodynamic (MHD) codes developed within the Center for Integrated Space weather modeling.

TL;DR: In this article, the authors investigate coronal energy flow during a simulated coronal mass ejection (CME) and find that the energy conservation properties of the code are quite good, conserving energy to within 4% for the entire simulation.