Contributed by P. Vemareddy. Posted on January 8, 2025
The coronal magnetic field evolution of the AR 11429 was simulated using time-dependent magneto-friction model. The model reproduced the magnetic structure that has remarkable correspondence with the spatial characteristics in coronal extreme ultraviolet images.
Contributed by Marion Weinzierl. Posted on December 12, 2015
Data-driven magnetofrictional model provides a more realistic description of the non-potential coronal magnetic field, but faces technical challenges that need to be addressed.