Speaker
Sanja Danilovic
(Stockholm University)
Description
Recent magnetohydrodynamic models show that many of the chromospheric features and their dynamics can be reproduced to some degree. The models demonstrate that the overall appearance of synthetic chromosphere depends mostly on the field configuration and the treatment of the small-scale dynamics. In this talk, the properties of these models are presented, as well as their comparison to observations. These results are then linked with outstanding questions, both in modeling and observations.
Primary author
Sanja Danilovic
(Stockholm University)
