Speaker
Jana Kasparova
(Astronomical Institute of the CAS)
Description
Using numerical RHD code Flarix we simulate the behaviour of MgII lines in the
flaring chromosphere heated by electron beams. This contribution will focus on the
role of partial redistribution, non-thermal collisional rates, and radiative losses.
The role of different types of the temporal heating profiles, e.g. a long duration
heating versus pulse heating will be assessed as well. The results will be discussed
in terms of recent IRIS observations.
Primary author
Jana Kasparova
(Astronomical Institute of the CAS)
