Nonequilibrium ionization and ambipolar diffusion in solar magnetic flux emergence processes
Context. Magnetic flux emergence from the solar interior has been shown to be a key mechanism for unleashing a wide variety of phenomena. However, there are still open questions concerning the rise of the magnetized plasma through the atmosphere, mainly in the chromosphere, where the plasma departs from local thermodynamic equilibrium (LTE) and is
Nóbrega-Siverio, D. et al.
Fecha de publicación:
1
2020