MHDSTS: a new explicit numerical scheme for simulations of partially ionised solar plasma
The interaction of plasma with magnetic field in the partially ionised solar atmosphere is frequently modelled via a single-fluid approximation, which is valid for the case of a strongly coupled collisional media, such as solar photosphere and low chromosphere. Under the single-fluid formalism the main non-ideal effects are described by a series of
González-Morales, P. A. et al.
Fecha de publicación:
7
2018