Partially ionized plasmas are found across the Universe in many different astrophysical
environments. They constitute an essential ingredient of the solar atmosphere, molecular …

Vortex flows, related to solar convective turbulent dynamics at granular scales and their
interplay with magnetic fields within intergranular lanes, occur abundantly on the solar …

With the advent of a new generation of solar telescopes and instrumentation, interpreting
chromospheric observations (in particular, spectropolarimetry) requires new, suitable …

Magnetohydrodynamic Alfvén waves have been a focus of laboratory plasma physics and
astrophysics for over half a century. Their unique nature makes them ideal energy …

Aims. Solar prominences contain a significant number of neutral species. The dynamics of
the ionised and neutral fluids composing the prominence plasma can be slightly different if …

The ambipolar diffusion approximation is used to model partially ionized plasma dynamics
in a single-fluid setting. To correctly apply the commonly used version of ambipolar diffusion …

To study acoustic wave propagation and the corresponding energy deposition in partially
ionized plasmas, we use a two-fluid computational model that treats neutrals and charged …

Our understanding of magnetic reconnection (MR) under chromospheric conditions remains
limited. Recent observations have demonstrated the important role of ion–neutral …

This work aims to provide an accurate description and calculations of collision frequencies
in conditions relevant to the solar atmosphere. To do so, we focus on the detailed …

We present a detailed guide to advanced collisionless fluid models that incorporate kinetic
effects into the fluid framework, and that are much closer to the collisionless kinetic …