This paper provides a comprehensive review of recent theoretical investigations concerning
magnetohydrodynamic (MHD) waves in partially ionized solar plasma. First, we examine the …

The low solar atmosphere is composed of mostly neutral particles, but the importance of the
magnetic field for understanding observed dynamics means that interactions between …

Abstract The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will
revolutionize our ability to measure, understand, and model the basic physical processes …

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

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 …

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 …

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 analyzed multiline observations of a quiescent prominence from the slit spectrograph
located at the Ondřejov Observatory. Dopplergrams and integrated intensity maps of the …

The ponderomotive force has been suggested to be the main mechanism to produce the so-
called first ionization potential (FIP) effect—the enrichment of low-FIP elements observed in …

The European Solar Telescope (EST) is a project aimed at studying the magnetic
connectivity of the solar atmosphere, from the deep photosphere to the upper …