In this review we focus on the fundamental theory of magnetohydrodynamic reconnection,
together with applications to understanding a wide range of dynamic processes in the solar …

Magnetic reconnection has been intensively studied in fully ionized plasmas. However,
plasmas are often partially ionized in astrophysical environments. The interactions between …

Magnetic reconnection is a key mechanism involved in solar eruptions and is also a prime
possibility to heat the low corona to millions of degrees. Here, we present ultra-high …

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 …

Context. Ultraviolet bursts are transients in the solar atmosphere with an increased
impulsive emission in the extreme UV lasting for one to several tens of minutes. They often …

Context. Ultraviolet (UV) bursts and Ellerman bombs (EBs) are small-scale magnetic
reconnection events taking place in the highly stratified, low solar atmosphere. The plasma …

We report a new, plasmoid-fed scenario for the formation of an eruptive prominence (PF 2),
involving reconnection and condensation. We use grid-adaptive resistive two-and-a-half …

We report our results from a set of high-resolution, two-fluid, non-linear simulations of the
magnetized Rayleigh Taylor instability (RTI) at the interface between a solar prominence …

Fast magnetic reconnection plays a fundamental role in driving explosive dynamics and
heating in the solar chromosphere. The reconnection time scale of traditional models is …