Magnetic fields play a fundamental role in the structure and dynamics of the solar corona. As
they are driven by their footpoint motions on the solar surface, which transport energy from …

We present a report of recent progress on the topic of understanding solar coronal mass
ejection (CME) onset from both modeling and observational viewpoints, as carried out from …

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 …

Context. Magnetic reconnection in the deep solar atmosphere can give rise to enhanced
emission in the Balmer hydrogen lines, a phenomenon referred to as Ellerman bombs. Aims …

The processes controlling the complex clump structure, phase distribution, and magnetic
field geometry that develop across a broad range of scales in the turbulent interstellar …

Previous studies have revealed that solar coronal jets triggered by the eruption of
minifilaments (MFs) conform to the famous magnetic-breakout mechanism. In such a …

We investigate observational signatures of explosive chromospheric evaporation during a
white-light flare (WLF) that occurred on 2022 August 27. Using the moment analysis …

We present two homologous quasi-periodic fast-mode propagating (QFP) wave trains
excited by two small-scale filament eruptions nearby a sunspot on 2017 September 12. By …

We present a method of conducting data-driven simulations of solar active regions and flux
emergence with the MURaM radiative magnetohydrodynamics (MHD) code. The horizontal …

We revise in detail and in a pedagogical way the analysis of the boundary layer theory of
warm tearing modes in slab, reduced magnetohydrodynamics (MHD), when magnetic …