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 …

Solar flares are energetic events taking place in the Sun's atmosphere, and their effects can
greatly impact the environment of the surrounding planets. In particular, eruptive flares, as …

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 …

Current state-of-the-art spectrographs cannot resolve the fundamental spatial
(subarcseconds) and temporal (less than a few tens of seconds) scales of the coronal …

Solar active region (AR) 12192 of 2014 October hosts the largest sunspot group in 24 years.
It is the most prolific flaring site of Cycle 24 so far, but surprisingly produced no coronal mass …

Eruptions, flares, and coronal mass ejection (CMEs) are due to physical phenomena mainly
driven by an initially force-free current-carrying magnetic field. We review some key …

M dwarf flares observed by the Transiting Exoplanet Survey Satellite (TESS) sometimes
exhibit a peak-bump light-curve morphology, characterized by a secondary, gradual peak …

Observations of coronal jets increasingly suggest that local fragmentation and intermittency
play an important role in the dynamics of these events. In this work, we investigate this …

Partial filament eruptions have often been observed; however, the physical mechanisms that
lead to filament splitting are not yet fully understood. In this study, we present a unique event …

We present a comprehensive study of the formation and eruption of an active region (AR)
sigmoid in AR 11283. To follow the quasi-static evolution of the coronal magnetic field, we …