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 …

Context. Solar active region (AR) 12673 in 2017 September produced the two largest flares
in Solar Cycle 24: the X9. 3 flare on September 6 and the X8. 2 flare on September 10. Aims …

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 …

Solar flares are powerful radiations occurring in the Sun's atmosphere. They are powered by
magnetic reconnection, a phenomenon that can convert magnetic energy into other forms of …

The study of circular ribbon (CR) flares is important to understand the three-dimensional
magnetic reconnection in the solar atmosphere. We investigate the slipping brightenings …

We study the early evolution of a hot-channel-like magnetic flux rope (MFR) toward eruption.
Combining with imaging observation and magnetic field extrapolation, we find that the hot …

Solar flares and coronal mass ejections are the most powerful explosions in the Sun. They
are major sources of potentially destructive space weather conditions. However, the …

We analyze a unique event with an M1. 8 confined circular-ribbon flare on 2016 February
13, with successive formations of two circular ribbons at the same location. The flare had two …

Slipping motions of magnetic field lines are a distinct signature of three-dimensional
magnetic reconnection, a fundamental process driving solar and stellar flares. While being a …

The solar eruption that occurred on 28 November 2023 (SOL2023-11-28) triggered an
intense geomagnetic storm on 1 December 2023. The associated terrestrial auroras …