The solar atmosphere is full of complicated transients manifesting the reconfiguration of the
solar magnetic field and plasma. Solar jets represent collimated, beam-like plasma …

Type II radio bursts are often associated with coronal shocks that are typically driven by
coronal mass ejections (CMEs) from the Sun. Here we conduct a case study of a type II radio …

Solid evidence of magnetic reconnection is rarely reported within sunspots, the darkest
regions with the strongest magnetic fields and lowest temperatures in the solar atmosphere …

We present observations of a blowout jet that experienced two distinct ejection stages. The
first stage started from the emergence of a small positive magnetic polarity, which was …

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 jets are fast‐moving, elongated brightenings related to ejections seen in both images
and spectra on all scales from barely visible chromospheric jets to coronal jets extending up …

We study a series of X-ray-bright, rapidly evolving active region coronal jets outside the
leading sunspot of AR 12259, using Hinode/X-ray telescope, Solar Dynamics Observatory …

Abstract On 2016 September 20, the Interface Region Imaging Spectrograph observed an
active region during its earliest emerging phase for almost 7 hr. The Helioseismic and …

We perform 2D resistive magnetohydrodynamic simulations of coronal jets driven by flux
emergence along the lower boundary. The reconnection layers are susceptible to the …

We report a strong minifilament eruption associated with Geostationary Operational
Environmental Satellite C1. 6 flare and WIND type-III radio burst. The minifilament, which lies …