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 …

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 …

We studied a blowout jet that occurred at the west limb of the Sun on 2014 August 29 using
high-resolution imaging/spectroscopic observations provided by the Solar Dynamics …

A highly important aspect of solar activity is the coupling between eruptions and the
surrounding coronal magnetic field topology, which determines the trajectory and …

Solar filament eruptions are often associated with solar flares and coronal mass ejections,
which have the greatest impact on space weather. However, the fine structures and the …

With high spatial and temporal resolution data from the Solar Dynamics Observatory and the
New Vacuum Solar Telescope (NVST), we present observations of recurrent jets confined by …

Particle acceleration in stellar flares is ubiquitous in the universe; however, our Sun is the
only astrophysical object where energetic particles and their source flares can both be …

With high spatial and temporal resolution, Hα data from the New Vacuum Solar Telescope, X-
ray images from the X-ray telescope on board Hinode and simultaneous observations from …

We have carried out a comprehensive study of the temperature structure of plasmoids, which
successively occurred in recurrent active region jets. The multithermal plasmoids were seen …

We investigate the topological evolution of coronal jet containing a sigmoid-like flux rope
using a nonlinear force-free field model obtained with the flux-rope insertion method and …