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 report on observations of recurrent jets by instruments on board the Interface Region
Imaging Spectrograph, Solar Dynamics Observatory (SDO), and Hinode spacecraft. Over a 4 …

Aims. We present a multiwavelength analysis of 20 EUV jets which occurred at the periphery
of active regions close to sunspots. We discuss the physical parameters of the jets and their …

In the present review article, we discuss the recent developments in studying the Kelvin–
Helmholtz (KH) instability of magnetohydrodynamic (MHD) waves propagating in various …

Solar jets are impulsive, collimated plasma ejections that are triggered by magnetic
reconnection. They are observed for many decades in various temperatures and …

Recent observations show that the buildup and triggering of minifilament eruptions that drive
coronal jets result from magnetic flux cancelation at the neutral line between merging …

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 …

Context. A subclass of broad extreme ultraviolet (EUV) and X-ray jets, called blowout jets,
have become a topic of research since they could be the link between standard collimated …

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 …

Context. Hot coronal jets are a basic observed feature of the solar atmosphere whose
physical origin is still actively debated. Aims. We study six recurrent jets that occurred in …