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 …

Abstract The Interface Region Imaging Spectrograph (IRIS) has been obtaining near-and far-
ultraviolet images and spectra of the solar atmosphere since July 2013. IRIS is the highest …

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 …

Different from the classical emerging-flux model for solar jets, recent studies proposed that
the great majority of solar coronal jets are triggered by minifilament eruptions and two …

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

Context. Coronal jets are ubiquitous in active regions and coronal holes. Aims. In this paper,
we study a coronal jet related to a C3. 4 circular-ribbon flare in the active region 12434 on …

In this paper, we report multiwavelength observations of subarcsecond blobs in coronal jets.
In AR 12149, a C5. 5 circular-ribbon flare occurred at∼ 04: 55 UT on 2014 August 24, which …

Context. Solar jets are an important field of study, as they may contribute to the mass and
energy transfer from the lower to the upper atmosphere. Aims. We use the Interface Region …

Using H α line core and off-band imaging data from the New Vacuum Solar Telescope in
China, we present a high-resolution observation on the entire life cycle of a solar …

Solar quiet-and coronal-hole region coronal jets frequently clearly originate from erupting
minifilaments, but active-region jets often lack an obvious erupting-minifilament source. We …