Solar filaments are an intriguing phenomenon, like cool clouds suspended in the hot corona.
Similar structures exist in the intergalactic medium as well. Despite being a long-studied …

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 …

We report the first observations of simultaneous large-amplitude longitudinal and transverse
oscillations of a quiescent filament trigged by a two-sided-loop jet formed by the magnetic …

To better understand the physical connections in sympathetic solar eruptions, we
investigated the interaction between two nearby filaments and their successive partial …

We report the smallest coronal jets ever observed in the quiet Sun with recent high-
resolution observations from the High Resolution Telescopes (HRI EUV and HRI Lyα) of the …

The fine magnetic structure is vitally important to understanding the formation, stabilization,
and eruption of solar filaments, but so far, it is still an open question yet to be resolved. Using …

We present the first observation of a solar filament formed by magnetic reconnection,
associated chromospheric evaporation, and subsequent coronal condensation. Driven by …

We present the formation process of a filament in NOAA active region 12765 from 2020 June
5 to 8, using observations from the New Vacuum Solar Telescope, the Solar Dynamics …

Context. Although solar filaments have been intensively studied, detailed observations that
show an entire process of filament maintenance are rare. Aims. The aim of this paper is to …

Context. Dynamic features such as chromospheric jets, transition region network jets,
coronal plumes, and coronal jets are abundant in the network regions of polar coronal holes …