Plasma in the Sun's hot corona expands into the heliosphere as a supersonic and highly
magnetized solar wind. This paper provides an overview of our current understanding of …

Decayless kink oscillations of an ensemble of loops are captured simultaneously by the
High Resolution Imager (HRI) of the Extreme Ultraviolet Imager (EUI) and the Atmospheric …

We present a clear case study on the occurrence of two successive X-class flares, including
a decade-class flare (X9. 3) and two coronal mass ejections (CMEs) triggered by shearing …

Using high spatial and temporal data from the New Vacuum Solar Telescope and the Solar
Dynamics Observatory, we present unambiguous observations of recurrent two-sided loop …

We present high-resolution observations of a magnetic reconnection event in the solar
atmosphere taken with the New Vacuum Solar Telescope, Atmospheric Imaging Assembly …

We present observations of the eruption and then reformation of a filament caused by its
nearby emerging magnetic flux. Driven by the emerging magnetic flux, the emerging positive …

Aims. To understand the formation mechanism of large plumes in solar prominences, we
investigate the formation process of two such phenomena. Methods. We studied the …

As one of the most common features in the solar atmosphere, filaments are significant not
only in solar physics but also in stellar and laboratory plasma physics. With the New Vacuum …

Solar prominences, intricate structures on the Sun's limb, have been a subject of fascination
owing to their threadlike features and dynamic behaviors. Utilizing data from the New …

ABSTRACT G-band bright points (GBPs) are thought to be the foot-points of magnetic flux
tubes. The aim of this paper is to investigate the relation between the diffusion regimes of …