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 …

Previous studies have revealed that solar coronal jets triggered by the eruption of
minifilaments (MFs) conform to the famous magnetic-breakout mechanism. In such a …

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 …

ABSTRACT The James Webb Space Telescope (JWST) will provide an opportunity to
investigate the atmospheres of potentially habitable planets. Aerosols significantly mute …

The current sheet is a characteristic structure of magnetic energy dissipation during the
magnetic reconnection process. So far, the width and depth of the current sheet are still …

Coronal loops are the building blocks of solar active regions. However, their formation
mechanism remains poorly understood. Here we present direct observational evidence for …

Fan-spine magnetic structure, as a fundamental three-dimensional topology in magnetic
reconnection theory, plays a crucial role in producing solar jets. However, how fan-spine …

Magnetic reconnection is believed to play an important role in the release and conversion of
energy among magnetized plasma systems. So far, we have been unable to understand …

Coronal rain (CR) is a crucial part of the mass cycle between the corona and chromosphere.
It includes flare-driven CR and two types of quiescent CR, along nonflaring active region …

Magnetic reconnection modulated by nonlocal disturbances in the solar atmosphere has
been investigated theoretically, but rarely observed. In this study, employing Hα and extreme …