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

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

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

Abstract On the Sun, Doppler shifts of bidirectional outflows from the magnetic-reconnection
site have been found only in confined regions through spectroscopic observations. Without …

Aims. We aim to study a high-resolution observation of an asymmetric inflow magnetic
reconnection between a filament and its surrounding magnetic loops in active region NOAA …

Abstract Employing Solar Dynamics Observatory/Atmospheric Imaging Assembly (AIA) multi-
wavelength images, we report the coronal condensation during the magnetic reconnection …

Magnetic reconnection is a fundamental process of topology change and energy release,
taking place in plasmas on the Sun, in space, in astrophysical objects and in the laboratory …

The structure of magnetic flux ropes injected into the solar wind during reconnection in the
coronal atmosphere is explored with particle-in-cell simulations and compared with in situ …

Using the high tempo-spatial resolution Hα images observed with the New Vacuum Solar
Telescope, we report solid observational evidence of magnetic reconnection between two …

The random walk of the footpoints of coronal loops in the rapidly evolving solar granulation
is expected to cause braiding of the field, which in turn should lead to a multitude of coronal …