The quiet Sun is the region of the solar surface outside of sunspots, pores, and plages. In
continuum intensity it appears dominated by granular convection. However, in polarized …

Abstract Properties of photospheric bright points (BPs) near an active region have been
studied in TiO λ 7058 Å images observed by the New Vacuum Solar Telescope of the …

We analysed line-of-sight magnetic fields and magnetic power spectra of an undisturbed
photosphere using magnetograms acquired by the Helioseismic and Magnetic Imager (HMI) …

By using a new method of forced-field extrapolation, we study the emerging flux region
AR11850 observed by the Interface Region Imaging Spectrograph and Solar Dynamical …

Photospheric bright points (PBPs) and chromospheric bright points (CBPs) reflect the cross
sections of magnetic flux tubes at different heights of the lower solar atmosphere. We aim to …

G-band bright points (GBPs) are regarded as good manifestations of magnetic flux
concentrations. We aim to investigate the relation between the dynamic properties of GBPs …

Multiwavelength bright points (BPs) are taken to be cross sections of magnetic flux tubes
extending from the surface of the photosphere upward to the higher photosphere. We aim to …

The Sun is a magnetic star, and the only spatio-temporally resolved astrophysical system
displaying turbulent MHD thermal convection. This makes it a privileged object of study to …

Six high-resolution TiO-band image sequences from the New Vacuum Solar Telescope
(NVST) are used to investigate the properties of intergranular bright points (igBPs). We …

The G-band bright points (GBPs) are driven by the granular convection flow, and appear
with different morphologies in the quiet Sun, such as points, elongated chains, and knees. A …