The purpose of this paper is to introduce the main scientific results made by the one-meter
New Vacuum Solar Telescope (NVST), which was put into commission on 2010. NVST is …

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 …

Photospheric bright points (BPs), the smallest magnetic elements in the photosphere, are
constantly moving and changing. Studying the characteristics of these small-scale strong …

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 …

Aims. The expansion with height of the solar photospheric magnetic field and the plasma
flows is investigated for three isolated bright points (BPs). Methods. The BPs were observed …

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 …

Magnetic bright points in the solar photosphere, visible in both continuum and G-band
images, indicate footpoints of kilogauss magnetic flux tubes extending to the corona. The …

Context. Magnetic bright points (MBPs) are small, bright, and conspicuous magnetic
structures observed in the solar photosphere and are widely recognized as tracers of …

Magnetic bright points (MBPs) are located in intergranular channels on the solar surface.
Studying the properties and evolution process of MBPs can help us to better understand …

Investigating the length scales of granules could help understand the dynamics of granules
in the photosphere. In this work, we detected and identified granules in an active region near …