Aims. We present the Stagger-grid, a comprehensive grid of time-dependent, three-
dimensional (3D), hydrodynamic model atmospheres for late-type stars with realistic …

In the following short review we will outline some of the possible interaction processes of
lower solar atmospheric plasma with the embedded small-scale solar magnetic fields. After …

On the basis of observations of solar granulation obtained with the New Solar Telescope of
Big Bear Solar Observatory, we explored proper motion of bright points (BPs) in a quiet-sun …

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 …

Aims. We aim to improve our picture of the low chromosphere in the quiet-Sun internetwork
by investigating the intensity, horizontal velocity, size and lifetime variations of small bright …

The overall structure and the fine structure of the solar photosphere outside active regions
are largely understood, except possibly the important roles of a turbulent near-surface …

We present a comprehensive analysis of the physical parameters and relationships of
umbral dots (UDs), which assists in our understanding of the physical properties of the Sun …

In this investigation, oscillation periods in Mg ii k-line intensity, brightness temperature, and
Doppler velocity obtained above magnetic bright points (MBPs) are investigated. For this …

In order to clarify a possible role of small-scale dynamo in formation of solar magnetic field,
we suggest an observational test for small-scale dynamo action based on statistics of anti …

Context. Chromospheric swirls are related to convectively driven vortex flows and
considered to play a significant role in the dynamics and heating of the upper solar …