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 …

Alfvén waves are considered to be viable transporters of the non-thermal energy required to
heat the Sun's quiescent atmosphere. An abundance of recent observations, from state-of …

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 …

It is amazing how wildly different-sized objects exist in the Universe! The red giant
Betelgeuse is so monstrously larger than our Sun that it could fill the orbit of Mars. But …

The physical processes that heat the solar corona and accelerate the solar wind remain
unknown after many years of study. Some have suggested that the wind is driven by waves …

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 use images of high spatial and temporal resolution, obtained with the Rapid Oscillations
in the Solar Atmosphere instrument at the Dunn Solar Telescope, to reveal how the …

We present high-cadence observations and simulations of the solar photosphere, obtained
using the Rapid Oscillations in the Solar Atmosphere imaging system and the MuRAM …

A number of observational and theoretical aspects of solar magnetoconvection are
considered in this review. We discuss recent developments in our understanding of the …

Bright points (BPs) in the solar photosphere are thought to be the radiative signatures (small-
scale brightness enhancements) of magnetic elements described by slender flux tubes or …