Waves and oscillations have been observed in the Sun's atmosphere for over half a century.
While such phenomena have readily been observed across the entire electromagnetic …

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 …

After emerging to the solar surface, the Sun's magnetic field displays a complex and intricate
evolution. The evolution of the surface field is important for several reasons. One is that the …

This publication provides an overview of magnetic fields in the solar atmosphere with the
focus lying on the corona. The solar magnetic field couples the solar interior with the visible …

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 …

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 …

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

The improved High-resolution Fast Imager (HiFI+) is a multiwavelength imaging filtergraph,
which was commissioned at the GREGOR solar telescope at Observatorio del Teide, Izaña …

Flow vorticity is a fundamental property of turbulent convection in rotating systems. Solar
supergranules exhibit a preferred sense of rotation, which depends on the hemisphere. This …

Small scale magnetic fields (magnetic elements) are ubiquitous in the solar photosphere.
Their interaction can provide energy to the upper atmospheric layers, and contribute to heat …