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 …

Observations of very quiet Sun using the Solar Optical Telescope/Spectro-Polarimeter
(SOT/SP) aboard the Hinode spacecraft reveal that the quiet internetwork regions are …

The magnetic field of the Sun is the underlying cause of the many diverse phenomena
combined under the heading of solar activity. Here we describe the magnetic field as it …

The infrared solar spectrum contains a wealth of physical data about our Sun, and is
explored using modern detectors and technology with new ground-based solar telescopes …

As we resolve ever smaller structures in the solar atmosphere, it has become clear that
magnetism is an important component of those small structures. Small-scale magnetism …

Magnetoconvection simulations on mesogranule and granule scales near the solar surface
are used to study the effect of convective motions on magnetic fields: the sweeping of …

Context. Owing to the limited spatial resolution and the weak polarization signal coming from
the quietest regions on the Sun, the organization of the magnetic field on the smallest scales …

The aim of this paper is to determine the flux emergence rate due to small-scale magnetic
features in the quiet Sun using high-resolution Hinode SOT NFI data. Small-scale magnetic …

Context. For many years, there seemed to be significant differences between the continuum
intensity distributions derived from observations and simulations of the solar photosphere …

Using turbulent MHD simulations (magnetic Reynolds numbers up to≈ 8000) and Hinode
observations, we study effects of turbulence on measuring the solar magnetic field outside …