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 …

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

Extreme-ultraviolet images from the Solar Dynamics Observatory often show loop-like fine
structure to be present where no minority-polarity flux is visible in magnetograms …

Context. Magnetic energy is required to heat the corona, the outer atmosphere of the Sun, to
millions of degrees. Aims. We study the nature of the magnetic energy source that is …

The magnetic network (NE) observed on the solar surface harbors a sizable fraction of the
total quiet Sun flux. However, its origin and maintenance are not well known. Here we …

Context. Magnetic reconnection in the quiet Sun is a phenomenon that is consistently
observed, however, its conditions of occurrence are not as well known as for more energetic …

The distribution and evolution of photospheric magnetic fields in sunspots, plages, and
network, and variations in their relative flux content, play key roles in radial velocity (RV) …

Context. Understanding the evolution of the solar magnetic field is of great importance for
heliosphere, dynamo, and irradiance studies, for example. While the contribution of the field …

Small-scale internetwork magnetic fields are important ingredients of the quiet Sun. In this
paper we analyze how they appear and disappear on the solar surface. Using high …

The energy for the coronal heating must be provided from the convection zone. However,
the amount and the method by which this energy is transferred into the corona depend on …