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 …

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 …

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 …

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 …

Small-scale internetwork (IN) features are thought to be the major source of fresh magnetic
flux in the quiet Sun. During its first science flight in 2009, the balloon-borne observatory …

The heating of the solar chromosphere remains one of the most important questions in solar
physics. Our current understanding is that small-scale internetwork (IN) magnetic fields play …

The removal of magnetic flux from the quiet-Sun photosphere is important for maintaining
the statistical steady state of the magnetic field there, for determining the magnetic flux …

The study of spatial and temporal scales on which small magnetic structures (magnetic
elements) are organized in the quiet Sun may be approached by determining how they are …

ABSTRACT G-band bright points (GBPs) are thought to be the foot-points of magnetic flux
tubes. The aim of this paper is to investigate the relation between the diffusion regimes of …