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 …

The Sunrise balloon-borne solar observatory consists of a 1 m aperture Gregory telescope,
a UV filter imager, an imaging vector polarimeter, an image stabilization system, and further …

The Sunrise balloon-borne solar observatory, consisting of a 1 m aperture telescope that
provides a stabilized image to a UV filter imager and an imaging vector polarimeter, carried …

Aims. We use new data from the High-resolution Coronal Imager (Hi-C) with its
unprecedented spatial resolution of the solar corona to investigate the structure of coronal …

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 solar atmosphere is known to be replete with magneto-hydrodynamic wave modes, and
there has been significant investment in understanding how these waves propagate through …

Arch-like loop structures filled with million Kelvin hot plasma form the building blocks of the
quiet-Sun corona. Both high-resolution observations and magnetoconvection simulations …

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 …

Aims. Within the quiet Sun corona imaged at 1 MK, much of the field of view consists of
diffuse emission that appears to lack the spatial structuring that is so evident in coronal loops …