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 …

Aims. Solar Orbiter, the first mission of ESA's Cosmic Vision 2015–2025 programme and a
mission of international collaboration between ESA and NASA, will explore the Sun and …

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 …

Magnetic flux emergence from the solar convection zone into the overlying atmosphere is
the driver of a diverse range of phenomena associated with solar activity. In this article, we …

In this article we review small-scale dynamo processes that are responsible for magnetic
field generation on scales comparable to and smaller than the energy carrying scales of …

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 …

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 …

Stars appear darker at their limbs than at their disk centres because at the limb we are
viewing the higher and cooler layers of stellar photospheres. Yet, limb darkening derived …

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 …