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 application of machine learning in solar physics has the potential to greatly enhance our
understanding of the complex processes that take place in the atmosphere of the Sun. By …

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 …

The chromosphere is a thin layer of the solar atmosphere that bridges the relatively cool
photosphere and the intensely heated transition region and corona. Compressible and …

Magnetic reconnection is a key mechanism involved in solar eruptions and is also a prime
possibility to heat the low corona to millions of degrees. Here, we present ultra-high …

Since the early 1970s, inversion techniques have become the most useful tool for inferring
the magnetic, dynamic, and thermodynamic properties of the solar atmosphere. Inversions …

Aims. This paper describes the Polarimetric and Helioseismic Imager on the Solar Orbiter
mission (SO/PHI), the first magnetograph and helioseismology instrument to observe the …

The production of science-ready data from major solar telescopes requires expertise beyond
that of the typical observer. This is a consequence of the increasing complexity of …

Abstract The joint Japan/US/UK Hinode mission includes the first large-aperture visible-light
solar telescope flown in space. One component of the Focal Plane Package of that …

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 …