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 …

Context. The heating of the solar corona by small heating events requires an increasing
number of such events at progressively smaller scales, with the bulk of the heating occurring …

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 …

After decades of observations of solar energetic particles from space-based observatories,
relevant questions on particle injection, transport, and acceleration remain open. To address …

Context. The Extreme Ultraviolet Imager (EUI) is part of the remote sensing instrument
package of the ESA/NASA Solar Orbiter mission that will explore the inner heliosphere and …

Aims. The Spectral Imaging of the Coronal Environment (SPICE) instrument is a high-
resolution imaging spectrometer operating at extreme ultraviolet wavelengths. In this paper …

Context. Recent observations by the Extreme Ultraviolet Imager (EUI) on board Solar Orbiter
have characterized prevalent small-scale transient brightenings in the corona above the …

The magnetometer instrument on the Solar Orbiter mission is designed to measure the
magnetic field local to the spacecraft continuously for the entire mission duration. The need …

Aims. Metis is the first solar coronagraph designed for a space mission and is capable of
performing simultaneous imaging of the off-limb solar corona in both visible and UV light …