S. Parenti

TL;DR: The Extreme Ultraviolet Imager (EUI) as discussed by the authors is part of the remote sensing instrument package of the ESA/NASA Solar Orbiter mission that will explore the inner heliosphere and observe the Sun from vantage points close to the Sun and out of the ecliptic.

TL;DR: The Spectral Imaging of the Coronal Environment (SPICE) instrument is a high-resolution imaging spectrometer operating at extreme ultraviolet (EUV) wavelengths as mentioned in this paper, which is used on the ESA/NASA Solar Orbiter mission.

TL;DR: The Spectral Imaging of the Coronal Environment (SPICE) instrument is a high-resolution imaging spectrometer operating at extreme ultraviolet wavelengths as discussed by the authors, which is used on the ESA/NASA Solar Orbiter mission.

TL;DR: In this article, the authors introduce the Science Activity Plan (SAP) of the Solar Orbiter, which groups objectives that require similar observations into solar Orbiter Observing Plans, resulting in a strategic, top-level view of the optimal opportunities for science observations during the mission lifetime.

TL;DR: The National Science Foundation's Daniel K. Inouye Solar Telescope (DKIST) will revolutionize our ability to measure, understand, and model the basic physical processes that control the structure and dynamics of the Sun and its atmosphere as discussed by the authors.