Javier Rodriguez-Pacheco

TL;DR: The first mission of ESA's Cosmic Vision 2015-2025 programme and a mission of international collaboration between ESA and NASA, was launched on 10 February 2020 04:03 UTC from Cape Canaveral and aims to address key questions of solar and heliospheric physics pertaining to how the Sun creates and controls the Heliosphere, and why solar activity changes with time.

TL;DR: In this paper, the authors assess the current status of research relating the origin at the Sun, the evolution through the inner heliosphere and the effects on the interplanetary counterparts of coronal mass ejections.

TL;DR: In this article, the authors conclude that the particle increases observed at multiple locations had a common single-source active region and the energetic particles filled a very broad region around the Sun, which was the source of a large flare, a fast and wide coronal mass ejection, and an EIT wave, accompanied by type II and type III radio emission.

TL;DR: The Spectrometer Telescope for Imaging X-rays (STIX) as mentioned in this paper is a hard X-ray imaging spectrometer, which covers the energy range from 4 to 150 keV and provides diagnostics of the hottest (⪆10 MK) flare plasma while quantifying the location, spectrum, and energy content of flare-accelerated nonthermal electrons.

TL;DR: The Solar Wind Analyser (SWA) suite as discussed by the authors is a suite of three sensors, including an electron analyser, a Proton and alpha particle sensor, and a heavy ion sensor.