Véronique Delouille

TL;DR: In this article, a feature recognition system for the Solar Dynamics Observatory (SDO) is presented, which can detect, trace, and analyze numerous phenomena, including flares, sigmoids, filaments, coronal dimmings, polarity inversion lines, sunspots, X-ray bright points, active regions, CORonal holes, EIT waves, and coronal mass ejections (CMEs), coronal oscillations).

TL;DR: In this paper, a set of segmentation procedures (known as the SPoCA-suite) is introduced to retrieve AR and CH properties on EUV images taken from SOHO-EIT, STEREO-EUVI, PROBA2-SWAP, and SDO-AIA.

TL;DR: In this paper, the authors analyzed forecasts submitted to the Community Coordinated Modeling Center at NASA's Goddard Space Flight Center over the last 6 years to answer the following questions: (1) How well do these models forecast the arrival time of CME-driven shocks? (2) What are the uncertainties associated with these forecasts? (3) Which model(s) perform best? (4) Have the models become more accurate during the past 6 years?

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: In this article, the solar UV radiometer LYRA is designed and manufactured by a Belgian-Swiss-German consortium (ROB, PMOD/WRC, IMOMEC, CSL, MPS and BISA) with additional international collaborations.