activity
20212025
most citedStereoscopy of extreme UV quiet Sun brightenings observed by Solar Orbiter/EUI

46 citations · 112 across the 6 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2025

Height-dependent thermal properties of extreme-ultraviolet campfires in the quiet Sun

O. Podladchikova, A. Warmuth, L. Harra +30

Small-scale impulsive energy-release events are widely considered a key ingredient of quiet-Sun coronal heating. We quantified the thermal-energy content of extreme ultraviolet (EU…

astro-ph.SR2023★ 1 cited

Initial radiometric calibration of the High-Resolution EUV Imager () of the Extreme Ultraviolet Imager (EUI) instrument onboard Solar Orbiter

S. Gissot, F. Auchère, D. Berghmans +21

The telescope was calibrated on ground at the Physikalisch-Technische Bundesanstalt (PTB), Germany's national metrology institute, using the Metrology L…

astro-ph.SR2023★ 16 cited

Beyond the disk: EUV coronagraphic observations of the Extreme Ultraviolet Imager on board Solar Orbiter

Auchère, F., Berghmans +58

Most observations of the solar corona beyond 2 Rs consist of broadband visible light imagery from coronagraphs. The associated diagnostics mainly consist of kinematics and derivati…

astro-ph.SR2023★ 19 cited

EUV fine structure and variability associated with coronal rain revealed by Solar Orbiter/EUI HRIEUV and SPICE

P. Antolin, A. Dolliou, F. Auchère +34

Coronal rain is the most dramatic cooling phenomenon of the solar corona and an essential diagnostic tool for the coronal heating properties. A puzzling feature of the solar corona…

astro-ph.SR2023★ 30 cited

First Perihelion of EUI on the Solar Orbiter mission

D. Berghmans, P. Antolin, F. Auchère +34

Context. The Extreme Ultraviolet Imager (EUI), onboard Solar Orbiter consists of three telescopes: the two High Resolution Imagers in EUV (HRIEUV) and in Lyman-α (HRILya), and the…

astro-ph.SR2021★ 46 cited

Stereoscopy of extreme UV quiet Sun brightenings observed by Solar Orbiter/EUI

A. N. Zhukov, M. Mierla, F. Auchère +27

The 3D fine structure of the solar atmosphere is still not fully understood as most of the available observations are taken from a single vantage point. The goal of the paper is to…