Showing 1–20 of 46 results
/ Date/ Name
Apr 8, 2022Automatic detection of small-scale EUV brightenings observed by the Solar Orbiter/EUIMar 30, 2012Signatures of the slow solar wind streams from active regions in the inner coronaSep 5, 2021Stereoscopy of extreme UV quiet Sun brightenings observed by Solar Orbiter/EUIMar 28, 2023Evidence of external reconnection between an erupting mini-filament and ambient loops observed by Solar Orbiter/EUIJan 13, 2023First Perihelion of EUI on the Solar Orbiter missionSep 25, 2022Solar coronal heating from small-scale magnetic braidsApr 18, 2020Solar physics in the 2020s: DKIST, parker solar probe, and solar orbiter as a multi-messenger constellationOct 21, 2021First observations from the SPICE EUV spectrometer on Solar OrbiterAug 4, 2021Stereoscopic Measurements of Coronal Doppler VelocitiesNov 25, 2024Coronal hole picoflare jets are progenitors of both fast and Alfvénic slow solar windAug 24, 2023Picoflare jets power the solar wind emerging from a coronal hole on the SunJul 26, 2023Initial radiometric calibration of the High-Resolution EUV Imager ($\textrm{HRI}_\textrm{EUV}$) of the Extreme Ultraviolet Imager (EUI) instrument onboard Solar OrbiterFeb 9, 2021The active region source of a type III radio storm observed by Parker Solar Probe during Encounter 2Jan 5, 2023Temperature of Solar Orbiter/EUI quiet Sun small scale brightenings: evidence for a cooler componentJun 8, 2023EUV brightenings in the quiet-Sun: Signatures in spectral and imaging data from the Interface Region Imaging SpectrographNov 1, 2024Spatial distributions of EUV brightenings in the quiet-SunMar 21, 2023Observational Evidence of S-Web Source of the Slow Solar WindMar 15, 2025A magnetic avalanche as the central engine powering a solar flareApr 18, 2023Ultra-high-resolution Observations of Persistent Null-point Reconnection in the Solar CoronaMay 19, 2023EUV fine structure and variability associated with coronal rain revealed by Solar Orbiter/EUI HRIEUV and SPICE