most citedSpectroscopic evidence of cool plasma in quiet Sun HRIEUV small scale brightenings

16 citations · 54 across the 6 of their papers we have counts for

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astro-ph.SR2025

Small EUV Brightenings in the Quiet Solar Atmosphere: New Insights from the Solar Orbiter Mission

Susanna Parenti

One of the many outcomes of the Solar Orbiter mission is the evidence for the solar atmosphere being filled by highly impulsive bursts, down to about 200 km scale: the limit of the…

astro-ph.SR2025★ 5 cited

The nature of small scale EUV solar brightenings investigated as impulsive heating of short loops in 1D hydrododynamics simulations

A. Dolliou, J. A. Klimchuk, S. Parenti +1

Small (400 to 4000 km) and short lived (10 to 200 km) extreme ultraviolet (EUV) brightenings, detected by the High Resolution Imager EUV (HRIEUV), have been found to be ubiquitous…

astro-ph.SR2024★ 14 cited

Spatial distributions of EUV brightenings in the quiet-Sun

C. J. Nelson, L. A. Hayes, D. Müller +16

The identification of large numbers of localised transient EUV brightenings, with small spatial scales, in the quiet-Sun corona has been one of the key early results from Solar Orb…

astro-ph.SR2024★ 3 cited

First Solar Orbiter observation of a dark halo in the solar atmosphere

Serena Maria Lezzi, David M. Long, Vincenzo Andretta +5

Solar active regions (ARs) are often surrounded by dark large areas of reduced emission compared to the quiet Sun, observed at various wavelengths corresponding to chromosphere, tr…

astro-ph.SR2024★ 16 cited

Spectroscopic evidence of cool plasma in quiet Sun HRIEUV small scale brightenings

A. Dolliou, S. Parenti, K. Bocchialini

Context: A large number of the small and the short-lived EUV brightenings have been detected in the quiet Sun (QS) over the past three years, by the High Resolution Imager of the E…

astro-ph.SR2024★ 16 cited

Observations of Fan-Spine Topology by Solar Orbiter/EUI: Rotational Motions and Indications of Alfvén Waves

E. Petrova, T. Van Doorsselaere, D. Berghmans +3

Torsional Alfvén waves do not produce any intensity variation and are, therefore, challenging to observe with imaging instruments. Previously, Alfvén wave observations were reporte…