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20242026
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astro-ph.SR2026

Sulfur fractionation in coronal plumes as observed by Solar Orbiter/SPICE

Slimane Mzerguat, Miho Janvier, Eric Buchlin +4

Coronal plumes are bright, narrow structures rooted in coronal holes that contribute to the solar wind. Their composition, particularly elemental fractionation as a function of fir…

astro-ph.SR2025

Picoflares in the Quiet Solar Corona: Solar Orbiter Observations Halfway to the Sun

O. Podladchikova, A. Warmuth, L. Harra +33

X-ray observations of the Sun led Eugene Parker to propose nanoflares as the basic energy-release units that heat the solar corona. Decades later, Solar Orbiter's Extreme Ultraviol…

astro-ph.SR2024

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

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

Searching for evidence of subchromospheric magnetic reconnection on the Sun

D. Baker, L. van Driel-Gesztelyi, A. W. James +13

Within the coronae of stars, abundances of those elements with low first ionization potential (FIP) often differ from their photospheric values. The coronae of the Sun and solar-ty…