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From the 1 of 6 linked papers with an AI index.

most citedPre-flare and active region plasma flows and structure seen by the short wavelength camera on SOLAR-C/EUVST

1 citations · 1 across the 2 of their papers we have counts for

collaborators

6 papers

astro-ph.SR2026

Exploring if a coronal dimming event can produce coronal hole-like properties

Adriana De-Sassi, Louise Harra, Krzysztof Barczynski +8

Coronal dimmings, or transient coronal holes, are manifested as a sudden reduction in extreme ultraviolet (EUV) and X-ray emission, often following solar eruptions. We investigate…

astro-ph.SR20261 cited

Pre-flare and active region plasma flows and structure seen by the short wavelength camera on SOLAR-C/EUVST

James McKevitt, Sarah Matthews, David H. Brooks +20

The paper uses forward modelling of the SOLAR-C/EUVST short‑wavelength camera to show how its high‑resolution EUV spectroscopy can resolve fine plasma flows and individual flux tub…

astro-ph.SR2026

Solar Orbiter observations of solar energetic electron events associated with hard microflares

Diane Mittaine, Andrea Francesco Battaglia, Laura Rodríguez-García +4

Generally, large solar flares accelerate electrons to high energies more efficiently than microflares. However, some microflares, known as hard microflares (HMFs), also produce hig…

astro-ph.SR2026

The Non-Eruptive Reconfiguration of a Quiescent Filament After a Nearby Active Region Emergence

James McKevitt, Louise Harra, Gherardo Valori +13

The unpredictability of solar filament eruptions presents major challenges for forecasting space weather, as such eruptions frequently drive coronal mass ejections (CMEs) that impa…

astro-ph.SR2024

Solar flares in the Solar Orbiter era: Short-exposure EUI/FSI observations of STIX flares

Hannah Collier, Laura A. Hayes, Stefan Purkhart +10

Aims: This paper aims to demonstrate the importance of short-exposure extreme ultraviolet (EUV) observations of solar flares in the study of particle acceleration, heating and ener…

astro-ph.SR2024

The observational evidence that all microflares that accelerate electrons to high energies are rooted in sunspots

Andrea Francesco Battaglia, Säm Krucker, Astrid M. Veronig +6

In general, large solar flares are more efficient at accelerating high-energy electrons than microflares. Nonetheless, we sometimes observe microflares that accelerate electrons to…