activity
20042025
most citedThe Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action

112 citations · 814 across the 21 of their papers we have counts for

collaborators

19 papers

astro-ph.SR2025★ 2 cited

Helical flows along coronal loops following the launch of a coronal mass ejection

Mohamed Nedal, David M. Long, Catherine Cuddy +2

Solar flares and coronal mass ejections (CMEs) are manifestations of energy release in the solar atmosphere, which can be accompanied by dynamic mass motions and waves in the surro…

astro-ph.SR2024

Spatially Resolved Plasma Composition Evolution in a Solar Flare -- The Effect of Reconnection Outflow

Andy S. H. To, David H. Brooks, Shinsuke Imada +6

Solar flares exhibit complex variations in elemental abundances compared to photospheric values. We examine the spatial and temporal evolution of coronal abundances in the X8.2 fla…

astro-ph.SR2023★ 27 cited

Observational Evidence of S-Web Source of the Slow Solar Wind

D. Baker, P. Demoulin, S. L. Yardley +25

From 2022 March 18-21, active region (AR) 12967 was tracked simultaneously by Solar Orbiter (SO) at 0.35 au and Hinode/EIS at Earth. During this period, strong blue-shifted plasma…

astro-ph.SR2020★ 15 cited

A new trigger mechanism for coronal mass ejections: the role of confined flares and photospheric motions in the formation of hot flux ropes

Alexander W James, Lucie M Green, Lidia van Driel-Gesztelyi +1

Context: Many previous studies have shown that the magnetic precursor of a coronal mass ejection (CME) takes the form of a magnetic flux rope, and a subset of them have become know…

astro-ph.SR2020★ 112 cited

The Solar Orbiter Science Activity Plan: translating solar and heliospheric physics questions into action

I. Zouganelis, A. De Groof, A. P. Walsh +182

Solar Orbiter is the first space mission observing the solar plasma both in situ and remotely, from a close distance, in and out of the ecliptic. The ultimate goal is to understand…

astro-ph.SR2020★ 23 cited

Can Sub-photospheric Magnetic Reconnection Change the Elemental Composition in the Solar Corona?

Deborah Baker, Lidia van Driel-Gesztelyi, David H. Brooks +6

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…