works on

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

collaborators

6 papers

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

The connection between solar coronal abundances and the underlying lower atmospheric properties

Paola Testa, Juan Martinez-Sykora, Bart De Pontieu +4

Elemental abundances in the solar corona and solar wind are often observed to differ from those in the solar photosphere, most commonly showing an enhancement of low first ionizati…

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

Radiative hydrodynamic simulations of FIP fractionation in solar flares

Jeffrey W. Reep, Luke Fushimi Benavitz, Andy S. H. To +5

Elemental abundances in solar flares are observed to vary both spatially and temporally, but the underlying mechanisms remain poorly understood. There is an interplay between advec…

astro-ph.SR2025

Systematic non-thermal velocity increase preceding soft X-ray flare onset: A large-scale Hinode/EIS study

Andy S. H. To, Abigail Burden, Deborah Baker +12

Non-thermal velocities, derived from spectral line broadening, can provide crucial insights into plasma dynamics before and during solar flares. To systematically study the pre-fla…

astro-ph.SR2025

Investigating Solar Wind Outflows from Open-Closed Magnetic Field Structures Using Coordinated Solar Orbiter and Hinode Observations

Nawin Ngampoopun, Roberto Susino, David H. Brooks +13

ESA/NASA's Solar Orbiter (SO) allows us to study the solar corona at closer distances and from different perspectives, which helps us to gain significant insights into the origins…