activity
20202026
most citedObservational Evidence of S-Web Source of the Slow Solar Wind

27 citations · 96 across the 16 of their papers we have counts for

collaborators

16 papers

astro-ph.IM2026

UK White Paper on Space-based total solar eclipse observations: structure and dynamics of the solar atmosphere

Lucie M. Green, Nicola Baresi, Huw Morgan +19

Our Sun is uniquely placed to enable a detailed study of astrophysical plasmas and how they are governed by the magnetic fields that thread through them. On the one hand, magnetic…

astro-ph.SR2026

Hinode EIS Observations of Plasma Composition Evolution and Radiative Cooling of Solar Flare Loops

Teodora Mihailescu, Peter R. Young, David H. Brooks +4

Plasma composition in flaring regions has been shown to have significant spatial and temporal variations, likely driven by dynamical processes that take place as a consequence of t…

astro-ph.SR2026

Probing the properties of active regions in the solar interface region using full-disk spectroheliograms

Éabha Power, David M. Long, Teodora Mihailescu +1

The composition of plasma in the solar corona is characterised by the First Ionisation Potential (FIP) bias, and is thought to be the result of a ponderomotive force acting in the…

astro-ph.SR2026★ 1 cited

Coronal Non-Thermal and Doppler Plasma Flows Driven by Photospheric Flux in 28 Active Regions

James McKevitt, Sarah Matthews, Deborah Baker +5

Magnetohydrodynamic (MHD) waves and/or the braiding of magnetic field lines are largely thought to be responsible for heating the solar corona, both being mechanisms which are driv…

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

Spectroscopic Observations of Supra-Arcade Downflows

Ryan J. French, Maria D. Kazachenko, Teodora Mihailescu +1

Despite their somewhat-frequent appearance in EUV imaging of off-limb flares, the origins of Supra-Arcade Downflows (SADs) remain a mystery. Appearing as dark, tendril-like downflo…

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…

astro-ph.SR2023

Intriguing Plasma Composition Pattern in a Solar Active Region: a Result of Non-Resonant Alfvén Waves?

Teodora Mihailescu, David H. Brooks, J. Martin Laming +6

The plasma composition of the solar corona is different from that of the solar photosphere. Elements that have a low first ionisation potential (FIP) are preferentially transported…

astro-ph.SR2023★ 11 cited

Slow Solar Wind Connection Science during Solar Orbiter's First Close Perihelion Passage

Stephanie L. Yardley, Christopher J. Owen, David M. Long +76

The Slow Solar Wind Connection Solar Orbiter Observing Plan (Slow Wind SOOP) was developed to utilise the extensive suite of remote sensing and in situ instruments on board the ESA…

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.SR2022★ 5 cited

The magnetic field environment of active region 12673 that produced the energetic particle events of September 2017

Stephanie L. Yardley, Lucie M. Green, Alexander W. James +2

Forecasting solar energetic particles (SEPs), and identifying flare/CMEs from active regions (ARs) that will produce SEP events in advance is extremely challenging. We investigate…

astro-ph.SR2022★ 16 cited

What determines active region coronal plasma composition?

Teodora Mihailescu, Deborah Baker, Lucie M. Green +4

The chemical composition of the solar corona is different from that of the solar photosphere, with the strongest variation being observed in active regions (ARs). Using data from t…

astro-ph.SR2021★ 12 cited

Evolution of Plasma Composition in an Eruptive Flux Rope

Deborah Baker, Lucie M. Green, David H. Brooks +8

Magnetic flux ropes are bundles of twisted magnetic field enveloping a central axis. They harbor free magnetic energy and can be progenitors of coronal mass ejections (CMEs), but i…

astro-ph.SR2021★ 7 cited

Plasma Upflows Induced by Magnetic Reconnection Above an Eruptive Flux Rope

Deborah Baker, Teodora Mihailescu, Pascal Demoulin +6

One of the major discoveries of Hinode's Extreme-ultraviolet Imaging Spectrometer (EIS) is the presence of upflows at the edges of active regions. As active regions are magneticall…

physics.plasm-ph2021★ 11 cited

First radiative shock experiments on the SG-II laser

Francisco Suzuki-Vidal, Thomas Clayson, Chantal Stehlé +17

We report on the design and first results from experiments looking at the formation of radiative shocks on the Shenguang-II (SG-II) laser at the Shanghai Institute of Optics and Fi…

astro-ph.EP2020★ 6 cited

Spatial variations of low mass negative ions in Titan's upper atmosphere

Teodora Mihailescu, Ravindra Desai, Oleg Shebanits +5

Observations with Cassini's Electron Spectrometer discovered negative ions in Titan's ionosphere, at altitudes between 1400 and 950 km. Within the broad mass distribution extending…