From the 2 of 6 linked papers with an AI index.
1 citations · 1 across the 2 of their papers we have counts for
6 papers
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…
Full-Disk Spectroscopy of the Solar Corona Across a Solar Cycle with Hinode/EIS
James McKevitt, Ignacio Ugarte-Urra, Peter R. Young
The paper presents 18 full-disk spectroscopic observations of the solar corona from Hinode/EIS spanning 2013‑2024, showing that coronal intensity varies with the solar cycle mainly…
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…
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…
UK White Paper on Magnetic Reconnection
Alexander J. B. Russell, James A. McLaughlin, Philippa Browning +25
Magnetic reconnection powers explosive releases of magnetic energy, heating and particle acceleration throughout the plasma universe. Knowledge of this universal process is vital t…
Near-continuous tracking of solar active region NOAA 13664 over three solar rotations
I. Kontogiannis, Y. Zhu, K. Barczynski +6
Magnetic flux emergence and decay in the Sun span from days to months. However, their tracking is typically limited to about half a solar rotation when relying on single-vantage-po…