collaborators

5 papers

astro-ph.SR2026

Constraining turbulent solar flare acceleration regions by connecting kinetic modeling and X-ray observations

Morgan Stores, Natasha Jeffrey, Ewan Dickson +2

Spatially-resolved X-ray observations are the key to understanding electron acceleration in solar flares. Currently, the underlying processes that efficiently energize solar flare…

astro-ph.IM2026

UK White Paper on Magnetohydrodynamic (MHD) seismology of solar and heliospheric plasmas

Valery M. Nakariakov, David B. Jess, Andrew N. Wright +6

Magnetohydrodynamic (MHD) seismology uses naturally occurring MHD waves to infer plasma properties that are otherwise hard to measure, especially magnetic field strength and topolo…

astro-ph.IM2025

Understanding Solar Flares and Energetic Events: Open questions, observational requirements, and instrumental needs over the coming decade

Malcolm K. Druett, Graham S. Kerr, Joel C. Allred +15

Solar flares are the largest energy-release events in the Solar System, allowing us to study fundamental physical phenomena under extreme conditions. Those include magnetic reconne…

astro-ph.IM2025

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…

astro-ph.SR2025

Estimating the Poynting flux of Alfvénic waves in polar coronal holes across Solar Cycle 24

Richard J. Morton, Micah J. Weberg, N. Balodhi +1

Alfvénic waves are known to be prevalent throughout the corona and solar wind. Determining the Poynting flux supplied by the waves is required for constraining their role in plasm…