activity
20242026
collaborators

10 papers

astro-ph.SR2026

Chromospheric dynamics and turbulence regulate the solar FIP effect

Andy S. H. To, J. Martin Laming, Jeffrey Reep +1

Elemental abundance variations in the solar corona, commonly characterised by First Ionisation Potential (FIP) bias, provide crucial diagnostics of chromospheric processes. The pon…

astro-ph.SR2026

Sungrazer comets as analogs of star-planet magnetic interactions

L-S. Guité, A. Strugarek, A. J. Finley +5

Star-planet magnetic interactions (SPMIs) can transfer energy from an exoplanet to its host star via Alfvén waves when the planet orbits within a sub-Alfvénic stellar wind. Simil…

astro-ph.SR2025

Decomposing wave activity in the solar atmosphere: Shocks, jets and swirls in the quiet Sun

George Cherry, Boris Gudiksen, Adam J. Finley +1

Context. There remains much mystery about how or if wave-energy in the photosphere can be transferred sufficiently upwards through the solar atmosphere to contribute to coronal hea…

astro-ph.SR2025

Reconstructing the Sun's Alfvén surface and wind braking torque with Parker Solar Probe

Adam J. Finley

The Alfvén surface -- where the solar wind exceeds the local Alfvén speed as it expands into interplanetary space -- is now routinely probed by NASA's Parker Solar Probe (PSP) in…

astro-ph.SR2025

Weakened Magnetic Braking Signals the Collapse of the Global Stellar Dynamo

Travis S. Metcalfe, Jennifer L. van Saders, Marc H. Pinsonneault +7

Weakened magnetic braking (WMB) was originally proposed in 2016 to explain anomalously rapid rotation in old field stars observed by the Kepler mission. The proximate cause was sug…

astro-ph.SR2025

The magnetic and spin-down properties of slowly rotating fully convective M dwarfs

Victor See, Louis Amard, Stefano Bellotti +19

The evolution of the magnetism, winds and rotation of low-mass stars are all linked. One of the most common ways to probe the magnetic properties of low-mass stars is with the Zeem…