activity
20242026
collaborators

8 papers

astro-ph.SR2026

Solar Wind Dependence on Source Distance from the Open-Closed Boundary

Chloe P. Wilkins, David I. Pontin, Anthony R. Yeates +2

The origin and variability of the slow solar wind remains an open question in solar physics, but is thought to be closely linked to dynamics at the Sun's open-closed magnetic flux…

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

Global Coronal Equilibria with Solar Wind Outflow II -- Optimizing the Outflow Model

Oliver Rice, Anthony Yeates

We expand upon our paper (Rice and Yeates, 2021) which introduced `Outflow Fields': alternatives to the widely-used potential field source surface (PFSS) extrapolations of the Sun'…

astro-ph.SR2026

Energy Bounds from Relative Magnetic Helicity in Spherical Shells

Anthony R. Yeates, Gunnar Hornig

Relative magnetic helicity is commonly used in solar physics to avoid the well known gauge ambiguity of standard magnetic helicity in magnetically open domains. But its physical in…

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

Witnessing Magnetic Reconnection in Tangled Superpenumbral Fibrils Around a Sunspot

Hechao Chen, Hui Tian, Eric R. Priest +8

Three-dimensional magnetic reconnection is a fundamental plasma process crucial for heating the solar corona and generating the solar wind, but resolving and characterizing it on t…