collaborators

6 papers

astro-ph.SR2026

Tracking Magnetic Topological Change in a Time-Dependent Coronal Model

Emily I. Mason, Cooper Downs, Roberto Lionello +2

We apply the slip-back mapping method of Titov et al. 2009 and Lionello et al. 2020 to a thermodynamic MHD simulation to track topological changes in the magnetic field at a range…

astro-ph.SR2026

Magnetic switchback formation: a review of proposed mechanisms

Peter F. Wyper, Jonathan Squire, Etienne Pariat +19

Magnetic switchbacks are large amplitude deflections of the magnetic field within the solar wind. They are Alfvénic in character and so are associated with a spike in velocity and…

astro-ph.SR2026

Magnetic Connectivity in the Time-Dependent Corona and Heliosphere

Roberto Lionello, Cooper Downs, Emily I. Mason +3

Magnetic flux fills the heliosphere, expands outward from the solar corona, and is fundamentally related to the structure and dynamics of the solar corona and solar wind. Open magn…

astro-ph.SR2025

First detection of acoustic-like flux in the middle solar corona

V. Andretta, L. Abbo, G. Jerse +28

Waves are thought to play a significant role in the heating of the solar atmosphere and the acceleration of the wind. Among the many types of waves observed in the Sun, the so-call…

astro-ph.SR2025

Investigating Solar Wind Outflows from Open-Closed Magnetic Field Structures Using Coordinated Solar Orbiter and Hinode Observations

Nawin Ngampoopun, Roberto Susino, David H. Brooks +13

ESA/NASA's Solar Orbiter (SO) allows us to study the solar corona at closer distances and from different perspectives, which helps us to gain significant insights into the origins…

astro-ph.SR2025

Metis Observations of Alfvénic Outflows Driven by Interchange Reconnection in a Pseudostreamer

P. Romano, P. Wyper, V. Andretta +33

This study presents observations of a large pseudostreamer solar eruption and, in particular, the post-eruption relaxation phase, as captured by Metis onboard the Solar Orbiter on…