activity
20132026
most citedA Breakout Model for Solar Coronal Jets with Filaments

146 citations · 1.1k across the 35 of their papers we have counts for

collaborators
Showing 2025Show all

6 papers · 1 filter

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

Solar Eruption Onset and Particle Acceleration in Nested-Null Topologies

Pankaj Kumar, Judith T. Karpen, Peter F. Wyper +3

The magnetic breakout model explains a variety of solar eruptions, ranging from small-scale jets to large-scale coronal mass ejections (CMEs). Most of our previous studies are focu…

astro-ph.SR2025

Determining the 3D Dynamics of Solar Flare Magnetic Reconnection

Joel T. Dahlin, Spiro K. Antiochos, Peter F. Wyper +2

Solar flares are major space weather events that result from the explosive conversion of stored magnetic energy into bulk motion, plasma heating, and particle acceleration. While t…

astro-ph.SR2025★ 2 cited

Helmet streamer influence on the evolution of magnetic flux ropes

M. Cécere, P. F. Wyper, G. Krause +2

Context: Solar eruptions are crucial for space weather studies. Understanding the mechanisms influencing their evolution is key to improving predictions of their geoeffectiveness.…

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…

astro-ph.SR2025★ 10 cited

Synthetic Remote-sensing and In-situ Observations of Fine-scale Structure in a Pseudostreamer Coronal Mass Ejection through the Solar Corona

B. J. Lynch, P. F. Wyper, E. Palmerio +11

Coronal pseudostreamer flux systems have a specific magnetic configuration that influences the morphology and evolution of coronal mass ejections (CMEs) from these regions. Here we…