TY - UNPB
T1 - UK White Paper on Magnetic Reconnection
T2 - White paper submitted to UK Space Frontiers 2035 on 28 November 2025
AU - Russell, Alexander
AU - Agudelo Rueda, Jeffersson Andres
AU - Bate, William
AU - Browning, Philippa
AU - Carter, Jennifer
AU - Del Zanna, Giulio
AU - Eastwood, Jonathan
AU - Franci, Luca
AU - Green, Lucie
AU - Hietala, Heli
AU - Hillier, Andrew
AU - Hornig, Gunnar
AU - Kumari, Anshu
AU - Lockwood, Mike
AU - MacTaggart, David
AU - Matthews, Sarah
AU - McKevitt, James
AU - McLaughlin, James
AU - Neukirch, Thomas
AU - Pontin, David
AU - Priest, Eric
AU - Reid , Jack
AU - Smith, Andy
AU - Snow, Ben
AU - Stawarz, Julia
AU - Walach, Maria-Theresia
AU - Wyper, Peter
AU - Yeates, Anthony
PY - 2025/12/12
Y1 - 2025/12/12
N2 - Magnetic reconnection powers explosive releases of magnetic energy, heating and particle acceleration throughout the plasma universe. Knowledge of this universal process is vital to understanding the Heliosphere, as it plays a key role in solar flares, coronal mass ejections, coronal heating, solar wind acceleration, geomagnetic storms, and interactions between the solar wind and planetary magnetospheres. As such, reconnection underpins multiple science objectives of multiple future space missions. The UK plays a leading role in this international field, through a combination of in situ measurements from Earth's magnetosphere and the solar wind, observations of the solar corona and chromosphere, and world-class numerical simulations and theory. This white paper identifies: Nine priority science objectives for reconnection research in the next decade; Recommendations to guide investment in theory, simulations and infrastructure; Mission priorities and required measurements to ensure the UK maintains and improves its world-class credentials in reconnection science.
AB - Magnetic reconnection powers explosive releases of magnetic energy, heating and particle acceleration throughout the plasma universe. Knowledge of this universal process is vital to understanding the Heliosphere, as it plays a key role in solar flares, coronal mass ejections, coronal heating, solar wind acceleration, geomagnetic storms, and interactions between the solar wind and planetary magnetospheres. As such, reconnection underpins multiple science objectives of multiple future space missions. The UK plays a leading role in this international field, through a combination of in situ measurements from Earth's magnetosphere and the solar wind, observations of the solar corona and chromosphere, and world-class numerical simulations and theory. This white paper identifies: Nine priority science objectives for reconnection research in the next decade; Recommendations to guide investment in theory, simulations and infrastructure; Mission priorities and required measurements to ensure the UK maintains and improves its world-class credentials in reconnection science.
KW - magnetic reconnection
U2 - 10.48550/arXiv.2512.11631
DO - 10.48550/arXiv.2512.11631
M3 - Working paper
BT - UK White Paper on Magnetic Reconnection
PB - arXiv
ER -