Electron and Ion Dynamics in Reconnection Diffusion Regions

Abstract Magnetic reconnection is a fundamental plasma process responsible for the sometimes explosive release of magnetic energy in space and laboratory plasmas. Inside the diffusion regions of magnetic reconnection, the plasma becomes demagnetized and decouples from the magnetic field, enabling the change in magnetic topology necessary to power the energy release over larger scales. Since it was launched in 2015, the Magnetospheric MultiScale (MMS) mission has significantly advanced the understanding of the particle dynamics key to magnetic reconnection by providing high-resolution, in-situ measurements able to resolve ion and electron kinetic scales, i.e. a fraction of a gyroradius, that have confirmed theoretical predictions, revealed new phenomena, and refined existing models. These breakthroughs are critical for understanding not only space plasmas but also laboratory and astrophysical plasmas where magnetic reconnection occurs. In this work, we review the ion and electron dynamics occurring within the diffusion regions, in the inflow, along the separatrices, and downstream of the diffusion regions, in different reconnection configurations: symmetric, asymmetric, antiparallel, and guide field reconnection.

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Publication Details

Journal
Space Science Reviews
Published
2025-08-01
DOI
https://doi.org/10.1007/s11214-025-01197-z
Citations
4
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
4.62

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article

Electron and Ion Dynamics in Reconnection Diffusion Regions

M. R. Argall, Naoki Bessho, J. R. Shuster, J. P. Eastwood et al.
4 citations
Space Science Reviews
Ionosphere and magnetosphere dynamics
4.62
article

Electron and Ion Dynamics in Reconnection Diffusion Regions

M. R. Argall, Naoki Bessho, J. R. Shuster, J. P. Eastwood, B. Lavraud, D. B. Graham, M. Hesse, Sergio Toledo‐Redondo, Hiroshi Hasegawa, Yi‐Hsin Liu, Y. V. Khotyaintsev, Li‐Jen Chen, C. Norgren, J. Egedal, Louis Richard, J. C. Holmes
article en
4 citations

Abstract

Abstract Magnetic reconnection is a fundamental plasma process responsible for the sometimes explosive release of magnetic energy in space and laboratory plasmas. Inside the diffusion regions of magnetic reconnection, the plasma becomes demagnetized and decouples from the magnetic field, enabling the change in magnetic topology necessary to power the energy release over larger scales. Since it was launched in 2015, the Magnetospheric MultiScale (MMS) mission has significantly advanced the understanding of the particle dynamics key to magnetic reconnection by providing high-resolution, in-situ measurements able to resolve ion and electron kinetic scales, i.e. a fraction of a gyroradius, that have confirmed theoretical predictions, revealed new phenomena, and refined existing models. These breakthroughs are critical for understanding not only space plasmas but also laboratory and astrophysical plasmas where magnetic reconnection occurs. In this work, we review the ion and electron dynamics occurring within the diffusion regions, in the inflow, along the separatrices, and downstream of the diffusion regions, in different reconnection configurations: symmetric, asymmetric, antiparallel, and guide field reconnection.

Space Science ReviewsVol. 221(5)
Dartmouth College (US), Ames Research Center (US), Centre National de la Recherche Scientifique (FR), Goddard Space Flight Center (US), Swedish Institute of Space Physics (SE), Los Alamos National Laboratory (US), University of Wisconsin–Madison (US), Université de Bordeaux (FR), University of New Hampshire (US), Laboratoire d'Astrophysique de Bordeaux (FR), Institute of Space and Astronautical Science (JP), University of Bergen (NO), Imperial College London (GB), University of Maryland, College Park (US), Universidad de Murcia (ES)
Swedish National Space Agency, Knut och Alice Wallenbergs Stiftelse, Norges Forskningsråd
Affordable and clean energy
Openalex Percentile: Top 5%
Ionosphere and magnetosphere dynamics
4.62
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