Characteristics of Energetic Electrons Near Active Magnetotail Reconnection Sites: Tracers of a Complex Magnetic Topology and Evidence of Localized Acceleration

Abstract We present detailed observations and reconstructed magnetic field topologies from a magnetic reconnection event observed directly by NASA's Magnetospheric Multiscale (MMS) mission. Comparing and contrasting energy and angular distributions of >50 keV electrons observed by three MMS...

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Main Authors: Drew L. Turner, Ian J. Cohen, Samuel T. Bingham, Grant K. Stephens, Mikhail I. Sitnov, Barry H. Mauk, Richard E. Denton, Trevor W. Leonard, Joseph F. Fennell, J. Bernard Blake, Roy B. Torbert, James L. Burch
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Language:English
Published: Wiley 2021-01-01
Series:Geophysical Research Letters
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Online Access:https://doi.org/10.1029/2020GL090089
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author Drew L. Turner
Ian J. Cohen
Samuel T. Bingham
Grant K. Stephens
Mikhail I. Sitnov
Barry H. Mauk
Richard E. Denton
Trevor W. Leonard
Joseph F. Fennell
J. Bernard Blake
Roy B. Torbert
James L. Burch
author_facet Drew L. Turner
Ian J. Cohen
Samuel T. Bingham
Grant K. Stephens
Mikhail I. Sitnov
Barry H. Mauk
Richard E. Denton
Trevor W. Leonard
Joseph F. Fennell
J. Bernard Blake
Roy B. Torbert
James L. Burch
author_sort Drew L. Turner
collection DOAJ
description Abstract We present detailed observations and reconstructed magnetic field topologies from a magnetic reconnection event observed directly by NASA's Magnetospheric Multiscale (MMS) mission. Comparing and contrasting energy and angular distributions of >50 keV electrons observed by three MMS spacecraft separated by only ∼18 km revealed a combination of chaotic motion and surprisingly coherent gyrophase bunching within a few thousand kilometers of the reconnection site. Such gyrophase‐bunched electrons have not been observed previously at these energies in relation to magnetic reconnection. Results indicate that the magnetic topology around the electron diffusion region was relatively stable over several seconds (i.e., more than a thousand electron gyro‐periods), and the observed gyrophase bunching may be the highest‐energy extent of coherent gyrophase structures observed at lower‐energies closer to the reconnection site. We hypothesize that the coherent gyrophase bunching was evidence of these energetic electrons being accelerated at the reconnection site and possibly also in the outflowing exhaust jets of the active reconnection. This case study exemplifies how energetic electrons can carry coherent signals of remote magnetic topologies and processes relevant to the physics of magnetic reconnection.
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spelling doaj-art-4d37a40041ac4154aafaff03b4759c2c2025-08-20T03:07:23ZengWileyGeophysical Research Letters0094-82761944-80072021-01-01482n/an/a10.1029/2020GL090089Characteristics of Energetic Electrons Near Active Magnetotail Reconnection Sites: Tracers of a Complex Magnetic Topology and Evidence of Localized AccelerationDrew L. Turner0Ian J. Cohen1Samuel T. Bingham2Grant K. Stephens3Mikhail I. Sitnov4Barry H. Mauk5Richard E. Denton6Trevor W. Leonard7Joseph F. Fennell8J. Bernard Blake9Roy B. Torbert10James L. Burch11Space Exploration Sector The Johns Hopkins University Applied Physics Laboratory Laurel MD USASpace Exploration Sector The Johns Hopkins University Applied Physics Laboratory Laurel MD USASpace Exploration Sector The Johns Hopkins University Applied Physics Laboratory Laurel MD USASpace Exploration Sector The Johns Hopkins University Applied Physics Laboratory Laurel MD USASpace Exploration Sector The Johns Hopkins University Applied Physics Laboratory Laurel MD USASpace Exploration Sector The Johns Hopkins University Applied Physics Laboratory Laurel MD USADepartment of Physics and Astronomy Dartmouth College Hanover NH USALaboratory for Atmospheric and Space Physics University of Colorado Boulder CO USADepartment of Space Sciences The Aerospace Corporation El Segundo CA USADepartment of Space Sciences The Aerospace Corporation El Segundo CA USADepartment of Physics and Astronomy University of New Hampshire Durham NH USASouthwest Research Institute San Antonio TX USAAbstract We present detailed observations and reconstructed magnetic field topologies from a magnetic reconnection event observed directly by NASA's Magnetospheric Multiscale (MMS) mission. Comparing and contrasting energy and angular distributions of >50 keV electrons observed by three MMS spacecraft separated by only ∼18 km revealed a combination of chaotic motion and surprisingly coherent gyrophase bunching within a few thousand kilometers of the reconnection site. Such gyrophase‐bunched electrons have not been observed previously at these energies in relation to magnetic reconnection. Results indicate that the magnetic topology around the electron diffusion region was relatively stable over several seconds (i.e., more than a thousand electron gyro‐periods), and the observed gyrophase bunching may be the highest‐energy extent of coherent gyrophase structures observed at lower‐energies closer to the reconnection site. We hypothesize that the coherent gyrophase bunching was evidence of these energetic electrons being accelerated at the reconnection site and possibly also in the outflowing exhaust jets of the active reconnection. This case study exemplifies how energetic electrons can carry coherent signals of remote magnetic topologies and processes relevant to the physics of magnetic reconnection.https://doi.org/10.1029/2020GL090089accelerationdiffusion regionelectronsmagnetic reconnectionplasma physics
spellingShingle Drew L. Turner
Ian J. Cohen
Samuel T. Bingham
Grant K. Stephens
Mikhail I. Sitnov
Barry H. Mauk
Richard E. Denton
Trevor W. Leonard
Joseph F. Fennell
J. Bernard Blake
Roy B. Torbert
James L. Burch
Characteristics of Energetic Electrons Near Active Magnetotail Reconnection Sites: Tracers of a Complex Magnetic Topology and Evidence of Localized Acceleration
Geophysical Research Letters
acceleration
diffusion region
electrons
magnetic reconnection
plasma physics
title Characteristics of Energetic Electrons Near Active Magnetotail Reconnection Sites: Tracers of a Complex Magnetic Topology and Evidence of Localized Acceleration
title_full Characteristics of Energetic Electrons Near Active Magnetotail Reconnection Sites: Tracers of a Complex Magnetic Topology and Evidence of Localized Acceleration
title_fullStr Characteristics of Energetic Electrons Near Active Magnetotail Reconnection Sites: Tracers of a Complex Magnetic Topology and Evidence of Localized Acceleration
title_full_unstemmed Characteristics of Energetic Electrons Near Active Magnetotail Reconnection Sites: Tracers of a Complex Magnetic Topology and Evidence of Localized Acceleration
title_short Characteristics of Energetic Electrons Near Active Magnetotail Reconnection Sites: Tracers of a Complex Magnetic Topology and Evidence of Localized Acceleration
title_sort characteristics of energetic electrons near active magnetotail reconnection sites tracers of a complex magnetic topology and evidence of localized acceleration
topic acceleration
diffusion region
electrons
magnetic reconnection
plasma physics
url https://doi.org/10.1029/2020GL090089
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