2D Reconstruction of Magnetotail Electron Diffusion Region Measured by MMS

Models for collisionless magnetic reconnection in near‐Earth space are distinctly characterized as 2D or 3D. In 2D kinetic models, the frozen‐in law for the electron fluid is usually broken by laminar dynamics involving structures set by the electron orbit size, while in 3D models the width of the e...

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Published inGeophysical research letters Vol. 49; no. 19
Main Authors Schroeder, J. M., Egedal, J., Cozzani, G., Khotyaintsev, Yu. V., Daughton, W., Denton, R. E., Burch, J. L.
Format Journal Article
LanguageEnglish
Published Washington John Wiley & Sons, Inc 16.10.2022
American Geophysical Union (AGU)
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Abstract Models for collisionless magnetic reconnection in near‐Earth space are distinctly characterized as 2D or 3D. In 2D kinetic models, the frozen‐in law for the electron fluid is usually broken by laminar dynamics involving structures set by the electron orbit size, while in 3D models the width of the electron diffusion region is broadened by turbulent effects. We present an analysis of in situ spacecraft observations from the Earth's magnetotail of a fortuitous encounter with an active reconnection region, mapping the observations onto a 2D spatial domain. While the event likely was perturbed by low‐frequency 3D dynamics, the structure of the electron diffusion region remains consistent with results from a 2D kinetic simulation. As such, the event represents a unique validation of 2D kinetic, and laminar reconnection models. Plain Language Summary Magnetic reconnection is a fundamental process that occurs in the near‐Earth space environment with implications for the safety and longevity of space‐borne electronics in which magnetic field lines rearrange and release energy. To understand whether reconnection is better described as occurring in a 2D‐plane without variation in the third direction versus 3D with variation in all directions, we analyze spacecraft data from the night‐side of Earth's magnetic field. We conclude for the considered event that the innermost region, where the field lines reconnect, remains consistent with results from a 2D simulation. Key Points The fluctuating measurements are consistent with a 2D reconnecting geometry, permitting a detailed spacecraft trajectory to be determined The Magnetospheric Multiscale Mission data is projected onto a 2D spatial domain, revealing the fine‐scale structure of the electron diffusion region (EDR) The EDR includes profiles with strong gradients in fields and flows, consistent with those observed in a matched 2D kinetic simulation
AbstractList Models for collisionless magnetic reconnection in near-Earth space are distinctly characterized as 2D or 3D. In 2D kinetic models, the frozen-in law for the electron fluid is usually broken by laminar dynamics involving structures set by the electron orbit size, while in 3D models the width of the electron diffusion region is broadened by turbulent effects. We present an analysis of in situ spacecraft observations from the Earth's magnetotail of a fortuitous encounter with an active reconnection region, mapping the observations onto a 2D spatial domain. While the event likely was perturbed by low-frequency 3D dynamics, the structure of the electron diffusion region remains consistent with results from a 2D kinetic simulation. As such, the event represents a unique validation of 2D kinetic, and laminar reconnection models.
Models for collisionless magnetic reconnection in near‐Earth space are distinctly characterized as 2D or 3D. In 2D kinetic models, the frozen‐in law for the electron fluid is usually broken by laminar dynamics involving structures set by the electron orbit size, while in 3D models the width of the electron diffusion region is broadened by turbulent effects. We present an analysis of in situ spacecraft observations from the Earth's magnetotail of a fortuitous encounter with an active reconnection region, mapping the observations onto a 2D spatial domain. While the event likely was perturbed by low‐frequency 3D dynamics, the structure of the electron diffusion region remains consistent with results from a 2D kinetic simulation. As such, the event represents a unique validation of 2D kinetic, and laminar reconnection models. Magnetic reconnection is a fundamental process that occurs in the near‐Earth space environment with implications for the safety and longevity of space‐borne electronics in which magnetic field lines rearrange and release energy. To understand whether reconnection is better described as occurring in a 2D‐plane without variation in the third direction versus 3D with variation in all directions, we analyze spacecraft data from the night‐side of Earth's magnetic field. We conclude for the considered event that the innermost region, where the field lines reconnect, remains consistent with results from a 2D simulation. The fluctuating measurements are consistent with a 2D reconnecting geometry, permitting a detailed spacecraft trajectory to be determined The Magnetospheric Multiscale Mission data is projected onto a 2D spatial domain, revealing the fine‐scale structure of the electron diffusion region (EDR) The EDR includes profiles with strong gradients in fields and flows, consistent with those observed in a matched 2D kinetic simulation
Models for collisionless magnetic reconnection in near‐Earth space are distinctly characterized as 2D or 3D. In 2D kinetic models, the frozen‐in law for the electron fluid is usually broken by laminar dynamics involving structures set by the electron orbit size, while in 3D models the width of the electron diffusion region is broadened by turbulent effects. We present an analysis of in situ spacecraft observations from the Earth's magnetotail of a fortuitous encounter with an active reconnection region, mapping the observations onto a 2D spatial domain. While the event likely was perturbed by low‐frequency 3D dynamics, the structure of the electron diffusion region remains consistent with results from a 2D kinetic simulation. As such, the event represents a unique validation of 2D kinetic, and laminar reconnection models. Plain Language Summary Magnetic reconnection is a fundamental process that occurs in the near‐Earth space environment with implications for the safety and longevity of space‐borne electronics in which magnetic field lines rearrange and release energy. To understand whether reconnection is better described as occurring in a 2D‐plane without variation in the third direction versus 3D with variation in all directions, we analyze spacecraft data from the night‐side of Earth's magnetic field. We conclude for the considered event that the innermost region, where the field lines reconnect, remains consistent with results from a 2D simulation. Key Points The fluctuating measurements are consistent with a 2D reconnecting geometry, permitting a detailed spacecraft trajectory to be determined The Magnetospheric Multiscale Mission data is projected onto a 2D spatial domain, revealing the fine‐scale structure of the electron diffusion region (EDR) The EDR includes profiles with strong gradients in fields and flows, consistent with those observed in a matched 2D kinetic simulation
Author Denton, R. E.
Egedal, J.
Cozzani, G.
Burch, J. L.
Schroeder, J. M.
Khotyaintsev, Yu. V.
Daughton, W.
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CitedBy_id crossref_primary_10_1063_5_0130417
crossref_primary_10_1029_2024GL108895
crossref_primary_10_1103_PhysRevLett_131_155101
crossref_primary_10_1029_2022JA030512
Cites_doi 10.1088/1742-6596/180/1/012055
10.1029/RG015i001p00113
10.1063/1.2937193
10.1029/2022JA030408
10.1103/PhysRevLett.110.135004
10.1103/PhysRevLett.127.215101
10.3847/1538-4357/aaf16f
10.1029/91JA00984
10.1029/rg013i001p00303
10.1038/s41467-022-30561-8
10.1029/2021GL093164
10.1080/14786440708521050
10.1007/s11214-015-0164-9
10.1029/GL004i003p00125
10.1103/PhysRevLett.123.225101
10.1029/2019JA027481
10.1146/annurev-astro-082708-101726
10.1029/1999ja001006
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References 2009; 47
2021; 48
1977; 15
2009; 180
2020
1991; 96
2021; 127
1975; 13
2022; 13
1977; 4
2016; 199
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2019; 123
2022; 127
2001; 106
e_1_2_7_6_1
e_1_2_7_5_1
e_1_2_7_4_1
e_1_2_7_3_1
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e_1_2_7_8_1
e_1_2_7_7_1
e_1_2_7_19_1
e_1_2_7_18_1
e_1_2_7_16_1
e_1_2_7_2_1
e_1_2_7_15_1
e_1_2_7_14_1
e_1_2_7_13_1
Paschmann G. (e_1_2_7_17_1) 1998; 1
e_1_2_7_12_1
e_1_2_7_11_1
e_1_2_7_10_1
e_1_2_7_21_1
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References_xml – volume: 13
  start-page: 303
  issue: 1
  year: 1975
  end-page: 336
  article-title: Theoretical models of magnetic‐field line merging 1
  publication-title: Reviews of Geophysics
– volume: 870
  issue: 1
  year: 2019
  article-title: Observations of an electron diffusion region in symmetric reconnection with weak guide field
  publication-title: The Astrophysical Journal
– volume: 1
  year: 1998
  article-title: Analysis methods for multi‐spacecraft data. ISSI scientific reports series SR‐001, ESA/ISSI
  publication-title: ISSI Scientific Reports Series, 1
– volume: 79
  issue: 6
  year: 2008
  article-title: Magnetic flux array for spontaneous magnetic reconnection experiments
  publication-title: Review of Scientific Instruments
– volume: 44
  start-page: 725
  issue: 354
  year: 1953
  end-page: 738
  article-title: Conditions for the occurrence of electrical discharges in astrophysical systems
  publication-title: Philosophical Magazine
– volume: 106
  start-page: 3783
  issue: A3
  year: 2001
  end-page: 3798
  article-title: Geospace Environment Modeling magnetic reconnection challenge: Simulations with a full particle electromagnetic code
  publication-title: Geospace environment modeling magnetic reconnection challenge: Simulations with a full particle electromagnetic code
– year: 2020
– volume: 180
  year: 2009
  article-title: Advances in petascale kinetic plasma simulation with VPIC and Roadrunner
  publication-title: Journal of Physics: Conference Series
– volume: 199
  start-page: 5
  issue: 1
  year: 2016
  end-page: 21
  article-title: Magnetospheric multiscale overview and science objectives
  publication-title: Space Science Reviews
– volume: 127
  issue: 7
  year: 2022
  article-title: Magnetic field annihilation in a magnetotail electron diffusion region with electron‐scale magnetic islands
  publication-title: Journal of Geophysical Research: Space Physics
– volume: 123
  issue: 22
  year: 2019
  article-title: Pressure tensor elements breaking the frozen‐in law during reconnection in earth’s magnetotail
  publication-title: Physical Review Letters
– volume: 48
  issue: 16
  year: 2021
  article-title: Upper‐hybrid waves driven by meandering electrons around magnetic reconnection x line
  publication-title: Geophysical Research Letters
– volume: 13
  issue: 1
  year: 2022
  article-title: Direct observations of anomalous resistivity and diffusion in collisionless plasma
  publication-title: Nature Communications
– volume: 96
  start-page: 11555
  issue: A7
  year: 1991
  end-page: 11567
  article-title: Forced magnetic reconnection in a plasma sheet with localized resistivity profile excited by lower hybrid drift type instability
  publication-title: Journal of Geophysical Research
– volume: 15
  start-page: 113
  issue: 1
  year: 1977
  end-page: 127
  article-title: A review of anomalous resistivity for the ionosphere
  publication-title: Reviews of Geophysics
– volume: 125
  issue: 2
  year: 2020
  article-title: Polynomial reconstruction of the reconnection magnetic field observed by multiple spacecraft
  publication-title: Journal of Geophysical Research: Space Physics
– volume: 4
  start-page: 125
  issue: 3
  year: 1977
  end-page: 128
  article-title: The lower‐hybrid‐drift instability as a source of anomalous resistivity for magnetic field line reconnection
  publication-title: Geophysical Research Letters
– volume: 110
  issue: 13
  year: 2013
– volume: 127
  issue: 21
  year: 2021
  article-title: Structure of a perturbed magnetic reconnection electron diffusion region in the earth’s magnetotail
  publication-title: Physical Review Letters
– volume: 47
  start-page: 291
  issue: 1
  year: 2009
  end-page: 332
  article-title: Magnetic reconnection in astrophysical and laboratory plasmas
  publication-title: Annual Review of Astronomy and Astrophysics
– ident: e_1_2_7_3_1
  doi: 10.1088/1742-6596/180/1/012055
– ident: e_1_2_7_16_1
  doi: 10.1029/RG015i001p00113
– ident: e_1_2_7_13_1
  doi: 10.1063/1.2937193
– ident: e_1_2_7_10_1
  doi: 10.1029/2022JA030408
– ident: e_1_2_7_2_1
– ident: e_1_2_7_14_1
  doi: 10.1103/PhysRevLett.110.135004
– ident: e_1_2_7_5_1
  doi: 10.1103/PhysRevLett.127.215101
– ident: e_1_2_7_20_1
  doi: 10.3847/1538-4357/aaf16f
– ident: e_1_2_7_11_1
  doi: 10.1029/91JA00984
– ident: e_1_2_7_19_1
  doi: 10.1029/rg013i001p00303
– ident: e_1_2_7_9_1
  doi: 10.1038/s41467-022-30561-8
– ident: e_1_2_7_15_1
  doi: 10.1029/2021GL093164
– ident: e_1_2_7_7_1
  doi: 10.1080/14786440708521050
– volume: 1
  year: 1998
  ident: e_1_2_7_17_1
  article-title: Analysis methods for multi‐spacecraft data. ISSI scientific reports series SR‐001, ESA/ISSI
  publication-title: ISSI Scientific Reports Series, 1
  contributor:
    fullname: Paschmann G.
– ident: e_1_2_7_4_1
  doi: 10.1007/s11214-015-0164-9
– ident: e_1_2_7_12_1
  doi: 10.1029/GL004i003p00125
– ident: e_1_2_7_8_1
  doi: 10.1103/PhysRevLett.123.225101
– ident: e_1_2_7_6_1
  doi: 10.1029/2019JA027481
– ident: e_1_2_7_21_1
  doi: 10.1146/annurev-astro-082708-101726
– ident: e_1_2_7_18_1
  doi: 10.1029/1999ja001006
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Snippet Models for collisionless magnetic reconnection in near‐Earth space are distinctly characterized as 2D or 3D. In 2D kinetic models, the frozen‐in law for the...
Models for collisionless magnetic reconnection in near-Earth space are distinctly characterized as 2D or 3D. In 2D kinetic models, the frozen-in law for the...
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SubjectTerms Aerospace environments
Diffusion
Dynamics
Earth
Electron diffusion
Electrons
Fluid flow
Geomagnetic field
Geomagnetic tail
Image reconstruction
Magnetic field
Magnetic fields
Magnetic reconnection
magnetosphere
magnetotail
Magnetotails
Modelling
Orbital mechanics
reconnection
Simulation
Spacecraft
Three dimensional models
Two dimensional models
Title 2D Reconstruction of Magnetotail Electron Diffusion Region Measured by MMS
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