Simultaneous Observation of the Inner and Outer Electron Diffusion Region in Reconnection with Large Guide Field

This paper presents a simultaneous observation of the inner and outer electron diffusion region (EDR) at the dayside magnetopause by the magnetospheric multiscale (MMS) spacecraft. The EDR was observed in magnetic reconnection with a large guide field. The inner EDR was characterized by positive ${\...

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Main Authors: Z. C. Tian, M. Zhou, H. Y. Man, Z. H. Zhong, X. H. Deng, D. J. Gershman, Y. V. Khotyaintsev, C. T. Russell
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/acf9f4
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author Z. C. Tian
M. Zhou
H. Y. Man
Z. H. Zhong
X. H. Deng
D. J. Gershman
Y. V. Khotyaintsev
C. T. Russell
author_facet Z. C. Tian
M. Zhou
H. Y. Man
Z. H. Zhong
X. H. Deng
D. J. Gershman
Y. V. Khotyaintsev
C. T. Russell
author_sort Z. C. Tian
collection DOAJ
description This paper presents a simultaneous observation of the inner and outer electron diffusion region (EDR) at the dayside magnetopause by the magnetospheric multiscale (MMS) spacecraft. The EDR was observed in magnetic reconnection with a large guide field. The inner EDR was characterized by positive ${\boldsymbol{J}}\cdot {{\boldsymbol{E}}}^{{\prime} }$ while the outer EDR is manifested by negative ${\boldsymbol{J}}\cdot {{\boldsymbol{E}}}^{{\prime} }$ and opposite out-of-plane electric field to that in the inner EDR. One pair of the spacecraft detected the inner EDR while the other pair encountered the outer EDR. Moreover, the two pairs were on the opposite side of the X-line as they observed the bidirectional accelerated electron jets. The fortuitous formation of MMS allows us to estimate the maximum length of the inner EDR as ∼36 d _e and the lower bound of the reconnection rate as 0.142 ± 0.041. These observations have far-reaching implications for understanding the electron physics in reconnection.
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spelling doaj.art-53d75d957c734c2fbe8e742b0cdf26c72023-10-26T13:05:40ZengIOP PublishingThe Astrophysical Journal1538-43572023-01-0195714210.3847/1538-4357/acf9f4Simultaneous Observation of the Inner and Outer Electron Diffusion Region in Reconnection with Large Guide FieldZ. C. Tian0https://orcid.org/0000-0002-8251-8297M. Zhou1H. Y. Man2Z. H. Zhong3https://orcid.org/0000-0003-0617-4418X. H. Deng4D. J. Gershman5https://orcid.org/0000-0003-1304-4769Y. V. Khotyaintsev6https://orcid.org/0000-0001-5550-3113C. T. Russell7https://orcid.org/0000-0003-1639-8298School of Physics and Materials Science, Nanchang University , Nanchang 330031, People’s Republic of China ; monmentum82@gmail.com; Institute of Space Science and Technology, Nanchang University , Nanchang 330031, People’s Republic of ChinaSchool of Physics and Materials Science, Nanchang University , Nanchang 330031, People’s Republic of China ; monmentum82@gmail.com; Institute of Space Science and Technology, Nanchang University , Nanchang 330031, People’s Republic of ChinaInstitute of Space Science and Technology, Nanchang University , Nanchang 330031, People’s Republic of ChinaSchool of Physics and Materials Science, Nanchang University , Nanchang 330031, People’s Republic of China ; monmentum82@gmail.com; Institute of Space Science and Technology, Nanchang University , Nanchang 330031, People’s Republic of ChinaInstitute of Space Science and Technology, Nanchang University , Nanchang 330031, People’s Republic of ChinaNASA Goddard Space Flight Center , Greenbelt, MD, USASwedish Institute of Space Physics , Uppsala, SwedenUniversity of California , Los Angeles, Los Angeles, CA, USAThis paper presents a simultaneous observation of the inner and outer electron diffusion region (EDR) at the dayside magnetopause by the magnetospheric multiscale (MMS) spacecraft. The EDR was observed in magnetic reconnection with a large guide field. The inner EDR was characterized by positive ${\boldsymbol{J}}\cdot {{\boldsymbol{E}}}^{{\prime} }$ while the outer EDR is manifested by negative ${\boldsymbol{J}}\cdot {{\boldsymbol{E}}}^{{\prime} }$ and opposite out-of-plane electric field to that in the inner EDR. One pair of the spacecraft detected the inner EDR while the other pair encountered the outer EDR. Moreover, the two pairs were on the opposite side of the X-line as they observed the bidirectional accelerated electron jets. The fortuitous formation of MMS allows us to estimate the maximum length of the inner EDR as ∼36 d _e and the lower bound of the reconnection rate as 0.142 ± 0.041. These observations have far-reaching implications for understanding the electron physics in reconnection.https://doi.org/10.3847/1538-4357/acf9f4Magnetic fieldsSolar magnetic reconnectionPlasma astrophysicsPlasma physicsSpace plasmas
spellingShingle Z. C. Tian
M. Zhou
H. Y. Man
Z. H. Zhong
X. H. Deng
D. J. Gershman
Y. V. Khotyaintsev
C. T. Russell
Simultaneous Observation of the Inner and Outer Electron Diffusion Region in Reconnection with Large Guide Field
The Astrophysical Journal
Magnetic fields
Solar magnetic reconnection
Plasma astrophysics
Plasma physics
Space plasmas
title Simultaneous Observation of the Inner and Outer Electron Diffusion Region in Reconnection with Large Guide Field
title_full Simultaneous Observation of the Inner and Outer Electron Diffusion Region in Reconnection with Large Guide Field
title_fullStr Simultaneous Observation of the Inner and Outer Electron Diffusion Region in Reconnection with Large Guide Field
title_full_unstemmed Simultaneous Observation of the Inner and Outer Electron Diffusion Region in Reconnection with Large Guide Field
title_short Simultaneous Observation of the Inner and Outer Electron Diffusion Region in Reconnection with Large Guide Field
title_sort simultaneous observation of the inner and outer electron diffusion region in reconnection with large guide field
topic Magnetic fields
Solar magnetic reconnection
Plasma astrophysics
Plasma physics
Space plasmas
url https://doi.org/10.3847/1538-4357/acf9f4
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