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Title: Electron diffusion region during magnetopause reconnection with an intermediate guide field: Magnetospheric multiscale observations

Journal Article · · Journal of Geophysical Research. Space Physics
DOI:https://doi.org/10.1002/2017JA024004· OSTI ID:1466266
ORCiD logo [1];  [2]; ORCiD logo [1]; ORCiD logo [1]; ORCiD logo [3]; ORCiD logo [4]; ORCiD logo [1]; ORCiD logo [5]; ORCiD logo [2];  [6]; ORCiD logo [7];  [2]; ORCiD logo [2]; ORCiD logo [2]; ORCiD logo [8]; ORCiD logo [9]; ORCiD logo [9]; ORCiD logo [10]; ORCiD logo [11]; ORCiD logo [1]
  1. NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States); Univ. of Maryland, College Park, MD (United States)
  2. NASA Goddard Space Flight Center (GSFC), Greenbelt, MD (United States)
  3. Univ. of Colorado, Boulder, CO (United States)
  4. Southwest Research Institute, San Antonio, TX (United States)
  5. Southwest Research Institute, San Antonio, TX (United States); Univ. of New Hampshire, Durham, NH (United States)
  6. Rice Univ., Houston, TX (United States)
  7. Denali Scientific, Healy, AK (United States)
  8. Univ. de Toulouse, Toulouse (France); Centre National de la Recherche Scientifique, Toulouse (France)
  9. Univ. of California, Los Angeles, CA (United States)
  10. Swedish Institute of Space Physics, Uppsala (Sweden)
  11. KTH Royal Institute of Technology, Stockholm (Sweden)

An electron diffusion region (EDR) in magnetic reconnection with a guide magnetic field approximately 0.2 times the reconnecting component is encountered by the four Magnetospheric Multiscale spacecraft at the Earth's magnetopause. The distinct substructures in the EDR on both sides of the reconnecting current sheet are visualized with electron distribution functions that are 2 orders of magnitude higher cadence than ever achieved to enable the following new findings: (1) Motion of the demagnetized electrons plays an important role to sustain the reconnection current and contributes to the dissipation due to the nonideal electric field, (2) the finite guide field dominates over the Hall magnetic field in an electron–scale region in the exhaust and modifies the electron flow dynamics in the EDR, (3) the reconnection current is in part carried by inflowing field–aligned electrons in the magnetosphere part of the EDR, and (4) the reconnection electric field measured by multiple spacecraft is uniform over at least eight electron skin depths and corresponds to a reconnection rate of approximately 0.1. Here, the observations establish the first look at the structure of the EDR under a weak but not negligible guide field.

Research Organization:
Univ. of Maryland, College Park, MD (United States)
Sponsoring Organization:
USDOE Office of Science (SC)
Grant/Contract Number:
SC0016278
OSTI ID:
1466266
Alternate ID(s):
OSTI ID: 1402346
Journal Information:
Journal of Geophysical Research. Space Physics, Vol. 122, Issue 5; ISSN 2169-9380
Publisher:
American Geophysical UnionCopyright Statement
Country of Publication:
United States
Language:
English
Citation Metrics:
Cited by: 49 works
Citation information provided by
Web of Science

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Cited By (8)

Structure of Electron‐Scale Plasma Mixing Along the Dayside Reconnection Separatrix journal November 2019
Assessing the Time Dependence of Reconnection With Poynting's Theorem: MMS Observations journal April 2018
Drift turbulence, particle transport, and anomalous dissipation at the reconnecting magnetopause journal June 2018
MMS Measurements of the Vlasov Equation: Probing the Electron Pressure Divergence Within Thin Current Sheets journal July 2019
Effects of the guide field on electron distribution functions in the diffusion region of asymmetric reconnection journal August 2019
Magnetic Reconnection in the Space Sciences: Past, Present, and Future journal January 2020
Observation of Nongyrotropic Electron Distribution Across the Electron Diffusion Region in the Magnetotail Reconnection journal December 2019
Universality of lower hybrid waves at Earth's magnetopause text January 2019

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