Spacecraft Observations of Oblique Electron Beams Breaking the Frozen-In Law During Asymmetric Reconnection
Author(s) -
J. Egedal,
A. Lê,
W. Daughton,
Blake Wetherton,
P. A. Cassak,
J. L. Burch,
B. Lavraud,
J. Dorelli,
D. J. Gershman,
L. A. Avanov
Publication year - 2018
Publication title -
physical review letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 3.688
H-Index - 673
eISSN - 1079-7114
pISSN - 0031-9007
DOI - 10.1103/physrevlett.120.055101
Subject(s) - magnetic reconnection , physics , magnetopause , electron , magnetic field , spacecraft , diffusion , field line , computational physics , magnetosphere , astronomy , nuclear physics , quantum mechanics
Fully kinetic simulations of asymmetric magnetic reconnection reveal the presence of magnetic-field-aligned beams of electrons flowing toward the topological magnetic x line. Within the ∼6d_{e} electron-diffusion region, the beams become oblique to the local magnetic field, providing a unique signature of the electron-diffusion region where the electron frozen-in law is broken. The numerical predictions are confirmed by in situ Magnetospheric Multiscale spacecraft observations during asymmetric reconnection at Earth's dayside magnetopause.
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