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Substorm‐Related Near‐Earth Reconnection Surge: Combining Telescopic and Microscopic Views
Author(s) -
Sergeev V. A.,
Apatenkov S. V.,
Nakamura R.,
Baumjohann W.,
Khotyaintsev Y. V.,
Kauristie K.,
Kamp M.,
Burch J. L.,
Ergun R. E.,
Lindqvist P.A.,
Torbert R.,
Russell C. T.,
Giles B. L.
Publication year - 2019
Publication title -
geophysical research letters
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.007
H-Index - 273
eISSN - 1944-8007
pISSN - 0094-8276
DOI - 10.1029/2019gl083057
Subject(s) - substorm , physics , geophysics , electrojet , magnetic reconnection , ionosphere , astrophysics , magnetosphere , field line , bulge , surge , amplitude , earth's magnetic field , magnetic field , stars , meteorology , quantum mechanics
A strong ~11‐min‐long surge of the lobe reconnection was observed during a substorm on the tailward side of the near‐Earth neutral line. In the southern lobe near the reconnection separatrix the MMS spacecraft observed short‐duration earthward electron beams providing the local Hall current, tailward propagating Alfven wave (AW) bursts with Poynting flux up to 10 −4 W/m 2 , and large‐amplitude E field spikes (e‐holes) and low hybrid waves. The reconnection surge was accompanied by substorm current wedge formation and fast poleward expansion of auroral bulge‐related westward electrojet in the conjugate ionosphere. During its meridional crossing above the expanding bulge the Metop‐2 spacecraft observed an intense energetic precipitation spike near the expected X line foot point and confirmed the dipolarized character of magnetic field lines inside of the bulge. Globally the observed average reconnection rate (< Ey > ~3.3 mV/m) was sufficient to produce the magnetic flux increase in the bulge, associated with observed fast poleward expansion (about 6° latitude in 5 min).