Open AccessFast tailward flows in the plasma sheet boundary layer during a substorm on 9 March 2008: THEMIS observations
Author(s) -
Du A. M.,
Nakamura R.,
Zhang T. L.,
Panov E. V.,
Baumjohann W.,
Luo H.,
Xu W. Y.,
Lu Q. M.,
Volwerk M.,
Retinò A.,
Zieger B.,
Angelopoulos V.,
Glassmeier K.H.,
McFadden J. P.,
Larson D.
Publication year - 2011
Publication title -
journal of geophysical research: space physics
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 1.67
H-Index - 298
eISSN - 2156-2202
pISSN - 0148-0227
DOI - 10.1029/2010ja015969
Subject(s) - substorm , plasma sheet , physics , geophysics , boundary layer , outflow , plasma , field line , magnetic field , magnetosphere , atmospheric sciences , mechanics , meteorology , quantum mechanics
Tailward flows in the plasma sheet boundary layer (PSBL) were observed simultaneously by the five Time History of Events and Macroscale Interactions during Substorms (THEMIS) probes at down‐tail distances X ∼ 7.6 to ∼17.6 R E for ∼10 min during an interval of successive substorm intensification in a storm time on 9 March 2008. The flows first occurred close to Earth and then propagated along the magnetic field lines in the PSBL with a speed of ∼150–350 km s −1 . We show that the occurrence of tailward flows is highly dependent on proximity to the plasma sheet boundary. Higher speeds occurred in the outer part of the PSBL, while either lower tailward speeds (or even earthward flows) were seen in the inner part of the PSBL. The tailward flow occurrence increased during magnetotail stretching and decreased or ceased during magnetic field dipolarizations. These PSBL tailward flows near the Earth can be understood as an outflow of the earthward flows that essentially empty the central plasma sheet. The tailward flows along the field line filled the void left behind by the dipolarization front.