Physics
Scientific paper
Dec 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993georl..20.2813a&link_type=abstract
Geophysical Research Letters (ISSN 0094-8276), vol. 20, no. 24, p. 2813-2816
Physics
8
Boundary Layer Plasmas, Geomagnetic Tail, Particle Acceleration, Plasma Layers, Flow Velocity, International Sun Earth Explorer 3, Ion Beams, Magnetic Storms
Scientific paper
No high-speed flows or discernible counterstreaming ion beams were observed during a series of plasma sheet boundary encounters resulting from solar wind-driven plasma sheet motions. We conclude that the boundary may be active primarily during plasma sheet 'recovery'. A temporal onset of flows in the inner plasma sheet (IPS) was associated with the appearance of counterstreaming beams embedded in an already isotropic plasma sheet boundary and close to the neutral sheet may have a common generation mechanism.
Angelopoulos Vassilis
Coroniti Ferdinan V.
Feldman William C.
Galland Kivelson Margaret
Gosling Jack T.
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