structure of the near-earth plasma sheet during tailward flows
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ID: 235371
2008
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Abstract
A detailed analysis of successive tailward flow bursts in the near-Earth
magnetotail (X~−19 RE) plasma sheet is performed on the basis of
in-situ multi-point observations by the Cluster spacecraft on 15 September
2001. The tailward flows were detected during a northward IMF interval, 2.5 h
after a substorm expansion. Each flow burst (Vx<300 km/s) was
associated with local auroral activation. Enhancements of the parallel and
anti-parallel ~1 keV electron flux were detected during the flows. The
spacecraft configuration enables to monitor the neutral sheet (Bx≈0)
and the level of Bx≈10–15 nT simultaneously, giving a
possibility to distinguish between closed plasmoid-like structures and open
NFTE-like surges. The data analysis shows NFTE-like structures and localized
current filaments embedded into the tailward plasma flow. 3-D shapes of the
structures were reconstructed using the four-point magnetic filed
measurements and the particle data.
| Reference Key |
runov2008annalesstructure
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|---|---|
| Authors | ;A. Runov;A. Runov;I. Voronkov;Y. Asano;W. Baumjohann;M. Fujimoto;R. Nakamura;T. Takada;M. Volwerk;M. Volwerk;Z. Vörös;Z. Vörös;M. Meurant;A. Fazakerley;H. Rème;A. Balogh |
| Journal | journal of food measurement and characterization |
| Year | 2008 |
| DOI |
10.5194/angeo-26-709-2008
|
| URL | |
| Keywords |
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