Cluster observations of ∂Bz/∂x during growth phase magnetotail stretching intervals

We study a statistics of ∂Bz/∂x in a thin stretching current sheet (substorm growth phases) observed by Cluster between 8 and 18 RE downtail. After 2005, spacecraft separation allowed to measure directly this derivative of Bz along the tail axis. The near‐tail events (within 14 RE) exhibited a strai...

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Veröffentlicht in:Journal of geophysical research. Space physics 2013-09, Vol.118 (9), p.5720-5730
Hauptverfasser: Petrukovich, A. A., Artemyev, A. V., Nakamura, R., Panov, E. V., Baumjohann, W.
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Sprache:eng
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Zusammenfassung:We study a statistics of ∂Bz/∂x in a thin stretching current sheet (substorm growth phases) observed by Cluster between 8 and 18 RE downtail. After 2005, spacecraft separation allowed to measure directly this derivative of Bz along the tail axis. The near‐tail events (within 14 RE) exhibited a straight decrease of an initially large positive ∂Bz/∂x to ∼1–2 nT/RE. In the more stretched middle tail, usually the small |∂Bz/∂x|
ISSN:2169-9380
2169-9402
DOI:10.1002/jgra.50550