Double Star/Cluster observation of neutral sheet oscillations on 5 August 2004

Details Double Star/Cluster observation of neutral sheet oscillations on 5 August 2004 Double Star/Cluster observation of neutral sheet oscillations on 5 August 2004

Nov 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005angeo..23.2909z&link_type=abstract

Annales Geophysicae, Volume 23, Issue 8, 2005, pp.2909-2914

Physics

14

Scientific paper

Previous Cluster observations have shown that the flapping motions of the Earth's magnetotail are of internal origin and that kink-like waves are emitted from the central part of the tail and propagate toward the tail flanks. The newly launched Double Star Program (DSP) TC-1 satellite allows us to investigate neutral sheet at 10-13 Re in the tail. Using conjunctions with Cluster we will have simultaneous observations at 10-13 and 16-19 Re of these flapping motions. In this paper, we present the first results of neutral sheet oscillations observed by the Cluster and Double Star satellites on 5 August 2004.

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