This paper was presented at the Eighth International Conference on Substorms (ICS-8), held at the University of Calgary, Alberta, Canada, 27-31 March, 2006, and published in Proceedings of the Eighth International Conference on Substorms, edited by M. Syrjäsuo and E.F. Donovan, pp. 65-70. It is available from http://ics8.ca/publication.htmlMetadata only entryWe present initial observations from an ongoing investigation into the dynamics of the magnetotail during a\ud period of multiple substorms. The investigation coordinates data from ground and space-based instruments including the\ud Cluster and IMAGE spacecraft, SuperDARN and ground magnetometers during the period 00:00UT to 05:00UT on 25th\ud August, 2003. The first substorm expansion phase, which is preceded by two pseudo-breakups at 00:38UT and 00:57UT,\ud takes place between 01:11UT and 01:50UT during which time IMAGE WIC(FUV) data for the Southern auroral oval\ud shows enhanced auroral activity almost solely in the post-midnight sector and the occurrence of auroral streamers within\ud the auroral bulge. SuperDARN map potential analysis shows a flow diversion with a northern hemisphere footprint that\ud is conjugate to a southern hemisphere auroral streamer. During this time, Cluster CIS and FGM instruments detect the\ud passage of under-populated flux tubes, or plasma bubbles, and a field rotation event, discussed as a flux rope. These\ud observations agree with current predictions on the relationship between streamers and under-populated flux tubes in the tail\ud from the Chen and Wolf model
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