Abstract
Bursty Bulk Flows (BBFs) are an important means of transporting magnetic flux and plasma through the Earth’s magnetosphere and can be explained as entropy depleted flux tubes (plasma bubbles) propagating earthward under the action of the interchange instability. For 10 years ESA’s Cluster spacecraft have been making measurements of BBFs in the magnetotail at spacecraft separations ranging from 100 to 10,000 km. Here we compare three BBFs observed by Cluster at three different spacecraft separations and discuss some of the similarities and differences between the features observed during each event, with particular reference to field-aligned currents and the newly-discovered wake region observed behind and around earthward moving flux tubes.
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Acknowledgements
The authors wish to acknowledge the ESA Cluster Active Archive and the FGM, CIS and PEACE instrument teams for providing the data employed in this study. Some data analysis was done with QSAS. The authors were funded by UK STFC grant number PP/E/001173/1.
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Walsh, A.P., Forsyth, C. (2011). Cluster Observations of Plasma Bubbles, BBFs and Their Wakes. In: Liu, W., Fujimoto, M. (eds) The Dynamic Magnetosphere. IAGA Special Sopron Book Series, vol 3. Springer, Dordrecht. https://doi.org/10.1007/978-94-007-0501-2_6
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DOI: https://doi.org/10.1007/978-94-007-0501-2_6
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