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Observations of Tailward Streaming Ions in the Near-Earth Tail During a Magnetospheric Substorm

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Part of the book series: NATO ASI Series ((ASIC,volume 509))

Abstract

A tailward moving plasmoid (flux rope) was observed by the GEOTAIL spacecraft at [-22, 5, -3 RE GSE] after a period with strong geomagnetic activity on November 27, 1995. The structure exhibited classic plasmoid like signatures; bipolar Bz, a strong core field and tailward streaming ions. Measurements from the solar wind and the ground show that the GEOTAIL-observations were correlated with a change in the IMF and a substorm onset. Together, these observations suggest that the flux rope was launched as a result of magnetic reconnection during substorm onset, and that the reconnection site was located earthward of -22 RE. To our knowledge, observations of similar substorm associated flux rope formation and tailward streaming ions at such distances have not been reported earlier.

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© 1998 Springer Science+Business Media Dordrecht

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Håland, S. et al. (1998). Observations of Tailward Streaming Ions in the Near-Earth Tail During a Magnetospheric Substorm. In: Moen, J., Egeland, A., Lockwood, M. (eds) Polar Cap Boundary Phenomena. NATO ASI Series, vol 509. Springer, Dordrecht. https://doi.org/10.1007/978-94-011-5214-3_30

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  • DOI: https://doi.org/10.1007/978-94-011-5214-3_30

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6195-7

  • Online ISBN: 978-94-011-5214-3

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