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Ionospheric convection and the substorm cycle

Lockwood, M. and Cowley, S.W.H. (1992) Ionospheric convection and the substorm cycle. In: the First International Conference on Substorms, ICS-1, 23-27 March 1992, Kiruna, Sweden, pp. 99-109. (in "Substorms 1, Proceedings of the First International Conference on Substorms, ICS-1", ed C. Mattock, ESA-SP-335 European Space Agency Publications, Nordvijk, The Netherlands)

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Abstract/Summary

During substorms, magnetic energy is stored and released by the geomagnetic tail in cycles of growth and expansion phases, respectively. Hence substorms are inherently non-steady phenomena. On the other hand, all numerical models (and most conceptual ones) of ionospheric convection produced to date have considered only steady-state situations. In this paper, we investigate the relationship of substorms to convection. In particular, it is shown that the steady-state convection pattern represents an average over several substorm cycles and does not apply on time scales shorter than the substorm cycle period of 1-2 hours. The flows driven by the growth and expansion phases of substorms are integral (indeed dominant) part of, as opposed to a transient addition to, the overall convection pattern.

Item Type:Conference or Workshop Item (Paper)
Refereed:Yes
Divisions:No Reading authors. Back catalogue items
Faculty of Science > School of Mathematical, Physical and Computational Sciences > Department of Meteorology
ID Code:38835
Publisher Statement:in "Substorms 1, Proceedings of the First International Conference on Substorms, ICS-1", ed C. Mattock, ESA-SP-335, ESA Special Publication SP 335 European Space Agency Publications, Nordvijk, The Netherlands ISBN 929092182X, 9789290921820

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