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Ionospheric Signatures of Magnetopause Processes

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Polar Cap Boundary Phenomena

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

Abstract

Whilst it is well-accepted that short-duration changes to the Interplanetary Magnetic Field (IMF) and solar wind cause high-latitude ionospheric transients observed by magnetic, optical and radar techniques, a coherent explanation of the zoo of signatures remains illusive. The paper describes some of the problems involved in the interpretation of dayside transient features, all of which result from time-and spatially-varying field-aligned currents. A brief discussion of how internal magnetospheric processes can directly affect the rate at which energy is transferred across the magnetopause is discussed. Further progress will require carefully-coordinated measurements from ground-based networks of observatories with complementary measurements from space.

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© 1998 Springer Science+Business Media Dordrecht

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Rodger, A.S. (1998). Ionospheric Signatures of Magnetopause Processes. 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_10

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  • DOI: https://doi.org/10.1007/978-94-011-5214-3_10

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-010-6195-7

  • Online ISBN: 978-94-011-5214-3

  • eBook Packages: Springer Book Archive

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