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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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
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