Abstract
It has recently become apparent that auroral radars are powerful tools for the investigation of ULF pulsations in the Pc5 range. Auroral radar observations of pulsation effects in the ionosphere are reviewed. The Stare radar system is described and its measurements of the pulsation electric field in the ionosphere outlined. It has been established that this electric field is entirely consistent with the field of a hydro-magnetic field-line resonance. The rotation of the pulsation magnetic field through 90° by the ionosphere is confirmed. Statistical studies of occurrence show some consistency with the behaviour expected for solar-wind driven instabilities on the magneto- pause. The use of Stare data to deduce equatorial plasma density, and height integrated ionospheric conductivities is also discussed. These measurements have been used to estimate energy input into the magnetosphere.
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Walker, A.D.M., Greenwald, R.A. (1981). Pulsation Structure in the Ionosphere Derived from Auroral Radar Data. In: Southwood, D.J. (eds) ULF Pulsations in the Magnetosphere. Advances in Earth and Planetary Sciences, vol 11. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-8426-4_7
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DOI: https://doi.org/10.1007/978-94-009-8426-4_7
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