Excitation of radioauroral pulsations and penetration of PiC waves through the ionosphere

Details Excitation of radioauroral pulsations and penetration of PiC waves through the ionosphere Excitation of radioauroral pulsations and penetration of PiC waves through the ionosphere

Sep 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981jatp...43..975k&link_type=abstract

(European Geophysical Society, Annual Meeting on Geomagnetic Pulsations, 7th, Budapest, Hungary, Aug. 24-29, 1980.) Journal of A

Physics

2

Geomagnetic Micropulsations, Ionospheric Propagation, Polar Substorms, Radio Auroras, Magnetic Signatures, Polarization Characteristics, Power Spectra, Radar Detection

Scientific paper

Radioauroral pulsations at T approximately equal to 4.5 s have been observed during a substorm. They appear as poleward propagating waves. The most intense Pi magnetic pulsations occur at T approximately equal to 9 s. Using the transformation theory of hydromagnetic waves through the ionosphere, it is concluded that the radioauroral pulsations have been generated by the electric field pulsations associated with intense poleward propagating hydromagnetic waves. Polarization characteristics of magnetic pulsations observed on the ground are also shown to be in agreement with this interpretation.

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