A sunset effect in variations of the eigenfrequencies of the ionospheric Alfven resonator

Details A sunset effect in variations of the eigenfrequencies of the ionospheric Alfven resonator A sunset effect in variations of the eigenfrequencies of the ionospheric Alfven resonator

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000jastp..62..249e&link_type=abstract

Journal of Atmospheric and Solar-Terrestrial Physics, Volume 62, Issue 4, p. 249-252.

Physics

2

Scientific paper

A method of detecting wavelike disturbances at heights of 200-400 km, based on the measurements of variations of the ionospheric Alfven resonator eigenfrequencies, is developed. The amplitude of these variations /ΔF increases significantly after the solar terminator crosses at sunset. The period of this variation varies in the interval from 30 to 60 min; the relative amplitude of the variation lies in the range 2-5%. /ΔF variations can be connected with the generation of internal gravity waves at heights about 200 km.

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