Solar cycle variations in the ionospheric Alfvén resonator 1985-1995.

Details Solar cycle variations in the ionospheric Alfvén resonator 1985-1995. Solar cycle variations in the ionospheric Alfvén resonator 1985-1995.

Mar 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000jastp..62..239b&link_type=abstract

J. Atmos. Sol.-Terr. Phys., Vol. 62, No. 4, p. 239 - 248

Physics

9

Earth Ionosphere: Solar Activity Cycles, Earth Ionosphere: Alfven Waves

Scientific paper

Based on long-term observations of the resonance structure in the electromagnetic background noise spectrum (resonance spectrum structure, RSS), recorded in the frequency range 0.1-10 Hz over one complete solar cycle (11 years, from 1985 to 1995), it was found that the resonance conditions for Alfvén waves in the ionosphere (ionospheric Alfvén resonator) are determined at midlatitudes by the level of solar activity. RSS are regularly observed in years of minimum solar activity, and are practically absent in years of maximum solar activity. It is shown that consideration of the ionospheric Alfvén resonator explains the dependence of the RSS on solar activity.

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