Height of the transition from O(+) ions to H(+) ions according to Aktivnyi-satellite data and the dependence of this height on solar activity

Details Height of the transition from O(+) ions to H(+) ions according to Aktivnyi-satellite data and the dependence of this height on solar activity Height of the transition from O(+) ions to H(+) ions according to Aktivnyi-satellite data and the dependence of this height on solar activity

Aug 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992ge%26ae..32...59a&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 32, no. 4, p. 59-63.

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Ionospheric Ion Density, Satellite Sounding, Solar Activity Effects, Solar Cycles, Hydrogen Ions, Oxygen Ions, Soviet Satellites

Scientific paper

Variations of the height (h sub T) at which O(+) and H(+) concentrations are equalized are investigated on the basis of mass-spectrometric measurements of the ion composition of the topside ionosphere performed with the Aktivnyi satellite during a period of high solar activity. A dependence of h sub T on the F10.7 index is obtained for the total solar-activity cycle.

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