Variations of the magnetospheric ion number densities near geostationary orbit with solar activity

Details Variations of the magnetospheric ion number densities near geostationary orbit with solar activity Variations of the magnetospheric ion number densities near geostationary orbit with solar activity

Feb 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989angeo...7...69s&link_type=abstract

Annales Geophysicae (ISSN 0980-8752), vol. 7, Feb. 1989, p. 69-75. Research supported by DOE and Southwest Research Institute.

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Magnetospheric Ion Density, Satellite Sounding, Solar Activity Effects, Geos 2 Satellite, Geosynchronous Orbits, Helium Ions, Oxygen Ions, Solar Terrestrial Interactions

Scientific paper

A large ion-composition data set consisting of 3-h averages has been assembled for the energy per charge range 0.9-15.9 keV/e. It includes all data collected by the Ion Composition Experiment on the ESA/GEOS-2 satellite from August 1, 1978 through August 24, 1985. Five ion species have been routinely identified: H(+), He(2+), He(+), O(2+), and O(+). Ions believed to be of ionospheric origin exhibit a very striking statistical correlation with solar EUV flux as measured by the F(10.7) index. The O(+) number density varies by a factor of 14 over the solar cycle.

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