Variations of ion composition in geostationary orbit during a geomagnetic storm

Details Variations of ion composition in geostationary orbit during a geomagnetic storm Variations of ion composition in geostationary orbit during a geomagnetic storm

Apr 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988izssr..52..824v&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Seriia Fizicheskaia (ISSN 0367-6765), vol. 52, April 1988, p. 824-826. In Russian.

Computer Science

Atmospheric Composition, Geomagnetism, Ionospheric Ion Density, Magnetic Storms, Hydrogen Ions, Oxygen Ions, Particle Acceleration, Positive Ions, Soviet Spacecraft, Synchronous Satellites

Scientific paper

Variations of ion composition in geostationary orbit during the geomagnetic storm of August 12-13, 1985 were measured with instrumentation at the Gorizont 1985-07A geostationary satellite. It is shown that a predominant acceleration of ions of ionospheric origin, H(+) and /N, O/(2+), occurs during the main storm phase. The filling of the geostationary orbit by solar ions occurs at the recovery phase and appears to be connected with dipolization of the geomagnetic field.

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