The magnitude and composition of the outflow of energetic ions from the ionosphere

Details The magnitude and composition of the outflow of energetic ions from the ionosphere The magnitude and composition of the outflow of energetic ions from the ionosphere

Apr 1984

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984jgr....89.2185c&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 89, April 1, 1984, p. 2185-2194. Research supported by the Lockheed Indep

Computer Science

Sound

50

Hydrogen Ions, Ionospheric Ion Density, Ionospheric Sounding, Oxygen Ions, Positive Ions, Explorer 12 Satellite, Ion Density (Concentration), Kp Index, Magnetic Storms, Mass Spectroscopy

Scientific paper

S3-3 spacecraft ion mass spectrometer data are used to determine the outflow from the high latitude ionosphere of terrestrial ions, in the 0.5-16 keV energy range, during both magnetically quiet times and magnetic storms. Ion populations having different histories were separated on a statistical basis to allow the use of all available data. The major outflow constituents were H(+) and O(+). Both the intensity of the outflow and its composition showed marked dependence on magnetic activity.

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