Oxygen charge state abundance in the inner magnetosphere

Details Oxygen charge state abundance in the inner magnetosphere Oxygen charge state abundance in the inner magnetosphere

Jul 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996aipc..383..145f&link_type=abstract

Workshop on the Earth's trapped particle environment. AIP Conference Proceedings, Volume 383, pp. 145-150 (1996).

Computer Science

Energetic Trapped Particles

Scientific paper

The CRRES Magnetospheric Ion Composition Sensor (MICS) was used to obtain the relative oxygen charge state abundances in the earth's inner magnetosphere (3+3 on average. As expected, O+ is the dominant oxygen ion at all times in the inner magnetosphere for energies >60 keV/Q. During average conditions the Q>=+4 ions have fluxes comparable to O+3 in the L=4.5-7.5 region and are about 50% of the O+3 fluxes in the L=3-5 regions. Thus, the average O+3 fluxes appear to represent a transition state between ionospheric and solar wind source oxygen.

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