Flow of oxygen ions in the solar wind acceleration region

Details Flow of oxygen ions in the solar wind acceleration region Flow of oxygen ions in the solar wind acceleration region

Jul 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990jgr....9510269e&link_type=abstract

Journal of Geophysical Research (ISSN 0148-0227), vol. 95, July 1, 1990, p. 10269-10272. Research supported by the Norges Almenv

Physics

14

Flow Velocity, Oxygen Ions, Oxygen Recombination, Solar Electrons, Solar Protons, Solar Wind, Ion Recombination, Solar Corona

Scientific paper

A solar wind model with protons, electrons, O VII and O VI ions is studied. It is found that ionization and recombination processes lead to an approximately constant density ratio of the oxygen states in the solar wind acceleration region. Although ionization and recombination have a significant effect on the flow speed of the O VI ions, these processes are not fast enough to bring the speed of O VI up to the flow speed of the O VII ions.

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