The scattering rate of solar 834 A radiation by magnetospheric O(+) and O(++)

Details The scattering rate of solar 834 A radiation by magnetospheric O(+) and O(++) The scattering rate of solar 834 A radiation by magnetospheric O(+) and O(++)

Sep 1990

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1990georl..17.1613m&link_type=abstract

Geophysical Research Letters (ISSN 0094-8276), vol. 17, Sept. 1990, p. 1613-1616.

Computer Science

Sound

18

Earth Magnetosphere, Oxygen Ions, Scattering Coefficients, Solar Radiation, Albedo, Ionospheric Disturbances, Solar Spectra

Scientific paper

Several recent proposals to image sunlit magnetospheric O(+) have been difficult to assess because of the lack of detailed knowledge of the solar spectrum at 834 A. An NRL solar spectrograph flown on a sounding rocket in 1962 actually had sufficient resolving power to allow the calculation of scattering rates. Using these solar data, examples of scattering rates for a range of thermal and bulk velocities are presented for both O(+) and O(++), and the effects of ionospheric albedo are estimated. The scattering rates are significantly lower than previously estimated for hot or moving plasma and exhibit substantial structure.

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