On the relationship of 6300 A airglow to parameters of the F-region of the ionosphere

Details On the relationship of 6300 A airglow to parameters of the F-region of the ionosphere On the relationship of 6300 A airglow to parameters of the F-region of the ionosphere

Jan 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978p%26ss...26...93h&link_type=abstract

Planetary and Space Science, vol. 26, Jan. 1978, p. 93-98. Research supported by the Australian Research Grants Committee.

Physics

Airglow, F Region, Oxygen Recombination, Oxygen Spectra, Radiative Recombination, Ion Recombination, Magnetic Effects, Wind Effects

Scientific paper

Variations in the intensity of 6300 A ionospheric airglow are explained in terms of variations of f0F2, i.e., its time derivative. It is suggested that the airglow is due to recombination of ions caused by atmospheric waves generated by magnetic activity and/or by a local neutral wind effect. This explanation is especially useful in predicting airglow when neutral atmosphere dynamics are not constant with time.

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