Airglow observations of the OI 7774 A multiplet at Arecibo during a magnetic storm

Details Airglow observations of the OI 7774 A multiplet at Arecibo during a magnetic storm Airglow observations of the OI 7774 A multiplet at Arecibo during a magnetic storm

Feb 1980

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980jgr....85..767b&link_type=abstract

Journal of Geophysical Research, vol. 85, Feb. 1, 1980, p. 767-773.

Physics

Airglow, Electron Density Profiles, Fine Structure, Magnetic Storms, Radar Scattering, Geomagnetism, Mathematical Models, Neutral Particles, Oxygen Ions, Radio Telescopes, Thermosphere

Scientific paper

The paper considers airglow observations of the OI 7774 A multiplet observed during a geomagnetic storm. Theoretical calculations using electron density profiles obtained with the incoherent scatter radar show that the measured intensities cannot be explained by either radiative or ion-ion recombination reactions. A possible correlation between the airglow enhancement and D(st) was found; excitation by heavy neutral atoms or ions precipitating into the thermosphere is proposed as a possible explanation for enhanced 7774 A emission during this magnetic storm.

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