Dawn-evening asymmetry of the 557.7-nm emission in the nightglow

Details Dawn-evening asymmetry of the 557.7-nm emission in the nightglow Dawn-evening asymmetry of the 557.7-nm emission in the nightglow

Jun 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991ge%26ae..31..482k&link_type=abstract

Geomagnetizm i Aeronomiia (ISSN 0016-7940), vol. 31, May-June 1991, p. 482-485. In Russian.

Physics

Dayglow, Emission Spectra, Satellite Orbits, Spectral Line Width, Diurnal Variations, Oxygen Spectra, Thermosphere, Upper Atmosphere

Scientific paper

An analysis of excitation mechanisms of the green oxygen line at 557.7
nm is used to explain the dawn-dusk asymmetry of the volume intensity
observed in AE-C satellite measurements. It is shown that the observed
asymmetry is associated with the change in solar zenith angle on the
satellite flight path.

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