Dayglow of the infrared atmospheric band system of O2 during a total eclipse of the sun

Details Dayglow of the infrared atmospheric band system of O2 during a total eclipse of the sun Dayglow of the infrared atmospheric band system of O2 during a total eclipse of the sun

May 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jatp...37..717w&link_type=abstract

Journal of Atmospheric and Terrestrial Physics, vol. 37, May 1975, p. 717-730. Research supported by the Science Research Counc

Physics

1

Dayglow, Infrared Radiation, Oxygen Spectra, Ozone, Photolysis, Solar Eclipses, Airborne Equipment, Mesosphere, Molecular Excitation, Molecular Spectroscopy, Radiance, Spectrophotometers

Scientific paper

A description is given of observations made at both 1.27 microns and 1.58 microns from the prototype supersonic airliner Concorde 001 over Africa during the total eclipse of June 30, 1973. It is pointed out that measurements of dayglow provide no evidence to suggest any other source of excited oxygen molecules than the photolysis of ozone. The variation of radiance during the eclipse is satisfactorily explained by the theory. No assumptions are, therefore, required concerning any change of ozone concentration during the eclipse.

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