Determination of the total ozone content in the atmosphere, based on spectrophotometric star observations

Details Determination of the total ozone content in the atmosphere, based on spectrophotometric star observations Determination of the total ozone content in the atmosphere, based on spectrophotometric star observations

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981fizao..17..706a&link_type=abstract

Akademiia Nauk SSSR, Izvestiia, Fizika Atmosfery i Okeana, vol. 17, July 1981, p. 706-715. In Russian.

Astronomy and Astrophysics

Astronomy

1

Atmospheric Attenuation, Atmospheric Composition, Earth Atmosphere, Ozonometry, Stellar Spectrophotometry, Absorption Spectra, Monochromatic Radiation, Mountains, Ultraviolet Spectra

Scientific paper

Astronomical methods are used to determine the total content of ozone at four mountain sites for various years and seasons in both the ultraviolet and the visible parts of the spectrum. Quasi-monochromatic coefficients of atmospheric extinction are determined, and more than 1000 spectral dependence curves of extinction coefficients are obtained. Results, obtained from two separate absorption bands, on ozone thickness, are in good agreement.

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