Absorption of XUV solar radiation in the atmosphere

Details Absorption of XUV solar radiation in the atmosphere Absorption of XUV solar radiation in the atmosphere

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974poast..22..261d&link_type=abstract

Postepy Astronomii, vol. 22, Oct.-Dec. 1974, p. 261-274. In Polish.

Astronomy and Astrophysics

Astronomy

Atmospheric Attenuation, Far Ultraviolet Radiation, Solar Radiation, Ultraviolet Absorption, Upper Atmosphere, Absorption Cross Sections, Absorption Spectra, Atmospheric Models, Molecular Absorption, Nitrogen, Optical Paths, Oxygen Atoms, Photoabsorption

Scientific paper

The absorption of extreme ultraviolet solar radiation by the N2, O2, and O components of the atmosphere at heights between 80 and 800 km is analyzed on the basis of the CIRA 1965 model of the neutral atmosphere, Hinteregger's (1970) data on solar radiation intensity, and Stolarski and Johnson's (1972) effective photoabsorption cross-sections. The optical paths and extinction of XUV radiation at various heights are calculated, and the behavior of the short-wave solar spectrum in the atmosphere is examined.

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