Astronomy and Astrophysics – Astronomy
Scientific paper
Mar 1982
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982kosis..20..312s&link_type=abstract
Kosmicheskie Issledovaniia, vol. 20, Mar.-Apr. 1982, p. 312-314. In Russian.
Astronomy and Astrophysics
Astronomy
Oxygen Atoms, Planetary Composition, Venus Atmosphere, Astronomical Spectroscopy, Atom Concentration, Atomic Energy Levels, Emission Spectra, Line Spectra, Spectral Energy Distribution, Ultraviolet Spectrometers, Upper Atmosphere, Venera 11 Satellite, Venera 12 Satellite
Scientific paper
The oxygen atom density in the upper atmosphere of Venus is estimated by comparing measurements of the total emission intensity in the O I 1304-A triplet line with results of theoretical calculations. The data were obtained by means of the multichannel UV diffraction spectrometer aboard the Venera 11 and Venera 12 probes. Oxygen atom densities of 3.7 x 10 to the 8th per cu cm and 4.0 x 10 to the 8th per cu cm were obtained from Venera 11 and Venera 12 data, respectively, for a height of 150 km.
Burgin M. S.
Sholokhov V. S.
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