Computer Science
Scientific paper
Apr 1984
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1984fizao..20..227b&link_type=abstract
Akademiia Nauk SSSR, Izvestiia, Fizika Atmosfery i Okeana (ISSN 0002-3515), vol. 20, April 1984, p. 227-230. In Russian.
Computer Science
Absorption Spectra, Atmospheric Composition, Ozone, Satellite Observation, Stellar Occultation, Upper Atmosphere, Altitude, Ozonosphere, Salyut Space Station, Satellite-Borne Instruments
Scientific paper
Stellar occultation measurements obtained from the Salyut-6 BST-1M telescope were used to study ozone concentrations in the upper atmosphere. The measurements were taken in the range of ozone absorption (2560 + or - 40 A), at heights ranging from approximately 70 to 100 km. The occultation sources used were the star Sirius and the UV-bright star Beta-Centaurus, with a tangent point in the region of the Marquesas Islands. The measurements are found to be in general agreement with those of previous studies up to the 80 km altitude range, but at altitudes exceeding 80 km distinct features were found which are considered to warrant further investigation.
Bakun V. N.
Chizhov A. F.
Grechko Gheorghy Mikhailovich
Ivanchenkov A. S.
Kovalenok V. V.
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