Computer Science
Scientific paper
Nov 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978kosis..16..895k&link_type=abstract
Kosmicheskie Issledovaniia, vol. 16, Nov.-Dec. 1978, p. 895-900. In Russian.
Computer Science
Atmospheric Chemistry, Mars Atmosphere, Mars 5 Spacecraft, Twilight Glow, Venera Satellites, Venus Atmosphere, Atmospheric Composition, Chemical Reactions, Concentration (Composition), Nitrogen, Optical Emission Spectroscopy, Sodium, Tables (Data), Venera 9 Satellite
Scientific paper
Threshold contents are tabulated for 17 elements and 6 diatomic molecules in the Martian and Venusian atmospheres. In particular, it is shown that the sodium content in these planetary atmospheres is smaller by an order of magnitude than in the earth's atmosphere. This finding is of interest in that the presence of the metals and ions studied (Fe, Al, Ca, Na, Ni, Cr, Mn, Ti, K, Co, Sc, Cu, Li, Sr, Ca(+), Ti(+), SC(+)) in planetary atmospheres must be attributed to evaporation of meteoric matter.
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