Computer Science
Scientific paper
Sep 1977
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977fizao..13..943n&link_type=abstract
Akademiia Nauk SSSR, Izvestiia, Fizika Atmosfery i Okeana, vol. 13, Sept. 1977, p. 943-948. In Russian.
Computer Science
1
Atmospheric Composition, Interplanetary Spacecraft, Planetary Atmospheres, Radio Spectroscopy, Remote Sensors, Ammonia, Atmospheric Attenuation, Carbon Monoxide, Jupiter Atmosphere, Microwave Resonance, Nitrous Oxides, Saturn (Planet), Venus Atmosphere, Water Vapor
Scientific paper
Consideration is given to the possibility of using interplanetary platforms for the remote sensing of trace components (N2O, CO and NH3) in the upper atmosphere of Venus and NH3 and H2O vapor in the atmospheres of Jupiter and Saturn. The limits of determining the relative concentrations of these gases using microwave resonance absorption spectroscopy are examined. The effective conditions under which this method can be used are determined from a comparison of minimum gas concentrations detected using this method with results of IR spectroscopy and with results on upper concentration limits, computed from component equilibrium conditions.
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