Computer Science – Numerical Analysis
Scientific paper
Jan 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980avest..13..129k&link_type=abstract
(Astronomicheskii Vestnik, vol. 13, July-Sept. 1979, p. 129-143.) Solar System Research, vol. 13, no. 3, Jan. 1980, p. 99-111. T
Computer Science
Numerical Analysis
Atmospheric Physics, Earth Atmosphere, Greenhouse Effect, Planetary Atmospheres, Atmospheric Composition, Carbon Dioxide Concentration, Climate, Jupiter Atmosphere, Mars Atmosphere, Numerical Analysis, Planetary Evolution, Solar Radiation, Venus Atmosphere
Scientific paper
Calculating the planetary greenhouse effect (GE) in terms of atmospheric chemical composition, degree of turbidity, and structural parameters is discussed regarding the earth, Venus, Mars and Jupiter. Climatic and anthropogenic effects on the earth's GE are considered, along with the determining effect of water vapor, the contribution of CO2 and ozone, the vertical temperature profile, clouds, and the absorption, scattering, and attenuation coefficients for a finely divided aerosol. The importance of CO2 and clouds for the Venusian GE, of CO2 and dusty aerosol, especially during dust storms, for the Martian GE, and of ammonia for Jupiter's GE, are also considered.
Kondrat'ev Ia. K.
Moskalenko N. I.
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