Planetary atmospheres

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Mar 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987rvgeo..25..297l&link_type=abstract

Reviews of Geophysics (ISSN 8755-1209), vol. 25, March 1987, p. 297-303.

Physics

Geophysics

2

Planetary Atmospheres, Planetology, Atmospheric Models, Atmospheric Temperature, Chemical Composition, Dust Storms, Erosion, Jupiter Atmosphere, Mars Atmosphere, Saturn Atmosphere, Venus Atmosphere, Water, Planets, Atmosphere, Spacecraft Observations, Earth-Based Observations, Vega Missions, Voyager 2, Origin, Formation, Evolution, Composition, Venus, Mars, Jupiter, Saturn, Titan, Satellites, Structure, Climate, Review, Dynamics, Gases, Features, Characteristics, Thermal Properties, Uranus, Clouds, Comparis

Scientific paper

Observations and theoretical models of planetary atmospheres published during the period 1983-1986 are reviewed, including Vega and Voyager data and results from ground-based remote sensing. Consideration is given to water-vapor and sulfur-compound distributions, electrical phenomena, and dynamics in the Venus atmosphere; dust storms, water cycles, and water and ice erosion on Mars; the compositions, temperature profiles, and dynamics of the Jovian and Saturnian atmospheres; chemical processes and zonal winds on Titan; and the radiation budgets and chemical compositions of the outer planets.

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