Cloud microphysics of the giant planets

Details Cloud microphysics of the giant planets Cloud microphysics of the giant planets

Jul 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jats...45.2066c&link_type=abstract

Journal of the Atmospheric Sciences (ISSN 0022-4928), vol. 45, July 15, 1988, p. 2066-2081.

Physics

32

Cloud Physics, Gas Giant Planets, Planetary Meteorology, Ammonia, Jupiter Atmosphere, Methane, Neptune Atmosphere, Saturn Atmosphere, Uranus Atmosphere, Water

Scientific paper

The characteristic time constants for the atmospheres of the giant planets were compared for the purpose of finding analogs for clouds in the atmospheres of these planets among the several types of cloud systems found on earth. The NH3 clouds on Jupiter and Saturn were found to be weakly precipitating systems, similar to the thicker cirrus clouds on earth, while the H2O clouds were found to be much more massive than the water clouds on earth. The CH4 and H2O clouds on Uranus and Neptune are completely unlike any cloud on earth, being 10 to 100 times more massive than the densest water clouds on earth. It is concluded that, while the microphysical characteristics of the clouds on Jupiter and Saturn are comparable to those of terrestrial stratus and cumulus clouds, the massive clouds on Uranus and Neptune reach conditions unlike anything on earth.

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