Differential rotation of the atmospheres of Jupiter and Saturn

Details Differential rotation of the atmospheres of Jupiter and Saturn Differential rotation of the atmospheres of Jupiter and Saturn

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979azh....56..595d&link_type=abstract

Astronomicheskii Zhurnal, vol. 56, May-June 1979, p. 595-605. In Russian.

Astronomy and Astrophysics

Astronomy

Atmospheric Circulation, Jupiter Atmosphere, Planetary Rotation, Saturn Atmosphere, Angular Momentum, Buoyancy, Correlation, Electrical Resistivity, Planetary Ionospheres

Scientific paper

It is suggested that angular-momentum transport caused by the different buoyancies of counterrotating compressible eddies may be the main cause of the accelerated rotation of the equatorial zones of Jupiter and Saturn. Calculations are performed in the mixing-length approximation, and the results are found to agree with observational data. The electrical conductivity of dense lower-atmospheric layers of the giant planets is estimated, and the role of an intrinsic magnetized ionosphere in the dynamics of observed atmospheric phenomena is shown to be important. A correlation between rotational velocity and equatorial flow width is predicted and tentatively confirmed by analysis of observational data on Jupiter.

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