Some dynamical parameters of the Jupiter atmosphere

Details Some dynamical parameters of the Jupiter atmosphere Some dynamical parameters of the Jupiter atmosphere

Feb 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986kfnt....2...48v&link_type=abstract

Kinematika i Fizika Nebesnykh Tel (ISSN 0233-7665), vol. 2, Jan.-Feb. 1986, p. 48-51. In Russian.

Physics

Atmospheric Circulation, Flow Stability, Jupiter Atmosphere, Adiabatic Conditions, Atmospheric Temperature, Couette Flow, Viscosity, Vortices

Scientific paper

The present study assumes that the first instability of Taylor-vortex type in thin-layer Couette spherical flow is responsible for the observed zonal structure of Jupiter. Based on this assumption, the depth of the planetary atmosphere (16,271 km) and the kinematic viscosity coefficient for large-scale circulation (not greater than about 1.9 x 10 to the 11th sq cm/sec) are calculated. The adiabatic variation of the atmospheric temperature with height is confirmed independently.

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