A review of Jovian atmospheric dynamics

Physics

Scientific paper

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Scientific paper

A brief review is presented of available knowledge of the fluid motions within Jupiter's atmosphere. Evidence is presented to support the contention that the observed cloud masses are probably not simply convected by the main zonal flows. It is likely that an understanding of wave motions within the atmosphere will be of great importance in interpreting data gathered both from the ground and from spacecraft. Permanent affiliation Departments of Aerospace and Mechanical Engineering, University of Southern California, Los Angeles, California 90007, U.S.A.

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