Possible Fluid Dynamical Interpretation of Some Reported Features in the Jovian Atmosphere
TONY MAXWORTHY 1 and
LARRY G. REDEKOPP 2
1 Departments of Mechanical and Aerospace Engineering, University of Southern California, Los Angeles 90007, and Planetary Atmospheres Section, Jet Propulsion Laboratory, Pasadena, California 91103
2 Department of Aerospace Engineering, University of Southern California, Los Angeles
Flow patterns of some of the features in the Voyager 1 imaging data for Jupiter appear to be consistent with those predicted by a solitary-wave theory.
Submitted on February 11, 1980
Revised on June 24, 1980