Other
Scientific paper
Oct 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976icar...29..261m&link_type=abstract
(IAU, NASA, and NSF, Jupiter Colloquium, 30th, Tucson, Ariz., May 18-23, 1975.) Icarus, vol. 29, Oct. 1976, p. 261-271.
Other
30
Jupiter Atmosphere, Jupiter Red Spot, Rossby Regimes, Shear Flow, Solitary Waves, Astronomical Models, Atmospheric Models, Eigenvalues, Propagation Modes, Wave Equations, Wave Interaction
Scientific paper
It is shown that solitary waves in a planetary zonal shear have a shape and flow field that are virtually identical to those observed around the Red Spot and numerous other features that have been seen in the Jovian atmosphere. It is suggested that the theoretically calculated interaction between solitary waves has many characteristics in common with the observed interactions between these same Jovian features, and available atmospheric models are shown to be consistent with the very restrictive requirements of the theory.
Maxworthy T.
Redekopp Larry G.
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