Other
Scientific paper
Feb 1978
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978icar...33..388m&link_type=abstract
Icarus, vol. 33, Feb. 1978, p. 388-409.
Other
4
Atmospheric Models, Jupiter Atmosphere, Jupiter Red Spot, Solitary Waves, Atmospheric Circulation, Barotropic Flow, Clouds, Flow Distribution, Gravitational Collapse, Shear Flow, Upper Atmosphere, Wave Interaction, Wave Propagation, S-Waves, Flow, Evolution, Morphology, Clouds, Jupiter, Atmosphere, Interactions, Solitary Waves
Scientific paper
Further evidence is presented that strengthens the case for the interpretation of many features in the Jovian atmosphere as solitary Rossby waves (solitons). These include: a mechanism whereby such waves can evolve from the instability of the basic shear flows; further interpretation of the interaction between observed features, and comparison with calculations of the interaction between planetary solitons of a restricted class; and calculations of soliton morphology for a type of shear flow other than the type considered originally by Maxworthy and Redekopp (1976).
Maxworthy T.
Redekopp Larry G.
Weidmann P. D.
No associations
LandOfFree
On the production and interaction of planetary solitary waves - Applications to the Jovian atmosphere does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with On the production and interaction of planetary solitary waves - Applications to the Jovian atmosphere, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and On the production and interaction of planetary solitary waves - Applications to the Jovian atmosphere will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-1035238