Computer Science – Numerical Analysis
Scientific paper
Mar 1980
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1980icar...41..400b&link_type=abstract
Icarus, vol. 41, Mar. 1980, p. 400-409. Research supported by the Science Research Council of England.
Computer Science
Numerical Analysis
Baroclinic Waves, Jupiter Atmosphere, Jupiter Red Spot, Shear Flow, Solitary Waves, Flow Distribution, Numerical Analysis, Shear Layers, Zonal Flow (Meteorology), Jupiter, Great Red Spot, Solitary Waves, Shear, Flow, Baroclinity, Atmosphere, Streamlines, Mathematical Models, Data, Velocity, Theoretical Studies
Scientific paper
A baroclinic model of the Jovian atmosphere is assumed. The zonal flow in the neighborhood of the Great Red Spot has been modeled by an unsymmetrical shear layer. The calculated solitary wave flow fields consist of various combinations of regions of closed streamlines and regions of reversed flow. Some of these flow fields closely resemble those observed around the Great Red Spot but the lack of accurate atmospheric data makes it difficult to determine the type of flow field that would be predicted by the theory.
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