Convective instability and vortices on a rotating sphere

Details Convective instability and vortices on a rotating sphere Convective instability and vortices on a rotating sphere

Oct 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987pmtf........91k&link_type=abstract

PMTF - Zhurnal Prikladnoi Mekhaniki i Tekhnicheskoi Fiziki (ISSN 0044-4626), Sept.-Oct. 1987, p. 91-101. In Russian.

Computer Science

Numerical Analysis

Convective Flow, Jupiter Red Spot, Planetary Rotation, Rotating Spheres, Vortices, Atmospheric Boundary Layer, Flow Stability, Numerical Analysis

Scientific paper

The paper is concerned with the problem of the formation and long existence of large-scale vortices in the atmospheres of rotating planets. By using the thin atmosphere approximation, the solution of the problem of stationary flow structures inside a spherical layer is investigated in the large. The interpretation of the great Red Spot on Jupiter in terms of the theory of normal eigenfunctions in a rotating atmosphere is discussed.

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