A possible explanation of the mechanism of formation of the equatorial jet on the surface of Jupiter

Physics

Scientific paper

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Fluid Jets, Jupiter (Planet), Planetary Surfaces, Cylindrical Bodies, Reynolds Number, Rotating Fluids, Shear Layers, Taylor Instability

Scientific paper

Formation of the equatorial jet of the Jovian surface was explained as a consequence of the Taylor-Proudman theorem. The asymptotic theory of motion of low viscosity fluids in a rotating spherical shear layer was included. The model shows the striated structure of the Jovian surface as the outflow of convective cells having the shape of axisymmetric rolls extended along the axis of rotation in the meridional direction. Depth of the layer was found to be of the order of 1000 kilometers.

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