Effect of rotation on the natural oscillation spectrum of Jupiter and Saturn

Physics

Scientific paper

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Jupiter (Planet), Oscillations, Planetary Radiation, Planetary Rotation, Radiation Spectra, Saturn (Planet), Adiabatic Conditions, Integral Equations, Perturbation Theory, Scalars

Scientific paper

The natural oscillation spectrum of Jupiter and Saturn (first calculated by Vorontsov et al., 1976) is conditioned by the gaseous-liquid structure of these planets. In the present paper, perturbation theory is used to analyze the effects of planetary rotation on the natural oscillation spectrum. A solution is obtained for the equation of small adiabatic oscillations.

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