Rotational distortion on the surfaces of Jupiter and Saturn

Details Rotational distortion on the surfaces of Jupiter and Saturn Rotational distortion on the surfaces of Jupiter and Saturn

Mar 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994em%26p...64..227m&link_type=abstract

Earth, Moon, and Planets, vol. 64, no. 3, p. 227-242

Physics

Boundary Conditions, Coefficients, Differential Equations, Jupiter (Planet), Numerical Integration, Planetary Rotation, Planetary Surfaces, Saturn (Planet), Surface Distortion, Amplitudes, Approximation, Density (Mass/Volume), Harmonics, Planetary Mass, Polynomials, Tables (Data)

Scientific paper

Having formulated the Clairaut second-order differential equations up to the fourth order in superficial distortion due to Hensen's coefficients in the previous article (El-Sharawy et al., 1989), we are now in a position to solve them. In this paper we shall discuss the methods of solving the Clairaut theory, to give an explicit form about the distortion of the surfaces of Jupiter and Saturn, numerically up to the fourth-order.

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