Hydrostatic equilibrium of three concentric masses in rotation

Details Hydrostatic equilibrium of three concentric masses in rotation Hydrostatic equilibrium of three concentric masses in rotation

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988hetc.rept.....h&link_type=abstract

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Physics

Angular Velocity, Gravitational Fields, Gravitational Waves, Hydrostatic Pressure, Concentricity, Earth Rotation, Planetary Mass, Radii, Rotation

Scientific paper

A system of three concentric homogeneous masses in rotation with angular velocity, omega, may represent a simple model of the earth-ocean-atmosphere system. Their hydrostatic pressures and gravitational potentials are determined. The hydrostatic pressure, P sub 1, and the gravitational potential, U sub 1, depend on R sup 2. The gravitational potential, U sub 4, depends on R sup -1 (R is the radius). The remaining parameters depend on R sup 2 and R sup -1. These pressures and potentials are important in the gravity waves research in the interface earth-ocean-atmosphere.

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