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Rotational Velocity of an Earth Model with a Liquid Core

Published online by Cambridge University Press:  14 August 2015

S. Takagi
S. Takagi*
Affiliation:
International Latitude Observatory, Mizusawa, Iwate, 023 Japan

Abstract

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There have been many papers discussing the rotation of the Earth (Jeffreys and Vicente, 1957; Molodenskij, 1961; Rochester, 1973; Smith, 1974; Shen and Mansinha, 1976). This report summarizes the application of the perturbation method of celestial mechanics to calculate the rotation of the Earth (Takagi, 1978). In this solution the Earth is assumed to consist of three components: a mantle, liquid outer core, and a solid inner core, each having a separate rotational velocity vector. Hamiltonian equations of motion were constructed to solve the rotational motion of the Earth.

Type
Part VIII: Geophysics
Information
Symposium - International Astronomical Union , Volume 82: Time and the Earth's Rotation , 1979 , pp. 313 - 314
Copyright
Copyright © Reidel 1979 

References

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