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Rotational Accelerations

Published online by Cambridge University Press:  27 June 2016

Wm. Markowitz*
Affiliation:
Marquette University, Milwaukee, Wisconsin 53233, U.S.A.

Abstract

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Rotational accelerations of the Earth arise from changes in speed of rotation: periodic, irregular, and secular. Changes are caused by winds, Earth tides, ocean tides, and motions of the core. The semimonthly lunar body tide produces the maximum acceleration.

Type
Research Article
Copyright
Copyright © Reidel 1972 

References

Guinot, B.: 1970a, Astron. Astrophys. 8, 26.Google Scholar
Guinot, B.: 1970b, in Mansinha, L. et al. (eds.), Earthquake Displacement Fields and the Rotation of the Earth, p. 60.Google Scholar
Markowitz, W.: 1959, Astron. J. 64, 106.CrossRefGoogle Scholar
Markowitz, W.: 1970, in Mansinha, L. et al. (eds.), Earthquake Displacement Fields and the Rotation of the Earth, p. 70.Google Scholar