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Geophysical Monograph Series

 

Keywords

  • Earth sciences—Mathematical models
  • Geophysics—Mathematical models

Index Terms

  • 1239 Geodesy and Gravity: Rotational variations
  • 7240 Seismology: Structure of mantle and core

Article

GEOPHYSICAL MONOGRAPH SERIES, VOL. 76, PP. 107-120, 1993

Topographic core-mantle coupling and fluctuations in the Earth's rotation

R. Hide

Robert Hooke Institute, The Observatory, Clarendon Laboratory, Parks Road Oxford 0X1 3PU, England, U.K.


R. W. Clayton

Seismological Laboratory, California Institute of Technology Pasadena, CA 91125. U.S.A.


B. H. Hager

Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA 02139, U.S.A.


M. A. Spieth

Jet Propulsion Laboratory, California Institute of Technology Pasadena, CA 91109, U.S.A.


C. V. Voorhdes

Geodynamics Branch Code 921, Goddard Space Flight Center, Greenbelt, MD 20771, U.S.A.


Astronomically-determined irregular fluctuations in the Earth's rotation vector on decadal time scales can be used to estimate the fluctuating torque on the lower surface of the Earth's mantle produced by magnetohydrodynamic flow in the underlying liquid metallic core. A method has been proposed for testing the hypothesis that the torque is due primarily to fluctuating dynamic pressure forces acting on irregular topographic features of the core-mantle boundary and also on the equatorial bulge. The method exploits (a) geostrophically-constrained models of fluid motions in the upper reaches of the core based on geomagnetic secular variation data, and (b) patterns of the topography of the CMB based on the mantle flow models constrained by data from seismic tomography, determinations of long wave-length anomalies of the Earth's gravitational field and other geophysical and geodetic data. According to the present study, the magnitude of the axial component of the torque implied by determinations of irregular changes in the length of the day is compatible with models of the Earth's deep interior characterized by the presence of irregular CMB topography of effective “height” no more than about 0.5 km (about 6% of the equatorial bulge) and strong horizontal variations in the properties of the D″ layer at the base of the mantle. The investigation is now being extended to cover a wider range of epochs and also the case of polar motion on decadal time scales produced by fluctuations in the equatorial components of the torque.

Citation: Hide, R., R. W. Clayton, B. H. Hager, M. A. Spieth, and C. V. Voorhdes (1993), Topographic core-mantle coupling and fluctuations in the Earth's rotation, in Relating Geophysical Structures and Processes: The Jeffreys Volume, Geophys. Monogr. Ser., vol. 76, edited by K. Aki and R. Dmowska, pp. 107–120, AGU, Washington, D. C., doi:10.1029/GM076p0107.

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