Inner core tilt and polar motion

Details Inner core tilt and polar motion Inner core tilt and polar motion

Nov 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002geoji.151..377d&link_type=abstract

Geophysical Journal International, Volume 151, Issue 2, pp. 377-392.

Astronomy and Astrophysics

Astronomy

14

Chandler Wobble, Earth'S Magnetic Field, Earth'S Rotation, Inner Core Viscosity, Inner Core Wobble, Markowitz Wobble

Scientific paper

A tilted inner core permits exchange of angular momentum between the core and the mantle through gravitational and pressure torques and, as a result, changes in the direction of Earth's axis of rotation with respect to the mantle. We have developed a model to calculate the amplitude of the polar motion that results from an equatorial torque at the inner core boundary which tilts the inner core out of alignment with the mantle. We specifically address the issue of the role of the inner core tilt in the decade polar motion known as the Markowitz wobble. We show that a decade polar motion of the same amplitude as the observed Markowitz wobble requires a torque of 1020 N m which tilts the inner core by 0.07 degrees. This result critically depends on the viscosity of the inner core; for a viscosity less than 5 × 1017 Pa s, larger torques are required. We investigate the possibility that a torque of 1020 N m with decadal periodicity can be produced by electromagnetic coupling between the inner core and torsional oscillations of the flow in the outer core. We demonstrate that a radial magnetic field at the inner core boundary of 3 to 4 mT is required to obtain a torque of such amplitude. The resulting polar motion is eccentric and polarized, in agreement with the observations. Our model suggests that equatorial torques at the inner core boundary might also excite the Chandler wobble, provided there exists a physical mechanism that can generate a large torque at a 14 month period.

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