bio photo

Mathieu Dumberry

email: dumberry@ualberta.ca

Professor

Department of Physics
University of Alberta
Edmonton, AB
T6G 2E1
Canada
Office: CCIS 3-093

Axial inner core rotation and oscillation

An axial inner core super-rotation of approximately 0.2 deg/yr with respect to the mantle is inferred from body-wave seismology (though this results remain controversial). As a fun historical note, Edmund Halley (of comet fame) was the first to suggest that the Earth comprised an inner core and that it was rotating at a different rate than the mantle (See Fig 1, below). This suggestion appears in a Philosophical Transaction of the Royal Society paper in 1692. Halley's suggestion was motivated by observations of the Earth's magnetic field, which was then thought to be purely produced by permanent magnetization. Halley's idea of a differentially rotating "inner core" with its own magnetization could explain the observed changes of the magnetic field.

It is unclear whether the differential inner core rotation inferred by seismic observations, if indeed correct, represents a steady rotation -- driven by a thermal wind profile in the region above and below the inner core -- or a time-dependent rotation. In my previous work on this topic (in collaboration with Jon Mound, University of Leeds), we show that bounds on each of these possible scenarios can be placed on the basis of angular momentum dynamics. In turn, this places useful constraints on quantities such as the inner core viscosity and the conductance at the base of the mantle. Together with my colleague Julien Aubert (IPGP, Paris), we have investigated this question using numerical models of the geodynamo. Our conclusion is that the present-day differential rotation of the inner core most likely represents a fragment of a long timescale (hundreds of years) time-dependent motion rather than a steady super-rotation.

Figure 1: Edmund Halley's model to explain the Earth's magnetic field changes. Color patches represent permanent magnetization.

Figure 2: Meridional slice showing the time-averaged zonal flow structure in a numerical simulation of the geodynamo using a decreasing viscosity from left to right. Red (blue) corresponds to eastward (westward) flow. The change in the flow structure near the inner core boundary leads to a change in the amplitude of the torque on the inner core, and to its differential rotation rate. The black lines are superimposed magnetic field lines. Figure taken from Aubert & Dumberry, GJI, 2011.


Some of my papers on this topic

  • Dumberry, M., 2011, A new twist on inner-core spin, Nature Geoscience, 4, 216-217.

  • Aubert, J., Dumberry, M., 2011, Steady and fluctuating inner core rotation in numerical geodynamo models, Geophys. J. Int., 184, 162-170.

  • Dumberry, M., 2010, Gravitationally driven inner core differential rotation, Earth Planet. Sci. Lett., 297, 387-394.

  • Dumberry, M. and Mound, J., 2010, Inner core-mantle gravitational locking and the super-rotation of the inner core, Geophys. J. Int., 181, 806-817.

  • Dumberry, M., 2007, Geodynamic constraints on the steady and time-dependent inner core axial rotation, Geophys. J. Int., 170, 886-895.