Topographic core-mantle coupling and polar motion on decadal time-scales
Topographic core-mantle coupling and polar motion on decadal time-scales
复制标题
十年时间尺度上的地形核幔耦合和极移
DOI:
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发表时间:
1996
期刊:
影响因子:
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通讯作者:
A. Jackson
中科院分区:
文献类型:
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作者:
R. Hide;D. Boggs;J. Dickey;D. Dong;R. Gross;A. Jackson
SUMMARY Associated with non-steady magnetohydrodynamic (MHD) flow in the liquid metallic core of the Earth, with typical relative speeds of a fraction of a millimetre per second, are fluctuations in dynamic pressure of about lo3 N m-2. Acting on the non-spherical core-mantle boundary (CMB), these pressure fluctuations give rise to a fluctuating net topographic torque Li(t) (i = 1,2,3twhere t denotes time--on the overlying solid mantle. Geophysicists now accept the proposal by one of us (RH) that L,(t) makes a significant and possibly dominant contribution to the total torque LT( t) on the mantle produced directly or indirectly by core motions. Other contributions are the ‘gravitational’ torque associated with fluctuating density gradients in the core, the ‘electromagnetic’ torque associated with Lorentz forces in the weakly electrically conducting lower mantle, and the ‘viscous’ torque associated with shearing motions in the boundary layer just below the CMB. The axial component L;(t) of LT(t) contributes to the observed fluctuations in the length of the day CLOD, an inverse measure of the angular speed of rotation of the solid Earth (mantle, crust and cryosphere)], and the equatorial components (Lf(t), L;(t)) = L*(t) contribute to the observed polar motion, as determined from measurements of changes in the Earth’s rotation axis relative to its figure axis. In earlier phases of a continuing programme of research based on a method for determining Li( t) from geophysical data (proposed independently about ten years ago by Hide and Le Mouel), it was shown that longitude-dependent irregular CMB topography no higher than about 0.5 km could give rise to values of L3(t) sufficient to account for the observed magnitude of LOD fluctuations on decadal time-scales. Here, we report an investigation of the equatorial components (L,(t), L2(t)) = L (t) of Li(t) taking into account just one topographic feature of the CMB-albeit possibly the most pronounced-namely the axisymmetric equatorial bulge, with an equatorial radius exceeding the polar radius by 9.5 kO.1 km (the mean radius of the core being 3485 2 km, 0.547 times that of the whole Earth). A measure of the local horizontal gradient of the fluctuating pressure field near the CMB can be obtained from the local Eulerian flow velocity in the ‘free stream’ below the CMB by supposing that nearly everywhere in the outer reaches of the core-the ‘polosphere’ (Hide 1995tgeostrophic balance obtains between the pressure gradient and Coriolis forces. The polospheric