On the dynamical implications of models of Bs in the Earth’s core
On the dynamical implications of models of Bs in the Earth’s core
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DOI:
10.1046/j.1365-246x.1999.00909.x
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发表时间:
1999-09
影响因子:
2.8
通讯作者:
S. Zatman;J. Bloxham
中科院分区:
文献类型:
--
作者:
S. Zatman;J. Bloxham
SUMMARY Recent work has shown that the zonal, equatorially symmetric, time-varying part of a model of the £ow at the surface of the Earth’s core can be well explained by only two standing waves, and that by making certain assumptions these waves may be inverted for rms Bs (the component of ¢eld pointing away from the rotation axis) and a quantity parametrizing friction or excitation (F) of the waves. Here, we discuss the two-wave ¢t, and describe the implications of models of rms Bs and friction/excitation for the dynamic state of the core, for the torque balance on axial cylinders, and for recent numerical simulations of the geodynamo.We ¢nd several possible explanations for why only two standing waves are needed to ¢t the data, including the possibility that it is due to the resolution of the core £ow model rather than conditions within the core itself.We ¢nd that the ¢ts of rms Bs and F suggest that the role of inertia should not be discounted in the core, and that care should be taken in constructing geodynamo simulations so that the eiective friction at the core^mantle boundarydoes not swamp the inertial term. A ratio of the magnitude of the two appears to be O(1) in the Earth’s core: we believe that, ideally, a numerical model of the Earth’s core should reproduce this result.