https://scholars.lib.ntu.edu.tw/handle/123456789/408056
標題: | From stable dipolar towards reversing numerical dynamos | 作者: | Annadurai G. Juang R.-S. Lee D.-J. |
關鍵字: | Geodynamo simulations;Geomagnetism;Reversals | 公開日期: | 2002 | 卷: | 131 | 期: | 1 | 起(迄)頁: | 29-45 | 來源出版物: | Physics of the Earth and Planetary Interiors | 摘要: | We are using a three-dimensional convection-driven numerical dynamo model without hyperdiffusivity to study the characteristics structure and time variability of the magnetic field in dependence of the Rayleigh number (Ra) for values up to 40 times supercritical. We also compare a variety of ways to drive the convection and basically find two dynamo regimes. At low Ra, the magnetic field at the surface of the model is dominated by the non-reversing axial dipole component. At high Ra, the dipole part becomes small in comparison to higher multipole components. At transitional values of Ra, the dynamo vacillates between the dipole-dominated and the multipolar regime, which includes excursions and reversals of the dipole axis. We discuss, in particular, one model of chemically driven convection, where for a suitable value of Ra, the mean dipole moment and the temporal evolution of the magnetic field resemble the known properties of the Earth's field from paleomagnetic data. ? 2002 Elsevier Science B.V. All rights reserved. |
URI: | https://scholars.lib.ntu.edu.tw/handle/123456789/408056 | ISSN: | 00319201 | DOI: | 10.1016/S0031-9201(02)00016-X |
顯示於: | 化學工程學系 |
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