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Detailed Reference Information |
Love, J.J. and Gubbins, D. (1996). Dynamos driven by poloidal flow exist. Geophysical Research Letters 23: doi: 10.1029/96GL00846. issn: 0094-8276. |
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We have discovered a class of dynamos driven by purely poloidal fluid motion, thereby demonstrating that toroidal motion is not essential for dynamo action and that there is no counterpart to the anti-dynamo theorem that purely toroidal motions cannot generate magnetic fields. The fully three-dimensional (3D) dynamo action of these models results from the pushing and twisting of magnetic field lines by helical motion in a manner akin to the &agr;2 mechanism of mean-field electrodynamics. No dynamo with dipole symmetry was found for an axisymmetric distribution of helicity; indeed, some azimuthal variation in helicity is required. Among the suite of dynamos that we have investigated, the poloidal flow dynamo with the smallest critical magnetic Reynolds number is very nearly the dynamo with the most nonaxisymmetric distribution of helicity. ¿ American Geophysical Union 1996 |
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Abstract |
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Keywords
Geomagnetism and Paleomagnetism, Dynamo theories, Solar Physics, Astrophysics, and Astronomy, Magnetic fields, Planetology, Fluid Planets, Magnetic fields and magnetism, Geomagnetism and Paleomagnetism, General or miscellaneous |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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