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- W2059647549 startingPage "229" @default.
- W2059647549 abstract "Motion of a conducting fluid distorts magnetic lines of force permeating the fluid. The magnetic field is dragged and amplified by the fluid motion. It has been thought that such an interaction between motions and magnetic fields is actually taking place within the earth's core. Time-dependent behaviour of magnetic lines of force deformed by a pair of convection cells is obtained by solving a non-steady equation of magnetic field in a conducting fluid with the intention of examining the fields above convective up-and downflows in the core's top layer. The computation is successively made for initially uniform as well as non-uniform fields by a method similar to the relaxation technique on the assumption that the fluid velocity is fixed and prescribed. The results obtained here qualitatively indicate that up- and down-flows in the core's top layer may possibly induce the non-dipole highs and lows at the earth's surface." @default.
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- W2059647549 date "1967-01-01" @default.
- W2059647549 modified "2023-10-18" @default.
- W2059647549 title "Magnetic Lines of Force Deformed by Motion of a Conducting Fluid (I)" @default.
- W2059647549 doi "https://doi.org/10.5636/jgg.19.229" @default.
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