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• W2016564826 abstract "For a model of an axially symmetric magnetosphere we have constructed a theory of standing Alfvén waves with large azimuthal wavenumbers, m ⪢ 1. It is supposed that the source for such waves can be provided by extraneous currents in the ionospheric E-layer. A monochromatic source excites an oscillation of the poloidal type on the magnetic shell, having an eigenfrequency of poloidal oscillation that coincides with the source frequency. This wave, while travelling across the magnetic shells, changes from the poloidal into the toroidal wave. On the magnetic shell, whose frequency of toroidal eigenoscillations coincides with the frequency of the wave concerned, it is totally absorbed due to energy dissipation in the ionosphere." @default.
• W2016564826 created "2016-06-24" @default.
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• W2016564826 date "1993-09-01" @default.
• W2016564826 modified "2023-10-10" @default.
• W2016564826 title "A theory of transverse small-scale standing Alfvén waves in an axially symmetric magnetosphere" @default.
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• W2016564826 doi "https://doi.org/10.1016/0032-0633(93)90055-7" @default.
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