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• W1619087029 abstract "The differential equation describing the response of the ionosphere to a horizontal wind-induced e.m.f. is derived and the appropriate boundary conditions are discussed. The equation is solved numerically to obtain the electric current distribution produced by several different models of the lunar semidiurnal tide. Tidal wind systems with large vertical wavelength are found to be much more efficient producers of current than wind systems of short wavelength. The current patterns produced by the lunar (2,2) mode with a maximum amplitude of 7.5 m/sec and a vertical wavelength of 85 km are very similar to the L current patterns deduced from geomagnetic observations." @default.
• W1619087029 created "2016-06-24" @default.
• W1619087029 creator A5088060589 @default.
• W1619087029 date "1970-07-01" @default.
• W1619087029 modified "2023-09-27" @default.
• W1619087029 title "The ionospheric wind dynamo—I" @default.
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• W1619087029 doi "https://doi.org/10.1016/0032-0633(70)90109-1" @default.
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