作者: R.N. Dewitt , S.-I. Akasofu
DOI: 10.1016/0032-0633(65)90109-1
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摘要: Abstract The distribution of the dynamo-induced electrostatic field obtained by Maeda and Kato is discussed in terms ionospheric winds, motion magnetospheric plasma resulting from further discussed. It suggested that can affect configuration radiation belts a certain similarity exists between flow patterns observed day-night asymmetry belts. A possible significance this regarding auroral phenomena suggested.