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- W2077776086 abstract "It is shown that the steady magnetospheric motion generated by the solar wind is current free in the first approximation, regardless of the driving mechanism. Also the sufficient condition for the hydromagnetic stability of cold plasma in the presence of an external magnetic field and a steady motion is obtained. Based on these theoretical estimations the damped-type geomagnetic pulsations associated with geomagnetic storms are interpreted as an interaction between hydromagnetic oscillations and magnetospheric motions caused by solar winds." @default.
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- W2077776086 title "Magnetospheric convections and damped-type geomagnetic pulsations associated with storms" @default.
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- W2077776086 doi "https://doi.org/10.1016/0032-0633(70)90178-9" @default.
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