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- W11092106 abstract "In contrast with the popular model of two sources of Pc pulsations, “external” and “internal”, a new concept assuming a common extra-magnetosphere origin is suggested, the idea being that the two distinct types of upstream waves in the solar wind lead to two types of Pc pulsations on the ground. The transverse monochromatic F — B dependent upstream waves are presumed responsible for generation of the solar wind-controlled Pcsw pulsations, while the multichromatic highly compressional upstream waves are presumed responsible for generation of the magnetosphere-controlled Pcmg pulsations. “High latitude entry” for Pcgw and “direct entry” through the sub-solar magnetopause into the magnetosphere for Pcmg is suggested and discussed. Experimental evidence supporting these hypotheses is presented." @default.
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- W11092106 date "1997-03-01" @default.
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- W11092106 title "Role of Solar Wind Wave Events in the Generation of Geomagnetic Pulsations" @default.
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- W11092106 doi "https://doi.org/10.1007/bf03325486" @default.
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