Sources of geomagnetic activity over the solar cycle: Relative importance of coronal mass ejections, high‐speed streams, and slow solar wind

Publisher： John Wiley & Sons Inc

E-ISSN： 2156-2202|105|A8|18203-18213

ISSN： 0148-0227

Source： Journal Of Geophysical Research, Vol.105, Iss.A8, 2000-08, pp. : 18203-18213

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