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Interplanetary Origin of Geomagnetic Activity in the Declining Phase of the Solar Cycle

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dc.contributor.author Tsurutani, B.T. en_US
dc.contributor.author Gonzalez, W.D. en_US
dc.contributor.author Gonzalez, A.L.C. en_US
dc.contributor.author Tang, F. en_US
dc.contributor.author Arballo, J.K. en_US
dc.contributor.author Okada, M. en_US
dc.date.accessioned 2004-10-04T21:21:08Z
dc.date.available 2004-10-04T21:21:08Z
dc.date.issued 1995-02 en_US
dc.identifier.citation Pasadena, CA en_US
dc.identifier.clearanceno 95-1551 en_US
dc.identifier.uri http://hdl.handle.net/2014/32203
dc.description.abstract Interplanetary magnetic field and plasma data are compared with ground-based geomagnetic Dst and AE indices to determine the causes of magnetic storms, substorms, and quiet during the descending phase of the solar cycle. The primary focus is on 1974 data characterized by the presence of two long-lasting corotating streams associated with coronal holes. en_US
dc.format.extent 922180 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Space Physics Magnetic Storms Geomagnetics Solar Corona Alfven Waves en_US
dc.title Interplanetary Origin of Geomagnetic Activity in the Declining Phase of the Solar Cycle en_US


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