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The Solar and Interplanetary Causes of Geomagnetic Activity and Quiet

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dc.contributor.author Gonzalez, W.D. en_US
dc.contributor.author Tsurutani, B.T. en_US
dc.contributor.author Tang, F. en_US
dc.date.accessioned 2004-10-03T05:09:49Z
dc.date.available 2004-10-03T05:09:49Z
dc.date.issued 1995-12 en_US
dc.identifier.citation San Francisco, CA en_US
dc.identifier.clearanceno 95-1126 en_US
dc.identifier.uri http://hdl.handle.net/2014/31444
dc.description.abstract This presentation will show that the three distinct phases of magnetic storms (initial, main, recovery) can each have considerably different characteristics during solar minimum and solar maximum. Illustrated will be the interplanetary causes of these differences; and, that a year during the descending phase of the solar cycle had significantly greater auroral activity than a year of solar maximum. en_US
dc.format.extent 41853 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other Space Physics Magnetic Storms Solar Cycles Sun en_US
dc.title The Solar and Interplanetary Causes of Geomagnetic Activity and Quiet en_US


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