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Magnetic cloud induced magnetic storms: a lack of classical substorm expansion phases

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dc.contributor.author Tsurutani, B. T. en_US
dc.contributor.author Zhou, X. Y. en_US
dc.contributor.author Gonzalez, W. D. en_US
dc.date.accessioned 2004-09-22T23:41:34Z
dc.date.available 2004-09-22T23:41:34Z
dc.date.issued 2001-05-15 en_US
dc.identifier.citation Journal of geophysical research en_US
dc.identifier.clearanceno 01-1151 en_US
dc.identifier.uri http://hdl.handle.net/2014/12830
dc.description.abstract The purpose of this paper will be to examine a specific but important subset of magnetic storms, those that are caused by large southward, smoothly rotating magnetic fields: interplanetary magnetic clouds. en_US
dc.format.extent 2756967 bytes
dc.format.mimetype application/pdf
dc.language.iso en_US
dc.subject.other magnetic storms substorm expansion phases en_US
dc.title Magnetic cloud induced magnetic storms: a lack of classical substorm expansion phases en_US


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