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

Tsurutani, B. T.; Zhou,  X. Y.; Gonzalez,  W. D.

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