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Spatial Relationship of Signatures of Interplanetary Coronal Mass Ejections
dc.contributor.authorRichardson, I. G.en_US
dc.contributor.authorCane, H. V.en_US
dc.contributor.authorLepri, Susan T.en_US
dc.contributor.authorZurbuchen, Thomas H.en_US
dc.contributor.authorGosling, J. T.en_US
dc.date.accessioned2011-11-15T16:05:41Z
dc.date.available2011-11-15T16:05:41Z
dc.date.issued2003-09-02en_US
dc.identifier.citationRichardson, I. G.; Cane, H. V.; Lepri, S. T.; Zurbuchen, T. H.; Gosling, J. T. (2003). "Spatial Relationship of Signatures of Interplanetary Coronal Mass Ejections." AIP Conference Proceedings 679(1): 681-684. <http://hdl.handle.net/2027.42/87650>en_US
dc.identifier.otherAPCPCS-679-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87650
dc.description.abstractInterplanetary coronal mass ejections (ICMEs) are characterized by a number of signatures. In particular, we examine the relationship between Fe charge states and other signatures during ICMEs in solar cycle 23. Though enhanced Fe charge states characterize many ICMEs, average charge states vary from event to event, are more likely to be enhanced in faster or flare‐related ICMEs, and do not appear to depend on whether the ICME is a magnetic cloud. © 2003 American Institute of Physicsen_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleSpatial Relationship of Signatures of Interplanetary Coronal Mass Ejectionsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelPhysicsen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/87650/2/681_1.pdf
dc.identifier.doi10.1063/1.1618686en_US
dc.identifier.sourceSOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conferenceen_US
dc.owningcollnamePhysics, Department of


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