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ICME Observations During the Ulysses Fast Latitude Scan

dc.contributor.authorForsyth, R. J.en_US
dc.contributor.authorRees, A.en_US
dc.contributor.authorReisenfeld, Daniel B.en_US
dc.contributor.authorLepri, Susan T.en_US
dc.contributor.authorZurbuchen, Thomas H.en_US
dc.date.accessioned2011-11-15T16:05:42Z
dc.date.available2011-11-15T16:05:42Z
dc.date.issued2003-09-02en_US
dc.identifier.citationForsyth, R. J.; Rees, A.; Reisenfeld, D. B.; Lepri, S. T.; Zurbuchen, T. H. (2003). "ICME Observations During the Ulysses Fast Latitude Scan." AIP Conference Proceedings 679(1): 715-720. <http://hdl.handle.net/2027.42/87651>en_US
dc.identifier.otherAPCPCS-679-1en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/87651
dc.description.abstractBetween November 2000 and October 2001 the Ulysses spacecraft performed a fast traversal of the heliospheric latitudes between 80°S and 80°N, a period close to the activity maximum of the current solar cycle. This paper provides an overview of the Ulysses observations of the transient solar wind structures associated with coronal mass ejections (ICMEs) during this period. Compared to the previous Ulysses fast latitude scan near solar minimum in 1995, many more ICME related signatures were observed in the present data set. Events were encountered spread over the full latitude range between 80°S and 80°N. Those at high northern latitudes, where fast solar wind from a northern polar coronal hole had become re‐established, were of the over‐expanding type first identified in Ulysses data at mid‐latitudes near solar minimum. The signatures of these events and their latitude dependence are discussed and some ongoing and possible future studies with this data set are described. © 2003 American Institute of Physicsen_US
dc.publisherThe American Institute of Physicsen_US
dc.rights© The American Institute of Physicsen_US
dc.titleICME Observations During the Ulysses Fast Latitude Scanen_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/2027.42/87651/2/715_1.pdf
dc.identifier.doi10.1063/1.1618693en_US
dc.identifier.sourceSOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conferenceen_US
dc.owningcollnamePhysics, Department of


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