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The Transition Between Fast and Slow Solar Wind from Composition Data
dc.contributor.authorHefti, S.en_US
dc.contributor.authorFisk, Lennard A.en_US
dc.contributor.authorGloeckler, Georgeen_US
dc.contributor.authorvon Steiger, R.en_US
dc.contributor.authorZurbuchen, Thomas H.en_US
dc.date.accessioned2006-09-11T13:50:46Z
dc.date.available2006-09-11T13:50:46Z
dc.date.issued1999-03en_US
dc.identifier.citationZurbuchen, T. H.; Hefti, S.; Fisk, L. A.; Gloeckler, G.; Von Steiger, R.; (1999). "The Transition Between Fast and Slow Solar Wind from Composition Data." Space Science Reviews 87 (1-2): 353-356. <http://hdl.handle.net/2027.42/43792>en_US
dc.identifier.issn0038-6308en_US
dc.identifier.issn1572-9672en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43792
dc.description.abstractThe transition between coronal hole associated fast solar wind and slow solar wind is studied using data from the high resolution mass spectrometer SWICS on ACE. We discuss the data in the framework of a recent theory about the global heliospheric magnetic field and conclude that the data are consistent with magnetic connections between field-lines in the fast and in the slow wind.en_US
dc.format.extent65716 bytes
dc.format.extent3115 bytes
dc.format.mimetypeapplication/pdf
dc.format.mimetypetext/plain
dc.language.isoen_US
dc.publisherKluwer Academic Publishers; Springer Science+Business Mediaen_US
dc.subject.otherPhysicsen_US
dc.subject.otherAstronomy, Astrophysics and Cosmologyen_US
dc.subject.otherCoronal Holesen_US
dc.subject.otherSolar Winden_US
dc.subject.otherIon Compositionen_US
dc.subject.otherUlyssesen_US
dc.subject.otherACEen_US
dc.subject.otherExtraterrestrial Physics, Space Sciencesen_US
dc.subject.otherElemental Fractionationen_US
dc.titleThe Transition Between Fast and Slow Solar Wind from Composition Dataen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAerospace Engineeringen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelEngineeringen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, USAen_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, USAen_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, USAen_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, USAen_US
dc.contributor.affiliationumDepartment of Atmospheric, Oceanic and Space Sciences, University of Michigan, Ann Arbor, USAen_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43792/1/11214_2004_Article_234059.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1023/A:1005126718714en_US
dc.identifier.sourceSpace Science Reviewsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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