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The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments

dc.contributor.authorvon Steiger, R.en_US
dc.contributor.authorZurbuchen, Thomas H.en_US
dc.contributor.authorGeiss, Johannesen_US
dc.contributor.authorGloeckler, Georgeen_US
dc.contributor.authorSchwadron, Nathan A.en_US
dc.contributor.authorFisk, Lennard A.en_US
dc.date.accessioned2006-09-11T13:51:54Z
dc.date.available2006-09-11T13:51:54Z
dc.date.issued2001-03en_US
dc.identifier.citationvon Steiger, R.; Zurbuchen, T.H.; Geiss, J.; Gloeckler, G.; Fisk, L.A.; Schwadron, N.A.; (2001). "The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments." Space Science Reviews 97 (1-4): 123-127. <http://hdl.handle.net/2027.42/43805>en_US
dc.identifier.issn0038-6308en_US
dc.identifier.issn1572-9672en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/43805
dc.description.abstractThe source region of solar wind plasma is observed to be directly reflected in the compositional pattern of both elemental and charge state compositions. Slow solar wind associated with streamers shows higher freeze-in temperatures and larger FIP enhancements than coronal hole associated wind. Also, the variability of virtually all compositional parameters is much higher for slow solar wind compared to coronal hole associated wind. We show that these compositional patterns persist even though stream-stream interactions complicate the identification based on in situ plasma parameters.en_US
dc.format.extent106858 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.otherExtraterrestrial Physics, Space Sciencesen_US
dc.subject.otherAstronomy, Astrophysics and Cosmologyen_US
dc.titleThe 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experimentsen_US
dc.typeArticleen_US
dc.subject.hlbsecondlevelAtmospheric, Oceanic and Space Sciencesen_US
dc.subject.hlbsecondlevelAerospace Engineeringen_US
dc.subject.hlbtoplevelScienceen_US
dc.subject.hlbtoplevelEngineeringen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDept. of AOSS, University of Michigan, Ann Arbor, MI , 48109, U.S.Aen_US
dc.contributor.affiliationumDept. of AOSS, University of Michigan, Ann Arbor, MI , 48109, U.S.Aen_US
dc.contributor.affiliationumDept. of AOSS, University of Michigan, Ann Arbor, MI , 48109, U.S.Aen_US
dc.contributor.affiliationumDept. of AOSS, University of Michigan, Ann Arbor, MI , 48109, U.S.Aen_US
dc.contributor.affiliationotherInternational Space Science Institute, Bern, Switzerlanden_US
dc.contributor.affiliationotherInternational Space Science Institute, Bern, Switzerlanden_US
dc.contributor.affiliationumcampusAnn Arboren_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/43805/1/11214_2004_Article_338816.pdfen_US
dc.identifier.doihttp://dx.doi.org/10.1023/A:1011886414964en_US
dc.identifier.sourceSpace Science Reviewsen_US
dc.owningcollnameInterdisciplinary and Peer-Reviewed


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