The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments
dc.contributor.author | von Steiger, R. | en_US |
dc.contributor.author | Zurbuchen, Thomas H. | en_US |
dc.contributor.author | Geiss, Johannes | en_US |
dc.contributor.author | Gloeckler, George | en_US |
dc.contributor.author | Schwadron, Nathan A. | en_US |
dc.contributor.author | Fisk, Lennard A. | en_US |
dc.date.accessioned | 2006-09-11T13:51:54Z | |
dc.date.available | 2006-09-11T13:51:54Z | |
dc.date.issued | 2001-03 | en_US |
dc.identifier.citation | von 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.issn | 0038-6308 | en_US |
dc.identifier.issn | 1572-9672 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/43805 | |
dc.description.abstract | The 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.extent | 106858 bytes | |
dc.format.extent | 3115 bytes | |
dc.format.mimetype | application/pdf | |
dc.format.mimetype | text/plain | |
dc.language.iso | en_US | |
dc.publisher | Kluwer Academic Publishers; Springer Science+Business Media | en_US |
dc.subject.other | Physics | en_US |
dc.subject.other | Extraterrestrial Physics, Space Sciences | en_US |
dc.subject.other | Astronomy, Astrophysics and Cosmology | en_US |
dc.title | The 3-D Heliosphere from the Ulysses and ACE Solar Wind Ion Composition Experiments | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Atmospheric, Oceanic and Space Sciences | en_US |
dc.subject.hlbsecondlevel | Aerospace Engineering | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.subject.hlbtoplevel | Engineering | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.contributor.affiliationum | Dept. of AOSS, University of Michigan, Ann Arbor, MI , 48109, U.S.A | en_US |
dc.contributor.affiliationum | Dept. of AOSS, University of Michigan, Ann Arbor, MI , 48109, U.S.A | en_US |
dc.contributor.affiliationum | Dept. of AOSS, University of Michigan, Ann Arbor, MI , 48109, U.S.A | en_US |
dc.contributor.affiliationum | Dept. of AOSS, University of Michigan, Ann Arbor, MI , 48109, U.S.A | en_US |
dc.contributor.affiliationother | International Space Science Institute, Bern, Switzerland | en_US |
dc.contributor.affiliationother | International Space Science Institute, Bern, Switzerland | en_US |
dc.contributor.affiliationumcampus | Ann Arbor | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/43805/1/11214_2004_Article_338816.pdf | en_US |
dc.identifier.doi | http://dx.doi.org/10.1023/A:1011886414964 | en_US |
dc.identifier.source | Space Science Reviews | en_US |
dc.owningcollname | Interdisciplinary and Peer-Reviewed |
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