The Composition of Interplanetary Coronal Mass Ejections
dc.contributor.author | Zurbuchen, Thomas H. | en_US |
dc.contributor.author | Fisk, Lennard A. | en_US |
dc.contributor.author | Lepri, Susan T. | en_US |
dc.contributor.author | von Steiger, R. | en_US |
dc.date.accessioned | 2011-11-15T16:05:45Z | |
dc.date.available | 2011-11-15T16:05:45Z | |
dc.date.issued | 2003-09-02 | en_US |
dc.identifier.citation | Zurbuchen, Thomas H.; Fisk, L. A.; Lepri, S. T.; von Steiger, R. (2003). "The Composition of Interplanetary Coronal Mass Ejections." AIP Conference Proceedings 679(1): 604-607. <http://hdl.handle.net/2027.42/87653> | en_US |
dc.identifier.other | APCPCS-679-1 | en_US |
dc.identifier.uri | https://hdl.handle.net/2027.42/87653 | |
dc.description.abstract | Interplanetary coronal mass ejection (ICME) associated plasma can exhibit signatures in elemental, ionic and isotopic composition. These signatures occur in less than 50% of all ICMEs, but are very indicative of ICME plasma. We review these compositional anomalies and briefly discuss a physical scenario that could be responsible for these anomalies. © 2003 American Institute of Physics | en_US |
dc.publisher | The American Institute of Physics | en_US |
dc.rights | © The American Institute of Physics | en_US |
dc.title | The Composition of Interplanetary Coronal Mass Ejections | en_US |
dc.type | Article | en_US |
dc.subject.hlbsecondlevel | Physics | en_US |
dc.subject.hlbtoplevel | Science | en_US |
dc.description.peerreviewed | Peer Reviewed | en_US |
dc.description.bitstreamurl | http://deepblue.lib.umich.edu/bitstream/2027.42/87653/2/604_1.pdf | |
dc.identifier.doi | 10.1063/1.1618667 | en_US |
dc.identifier.source | SOLAR WIND TEN: Proceedings of the Tenth International Solar Wind Conference | en_US |
dc.owningcollname | Physics, Department of |
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