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dc.contributor.author Jones, R. A.
dc.contributor.author Breen, A. R.
dc.contributor.author Fallows, R. A.
dc.contributor.author Canals, A.
dc.contributor.author Bisi, M. M.
dc.contributor.author Lawrence, G.
dc.date.accessioned 2007-11-06T10:34:43Z
dc.date.available 2007-11-06T10:34:43Z
dc.date.issued 2007-08
dc.identifier.citation Jones , R A , Breen , A R , Fallows , R A , Canals , A , Bisi , M M & Lawrence , G 2007 , ' Interaction between coronal mass ejections and the solar wind ' Journal of Geophysical Research: Space Physics , vol 112 , no. A8 , pp. 8107 . , 10.1029/2006JA011875 en
dc.identifier.issn 2169-9402
dc.identifier.other PURE: 72713
dc.identifier.other dspace: 2160/350
dc.identifier.uri http://hdl.handle.net/2160/350
dc.identifier.uri http://www.agu.org/journals/ja en
dc.description Jones, R. A.; Breen, A. R.; Fallows, R. A.; Canals, A.; Bisi, M. M.; Lawrence, G. (2007). Interaction between coronal mass ejections and the solar wind, Journal of Geophysical Research, 112, Issue A8 RAE2008 en
dc.description.abstract Observations suggest that the interplanetary extensions of coronal mass ejections (iCMEs) may be accelerated or decelerated in their passage through the solar wind. Interplanetary scintillation measurements (IPS) can detect the passage of iCMEs beyond the field of view of the Large-Angle and Spectrometric Coronagraph coronagraphs and can provide information on their velocities. The European Incoherent Scatter Radar and the Multi Element Radio Linked Interferometer Network systems, with a field of view covering 10-120 solar radii, can provide information on iCMEs in the inner regions of the solar wind. IPS observations can also provide solar wind velocity measurements ahead of the iCME, and using this information, we consider the velocity profile of a number of clearly defined iCMEs and the relationship between iCME velocities and that of the background solar wind. The results provide additional confirmation that iCMEs converge toward the velocity of the solar wind ahead of the event and that most of the resulting acceleration or deceleration occurs in the innermost regions of the solar wind. en
dc.format.extent 1 en
dc.language.iso eng
dc.relation.ispartof Journal of Geophysical Research: Space Physics en
dc.title Interaction between coronal mass ejections and the solar wind en
dc.type Text en
dc.type.publicationtype Article (Journal) en
dc.identifier.doi http://dx.doi.org/10.1029/2006JA011875
dc.contributor.institution Institute of Mathematics & Physics (ADT) en
dc.contributor.institution Mathematics and Physics en
dc.description.status Peer reviewed en


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