Show simple item record Bisi, Mario Mark Breen, Andrew Fallows, Richard A. Habbal, Shadia Rifai Jones, R. A. 2008-12-04T16:43:17Z 2008-12-04T16:43:17Z 2007-06-01
dc.identifier.citation Bisi , M M , Breen , A , Fallows , R A , Habbal , S R & Jones , R A 2007 , ' Large-scale structure of the fast solar wind ' Journal of Geophysical Research: Space Physics , vol 112 , no. A6 . DOI: 10.1029/2006JA012166 en
dc.identifier.issn 2169-9402
dc.identifier.other PURE: 90313
dc.identifier.other PURE UUID: 8d92b26e-e765-4cda-ae92-e4aeb7bcfed3
dc.identifier.other dspace: 2160/1383
dc.description Breen, Andrew; Bisi, M.M.; Fallows, R.A.; Habbal, S.R., (2007) 'Large-scale structure of the fast solar wind', Journal of Geophysical Research 112(A6) pp.A06101 RAE2008 en
dc.description.abstract We present the results of a comprehensive study of the fast solar wind near solar minimum conditions using interplanetary scintillation (IPS) data taken with the EISCAT system in northern Scandinavia, and a recent extremely long baseline observation using both EISCAT and MERLIN systems. The results from IPS observations suggest that the fast wind inside 100 solar radii (R ) can be represented by a two-mode model in some cases but this distinction is much less clear by in situ distances beyond 1 astronomical unit (215 R ). Two distinct fast streams are seen in the extremely long baseline IPS observation; comparison of the IPS line of sight with a synoptic map of white light indicates the faster mode overlies the polar crown and the slower fast mode overlies an equatorial extension of the polar coronal hole. en
dc.language.iso eng
dc.relation.ispartof Journal of Geophysical Research: Space Physics en
dc.rights en
dc.subject EISCAT en
dc.subject interplanetary scintillation (IPS) en
dc.subject solar wind en
dc.title Large-scale structure of the fast solar wind en
dc.type /dk/atira/pure/researchoutput/researchoutputtypes/contributiontojournal/article en
dc.contributor.institution Department of Physics en
dc.description.status Peer reviewed en

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