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dc.contributor.author Fallows, R. A.
dc.contributor.author Breen, A. R.
dc.contributor.author Bisi, M. M.
dc.contributor.author Jones, R. A.
dc.contributor.author Dorrian, Gareth David
dc.date.accessioned 2013-07-13T04:15:08Z
dc.date.available 2013-07-13T04:15:08Z
dc.date.issued 2007-12-01
dc.identifier.citation Fallows , R A , Breen , A R , Bisi , M M , Jones , R A & Dorrian , G D 2007 , ' Interplanetary scintillation using EISCAT and MERLIN: extremely long baselines at multiple frequencies ' Astronomical and Astrophysical Transactions , vol 26 , no. 6 , pp. 489-500 . DOI: 10.1080/10556790701612197 en
dc.identifier.issn 1055-6796
dc.identifier.other PURE: 1201261
dc.identifier.other PURE UUID: 53b4cceb-df04-45f6-bea4-83eb41591e88
dc.identifier.other Bibtex: urn:e9c9e1629e43d888d396972750cf4e57
dc.identifier.other handle.net: 2160/9252
dc.identifier.uri http://hdl.handle.net/2160/9252
dc.description Special Issue: International Colloquium ‚Scattering and Scintillation in Radioastronomy’, June 19–23 2006, Pushchino, Moscow Region, Russia en
dc.description.abstract Improvements to two of the radio telescopes of European Incoherent SCATter radar (EISCAT) allow measurements of Interplanetary Scintillation (IPS) at 1.4 GHz, and this has prompted two major developments in studies of IPS. Simultaneous observations between EISCAT and MERLIN allow baselines of up to 2000 km, significantly improving velocity resolution and making possible much greater accuracy in determining the direction of flow than previously, as well as demonstrating that density variations in the slow solar wind remain partially correlated for at least 8 s. Initial results suggest two fast solar wind modes, and there is evidence for super-radial (meridional) expansion of the fast solar wind. Trials have been conducted using different observing frequencies at different sites, including the use of the EISCAT Svalbard Radar for IPS for the first time. Observations at 500, 928 and 1420 MHz with baselines of up to 1200 km have been carried out. The results are found to be consistent between single- and dual-frequency correlations, allowing the range of observations possible with the EISCAT system to be expanded. en
dc.format.extent 12 en
dc.language.iso eng
dc.relation.ispartof Astronomical and Astrophysical Transactions en
dc.rights en
dc.subject solar wind en
dc.subject interplanetary scintillation en
dc.subject coronal mass ejections en
dc.title Interplanetary scintillation using EISCAT and MERLIN: extremely long baselines at multiple frequencies en
dc.type /dk/atira/pure/researchoutput/researchoutputtypes/contributiontojournal/article en
dc.identifier.doi https://doi.org/10.1080/10556790701612197
dc.contributor.institution Department of Physics en
dc.description.status Peer reviewed en


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