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dc.contributor.authorMcCrea, Ian W.
dc.contributor.authorAikio, Anita
dc.contributor.authorAlfonsi, Lucilla
dc.contributor.authorBelova, Evgenia
dc.contributor.authorBuchert, Stephan C.
dc.contributor.authorClilverd, Mark
dc.contributor.authorEngler, Norbert
dc.contributor.authorGustavsson, Björn Johan
dc.contributor.authorHeinselman, C.
dc.contributor.authorKero, Johan
dc.contributor.authorKosch, Mike
dc.contributor.authorLamy, Herve
dc.contributor.authorLeyser, Thomas
dc.contributor.authorOgawa, Yasunobu
dc.contributor.authorOksavik, Kjellmar
dc.contributor.authorPellinen-Wannberg, Asta
dc.contributor.authorPitout, Frederic
dc.contributor.authorRapp, Markus
dc.contributor.authorStanislawska, Iwona
dc.contributor.authorVierinen, Juha
dc.date.accessioned2016-04-18T09:34:18Z
dc.date.available2016-04-18T09:34:18Z
dc.date.issued2015-07-29
dc.PublishedProgress in Earth and Planetary Science (2015) 2:21eng
dc.identifier.issn2197-4284en_US
dc.identifier.urihttps://hdl.handle.net/1956/11922
dc.description.abstractThe EISCAT (European Incoherent SCATer) Scientific Association has provided versatile incoherent scatter (IS) radar facilities on the mainland of northern Scandinavia (the EISCAT UHF and VHF radar systems) and on Svalbard (the electronically scanning radar ESR (EISCAT Svalbard Radar) for studies of the high-latitude ionised upper atmosphere (the ionosphere). The mainland radars were constructed about 30 years ago, based on technological solutions of that time. The science drivers of today, however, require a more flexible instrument, which allows measurements to be made from the troposphere to the topside ionosphere and gives the measured parameters in three dimensions, not just along a single radar beam. The possibility for continuous operation is also an essential feature. To facilitatefuture science work with a world-leading IS radar facility, planning of a new radar system started first with an EU-funded Design Study (2005–2009) and has continued with a follow-up EU FP7 EISCAT_3D Preparatory Phase project (2010–2014). The radar facility will be realised by using phased arrays, and a key aspect is the use of advanced software and data processing techniques. This type of software radar will act as a pathfinder for other facilities worldwide. The new radar facility will enable the EISCAT_3D science community to address new, significant science questions as well as to serve society, which is increasingly dependent on space-based technology and issues related to space weather. The location of the radar within the auroral oval and at the edge of the stratospheric polar vortex is also ideal for studies of the long-term variability in the atmosphere and global change. This paper is a summary of the EISCAT_3D science case, which was prepared as part of the EU-funded Preparatory Phase project for the new facility. Three science working groups, drawn from the EISCAT user community, participated in preparing this document. In addition to these working group members, who are listed as authors, thanks are due to many others in the EISCAT scientific community for useful contributions, discussions, and support.en_US
dc.language.isoengeng
dc.publisherSpringeren_US
dc.relation.urihttp://www.progearthplanetsci.com/content/2/1/21
dc.rightsAttribution CC BYeng
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/eng
dc.subjectEISCATeng
dc.subjectEISCAT_3Deng
dc.subjectRadareng
dc.subjectIncoherent scattereng
dc.subjectAtmospheric scienceeng
dc.subjectSpace physicseng
dc.subjectPlasma physicseng
dc.subjectSolar system researcheng
dc.subjectSpace weathereng
dc.subjectRadar techniqueseng
dc.titleThe science case for the EISCAT_3D radaren_US
dc.typePeer reviewed
dc.typeJournal article
dc.date.updated2016-03-16T07:45:50Z
dc.description.versionpublishedVersionen_US
dc.rights.holderCopyright 2015 the authorsen_US
dc.identifier.doihttps://doi.org/10.1186/s40645-015-0051-8
dc.identifier.cristin1317426
dc.relation.projectNorges forskningsråd: 223252


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