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dc.contributor.authorMasson, A.
dc.contributor.authorSantolík, O.
dc.contributor.authorCarpenter, D.L.
dc.contributor.authorDarrouzet, F.
dc.contributor.authorDécréau, P.M.E.
dc.contributor.authorEl-Lemdani Mazouz, F.
dc.contributor.authorGreen, J.L.
dc.contributor.authorGrimald, S.
dc.contributor.authorMoldwin, M.B.
dc.contributor.authorNěmec, F.
dc.contributor.authorSonwalkar, V.S.
dc.date2009
dc.date.accessioned2016-04-06T08:39:21Z
dc.date.available2016-04-06T08:39:21Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3332
dc.descriptionThis paper highlights significant advances in plasmaspheric wave research with CLUSTER and IMAGE observations. This leap forward was made possible thanks to the new observational capabilities of these space missions. On one hand, the multipoint view of the four CLUSTER satellites, a unique capability, has enabled the estimation of wave characteristics impossible to derive from single spacecraft measurements. On the other hand, the IMAGE experiments have enabled to relate large-scale plasmaspheric density structures with wave observations and provide radio soundings of the plasmasphere with unprecedented details. After a brief introduction on CLUSTER and IMAGE wave instrumentation, a series of sections, each dedicated to a specific type of plasmaspheric wave, put into context the recent advances obtained by these two revolutionary missions. © 2009 Springer Science+Business Media B.V.
dc.languageeng
dc.titleAdvances in plasmaspheric wave research with CLUSTER and IMAGE observations
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeCLUSTER
dc.subject.freeDensity structures
dc.subject.freeIMAGE
dc.subject.freeMultipoint
dc.subject.freePlasmasphere
dc.subject.freeRadio soundings
dc.subject.freeSpace missions
dc.subject.freeWave characteristics
dc.subject.freeSpace flight
dc.subject.freeWaves
dc.subject.freeMagnetosphere
dc.source.titleSpace Science Reviews
dc.source.volume145
dc.source.issue1-2
dc.source.page137-191
Orfeo.peerreviewedYes
dc.identifier.doi10.1007/s11214-009-9508-7
dc.identifier.scopus2-s2.0-84861338930


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