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dc.contributor.authorPierrard, V.
dc.contributor.authorVoitenko, Y.
dc.date2016
dc.date.accessioned2016-10-26T11:01:27Z
dc.date.available2016-10-26T11:01:27Z
dc.identifier.isbn978-1-4673-8801-6
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/4463
dc.descriptionPlasmapause positions observed by CLUSTER/WHISPER show a strong MLT dependence with the geomagnetic activity and solar wind indices. This is in very good agreement with the mechanism of interchange instability that predicted such a MLT dependence. Typical examples of plasmapause positions obtained with CLUSTER/WHISPER and the three dimensional dynamic model of the plasmasphere developed at BIRA-IASB illustrate the time delay and the MLT dependence associated to the formation of the plasmapause.
dc.languageeng
dc.titleMLT dependence of the plasmapause from satellite observations and quasi-interchange instability mechanism
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleURSI Asia-Pacific Radio Science Conference (URSI AP-RASC)
dc.source.page629-630
Orfeo.peerreviewedNo
dc.identifier.doi10.1109/URSIAP-RASC.2016.7601369


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