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dc.contributor.authorLichtenberger, J.
dc.contributor.authorSantolik, O.
dc.contributor.authorSolymosi, J.
dc.contributor.authorGraclík, L.
dc.contributor.authorDarrouzet, F.
dc.contributor.authorDemekhov, A.
dc.contributor.authorKudrin, A.
dc.contributor.authorLehtinen, N.
dc.date2017
dc.date.accessioned2017-12-22T14:32:04Z
dc.date.available2017-12-22T14:32:04Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/6354
dc.descriptionRecent advances in the monitoring of the plasmasphere (e.g. the PLASMON FP7-Space project, http://plasmon.elte.hu, Lichtenberger et al., Space Weather Space Clim. 3 2013, A23 DOI: 10.1051/swsc/2013045) http) makes the continuous monitoring of the plasmasphere possible. But this monitoring capability totally depends on natural and sporadic phenomena, preventing systematic monitoring required for operational Space Weather models and forecasts.
dc.languageeng
dc.titleDeveloping a VLF transmitter for LEO satellites: Probing of plasmasphere and radiation belts - The POPRAD proposal
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeVLF transmitter
dc.subject.freeLEO satellites
dc.subject.freeradiation belts
dc.subject.freePLASMON FP7-Space project
dc.subject.freeplasmasphere monitoring
dc.subject.freeplasmasphere probing
dc.subject.freesporadic phenomena
dc.subject.freesystematic monitoring
dc.source.title2017 XXXIInd General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 19-26 August 2017, Montreal, Canada
Orfeo.peerreviewedNo
dc.identifier.doi10.23919/URSIGASS.2017.8105199


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