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dc.contributor.authorRipoll, J.-F.
dc.contributor.authorThaller, S.A.
dc.contributor.authorHartley, D.P.
dc.contributor.authorCunningham, G.S.
dc.contributor.authorPierrard, V.
dc.contributor.authorKurth, W.S.
dc.contributor.authorKletzing, C.A.
dc.contributor.authorWygant, J.R.
dc.date2023
dc.date.accessioned2023-10-09T10:15:12Z
dc.date.available2023-10-09T10:15:12Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/11151
dc.descriptionWe deduce the cold electron plasma density from NASA Van Allen Probes measurements throughout 2012-2019. We then extract two of the plasmasphere boundaries. We first use the gradient method for locating the plasmapause at L pp and, then, the 100 cm−3 density threshold for the plasmasphere outer edge located at L 100 . The sharp gradient of the plasmapause is only defined in 53% of cases, while L 100 is defined for ∼85% of cases. Differences and similarities between L pp and L 100 are discussed. L 100 is demonstrated to bound the plasmasphere at large L-shell in the dusk where L pp gradients often lack. We generate new empirical density models of the plasmasphere boundaries binned by L-shell, magnetic local time (MLT), and the maximum of the Kp index over 24 hours (Kp*).
dc.languageeng
dc.titleObservations and statistics of the plasmasphere boundaries from the Van Allen Probes
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeSpace vehicles
dc.subject.freeGradient methods
dc.subject.freeUncertainty
dc.subject.freeNASA
dc.subject.freePlasma measurements
dc.subject.freeLabeling
dc.subject.freeIndexes
dc.source.title2023 XXXVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 19-26 Aug. 2023, Sapporo, Japan
Orfeo.peerreviewedNo
dc.identifier.doi10.23919/URSIGASS57860.2023.10265488
dc.identifier.url


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