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dc.contributor.authorRipoll, J.-F.
dc.contributor.authorPierrard, V.
dc.contributor.authorCunningham, G.S.
dc.contributor.authorChu, X.
dc.contributor.authorSorathia, K.A.
dc.contributor.authorHartley, D.P.
dc.contributor.authorThaller, S.A.
dc.contributor.authorMerkin, V.G.
dc.contributor.authorDelzanno, G.L.
dc.contributor.authorDe Pascuale, S.
dc.contributor.authorUkhorskiy, A.Y.
dc.date2023
dc.date.accessioned2023-02-27T21:12:43Z
dc.date.available2023-02-27T21:12:43Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/10759
dc.descriptionThis review focusses strictly on existing plasma density models, including ionospheric source models, empirical density models, physics-based and machine-learning density models. This review is framed in the context of radiation belt physics and space weather codes. The review is limited to the most commonly used models or to models recently developed and promising. A great variety of conditions is considered such as the magnetic local time variation, geomagnetic conditions, ionospheric source regions, radial and latitudinal dependence, and collisional vs. collisionless conditions. These models can serve to complement satellite observations of the electron plasma density when data are lacking, are for most of them commonly used in radiation belt physics simulations, and can improve our understanding of the plasmasphere dynamics.
dc.languageeng
dc.titleModeling of the cold electron plasma density for radiation belt physics
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeelectron density
dc.subject.freeplasmasphere
dc.subject.freeplasmapause
dc.subject.freeempirical models
dc.subject.freephysical models
dc.subject.freemachine learning
dc.subject.freeradiation belts
dc.source.titleFrontiers in Astronomy and Space Sciences
dc.source.volume10
dc.source.pageA1096595
Orfeo.peerreviewedYes
dc.identifier.doi10.3389/fspas.2023.1096595
dc.identifier.scopus


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