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dc.contributor.authorPierrard, V.
dc.date2021
dc.date.accessioned2021-11-05T13:46:10Z
dc.date.available2021-11-05T13:46:10Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/8094
dc.descriptionAt BIRA-IASB, we develop kinetic models for the solar wind and its interactions with the magnetosphere of the Earth and other planets. Recent progresses were made especially for the solar wind for which our kinetic model takes into account the suprathermal particles observed in situ in this space plasma. In the magnetosphere, predictive kinetic models are also developed for different regions and especially for the plasmasphere. The model is coupled to the ionosphere and is dynamically influenced by the solar wind variations and geomagnetic activity. Radio waves are used to make observations needed for forecast, for boundary conditions and comparisons with model results.
dc.languageeng
dc.titleSpace weather models for the solar wind and the plasmasphere
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeEarth
dc.subject.freePredictive models
dc.subject.freeBoundary conditions
dc.subject.freeKinetic theory
dc.subject.freePlasmas
dc.subject.freeMagnetosphere
dc.subject.freeWind forecasting
dc.source.title2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 28 August - 4 September 2021, Rome, Italy
Orfeo.peerreviewedNo
dc.identifier.doi10.23919/URSIGASS51995.2021.9560556
dc.identifier.scopus


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