Space weather models for the solar wind and the plasmasphere

dc.contributor.author	Pierrard, V.
dc.date	2021
dc.date.accessioned	2021-11-05T13:46:10Z
dc.date.available	2021-11-05T13:46:10Z
dc.identifier.uri	https://orfeo.belnet.be/handle/internal/8094
dc.description	At 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.language	eng
dc.title	Space weather models for the solar wind and the plasmasphere
dc.type	Conference
dc.subject.frascati	Physical sciences
dc.audience	Scientific
dc.subject.free	Earth
dc.subject.free	Predictive models
dc.subject.free	Boundary conditions
dc.subject.free	Kinetic theory
dc.subject.free	Plasmas
dc.subject.free	Magnetosphere
dc.subject.free	Wind forecasting
dc.source.title	2021 XXXIVth General Assembly and Scientific Symposium of the International Union of Radio Science (URSI GASS), 28 August - 4 September 2021, Rome, Italy
Orfeo.peerreviewed	No
dc.identifier.doi	10.23919/URSIGASS51995.2021.9560556
dc.identifier.scopus