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dc.contributor.authorTam, S.W.Y.
dc.contributor.authorChang, T.
dc.contributor.authorPierrard, V.
dc.date2007
dc.date.accessioned2016-09-27T11:09:46Z
dc.date.available2016-09-27T11:09:46Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/4404
dc.descriptionThe polar wind, a plasma outflow along open geomagnetic field lines from the Earth's ionosphere, has been the subject of many theoretical studies. Since the proposal of its existence more than 30 years ago, the polar wind has been described by various theoretical modeling approaches. In this paper, we first describe the two traditional modeling approaches for the classical polar wind: moment-based models and collisionless kinetic calculations; and discuss how other models of the outflow were formed by combining these two traditional approaches. We then discuss how kinetic calculations have been improved to take into account the effects of Coulomb collisions, which may contribute to the formation of double-peaked H+ velocity distributions in the polar wind. As observations of escaping O+ fluxes have guided theoreticians to go beyond the classical polar wind description, we discuss how models were modified or constructed in order to take into account the various non-classical effects, including those due to photoelectrons, which may also provide an explanation for the satellite observations of day-night asymmetries in addition to the acceleration of the O+ ions.
dc.languageeng
dc.relation.ispartofseries
dc.titleKinetic modeling of the polar wind
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.subject.freeGeomagnetism
dc.subject.freeIonosphere
dc.subject.freeMathematical models
dc.subject.freePhotoelectrons
dc.subject.freeSatellite observatories
dc.subject.freeVelocity distribution
dc.subject.freeCoulomb collisions
dc.subject.freeDay-night asymmetries
dc.subject.freeIon acceleration
dc.subject.freePolar wind
dc.subject.freeSolar wind
dc.source.titleJournal of Atmospheric and Solar-Terrestrial Physics
dc.source.volume69
dc.source.issue16
dc.source.page1984-2027
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/j.jastp.2007.08.006
dc.identifier.scopus2-s2.0-36148984633


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