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dc.contributor.authorLemaire, J.
dc.contributor.authorScherer, M.
dc.date1970
dc.date.accessioned2017-08-23T12:46:56Z
dc.date.available2017-08-23T12:46:56Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/5978
dc.descriptionA model of a polar ion-exosphere in which the geomagnetic field lines are open is developed. The electrostatic field in this region has been calculated by taking into account two fundamental conditions: (1) quasi-neutrality has to be satisfied everywhere in the exosphere; (2) escape fluxes of electrons and ions have to be equal. The density distributions are calculated for different evaporative models in the case of two (O+ and e) and three (O+, H+ and e) constituents. In addition, the mean velocity, pressure and temperature distributions of the several constituents are derived.
dc.languageeng
dc.titleModel of the polar ion-exosphere
dc.typeArticle
dc.subject.frascatiEarth and related Environmental sciences
dc.audienceScientific
dc.source.titlePlanetary and Space Science
dc.source.volume18
dc.source.issue1
dc.source.page103-120
Orfeo.peerreviewedYes
dc.identifier.doi10.1016/0032-0633(70)90070-X
dc.identifier.scopus2-s2.0-0000850350


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