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dc.contributor.authorPierrard, V.
dc.contributor.authorBonhome, M.P.D.
dc.contributor.authorHalekas, J.
dc.contributor.authorAudoor, C.
dc.contributor.authorWhittlesey, P.
dc.contributor.authorLivi, R.
dc.date2023
dc.date.accessioned2023-10-09T10:15:10Z
dc.date.available2023-10-09T10:15:10Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/11150
dc.descriptionThe new observations of Parker Solar Probe and Solar Orbiter are used to constrain and compare with the exospheric model of the solar wind. The observations at low radial distances show suprathermal electrons already well present in the Strahl in the antisunward direction and a deficit in the sunward direction, confirming the exospheric feature of almost no incoming particles. The presence of suprathermal Strahl electrons at the exobase increases the velocity to higher values, as well as a low exobase, because that increases the electric potential acccelerating the wind. That causes a clear difference between the slow wind and the higher speed wind originating from low density solar corona. The kinetic exospheric model of the solar wind is also improved by considering regularized Kappa distributions that have no diverging moments through consideration of a cut-off at relativistic velocities. The model becomes valid even for kappa indices lower than 2, which is important since low values of kappa are observed in the fast solar wind.
dc.languageeng
dc.titleSolar Wind Kappa Exospheric Model Constrained by PSP
dc.typeArticle
dc.subject.frascatiPhysical sciences
dc.audienceGeneral public
dc.subject.freesolar wind
dc.subject.freeexospheric models
dc.subject.freeregularized kappa
dc.subject.freeParker Solar Probe
dc.subject.freesuprathermal electrons
dc.subject.freevelocity distributions
dc.subject.freeacceleration
dc.subject.freesolar corona
dc.subject.freespace plasmas
dc.source.titleEncyclopedia
Orfeo.peerreviewedNo
dc.identifier.urlhttps://encyclopedia.pub/video/video_detail/932


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