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hal.structure.identifierLaboratoire de Physique des Plasmas [LPP]
dc.contributor.authorNGUYEN, G.
hal.structure.identifierLaboratoire de Physique des Plasmas [LPP]
dc.contributor.authorAUNAI, Nicolas
hal.structure.identifierLaboratoire de Physique des Plasmas [LPP]
dc.contributor.authorMICHOTTE DE WELLE, Bayane
hal.structure.identifierLaboratoire de Physique des Plasmas [LPP]
dc.contributor.authorJEANDET, A.
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierInstitut de recherche en astrophysique et planétologie [IRAP]
dc.contributor.authorLAVRAUD, B.
hal.structure.identifierLaboratoire de Physique des Plasmas [LPP]
dc.contributor.authorFONTAINE, D.
dc.date.issued2022
dc.identifier.issn2169-9380
dc.description.abstractEnIn a companion statistical study, we showed that the expression of the magnetopause surface as a power law of an elliptic function of the zenith angle θ holds at lunar distances, that the flaring of the magnetopause surface is influenced by the Interplanetary Magnetic Field (IMF) B<SUB>y</SUB> component and that the IMF B<SUB>x</SUB> component had no influence on the stand-off distance. As a follow-up to these statistical results, this paper presents a new empirical analytical asymmetric and non-indented model of the magnetopause location and shape. This model is obtained from fitting of 15,349 magnetopause crossings using 17 different spacecraft and is parametrized by the upstream solar wind dynamic and magnetic pressures, the IMF clock angle and the Earth dipole tilt angle. The constructed model provides a more accurate prediction of the magnetopause surface location than current Magnetopause surface models, especially on the night side of the magnetosphere.
dc.language.isoen
dc.publisherAmerican Geophysical Union/Wiley
dc.rights.urihttp://hal.archives-ouvertes.fr/licences/copyright/
dc.subject.enMagnetopause
dc.subject.enMagnetosphere
dc.subject.enSolar Wind
dc.subject.enInterplanetary Magnetic Field
dc.title.enMassive Multi-Mission Statistical Study and Analytical Modeling of the Earth's Magnetopause: 3. An Asymmetric Non Indented Magnetopause Analytical Model
dc.typeArticle de revue
dc.identifier.doi10.1029/2021JA030112
dc.subject.halPlanète et Univers [physics]
bordeaux.journalJournal of Geophysical Research Space Physics
bordeaux.volume127
bordeaux.peerReviewedoui
hal.identifierinsu-03672057
hal.version1
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//insu-03672057v1
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