Magnetosphere‐Ionosphere‐Thermosphere Coupling study at Jupiter Based on Juno’s First 30 Orbits and Modeling Tools
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
hal.structure.identifier | Centre de Physique Théorique [CPHT] | |
dc.contributor.author | AL SAATI, S. | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
hal.structure.identifier | Laboratoire d'Astrophysique de Bordeaux [Pessac] [LAB] | |
dc.contributor.author | CLÉMENT, N. | |
hal.structure.identifier | Dublin Institute for Advanced Studies [DIAS] | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | LOUIS, C. | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | BLANC, M. | |
dc.contributor.author | WANG, Y. | |
hal.structure.identifier | Institut de recherche en astrophysique et planétologie [IRAP] | |
dc.contributor.author | ANDRÉ, N. | |
hal.structure.identifier | Laboratoire d'études spatiales et d'instrumentation en astrophysique = Laboratory of Space Studies and Instrumentation in Astrophysics [LESIA] | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | LAMY, L. | |
dc.contributor.author | BONFOND, B. | |
hal.structure.identifier | Laboratoire d'Astrophysique de Marseille [LAM] | |
dc.contributor.author | COLLET, B. | |
dc.contributor.author | ALLEGRINI, F. | |
dc.contributor.author | BOLTON, S. | |
dc.contributor.author | CLARK, G. | |
dc.contributor.author | CONNERNEY, J. | |
dc.contributor.author | GÉRARD, J.‐c. | |
dc.contributor.author | GLADSTONE, G. | |
dc.contributor.author | KOTSIAROS, S. | |
dc.contributor.author | KURTH, W. | |
dc.contributor.author | MAUK, B. | |
dc.date.issued | 2022-09-24 | |
dc.identifier.issn | 2169-9380 | |
dc.description.abstractEn | • We analyze the first 30 orbits of Juno to retrieve the properties of current systems and plasma flows associated with Jovian main auroras. • Southern hemisphere results are consistent with ionospheric plasma sub-corotation. • The two opposite patterns, sub-corotation and super-corotation, are observed in the northern hemisphere. | |
dc.language.iso | en | |
dc.publisher | American Geophysical Union/Wiley | |
dc.title.en | Magnetosphere‐Ionosphere‐Thermosphere Coupling study at Jupiter Based on Juno’s First 30 Orbits and Modeling Tools | |
dc.type | Article de revue | |
dc.identifier.doi | 10.1029/2022JA030586 | |
dc.subject.hal | Planète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP] | |
bordeaux.journal | Journal of Geophysical Research Space Physics | |
bordeaux.peerReviewed | oui | |
hal.identifier | hal-03806919 | |
hal.version | 1 | |
hal.popular | non | |
hal.audience | Internationale | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-03806919v1 | |
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