biostudies-literatureUnknown127(10)Al Saati SNational Aeronautics and Space AdministrationFonds De La Recherche Scientifique - FNRSBelgian Federal Science Policy OfficeThe dynamics of the Jovian magnetosphere is controlled by the interplay of the planet's fast rotation, its solar-wind interaction and its main plasma source at the Io torus, mediated by coupling processes involving its magnetosphere, ionosphere, and thermosphere. At the ionospheric level, these processes can be characterized by a set of parameters including conductances, field-aligned currents, horizontal currents, electric fields, transport of charged particles along field lines including the fluxes of electrons precipitating into the upper atmosphere which trigger auroral emissions, and the particle and Joule heating power dissipation rates into the upper atmosphere. Determination of these key parameters makes it possible to estimate the net transfer of momentum and energy between JovianJournal of geophysical research. Space physicse2022JA030586https://www.ebi.ac.uk/biostudies/studies/S-EPMC9787687biostudies-literatureMagnetosphere-Ionosphere-Thermosphere Coupling Study at Jupiter Based on Juno's First 30 Orbits and Modeling Tools.PMC9787687Clark GGladstone GRAl Saati SBolton SClement NBlanc MGerard JCKurth WSBonfond BCollet BAllegrini FConnerney JEPLamy LAndre NLouis CWang YKotsiaros SMauk BfalseMagnetosphere-Ionosphere-Thermosphere Coupling Study at Jupiter Based on Juno's First 30 Orbits and Modeling Tools.The dynamics of the Jovian magnetosphere is controlled by the interplay of the planet's fast rotation, its solar-wind interaction and its main plasma source at the Io torus, mediated by coupling processes involving its magnetosphere, ionosphere, and thermosphere. At the ionospheric level, these processes can be characterized by a set of parameters including conductances, field-aligned currents, horizontal currents, electric fields, transport of charged particles along field lines including the fluxes of electrons precipitating into the upper atmosphere which trigger auroral emissions, and the particle and Joule heating power dissipation rates into the upper atmosphere. Determination of these key parameters makes it possible to estimate the net transfer of momentum and energy between Jovian2022-01-01T00:00:00Z2022 Oct2026-05-28T04:38:45.09Z2025-04-19T09:53:54.542ZS-EPMC97876873659132110.1029/2022JA030586