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At the ionospheric level, these processes can be characterized by a set of parameters including conductances, field\u2010aligned 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 Jovian upper atmosphere and equatorial magnetosphere. A method based on a combined use of Juno multi\u2010instrument data and three modeling tools was developed by Wang et\u00a0al. (2021, <jats:ext-link xmlns:xlink=\"http:\/\/www.w3.org\/1999\/xlink\" xlink:href=\"https:\/\/doi.org\/10.1029\/2021ja029469\">https:\/\/doi.org\/10.1029\/2021ja029469<\/jats:ext-link>) and applied to an analysis of the first nine orbits to retrieve these parameters along Juno's magnetic footprint. We extend this method to the first 30 Juno science orbits and to both hemispheres. Our results reveal a large variability of these parameters from orbit to orbit and between the two hemispheres. They also show dominant trends. Southern current systems are consistent with the generation of a region of sub\u2010corotating ionospheric plasma flows, while both super\u2010corotating and sub\u2010corotating plasma flows are found in the north. These results are discussed in light of the previous space and ground\u2010based observations and currently available models of plasma convection and current systems, and their implications are assessed.<\/jats:p>","DOI":"10.1029\/2022ja030586","type":"journal-article","created":{"date-parts":[[2022,9,24]],"date-time":"2022-09-24T15:58:17Z","timestamp":1664035097000},"update-policy":"https:\/\/doi.org\/10.1002\/crossmark_policy","source":"Crossref","is-referenced-by-count":20,"title":["Magnetosphere\u2010Ionosphere\u2010Thermosphere Coupling Study at Jupiter Based on Juno's First 30 Orbits and Modeling Tools"],"prefix":"10.1029","volume":"127","author":[{"ORCID":"https:\/\/orcid.org\/0000-0002-9524-8687","authenticated-orcid":false,"given":"S.","family":"Al Saati","sequence":"first","affiliation":[{"name":"IRAP CNRS Universit\u00e9 Toulouse III\u2010Paul Sabatier CNES  Toulouse France"},{"name":"CPHT CNRS Institut Polytechnique de Paris  Palaiseau France"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-9928-2981","authenticated-orcid":false,"given":"N.","family":"Cl\u00e9ment","sequence":"additional","affiliation":[{"name":"IRAP CNRS Universit\u00e9 Toulouse III\u2010Paul Sabatier CNES  Toulouse France"},{"name":"Laboratoire d\u2019Astrophysique de Bordeaux Universit\u00e9 de Bordeaux  Bordeaux France"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-9552-8822","authenticated-orcid":false,"given":"C.","family":"Louis","sequence":"additional","affiliation":[{"name":"IRAP CNRS Universit\u00e9 Toulouse III\u2010Paul Sabatier CNES  Toulouse France"},{"name":"School of Cosmic Physics DIAS Dunsink Observatory Dublin Institute for Advanced Studies  Dublin Ireland"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-1290-7350","authenticated-orcid":false,"given":"M.","family":"Blanc","sequence":"additional","affiliation":[{"name":"IRAP CNRS Universit\u00e9 Toulouse III\u2010Paul Sabatier CNES  Toulouse France"},{"name":"LAM Pyth\u00e9as Aix Marseille Universit\u00e9 CNRS CNES  Marseille France"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-8736-5541","authenticated-orcid":false,"given":"Y.","family":"Wang","sequence":"additional","affiliation":[{"name":"State Key Laboratory of Space Weather National Space Science Center Chinese Academy of Sciences  Beijing China"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-8017-5676","authenticated-orcid":false,"given":"N.","family":"Andr\u00e9","sequence":"additional","affiliation":[{"name":"IRAP CNRS Universit\u00e9 Toulouse III\u2010Paul Sabatier CNES  Toulouse France"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-8428-1369","authenticated-orcid":false,"given":"L.","family":"Lamy","sequence":"additional","affiliation":[{"name":"LAM Pyth\u00e9as Aix Marseille Universit\u00e9 CNRS CNES  Marseille France"},{"name":"LESIA Observatoire de Paris Universit\u00e9 PSL CNRS Sorbonne Universit\u00e9 Universit\u00e9 de Paris  Meudon France"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-2514-0187","authenticated-orcid":false,"given":"B.","family":"Bonfond","sequence":"additional","affiliation":[{"name":"University of Li\u00e8ge  Li\u00e8ge Belgium"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-1314-9632","authenticated-orcid":false,"given":"B.","family":"Collet","sequence":"additional","affiliation":[{"name":"LAM Pyth\u00e9as Aix Marseille Universit\u00e9 CNRS CNES  Marseille France"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-0696-4380","authenticated-orcid":false,"given":"F.","family":"Allegrini","sequence":"additional","affiliation":[{"name":"SwRI  San Antonio TX USA"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-9115-0789","authenticated-orcid":false,"given":"S.","family":"Bolton","sequence":"additional","affiliation":[{"name":"SwRI  San Antonio TX USA"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-5264-7194","authenticated-orcid":false,"given":"G.","family":"Clark","sequence":"additional","affiliation":[{"name":"JHU\u2010APL  Laurel MD USA"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-7478-6462","authenticated-orcid":false,"given":"J. 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