{"status":"ok","message-type":"work","message-version":"1.0.0","message":{"indexed":{"date-parts":[[2026,10,8]],"date-time":"2026-10-08T22:40:15Z","timestamp":1791499215530,"version":"4.3.4"},"reference-count":48,"publisher":"American Geophysical Union (AGU)","issue":"12","license":[{"start":{"date-parts":[[2024,11,27]],"date-time":"2024-11-27T00:00:00Z","timestamp":1732665600000},"content-version":"vor","delay-in-days":0,"URL":"http:\/\/creativecommons.org\/licenses\/by-nc-nd\/4.0\/"}],"content-domain":{"domain":["agupubs.onlinelibrary.wiley.com"],"crossmark-restriction":true},"short-container-title":["JGR Space Physics"],"published-print":{"date-parts":[[2024,12]]},"abstract":"<jats:title>Abstract<\/jats:title><jats:p>Juno's highly elliptical polar orbits provide unprecedented in\u2010situ observations of the electrodynamic interaction between Jupiter and its volcanic moon Io. These observations occur in regions never sampled before both near Io's orbit and near Jupiter's ionosphere and at distances between the two. Magnetic field data obtained during multiple traversals of magnetic field lines mapping to Io's orbit reveal remarkably rich and complex magnetic signatures near flux tubes connected to Io's orbital position. Here we present a methodology to model the distribution of currents along Io's flux tube (IFT) and Alfv\u00e9n wings in such a way as to match the magnetic field signature observed during Juno's traversals of the IFT and Alfv\u00e9n wings downstream of Io. We obtain the location, size and morphology of the current\u2010carrying region as well as the distribution of currents within the IFT and Alfv\u00e9n wings. The observed field\u2010aligned currents exhibit strong filamentation, with upward and downward currents splitting into secondary cells rather than forming uniform structures. Additionally, there is a strong correlation between total field\u2010aligned current intensity, particle energy flux, and Poynting flux, indicating efficient energy transfer and coupling in the Jupiter\u2010Io system. Using all of Juno's traversals up to perijove (PJ) pass 42, we estimate the strength of the interaction with regards to distance along Io's extended tail, Io's position in the plasma torus and the magnetic field intensity at the footprint in Jupiter's ionosphere, illuminating the interaction of Jovian magnetospheric plasma with Io and setting important constraints in the Io\u2010Jupiter interaction.<\/jats:p>","DOI":"10.1029\/2024ja032591","type":"journal-article","created":{"date-parts":[[2024,11,28]],"date-time":"2024-11-28T06:13:00Z","timestamp":1732774380000},"update-policy":"https:\/\/doi.org\/10.1002\/crossmark_policy","source":"Crossref","is-referenced-by-count":6,"title":["Juno Observations Set New Constraints on the Electrodynamic Interaction Between Io and Jupiter"],"prefix":"10.1029","volume":"129","author":[{"ORCID":"https:\/\/orcid.org\/0000-0003-2636-5545","authenticated-orcid":false,"given":"S.","family":"Kotsiaros","sequence":"first","affiliation":[{"name":"Aurora Technology BV for ESA \u2010 European Space Agency European Space Astronomy Centre (ESA\/ESAC)  Villanueva de La Ca\u00f1ada Spain"},{"name":"DTU Space Technical University of Denmark (DTU)  Kongens Lyngby Denmark"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0001-7478-6462","authenticated-orcid":false,"given":"J. 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P.","family":"Connerney","sequence":"additional","affiliation":[{"name":"Space Research Corporation  Annapolis MD USA"},{"name":"Nasa Goddard Space Flight Center  Greenbelt MD USA"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-1413-1231","authenticated-orcid":false,"given":"J.","family":"Saur","sequence":"additional","affiliation":[{"name":"Institut f\u00fcr Geophysik und Meteorologie Universit\u00e4t zu K\u00f6ln  Cologne Germany"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-9662-6272","authenticated-orcid":false,"given":"A.","family":"Kokkalis","sequence":"additional","affiliation":[{"name":"National Institute of Aquatic Resources (DTU Aqua)  Kongens Lyngby Denmark"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0002-3736-2123","authenticated-orcid":false,"given":"M.","family":"Herceg","sequence":"additional","affiliation":[{"name":"DTU Space Technical University of Denmark (DTU)  Kongens Lyngby Denmark"}],"role":[{"vocabulary":"crossref","role":"author"}]},{"ORCID":"https:\/\/orcid.org\/0000-0003-0351-7825","authenticated-orcid":false,"given":"Y. 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