Abstract :
[en] At Jupiter, the plasma is concentrated near the centrifugal equator, forming a magnetodisc. The planet's dipole tilt induces periodic disc flapping, generating magnetic oscillations observed by spacecraft. While centrifugal forces are theorized to drive interchange instability in this system, direct detection of such structures remains challenging due to flapping-induced variabilities. However, in situ and remote sensing data reveal ∼tens-of-minute periodicities proposed to link to interchange dynamics. Using unique Juno observations, we analyze two events to: (a) resolve highly variable magnetic curvature changes during successive plasma sheet crossings and (b) identify periodic ∼30-min fluctuations in plasma measurements in the magnetodisc while Juno occupied a magnetically favorable location. These findings provide the first direct examination of interchange-related magnetic curvature evolution and plasma signatures, to advance our understanding of the magnetodisc's 3D structure and instability-driven dynamics.
Funding text :
ZY acknowledges the General Program of the National Natural Science Foundation of China (Grant 42374212), the Research Grants Council (RGC) General Research Fund (Grant 17309124), and Project (JLFS/P\u2010702/24) of Hong Kong RGC Co\u2010funding Mechanism on Joint Laboratories with the Chinese Academy of Science. BZ is supported by the General Program of National Natural Science Foundation of China (Grant 42374216) and Research Grants Council (RGC) General Research Fund (Grants 17309224, 17308723, 17315222). YX is supported by the China Postdoctoral Science Foundation under Grant 2025M770390 and the Postdoctoral Fellowship Program of CPSF under Grant GZB20250099. The work at Southwest Research Institute is funded by NASA's New Frontiers Program for Juno through contract NNM06AA75C.
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