Whistler‐Mode Waves and Associated Electron Distributions in Jupiter's Middle and Outer Magnetosphere

Abstract Whistler‐mode waves play a crucial role in shaping magnetospheric electron dynamics. Using Juno's observations, we investigate these waves in Jupiter's post‐midnight‐to‐dawn magnetosphere, spanning 20–80 Jupiter radii. Our survey reveals that whistler‐mode waves predominantly occur in the lobes, while the magnetodisk remains largely devoid of such waves. Simultaneous electron measurements from JADE‐E, combined with dispersion relation analysis, indicate that these waves are likely driven by a mono‐directional electron population between 0.1 and 10 keV propagating anti‐Jupiter‐ward. Further controlled studies show that a local flux minimum at 0.3 keV in the electron energy spectrum, which is commonly detected during whistler‐mode waves, is critical for wave growth. Based on their direction of motion, we suggest that these mono‐directional electrons and the whistler‐mode waves they generate are related to magnetosphere‐ionosphere coupling. Our findings offer new insights into the interplay between whistler‐mode waves and electrons in Jupiter's magnetosphere.

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Publication Details

Journal
Geophysical Research Letters
Published
2025-09-18
DOI
https://doi.org/10.1029/2025gl116543
Citations
1
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
1.15

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article

Whistler‐Mode Waves and Associated Electron Distributions in Jupiter's Middle and Outer Magnetosphere

F. Allegrini, Michel Blanc, W. S. Kŭrth, Zhi‐Yang Liu et al.
1 citations
Geophysical Research Letters
Astro and Planetary Science
1.15
article

Whistler‐Mode Waves and Associated Electron Distributions in Jupiter's Middle and Outer Magnetosphere

F. Allegrini, Michel Blanc, W. S. Kŭrth, Zhi‐Yang Liu, Liming Li, J. E. P. Connerney, R. W. Ebert, J. Rabia, S. J. Bolton, Nicolás André
article en
1 citations

Abstract

Abstract Whistler‐mode waves play a crucial role in shaping magnetospheric electron dynamics. Using Juno's observations, we investigate these waves in Jupiter's post‐midnight‐to‐dawn magnetosphere, spanning 20–80 Jupiter radii. Our survey reveals that whistler‐mode waves predominantly occur in the lobes, while the magnetodisk remains largely devoid of such waves. Simultaneous electron measurements from JADE‐E, combined with dispersion relation analysis, indicate that these waves are likely driven by a mono‐directional electron population between 0.1 and 10 keV propagating anti‐Jupiter‐ward. Further controlled studies show that a local flux minimum at 0.3 keV in the electron energy spectrum, which is commonly detected during whistler‐mode waves, is critical for wave growth. Based on their direction of motion, we suggest that these mono‐directional electrons and the whistler‐mode waves they generate are related to magnetosphere‐ionosphere coupling. Our findings offer new insights into the interplay between whistler‐mode waves and electrons in Jupiter's magnetosphere.

Geophysical Research LettersVol. 52(18)
University of Iowa (US), Southwest Research Institute (US), Centre National de la Recherche Scientifique (FR), Goddard Space Flight Center (US), Université Toulouse III - Paul Sabatier (FR), Université Fédérale de Toulouse Midi-Pyrénées (FR), Institut Superieur de l'Aeronautique et de l'Espace (ISAE-SUPAERO) (FR), Aix-Marseille Université (FR), China University of Geosciences (Beijing) (CN), Laboratoire d’Astrophysique de Marseille (FR), Institut de Recherche en Astrophysique et Planétologie (FR), The University of Texas at San Antonio (US)
National Aeronautics and Space Administration, Centre National d’Etudes Spatiales, Nuclear Safety and Security Commission, Centre National de la Recherche Scientifique
Openalex Percentile: Top 16%
Astro and Planetary Science
1.15
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