Statistical Survey of Interchange Events in the Jovian Magnetosphere Using Juno Observations

Abstract Interchange instability is known to drive fast radial transport of electrons and ions in Jupiter's inner and middle magnetosphere. In this study, we conduct a statistical survey to evaluate the properties of energetic particles and plasma waves during interchange events using Juno data from 2016 to 2023. We present representative examples of interchange events followed by a statistical analysis of the spatial distribution, duration and spatial extent. Our survey indicates that interchange instability is predominant at M ‐shells from 6 to 26, peaking near 17 with an average duration of minutes and a corresponding M ‐shell width of <∼0.05. During interchange events, the associated plasma waves, such as whistler‐mode, Z‐mode, and electron cyclotron harmonic waves exhibit a distinct preferential location. These findings provide valuable insights into particle transport and the source region of plasma waves in the Jovian magnetosphere, as well as in other magnetized planets within and beyond our solar system.

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Publication Details

Journal
Geophysical Research Letters
Published
2024-10-05
DOI
https://doi.org/10.1029/2024gl110300
Citations
10
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
3.32

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article

Statistical Survey of Interchange Events in the Jovian Magnetosphere Using Juno Observations

Qianli Ma, Wen Li, Sheng Huang, B. H. Mauk et al.
10 citations
Geophysical Research Letters
Ionosphere and magnetosphere dynamics
3.32
article

Statistical Survey of Interchange Events in the Jovian Magnetosphere Using Juno Observations

Qianli Ma, Wen Li, Sheng Huang, B. H. Mauk, F. Allegrini, W. S. Kŭrth, Luisa Capannolo, Alec Daly, Xiaochen Shen, S. J. Bolton, G. B. Hospodarsky, G. Clark
article en
10 citations

Abstract

Abstract Interchange instability is known to drive fast radial transport of electrons and ions in Jupiter's inner and middle magnetosphere. In this study, we conduct a statistical survey to evaluate the properties of energetic particles and plasma waves during interchange events using Juno data from 2016 to 2023. We present representative examples of interchange events followed by a statistical analysis of the spatial distribution, duration and spatial extent. Our survey indicates that interchange instability is predominant at M ‐shells from 6 to 26, peaking near 17 with an average duration of minutes and a corresponding M ‐shell width of <∼0.05. During interchange events, the associated plasma waves, such as whistler‐mode, Z‐mode, and electron cyclotron harmonic waves exhibit a distinct preferential location. These findings provide valuable insights into particle transport and the source region of plasma waves in the Jovian magnetosphere, as well as in other magnetized planets within and beyond our solar system.

Geophysical Research LettersVol. 51(19)
Boston University (US), University of Iowa (US), Southwest Research Institute (US), University of California, Los Angeles (US), Johns Hopkins University Applied Physics Laboratory (US), The University of Texas at San Antonio (US)
National Science Foundation, National Aeronautics and Space Administration, Nuclear Safety and Security Commission, Planetary Science Division
Openalex Percentile: Top 8%
Ionosphere and magnetosphere dynamics
3.32
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