Acceleration of Energetic Electrons in Jovian Middle Magnetosphere by Whistler‐Mode Waves

Abstract An abundant multi‐MeV electron population beyond the orbit of Io is required to explain the intense inner radiation belt (electrons MeV) at Jupiter and its synchrotron radiation. In order to better understand the synergistic effect of radial transport and local wave‐particle interactions driven by whistler‐mode waves on the formation of Jupiter's radiation belt, we perform 3‐D Fokker‐Planck simulations for Jovian energetic electrons with the Versatile Electron Radiation Belt code. An empirical model of Jovian whistler‐mode waves updated with measurements from the Juno extended mission is used to quantify the local acceleration and pitch angle scattering. Resonant cyclotron acceleration by whistler‐mode waves leads to significant enhancement in the intensity of electrons above 1 MeV in the middle magnetosphere. Radial diffusion is capable of transporting MeV electrons accelerated by outer‐belt whistler‐mode waves into the region, where they are further accelerated adiabatically to energies of about 10 MeV.

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Publication Details

Journal
Journal of Geophysical Research Space Physics
Published
2024-12-01
DOI
https://doi.org/10.1029/2024ja032735
Citations
2
Primary Topic
Ionosphere and magnetosphere dynamics
Type
article
Field-Weighted Citation Impact
0.66

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article

Acceleration of Energetic Electrons in Jovian Middle Magnetosphere by Whistler‐Mode Waves

R. B. Horne, T. F. Averkamp, P. Kollmann, N. Krupp et al.
2 citations
Journal of Geophysical Research Space Physics
Ionosphere and magnetosphere dynamics
0.66
article

Acceleration of Energetic Electrons in Jovian Middle Magnetosphere by Whistler‐Mode Waves

R. B. Horne, T. F. Averkamp, P. Kollmann, N. Krupp, A. Saikin, Alexander Drozdov, E. E. Woodfield, Yixin Hao, Dedong Wang, J. D. Menietti, Yuri Shprits, S. J. Bolton, E. Roussos, G. B. Hospodarsky
article en
2 citations

Abstract

Abstract An abundant multi‐MeV electron population beyond the orbit of Io is required to explain the intense inner radiation belt (electrons MeV) at Jupiter and its synchrotron radiation. In order to better understand the synergistic effect of radial transport and local wave‐particle interactions driven by whistler‐mode waves on the formation of Jupiter's radiation belt, we perform 3‐D Fokker‐Planck simulations for Jovian energetic electrons with the Versatile Electron Radiation Belt code. An empirical model of Jovian whistler‐mode waves updated with measurements from the Juno extended mission is used to quantify the local acceleration and pitch angle scattering. Resonant cyclotron acceleration by whistler‐mode waves leads to significant enhancement in the intensity of electrons above 1 MeV in the middle magnetosphere. Radial diffusion is capable of transporting MeV electrons accelerated by outer‐belt whistler‐mode waves into the region, where they are further accelerated adiabatically to energies of about 10 MeV.

Journal of Geophysical Research Space PhysicsVol. 129(12)
University of Iowa (US), Southwest Research Institute (US), British Antarctic Survey (GB), University of California, Los Angeles (US), University of Potsdam (DE), Johns Hopkins University Applied Physics Laboratory (US), Max Planck Institute for Solar System Research (DE), GFZ Helmholtz Centre for Geosciences (DE)
National Aeronautics and Space Administration, Sight Research UK, Natural Environment Research Council, Science and Technology Facilities Council
Openalex Percentile: Top 27%
Ionosphere and magnetosphere dynamics
0.66
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