EGU21-8779, updated on 04 Mar 2021
https://doi.org/10.5194/egusphere-egu21-8779
EGU General Assembly 2021
© Author(s) 2021. This work is distributed under
the Creative Commons Attribution 4.0 License.

The Formation of Saturn’s and Jupiter’s Electron Radiation Belts by Magnetospheric Electric Fields

Yixin Hao1, Yixin Sun1, Elias Roussos2, Ying Liu1, Peter Kollmann3, Chongjing Yuan4, Norbert Krupp2, Chris Paranicas3, Xuzhi Zhou1, Go Murakami5, Hajime Kita5, and Qiugang Zong1
Yixin Hao et al.
  • 1(yixinhao@pku.edu.cn) Institute of Space Physics and Applied Technology, Peking University, 100871, Beijing, Peopleʼs Republic of China
  • 2Max Planck Institute for Solar System Research, D-37077, Goettingen, Germany
  • 3Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA
  • 4Institute of Geology and Geophysics, Chinese Academy of Sciences, 100029, Beijing, Peopleʼs Republic of China
  • 5Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Japan

The existence of planetary radiation belts with relativistic electron components means that powerful acceleration mechanisms are operating within their volume. Mechanisms that bring charged particles planetward toward stronger magnetic fields can cause their heating. On the basis that electron fluxes in Saturn’s radiation belts are enhanced over discrete energy intervals, previous studies have suggested that rapid inward plasma flows may be controlling the production of their most energetic electrons. However, rapid plasma inflows languish in the planet’s inner magnetosphere, and they are not spatially appealing as a mechanism to form the belts. Here we show that slow, global-scale flows resulting from transient noon-to-midnight electric fields successfully explain the discretized flux spectra at quasi- and fully relativistic energies, and that they are ultimately responsible for the bulk of the highest energy electrons trapped at Saturn. This finding is surprising, given that plasma flows at Saturn are dominated by the planetary rotation; these weak electric field perturbations were previously considered impactful only over a very narrow electron energy range where the magnetic drifts of electrons cancel out with corotation. We also find quantitative evidence that ultrarelativistic electrons in Jupiterʼs radiation belts are accelerated by the same mechanism. Given that similar processes at Earth drive a less efficient electron transport compared to Saturn and Jupiter, the conclusion is emerging that global-scale electric fields can provide powerful relativistic electron acceleration, especially at strongly magnetized and fast-rotating astrophysical objects.

How to cite: Hao, Y., Sun, Y., Roussos, E., Liu, Y., Kollmann, P., Yuan, C., Krupp, N., Paranicas, C., Zhou, X., Murakami, G., Kita, H., and Zong, Q.: The Formation of Saturn’s and Jupiter’s Electron Radiation Belts by Magnetospheric Electric Fields, EGU General Assembly 2021, online, 19–30 Apr 2021, EGU21-8779, https://doi.org/10.5194/egusphere-egu21-8779, 2021.

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