Preprints
https://doi.org/10.5194/egusphere-2026-2055
https://doi.org/10.5194/egusphere-2026-2055
15 Apr 2026
 | 15 Apr 2026
Status: this preprint is open for discussion and under review for Annales Geophysicae (ANGEO).

RADEM observations of the Van Allen belts during the JUICE Lunar-Earth Gravity Assist

Marco Pinto, André Rodrigues, Elias Roussos, Daniel Schmid, Martin Volwerk, Stavros Kotsiaros, Patrick Brown, Michele Dougherty, Luísa Arruda, and Olivier Witasse

Abstract. On 19–20 August 2024, the European Space Agency (ESA) Jupiter Icy Moons Explorer (JUICE) mission performed the first ever Lunar–Earth Gravity Assist (LEGA) manoeuvre. The mission was launched on April 14, 2023, and is currently on an 8-year interplanetary cruise to the Jovian system. It is equipped with the RADiation-hard Electron Monitor (RADEM), a facility instrument designed to measure the most energetic particle populations (electrons, protons and ions) in the Jovian environment where JUICE will operate. During LEGA, JUICE crossed the Van Allen belts, providing a unique opportunity to evaluate the in-flight response of RADEM and to optimize its configuration for the Jupiter phase. In this paper, we report RADEM observations of the Van Allen belts, showing clear sensitivity to trapped electrons and protons. We also discuss how the Earth-flyby geometry, including pitch-angle effects, influenced the measurements and the implications for future operations. The observations also demonstrate that while RADEM is a facility instrument, it has the potential to enhance the scientific return of the JUICE mission by monitoring a key energy range in Jupiter's radiation belts that no other instrument on JUICE is covering.

Competing interests: At least one of the (co-)authors is a member of the editorial board of Annales Geophysicae.

Publisher's note: Copernicus Publications remains neutral with regard to jurisdictional claims made in the text, published maps, institutional affiliations, or any other geographical representation in this paper. While Copernicus Publications makes every effort to include appropriate place names, the final responsibility lies with the authors. Views expressed in the text are those of the authors and do not necessarily reflect the views of the publisher.
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Marco Pinto, André Rodrigues, Elias Roussos, Daniel Schmid, Martin Volwerk, Stavros Kotsiaros, Patrick Brown, Michele Dougherty, Luísa Arruda, and Olivier Witasse

Status: open (until 27 May 2026)

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Marco Pinto, André Rodrigues, Elias Roussos, Daniel Schmid, Martin Volwerk, Stavros Kotsiaros, Patrick Brown, Michele Dougherty, Luísa Arruda, and Olivier Witasse
Marco Pinto, André Rodrigues, Elias Roussos, Daniel Schmid, Martin Volwerk, Stavros Kotsiaros, Patrick Brown, Michele Dougherty, Luísa Arruda, and Olivier Witasse
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Latest update: 15 Apr 2026
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Short summary
During its flyby of the Moon and Earth, the Jupiter Icy Moons Explorer crossed Earth's radiation belts and gave us a rare chance to test the Radiation Hard Electron Monitor in space. By studying how its measurements changed along the path, we showed that the instrument can clearly detect trapped electrons and protons. This gives confidence for future operations at Jupiter, where the radiation environment is far harsher and these measurements will be especially valuable.
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