Map of Jupiter's Radiation Environment From Juno's In‐Situ Observations

Abstract Since its orbit insertion on 4 July 2016, the Juno spacecraft has orbited Jupiter in a highly elliptical, polar orbit. With every orbit, Juno's line of apsides migrates, increasing the angle relative to the Jovian equator. Therefore, the spacecraft traverses across the inner regions of the radiation belt, where energetic particles are trapped. The most energetic particle fluxes (electrons with energy >20 MeV) are continuously monitored by an instrument that is part of the Magnetic Field investigation, the micro Advanced Stellar Compass (μASC), which serves as an attitude reference for the magnetic sensor. In the regions traversed thus far in the mission, the μASC has obtained in‐situ measurements of high‐energy particle fluxes from those on open field lines to Io's L‐shell, densely covering the flux environment. We present a map of the radiation environment within Jupiter's magnetosphere based on in‐situ measurements acquired in regions not well sampled by prior missions.

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Publication Details

Journal
Journal of Geophysical Research Planets
Published
2025-02-28
DOI
https://doi.org/10.1029/2024je008549
Citations
2
Primary Topic
Astro and Planetary Science
Type
article
Field-Weighted Citation Impact
2.31

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Map of Jupiter's Radiation Environment From Juno's In‐Situ Observations

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article

Map of Jupiter's Radiation Environment From Juno's In‐Situ Observations

Stavros Kotsiaros, Leonardo Ghizoni, J. E. P. Connerney, Peter S. Jørgensen, John Leif Jørgensen, Julia Sushkova, Matija Herceg, S. J. Bolton, Mathias Benn, Troelz Denver
article en
2 citations

Abstract

Abstract Since its orbit insertion on 4 July 2016, the Juno spacecraft has orbited Jupiter in a highly elliptical, polar orbit. With every orbit, Juno's line of apsides migrates, increasing the angle relative to the Jovian equator. Therefore, the spacecraft traverses across the inner regions of the radiation belt, where energetic particles are trapped. The most energetic particle fluxes (electrons with energy >20 MeV) are continuously monitored by an instrument that is part of the Magnetic Field investigation, the micro Advanced Stellar Compass (μASC), which serves as an attitude reference for the magnetic sensor. In the regions traversed thus far in the mission, the μASC has obtained in‐situ measurements of high‐energy particle fluxes from those on open field lines to Io's L‐shell, densely covering the flux environment. We present a map of the radiation environment within Jupiter's magnetosphere based on in‐situ measurements acquired in regions not well sampled by prior missions.

Journal of Geophysical Research PlanetsVol. 130(3)
Southwest Research Institute (US), Department of Space (IN), Technical University of Denmark (DK)
National Aeronautics and Space Administration, Lockheed Martin, Southwest Research Institute, Jet Propulsion Laboratory
Openalex Percentile: Top 13%
Astro and Planetary Science
2.31
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