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Intervals of Intense Energetic Electron Beams Over Jupiter's Poles

Paranicas, C; Mauk, BH; Haggerty, DK; Clark, G; Kollmann, P; Rymer, AM; Bonfond, B; ... Bolton, SJ; + view all (2018) Intervals of Intense Energetic Electron Beams Over Jupiter's Poles. Journal of Geophysical Research: Space Physics , 123 (3) pp. 1989-1999. 10.1002/2017ja025106. Green open access

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Abstract

Juno's Jupiter Energetic particle Detector Instrument often detects energetic electron beams over Jupiter's polar regions. In this paper, we document a subset of intense magnetic field‐aligned beams of energetic electrons moving away from Jupiter at high magnetic latitudes both north and south of the planet. The number fluxes of these beams are often dominated by electrons with energies above about 1 MeV. These very narrow beams can create broad angular responses in the Jupiter Energetic particle Detector Instrument with unique signatures in the detector count rates, probably because of >10 MeV electrons. We use these signatures to identify the most intense beams. These beams occur primarily above the swirl region of the polar cap aurora. This polar region is described as being of low brightness and high absorption and the most magnetically “open” at Jupiter.

Type: Article
Title: Intervals of Intense Energetic Electron Beams Over Jupiter's Poles
Open access status: An open access version is available from UCL Discovery
DOI: 10.1002/2017ja025106
Publisher version: https://doi.org/10.1002/2017JA025106
Language: English
Additional information: © 2018 The Authors. This is an open access article under the terms of the Creative Commons Attribution‐NonCommercial‐NoDerivs License (http://creativecommons.org/licenses/by-nc-nd/4.0/).
Keywords: MeV electron beams, swirl region, Jupiter, Jovian aurora
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Space and Climate Physics
URI: https://discovery.ucl.ac.uk/id/eprint/10077596
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