UCL Discovery
UCL home » Library Services » Electronic resources » UCL Discovery

Cassini CAPS-ELS Observations of Low-Energy Electron Beams Within Enceladus Mid-Latitude Flux Tubes

Rabia, J; Hadid, LZ; André, N; Nénon, Q; Chust, T; Pisa, D; Parsec-Wallis, A; ... Rymer, AM; + view all (2025) Cassini CAPS-ELS Observations of Low-Energy Electron Beams Within Enceladus Mid-Latitude Flux Tubes. Geophysical Research Letters , 52 (22) , Article e2025GL119448. 10.1029/2025GL119448. Green open access

[thumbnail of Coates_Geophysical Research Letters - 2025 - Rabia - Cassini CAPS‐ELS Observations of Low‐Energy Electron Beams Within Enceladus.pdf]
Preview
Text
Coates_Geophysical Research Letters - 2025 - Rabia - Cassini CAPS‐ELS Observations of Low‐Energy Electron Beams Within Enceladus.pdf

Download (594kB) | Preview

Abstract

The electrodynamic interaction between Saturn's magnetosphere and Enceladus accelerates electrons along magnetic field lines. These electrons propagate inside magnetic flux tubes connecting the moon to the giant planet, generating distinctive auroral hiss and auroral footprint signatures, both previously observed by the Cassini spacecraft. In this study, we analyze low-energy electron measurements made during multiple mid-latitude crossings of magnetic flux tubes connected to Enceladus' wake. We show that the properties of the observed electrons are consistent with those of electrons inducing Enceladus' auroral hiss, and discuss the physical processes responsible for their pitch-angle distributions and acceleration. Field-aligned electron beams have very different properties from those triggering the Enceladus ultraviolet footprint, with a much lower characteristic energy and energy flux. Observations of electron beams resulting from the moon-magnetosphere interactions up to 30° downstream of the moon reveal that the coupling system between Enceladus and Saturn is significantly more extended than previously anticipated.

Type: Article
Title: Cassini CAPS-ELS Observations of Low-Energy Electron Beams Within Enceladus Mid-Latitude Flux Tubes
Open access status: An open access version is available from UCL Discovery
DOI: 10.1029/2025GL119448
Publisher version: https://doi.org/10.1029/2025GL119448
Language: English
Additional information: Copyright © 2025. The Author(s). This is an open access article under the terms of the Creative Commons Attribution License, https://creativecommons.org/licenses/by/4.0/, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
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/10218240
Downloads since deposit
4Downloads
Download activity - last month
Download activity - last 12 months
Downloads by country - last 12 months

Archive Staff Only

View Item View Item