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Ion Cyclotron Waves Associated With Ionospheric Outflow at Jupiter
Journal article   Open access   Peer reviewed

Ion Cyclotron Waves Associated With Ionospheric Outflow at Jupiter

E. A Skinner, A. H Sulaiman, J. R Szalay, N. S Kruegler, R. L Lysak, Y Sarkango, W. S Kurth, G Clark and S. J Bolton
Geophysical research letters, Vol.53(10), e2026GL121914
05/28/2026
DOI: 10.1029/2026GL121914
url
https://doi.org/10.1029/2026GL121914View
Published (Version of record) Open Access

Abstract

The mechanism driving ion outflow from Jupiter's auroras remains to be determined. H+${\mathrm{H}}^{+}$outflow has been observed with highly field‐aligned pitch angles consistent with acceleration by high‐altitude electrostatic potential structures. However, the cold ionospheric ions require a pre‐acceleration mechanism to reach Jupiter's large escape speed and access the potential structures. Here we present case studies of H+${\mathrm{H}}^{+}$outflow coincident with intense H+${\mathrm{H}}^{+}$ion cyclotron waves (ICWs). We invoke resonant wave heating to suggest a causality between the two phenomena. We further investigate Landau resonance with auroral electron beams as a plausible source of free energy using cold plasma theory, finding that electron energies between 10 and 100 keV produce results consistent with ICW observations. H2+${\mathrm{H}}_{2}^{+}$and H3+${\mathrm{H}}_{3}^{+}$ICWs are likewise present, which we suggest indicates that Jovian ion outflow is a multi‐species process.
Auroras Ionosphere Acceleration Antennas Cold plasmas Electric fields Electron beams Electrostatic properties Energy Free energy Hydrogen Ion cyclotron waves Ionospheric ions Jupiter Magnetic fields Outflow Pitch (inclination) Plasma Spacecraft

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