Comprehensive characterization of water group ion composition and distributions in Saturn's magnetosphere with Cassini plasma spectrometer data
Author(s)
Type
Journal Article
Abstract
Saturn's magnetosphere is continuously supplied with neutrals from the Enceladus plume and the icy rings, which undergo ionization and charge-exchange to form a complex water-group plasma environment. While the Cassini Plasma Spectrometer (CAPS) instrument has provided extensive compositional information, detailed separation of individual water-group ion species in time-of-flight (TOF) data has not previously been achieved. In this study, we perform forward modeling of CAPS-IMS energy-per-charge (E/Q) and TOF spectra obtained between 2004 and 2012 to resolve O+, OH+, H2O+, and H3O+ and to characterize their plasma properties, including number density, temperature, and thermodynamic κ. Our results demonstrate that O+ is the dominant thermal ion species throughout Saturn's magnetosphere, comprising up to ∼70% of the total ion population beyond ∼5 Saturn radii (RS). In contrast, molecular ions such as OH+, H2O+, and H3O+ dominate closer to Enceladus but rapidly dissociate into atomic ions between ∼5 and 10 RS. This radial region is also characterized by the steepest increase in plasma flow speed, which rises from ∼40% to ∼80% of rigid corotation. Simultaneously, ion velocity distributions approach Maxwell–Boltzmann equilibrium, as indicated by high kappa values. These findings provide new constraints on the ion–neutral chemistry that regulates the balance between molecular and atomic ions in Saturn's magnetosphere. They also emphasize the critical role of the 5–10 RS region as a transition zone for both plasma composition and dynamics. Our results refine previous CAPS-based studies and underscore the need to incorporate seasonal variability and ionospheric coupling into future global models of Saturn's plasma environment.
Date Issued
2026-04-01
Date Acceptance
2026-03-18
Citation
Journal of Geophysical Research (JGR): Space Physics, 2026, 131 (4)
ISSN
2169-9380
Publisher
American Geophysical Union
Journal / Book Title
Journal of Geophysical Research (JGR): Space Physics
Volume
131
Issue
4
Copyright Statement
© 2026. The Author(s). This is an open access article under the terms of the Creative Commons Attribution License, which permits use, distribution and reproduction in any medium, provided the original work is properly cited.
License URL
Publication Status
Published
Article Number
e2025JA034738
Date Publish Online
2026-03-30