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            <description>This collection contains the documentation associated with the lobal Survey of Individual Water Group Ion 
                Properties in Saturn’s Magnetosphere: Cassini CAPS Observations data bundle</description>
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                    <given_name>Thomas</given_name>
                    <family_name>Kim</family_name>
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            <reference_text>Kim et al (2026), Comprehensive Characterization of Water Group Ion Composition and 1 
                Distributions in Saturn’s Magnetosphere with Cassini Plasma Spectrometer Data,  J. Geophys. Res. Space Physics. (Accepted)</reference_text>
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                - Enceladus-origin OH+, H2O+, and H3O+ dissociate within 5-10 Saturn radii, leaving O+  
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                - Ionosphere-plasma coupling is strongest at 5-10 Saturn radii, where flow speeds reach  
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                - O+ ions make up nearly 70% of Saturn’s thermal plasma population across the 25 
                magnetosphere out to 16 Saturn radii. </description> 
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