The roles of charge exchange and dissociation in spreading Saturn's neutral clouds
B. L. Fleshman, P. A. Delamere, F. Bagenal, T. Cassidy

TL;DR
This study investigates the processes of charge exchange and dissociation in shaping Saturn's neutral clouds, introducing new modeling approaches and considering ion gyrophase effects, leading to refined understanding of neutral cloud distributions.
Contribution
It presents a novel modeling approach for charge exchange that tracks ions within a neutral background and examines the impact of ion gyrophase on neutral cloud densities.
Findings
High-speed dissociation extends OH influence from 9 to 15 Rs.
Gyrophase significantly affects OH and oxygen densities but not H2O.
Charge exchange produces more extended oxygen clouds than H2O, with OH being the most confined.
Abstract
Neutrals sourced directly from Enceladus's plumes are initially confined to a dense neutral torus in Enceladus's orbit around Saturn. This neutral torus is redistributed by charge exchange, impact/photodissociation, and neutral-neutral collisions to produce Saturn's neutral clouds. Here we consider the former processes in greater detail than in previous studies. In the case of dissociation, models have assumed that OH is produced with a single speed of 1 km/s, whereas laboratory measurements suggest a range of speeds between 1 and 1.6 km/s. We show that the high-speed case increases dissociation's range of influence from 9 to 15 Rs. For charge exchange, we present a new modeling approach, where the ions are followed within a neutral background, whereas neutral cloud models are conventionally constructed from the neutrals' point of view. This approach allows us to comment on the…
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