Overview of Cassini CAPS observations of thermal plasma in Saturn’s magnetosphere (Invited)

Physics – Plasma Physics

Scientific paper

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[5737] Planetary Sciences: Fluid Planets / Magnetospheres, [7846] Space Plasma Physics / Plasma Energization, [7859] Space Plasma Physics / Transport Processes

Scientific paper

In situ plasma measurements from the Cassini Plasma Spectrometer (CAPS) have provided crucial clues to a) sources of plasma in Saturn’s magnetosphere, b) heating and acceleration processes that affect that plasma, c) transport and dynamics of the plasma, and d) the plasma’s consequences. These clues include determination of the ion composition and the spatial distribution of plasma densities, temperatures, and flow velocities. They also include details of the ion and electron energy and angular distributions, which provide signatures of the physical processes that are operating. We will give a brief overview of some of the CAPS observations that bear on the important physics associated with Saturn’s magnetospheric plasma.

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