Caption: 
During the Cassini Orbiter’s passes through Saturn’s inner magnetosphere, the Cassini Plasma Spectrometer has measured double-peaked “butterfly” pitch angle distributions in the cold, dense plasma adjacent to the fingers of hot, tenuous plasmas thought to be injected from the outer magnetosphere. The electron fluxes were observed to peak at specific pitch angles, which are correlated with electron energy and vary systematically with radial distance from the planet. These observations are interpreted as evidence for plasma outflow from sources near the orbits of Tethys and Dione. 