During their respective missions, the spacecraft Voyager and Cassini measured
several Saturn magnetosphere parameters at different radial distances. As a result of
information gathered throughout the journey, Voyager 1 discovered hot and cold electron
distribution components, number density, and energy in the 6–18 Rs range. Observations
made by Voyager of intensity fluctuations in the 20–30 keV range show electrons are
situated in the resonance spectrum’s high energy tail. Plasma waves in the magnetosphere
can be used to locate Saturn’s inner magnetosphere’s plasma clusters, which are
controlled by Saturn’s spin. Electromagnetic electron cyclotron (EMEC) wave ring
distribution function has been investigated. Kinetic and linear approaches have been
used to study electromagnetic cyclotron (EMEC) wave propagation. EMEC waves’ stability
can be assessed by analyzing the dispersion relation’s effect on the ring distribution
function. The primary goal of this study is to determine the impact of the magnetosphere
parameters which is observed by Cassini. The magnetosphere of Saturn has also been
observed. When the plasma parameters are increased as the distribution index, the
growth/damping rate increases until the magnetic field model affects the magnetic field
at equator, as can be seen in the graphs. We discuss the outputs of our model in the
context of measurements made in situ by the Cassini spacecraft.