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.

1. INTRODUCTION
2. Mathematical Formulation
3. PLA SMA PARAMETERS
4. RESULT AND DISCUSSION
5. CONCLUSION
ACKNOWLEDGMENTS
References

• Annex Edappattu Haridas(Department of Physics, Amity Institute of Applied Sciences, Amity University, Noida, Uttar Pradesh 201303, India)
• Shefali Kanwar(Department of Physics, Amity Institute of Applied Sciences, Amity University, Noida, Uttar Pradesh 201303, India)
• Rama Shankar Pandey(Department of Physics, Amity Institute of Applied Sciences, Amity University, Noida, Uttar Pradesh 201303, India) Corresponding author