The article reviews the intricate relationship between Io and the Jupiter magnetosphere, emphasizing Io's volcanic activity as a significant source of mass. The interaction between the fast-moving plasma and Io's atmosphere leads to various effects, contributing to mass loss. It explores current knowledge, particularly gaps regarding transient phenomena in the plasma torus and the neutral clouds. Future observational strategies leveraging spacecraft and Earth-based methods, along with improved modeling, are discussed as vital to enhancing understanding of the Io-Jupiter system.
The interactions between Io and the magnetosphere significantly affect its atmosphere and contribute to mass loss, with a variety of plasma-induced effects observed.
This review aims to clarify the understanding of the Io-Jupiter system, particularly focusing on volcanic activity, thermal dynamics, and mass supply variability.
Despite substantial research, there remain gaps in understanding transient events within the plasma torus, neutral clouds, and inconsistencies in the data.
Future observations via spacecraft and Earth-based methods are essential for modeling the complex interactions within the Io plasma torus and its contributions to the magnetosphere.
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