Analysis of Jovian nKOM Radio Emissions Using Juno Waves/Data

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Jupiter possesses an exceptionally strong magnetic field, and within its magnetosphere lies a vast distribution of plasma released from its volcanically active moon, Io. This plasma forms a structure known as the Io plasma torus, from which narrowband kilometric radiation (nKOM) is emitted.
The objective of my research is to investigate the long-term variations in the occurrence frequency and intensity of nKOM emissions, in order to clarify their relationship with magnetospheric dynamics such as injection phenomena within Jupiter’s magnetosphere.

This post is also available in: Japanese