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Radio telescopic observations revealed Io's influence on the Jovian magnetosphere, as demonstrated by decametric wavelength bursts tied to the orbital period of Io.
The complex interplay between Jupiter and its volcanic moon, Io, produces "radio noise storms", which can be heard on the radio band from about 15 MHz up to 38 MHz.
Radio tracking provided an improved estimate of Io's mass, which, along with the best available information of Io's size, suggested that Io had the highest density of the four Galilean satellites, and was composed primarily of silicate rock rather than water ice.
The location of Io and its auroral footprint with respect to Earth and Jupiter has a strong influence on Jovian radio emissions from our vantage point: when Io is visible, radio signals from Jupiter increase considerably.
Bursts of increased radio emission are correlated with the position of Io, the innermost of the four Galilean moons of Jupiter.
The influence of Io on the Jovian magnetosphere and its radio emissions has been studied for more than three decades.
"There is an example of this in our solar system," he observes: The volcanic moon Io, the innermost of Jupiter's large satellites, triggers radio emissions from Jupiter's magnetic field and even auroras in the planet's atmosphere.
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