The study of the dynamic spectra of hectometric Jovian emission (f<1.3 MHz) for the period January to June 1978 from the planetary radio astronomy (PRA) experiment on the Voyager 1 and 2 spacecraft shows that its shape is stable with the rotation of the planet. However, there are noticeable differences between the spectra observed at one‐month intervals by one spacecraft, or simultaneously by the two spacecraft, which can be clearly related neither to an effect of Io nor to the Jovicentric declination of the observer.
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Lecacheux et al. (1980) studied this question.
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