Modulation of Jovian interplanetary electrons and the longitude variation of decametric emissions

Mathematics – Probability

Scientific paper

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Decametric Waves, Energy Spectra, High Energy Electrons, Interplanetary Medium, Jupiter (Planet), Radio Emission, Modulation, Planetary Environments, Planetary Magnetospheres, Ultrahigh Frequencies

Scientific paper

The relationship between modulation of the intensity and energy spectrum of relativistic interplanetary electrons originating from Jupiter's magnetosphere and longitudinal asymmetry in decametric radio emissions from the surface is discussed. Modulation minima are correlated with the time when the subsolar point on Jupiter is near the longitude of the most frequent non-Io-related decametric emissions. The probability of observing such emissions is graphed as a function of the System III central meridian longitude of an observer and the angle of Io past superior conjunction. It is suggested that the modulation of interplanetary electrons and the longitudinal asymmetry of decametric emissions may be due to the same unknown longitudinally asymmetric feature on Jupiter.

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