Jupiter's low-frequency radio spectrum from Cassini/Radio and Plasma Wave Science (RPWS) absolute flux density measurements : Cassini flyby of Jupiter

By Philippe Zarka, B. Cecconi, W. Kurth. 2004

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Predicting low-frequency radio fluxes of known extrasolar planets (2007, background): “As was mentioned above, the analysis of the jovian radio emission allows to define three terms for the typical radio spectrum: (a) the power during average conditions, (b) the average power during periods of high activity, and (c) the peak power (Zarka et al., 2004).”
Science with a lunar low-frequency array: From the dark ages of the Universe to nearby exoplanets (2009, background): “One possibility is that they have “light house beams” similar to pulsars, with intrinsically continuous emission that is confined to a solid angle and bursts being observed when the emission beam sweeps over the telescope (e.g., Zarka et al., 2004).”
The electron–cyclotron maser for astrophysical application (2006, background): “Radio emissions from Jupiter and Saturn, the nearest outer strongly magnetized planets in the solar system, have been known (Zarka et al. 1986, 2004; Zarka 1992a,b, 1998, 2004) for a long time from ground-based observations.”
Plasma interactions of exoplanets with their parent star and associated radio emissions (2006, background): “The best available estimate for the average detected power of Io–induced radio emissions, derived from integration over time, emission bandwidth and beaming pattern, is ∼1010 W (Kaiser et al., 2000 ; Queinnec and Zarka, 2001; Zarka et al., 2004).”