Satellite influence on Jupiter's radio emission

Details Satellite influence on Jupiter's radio emission Satellite influence on Jupiter's radio emission

Apr 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003eaeja.....4797h&link_type=abstract

EGS - AGU - EUG Joint Assembly, Abstracts from the meeting held in Nice, France, 6 - 11 April 2003, abstract #4797

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Jupiter decameter wavelength radio emissions have a well-known correlation with the orbital phase of Io. Recent analysis of Galileo spacecraft data show that Callisto, and to a lesser extent Ganymede, influence Jovian radio emission as well. Additional data analysis from the Voyager 1 and 2 spacecraft confirm the Callisto effect. These results are best displayed as Frequency-Time spectrograms of emission intensity where the satellite longitude is constant, and as occurrence probability graphs of satellite phase versus Jovian longitude. Statistical analyses showing significance of these effects will be presented and long-term stability of Jupiter's radio emission will be discussed

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