Abstract An eleven-year homogeneous series of observations collected at Nançay Observatory in France from 1978 to 1988 forms the basic for detailed statistics on the Jovian radio emission in the range of 15–40 MHz. The Jovian radio sources are studied by means of high resolution histograms of occurrence probability for intervals as small as 2° in the Jovian System III longitude and Io phase. The histograms clearly exhibit a substantial shift in the source Io-A and source Io-B positions which is correlated with the declination D E of the Earth. These results can be interpreted in terms of a Jovian source model which is localised in longitude and corotates with the Jovian magnetosphere, and where the radiation is beamed into a System III hollow conical sheet.
The variability of Jovian decametric radiation from 1978 to 1988
Advances in Space Research ; 12 , 8 ; 95-98
1992-01-01
4 pages
Article (Journal)
Electronic Resource
English
B and C ''sources'' of Jovian decametric radiation.
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