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[en] The paper deals with the long-term fluctuations of the jovian emission at hectometre and kilometre wavelengths. Observations from the Planetary Radio Astronomy (PRA) experiment aboard the two Voyager space-craft are used. The emissions are shown to be strongly affected by the magnetic sector structure at Jupiter. The position of the sources of emission in the jovian magnetosphere is discussed. (author)
Journal
Nature (London); ISSN 0028-0836; 
; v. 306(5945); p. 767-768
; v. 306(5945); p. 767-768