We report on the analysis of Jovian millisecond radio bursts (S-bursts
) observed at the radio station Graz-Lustbuhel on 4 January 1993 and s
imultaneously recorded at two other stations Nancay in France and Khar
ko in Ukraine. The three radiotelescopes are separated in longitude by
approximately 15-degrees, but located at nearly the same northern lat
itude (congruent-to 48-degrees). This network allows us to use differe
nt receivers with complementary characteristics (multichannel, spectro
-analyser, spectro-polarimeter). At the Lustbuhel Observatory we have
recorded the Jovian S-bursts with high time resolution of 2 ms, suffic
ient to see the individual S-bursts and to study their phenomenology.
The high resolution spectra permitted us to analyse more than 900 S-bu
rsts, in particular the drift-rate being determined at round -33 MHz s
-1, on average. On the other hand, from the Nancay (France) data we di
stinguished fifteen S-burst patterns during half an hour with mainly r
ight-hand polarization, in the frequency range 15 MHz to 31 MHz. If we
take into account the spectra of different S-bursts (Riihimaa 1991) w
e find that the drift of the S-burst pattern is a function of the stru
cture, like the type b and type f. We have concluded that the source e
missions of an S-burst pattern with positive and negative drift seem t
o be different. Concerning the existence of correlation between the S-
and L- bursts a confirmation is shown with respect to previous works.