One of the main, unresolved questions about the nature of quasars is the
position of the acceleration site responsible for the highest energies. The
attempt to investigate this question in the energy regime with the highest
resolution, the radio band, has the downside that no theoretical model exists
that can connect these two regimes. The model in this work tries to shrink this
gap by extending the general synchrotron self Compton (SSC) model up to length
scales in the order of the resolution of radio observations. The resulting
spectral energy distributions (SED) show a qualitative improvement in the
representation of the radio spectrum. Furthermore the obtained emission
morphology shows similar properties to the radio structures observed in jets of
quasars. A complete and quantitative connection will however need either much
higher numerical effort or an improved methodology
