  Radio observations of novae in outburst are of particular interest due to the
physical parameters that may be retrieved from fitting the radio light curves.
Most models that have fitted previous data assumed spherical symmetry however,
it is becoming more and more clear that this is not the case. We explore
morpho-kinematical techniques to retrieve the free-free radio light curves of
non-spherical models and explore the effects of a non-spherical outburst on the
physical parameters. In particular, we find that we may have been over
estimating the ejected masses in the outburst of non-spherical novae.
