The interrelations between the physical parameters of a cometary nucle
us, and the morphology of the dust tail and its streamers are systemat
ically investigated by means of a model developed by Bei ss er (1990a)
, involving a rotating nucleus. The analysis of streamers in the tail,
using direct modeling and synchrone grids, provides a suitable tool t
o deduce substantial informations on the nucleus' state of rotation. O
pportunities and limitations of this analysis are discussed. Dust emis
sion parameters like the distribution of active regions on the nucleus
, or the emission characteristics can only be determined if certain ot
her physical properties of the nucleus have been independently measure
d before.