We present in this paper the technical characteristics of a new polarimetri
c unit dedicated to the MuSiCoS echelle spectrograph. The first test runs i
ndicate that our instrument is very good at measuring polarisation or depol
arisation structures in line profiles. It is therefore one of the very few
facilities worldwide for studying magnetic topologies of active and chemica
lly peculiar stars through rotational modulation of linearly and circularly
polarised Zeeman signatures in line profiles. It is also a very interestin
g tool for investigating geometries of non-axisymmetric circumstellar envir
onments through depolarisation of spectral lines formed within the scatteri
ng envelope.