In this paper, I have analysed the subarcsecond polarization structure
of two high-z compact steep-spectrum quasars. Morphology suggests tha
t the jets are interacting strongly with intergalactic medium. Models
of bending by ram pressure equilibrium in a cooling flow and alignment
of magnetic field lines by jet-IGM shock suggest that the CSS jets ar
e light, supersonic and mildly relativistic. Particle energy index var
iations along the jet suggests replenishment triggered by such interac
tions.