The formation of supersonic, radiatively cooled plasma jets with applications tolaboratory astrophysics has been an active area of research on the MAGPIE generator. Oneof the ways of producing astrophysically-relevant jets in the laboratory is by using theablation of plasma from a radial foil Z-pinch. In this configuration a ~1.4 MA, 250ns current pulse is introduced into an aluminium disk with a thickness of 15μm. The ablated plasma from the foil converges on the axis, producing asteady and collimated jet with a typical axial velocity of ~100 km/s. The setupallows for the addition of argon above the foil for jet-ambient interaction studies. Theinteraction is characterised by the formation of several shock features, which arepresented and discussed from experimental data and numerical simulations.