  We present new optical observations of the HH 111 Herbig-Haro jet using the
Gemini Multi Object Spectrograph in its Integral Field Unit mode. Eight fields
of 5" x 3.5" have been positioned along and across the HH 111 jet, covering the
spatial region from knot E to L in HH 111 (namely, knots E, F, G, H, J, K and
L). We present images and velocity channel maps for the [O I] 6300+6360,
Halpha, [N II] 6548+6583 and [S II] 6716+6730 lines, as well as for the [S
II]6716/6730 line ratio. We find that the HH 111 jet has an inner region with
lower excitation and higher radial velocity, surrounded by a broader region of
higher excitation and lower radial velocity. Also, we find higher electron
densities at lower radial velocities. These results imply that the HH 111 jet
has a fast, axial region with lower velocity shocks surrounded by a lower
velocity sheath with higher velocity shocks.
