  We present new details of the structure and morphology of the jets and
outflows in HH46/47 as seen in Spitzer infrared images from IRAC and MIPS,
reprocessed using the ``HiRes'' deconvolution technique. HiRes improves the
visualization of spatial morphology by enhancing resolution (to sub-arcsec
levels in IRAC bands) and removing the contaminating side lobes from bright
sources. In addition to sharper views of previously reported bow shocks, we
have detected: (i) the sharply-delineated cavity walls of the wide-angle
biconical outflow, seen in scattered light on both sides of the protostar, (ii)
several very narrow jet features at distances 400 AU to 0.1 pc from the star,
and, (iii) compact emissions at MIPS 24 micron coincident with the jet heads,
tracing the hottest atomic/ionic gas in the bow shocks.
