  We present ultraviolet emission-line maps of the narrow-line region (NLR) of
NGC 1068. The maps span 115--318 nm, the biconical ionization cone, several
posited jet/ISM interactions, and the compact knots whose optical spectra we
reported previously resemble kinematically the quasar Associated Absorption
Line systems. Across the NLR, we find that ultraviolet flux ratios are
consistent with photoionization, not shock excitation, even for gas blueshifted
abruptly to 3000 \kms relative to galaxy systemic velocity or for gas projected
near the radio jet. The knots may be radiatively accelerated, photoablated
fragments of molecular clouds.
