  We present images from a long term program (MOJAVE: Monitoring of Jets in AGN
with VLBA Experiments) to survey the structure and evolution of parsec-scale
jet phenomena associated with bright radio-loud active galaxies in the northern
sky. The observations consist of 2424 15 GHz VLBA images of a complete
flux-density limited sample of 135 AGN above declination -20 degrees, spanning
the period 1994 August to 2007 September. These data were acquired as part of
the MOJAVE and 2 cm Survey programs, and from the VLBA archive. The sample
selection criteria are based on multi-epoch parsec-scale (VLBA) flux density,
and heavily favor highly variable and compact blazars. The sample includes
nearly all the most prominent blazars in the northern sky, and is well-suited
for statistical analysis and comparison with studies at other wavelengths. Our
multi-epoch and stacked-epoch images show 94% of the sample to have apparent
one-sided jet morphologies, most likely due to the effects of relativistic
beaming. Of the remaining sources, five have two-sided parsec-scale jets, and
three are effectively unresolved by the VLBA at 15 GHz, with essentially all of
the flux density contained within a few tenths of a milliarcsecond.
