Detailed simulations of tidally induced structure in disk galaxies hav
e either concentrated on specific systems or consisted of a few encoun
ters with relatively small numbers of particles and no self-gravity. O
bservers need a ''dictionary'' of simulations that covers many encount
er parameters with fine morphological resolution and includes effects
of self-gravitation. Observers can then search the dictionary for the
parameters that best match a particular observed morphology. Alternati
vely, the dictionary can be used with observational samples for statis
tical studies of system parameters. To fill this need, we present a su
rvey of model tidal encounters using a self-gravitating, 180,000 parti
cle, two-component (''stars'' and ps'') disk. A wide variety of fascin
ating morphologies results. There are 86 different encounters that var
y orbit tilt, perigalacticon distance, galaxy to companion mass ratio,
and the amount of halo dark matter relative to the disk. For morpholo
gical comparisons, over 1700 images of the entire survey are available
in video form. While there is a rich variety of tidal structure cover
ing much of this parameter space, some general patterns may be remarke
d. There is a strong orbital inclination dependence of the symmetry of
tidal patterns, most symmetric for planar orbits and nearly one-sided
for polar encounters. Retrograde encounters produce only broad fanlik
e global patterns, but rich small-scale internal structure. In both ki
nds of encounter, our numerical resolution allows us to track internal
spiral structure driven by the outer material arms, especially in the
lighter halo simulations. We note also that polar encounters generate
series of expanding, essentially non-rotating loops resembling shell
structures in some respects.