  We present a large grid of computed far- and mid-ultraviolet spectra (850
Angstroms to 2000 Angstroms) of the integrated light from steady-state
accretion disks in luminous cataclysmic variables. The spectra are tabulated at
0.25 Angstrom intervals with an adopted FWHM resolution of 1.0 Angstrom, so
they are suitable for use with observed spectra from a variety of modern
space-borne observatories. Twenty-six different combinations of white dwarf
mass M(wd) and mass accretion rate dM/dt are considered, and spectra are
presented for six different disk inclinations, i. The disk models are computed
self-consistently in the plane-parallel approximation, assuming LTE and
vertical hydrostatic equilibrium, by solving simultaneously the radiative
transfer, hydrostatic equilibrium, and energy balance equations. Irradiation
from external sources is neglected. Local spectra of disk annuli are computed
taking into account line transitions from elements 1-28 (H through Ni). Limb
darkening as well as Doppler broadening and blending of lines are taken into
account in computing the integrated disk spectra. The radiative properties of
the models are discussed, including the dependence of ultraviolet fluxes and
colors on M(wd), dM/dt, and i. The appearance of the disk spectra is
illustrated, with regard to changes in the same three parameters. Finally,
possible future improvements to the present models and spectra are discussed.
The synthetic spectra are available as machine-readable ASCII files via ftp.
