  We present a synthetic spectral analysis of IUE archival and FUSE FUV spectra
of the peculiar dwarf nova WW Ceti. During the quiescence of WW Ceti, a white
dwarf with Twd=26,000K can account for the FUV flux and yields the proper
distance. However, the best agreement with the observations is provided by a
two-temperature white dwarf model with a cooler white dwarf at Twd=25,000K
providing 75% of the FUV flux and a hotter region (accretion belt or optically
thick disk ring) with T=40,000K contributing 25% of the flux for the proper
distance. We find from the FUSE spectrum that the white dwarf is rotating with
a projected rotational velocity V sin{i} = 600 km/s. Our temperature results
provide an additional data point in the distribution of Twd versus orbital
period above the CV period gap where few Twds are available.
