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We present a synthetic spectral analysis of IUE archival and FUSE FUV spectraof the peculiar dwarf nova WW Ceti. During the quiescence of WW Ceti, a whitedwarf with Twd=26,000K can account for the FUV flux and yields the properdistance. However, the best agreement with the observations is provided by atwo-temperature white dwarf model with a cooler white dwarf at Twd=25,000Kproviding 75% of the FUV flux and a hotter region (accretion belt or opticallythick disk ring) with T=40,000K contributing 25% of the flux for the properdistance. We find from the FUSE spectrum that the white dwarf is rotating witha projected rotational velocity V sin{i} = 600 km/s. Our temperature resultsprovide an additional data point in the distribution of Twd versus orbitalperiod above the CV period gap where few Twds are available.Comment: 25 pages, 3 tables, 8 figures (including 2 color ones), final versio

A Far-Ultraviolet Study of the Hot White Dwarf in the Dwarf Nova WW Ceti