  We present a synthetic spectral analysis of Far Ultraviolet Spectroscopic
Explorer (FUSE) and Hubble Space Telescope/Space Telescope Imaging Spectrograph
(HST/STIS) spectra of 5 dwarf novae above and below the period gap during
quiescence. We use our synthetic spectral code, including options for the
treatment of the hydrogen quasi-molecular satellite lines (for low temperature
stellar atmospheres), NLTE approximation (for high temperature stellar
atmospheres), and for one system (RU Peg) we model the interstellar medium
(ISM) molecular and atomic hydrogen lines. In all the systems presented here
the FUV flux continuum is due to the WD. These spectra also exhibit some broad
emission lines. In this work we confirm some of the previous FUV analysis
results but we also present new results. For 4 systems we combine the FUSE and
STIS spectra to cover a larger wavelength range and to improve the spectral
fit. This work is part of our broader HST archival research program, in which
we aim to provide accurate system parameters for cataclysmic variables above
and below the period gap by combining FUSE and HST FUV spectra.
