The short-period cataclysmic variable WZ Sge underwent its first dwarf nova outburst in 23 years in 2001 July. Here we describe 905-1187 ? spectra obtained with the Far Ultraviolet Spectroscopic Explorer (FUSE) during the outburst and within the first few months after the outburst. The first spectrum, obtained about 7 days after the outburst began and 6.4 days past optical maximum, is dominated by a broad (50-60 ? equivalent width) feature due to O VI and can be characterized in terms of emission from a highly inclined disk modulated by the effects of a highly ionized wind. WZ Sge is fainter in later observations (starting about 45 days after optical maximum) and increasingly "red" in the far ultraviolet. The spectral shape increasingly resembles that expected from a metal-enriched white dwarf photosphere, although it seems likely that some disk contribution remains at least through the second FUSE observation, when the visible light curve showed the system to be undergoing a rebrightening event. The absorption lines observed on September 29 and in early November, when the visible light curve was in a fairly steady decline toward quiescence, are narrow, with widths (FWHM) of the order of 0.7-1.3 ? (200-400 km s-1). The most natural explanation for these spectra is that the continuum arises from a relatively massive, slowly rotating white dwarf and that the lines are created by a combination of metals in the atmosphere and absorbing material along the line of sight to the white dwarf. If the white dwarf has log g = 8.5, then the white dwarf cooled from ~25,000 K on September 29 to 23,000 K in early November.
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