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We carry out a spectral analysis of the archival FUSE spectrum of the VY Sclnova-like cataclysmic variable MV Lyrae obtained in the high state. We findthat standard disk models fail to fit the flux in the shorter wavelengths ofFUSE (< 950$A). An improved fit is obtained by including a modeling of theboundary layer at the inner edge of the disk. The result of the modeling showsthat in the high state the disk has a moderate accretion rate of about 2.E09solar mass per year, a low inclination, a boundary layer with a temperature ofaround 100,000K, and size 0.20Rwd, and the white dwarf is possibly heated up toa temperature of 50,000K or higher.

FUSE Observational Evidence of the Boundary Layer of MY Lyrae in the High State