91 cataclysmic variables from a sample of 162 systems with known or su
spected binary periods were detected during the ROSAT XRT-PSPC All Sky
Survey. Among the non-magnetic systems, the X-ray to optical/ultravio
let flux ratio decreases along the sequence SU UMa type - U Gem type -
Z Cam type - UX UMa type, due mainly to variations in the optical/ult
raviolet flux. 8 of the 10 brightest systems in terms of total PSPC co
untrate are magnetic systems. The 0.5-2.5 keV X-ray luminosities range
up to similar to 10(32)erg/s, the highest luminosities being those of
four faraway DQ Her type systems. The other types of cataclysmic vari
ables all have similar 0.5-2.5 keV luminosity distributions. In an App
endix we compare the X-ray properties of cataclysmic variables with th
ose of the dim X-ray sources in globular clusters.