  We report a new analysis of diffuse EUV emission in clusters of galaxies. We
find the cluster emission is strongly influenced by the variation of the
telescope sensitivity over the field of view and upon the details of the
subtraction of the EUV emission for the X-ray plasma. We investigate these
effects on Abell 1795, Abell 2199, and the Coma cluster. When we use the
appropriate correction factors, we find there is no evidence for any excess EUV
emission in Abell 1795 or Abell 2199, However, we do find extended EUV emission
in the Coma cluster and in the Virgo cluster using our new analysis
proceedures, confirming that in these clusters some as yet unidentified process
is operative.
