We present uniformly reduced and measured equivalent widths, FWHM and
observed line fluxes for 94 ''single'' WR stars (34 galactic WN, 22 ga
lactic WC, 31 LMC WN and 7 LMC WC) based on the archive IUE spectra of
WR stars gathered from different observational runs and from differen
t epochs. The spectra are used for spectral classification in the ultr
aviolet region and for searching correlations among the strength and w
idths of emission Lines of different ions. Some correlations with opti
cal and near IR lines observed by other authors are given as well. The
set of spectra we use is almost complete to 12 magnitude and represen
tative according to spectral subtype of WR stars.