We report on extreme-ultraviolet (EUV) spectroscopic observations of t
he B bright giant epsilon Canis Majoris made during the ORFEUS-SPAS II
mission. We assess the performance of the instrument in the EUV and f
ind that the effective area is roughly 3 times that of the Extreme-Ult
raviolet Explorer long-wavelength spectrometer and that the spectral r
esolution is lambda/Delta lambda approximate to 1250. We identify most
of the features, qualitatively compare different models, and examine
the wind-broadened O V and Si IV lines, which display blue-edge veloci
ties up to 800 km s(-1).