High-resolution, time-resolved spectroscopic observations of Z CMa car
ried out on 1997 January 14-17 are presented. Large night-to-night and
hour-to-hour variations in H-alpha, H-beta and Na I D P Cygni absorpt
ions, as well as an H-beta emission peak, were observed. Variations in
the red wings of the hydrogen emission lines were also detected. The
high-velocity wide-emission component on the blue side of H-alpha appe
ared on January 17. The observations are discussed in the framework of
current wind models.