WZ Sge: short-term variations in optical spectra Accorging to the report from Dr. Sadakane, observing at Okayama Astrophysical Observatory, both emission and absorption components of H-beta show strong short-term variation (reported on July 24). Since the object is very bright, even small telescope will be able to obtain time-resolved low resolution spectra. Such time-series spectroscopy will provide enormous hints for the dwarf nova outburst and the early superhump. Observations are strongly encouraged. If possible, observations covering more than one orbital period are prefered. Regards, VSNET Collaboration team