Dear colleagues, I have just concluded the analysis of my August 10/11 CCD time-series photometry run of WZ Sge. The sky was of moderate quality, with some cloud fields hampering the observing session. Nevertheless, we got a pretty interesting light curve, that is presented at my web site (address below). There are some striking differences with WZ Sge's behaviour of the night before. First of all, the 'secondary superhump' now is dominating the true superhump, both being almost equal now [this confirms the findings of G. Masi and others, as discussed by T. Kato in vsnet-alert 6255]. More pronounced is also a small hump, that emerges just after an eclipse of WZ Sge. Please note that the depth of the eclipses is very small, in the order of about 0.05 mag. The plateau, that we observed yesterday, seems to have disappeared completely. I'm wondering what suprises this night will bring ? I have started a new session at about 21:20 UT and will continue till about 03:00 UT. Sky conditions are more or less okay, with some cirrus clouds. Tonny Vanmunster CBA Belgium Observatory http://vsnet.lunarpages.com/cbabelgium email : Tonny.Vanmunster@advalvas.be