V592 Her: possible superhump emergence Dear Colleagues, Gordon Garradd (Loomberah NSW Australia) has kindly provided a set of time-series CCD photometry of V592 Her (will be posted separately to vsnet-obs). A preliminary analysis of relative maginitudes of V592 Her to the comparison suggests the existence of ~0.2-mag hump with a possible period close to the spectroscopic period detected by Mennickent et al. The likely humps are singly peaked. This feature may indicate V592 Her may be experiencing the stage of rapid evolution of "true" superhumps. During this stage, another WZ Sge star EG Cnc experienced a recovery from the initial rapid decay (sometimes called "glitch"). Snapshot observations are equally important whether the same phenomenon occurs in V592 Her. Independent confirmations and follow-up observations of hump features are strongly encouraged. Regards, Taichi Kato