Rapid fading of V592 Her A preliminary analysis of Sep. 20 images of V592 Her, taken at Ouda team rooftop station (K. Matsumoto) has shown the star entered a rapidly fading stage. Dwarf novae of the similar type may show early recovery to "second superoutbursts" (AL Com and USNO 1425.09823278), or repetitive rebrightenings (EG Cnc). Observers with CCDs and suitable telescopes are strongly urged to continue monitoring the object's behavior after this stage. YYMMDD(UT) mag observer 980910.482 16.01C (Ouda team) 980910.830 164C (T. Vanmunster) 980911.478 16.23C (Ouda team) 980912.481 16.15C (Ouda team) 980913.198 <149 (G. Hanson) 980913.397 16.11C (G. Garradd) 980913.440 <138 (H. Itoh) 980913.465 16.17C (Ouda team) 980913.476 <128 (N. Makiguchi) 980913.780 <149 (T. Kinnunen) 980914.126 <149 (G. Hanson) 980914.448 <128 (N. Makiguchi) 980914.464 <138 (H. Itoh) 980914.799 156 (L. T. Jensen, CCD unfiltered) 980915.182 <149 (G. Hanson) 980915.460 16.11C (Ouda team) 980915.824 152 (L. T. Jensen, CCD unfiltered) 980916.378 15.52C (G. Garradd) 980916.449 <137 (N. Makiguchi) 980916.476 16.19C (Ouda team) 980916.490 <138 (H. Itoh) 980916.523 <128 (T. Watanabe) 980916.841 158 (L. T. Jensen, CCD unfiltered) 980917.128 <149 (G. Hanson) 980919.838 <147 (G. Poyner) 980920.437 <143 (T. Watanabe) 980920.463 <142 (H. Itoh) 980920.471 19.2:C (Ouda team) 980920.501 <136 (N. Makiguchi) Regards, Taichi Kato