Dramatic fading of SW UMa T. Kinnunen reports the SU UMa-type dwarf nova SW UMa is dramatically fading from one of its rare superoutbursts. Observers are urged to monitor whether there may be any rebrightening(s) which are usually associated with ultrashort orbital-period systems. A search for late superhumps would be also important. Recent observations: YYMMDD(UT) mag observer 971031.474 117 (G. Hanson) 971031.806 120 (R. J. Bouma) 971031.842 113 (H. Itoh) 971101.133 125 (P. Schmeer) 971101.422 117 (G. Hanson) 971101.935 125 (P. Schmeer) 971102.130 123 (T. Kinnunen) 971102.483 117 (G. Hanson) 971102.790 125 (T. Kinnunen) 971103.100 126 (P. Schmeer) 971103.444 120 (G. Hanson) 971103.596 122 (T. Watanabe) 971103.733 126 (B. H. Granslo) 971103.780 125 (T. Kinnunen) 971103.882 130 (M. Westlund) 971104.011 131 (L. T. Jensen, CCD unfiltered) 971104.960 151 (T. Kinnunen) Regards, Taichi Kato