We have observed 7045 frames of SW UMa from Feb. 12 to 18 and Dr. Martin also observed 535 frames on Feb. 17 and 18. We did not detect the super-QPO during the very early stage of superoutburst. From Feb. 15, the object is gradually faded with the rate of 0.13 mag/d. The amplitude of superhump is constant after fully evolved to about 2.0 mag. Tonight we are now observing SW UMa. The object is sometimes visible on display through thin cloud, but the condition is not good. The other site observations are encouraged. Regards, Makoto Uemura and Taichi Kato