Panels a)–c) are running difference images based on the observations in EUV 193 Å by SDO/AIA. The arrows in panels a) and c) mark the wavefront of the EUV waves. The red line OP is the slit for making the time-distance images of panel e). Panel d) is a running difference image made with LASCO C2. The slopes of dashed lines, green lines, and red lines give the propagating speeds of the expanding erupted filament, EUV waves, and reflected EUV waves during the toroidal filament eruptions.