Azimuthal velocity, the surface density, the pressure, and the midplane temperature for five time steps centered around the second outburst. The dashed lines denote the initial conditions of the simulations. The dash-dotted line in the upper left panel gives the azimuthal velocity for pure Keplerian rotation. In the lower right panel we have included a zoom-in of Fig. 6 for better identification of the exact location of the plot times.