Superfluorescence[1] (SF) emission profiles are computed using one-way coupled Maxwell-Bloch equations. Transverse effects[2] are included in the full three-spatial-dimension case as well as in the cylindrical-symmetry case. Initiating quantum fluctuations[3–5] are approximated by a random polarization source with a completely random phase and root-mean-square tipping angle of 2/ N, where N is the number of atoms in each volume element. These fluctuations reduce the tail of the output obtained with transverse effects alone[6]. In fact, the fluctuations in output pulse shapes encompass the Cs data of Gibbs, Vrehen and Hikspoors[7]; see Fig. 1. The standard deviation for the delay time is found to be (12.5±4)% for Fresnel number of 0.8 compared with the value (10±2)% recently measured by Vrehen and der Weduwe[8], also for Cs. The Fresnel-number dependence of the standard deviation is shown in Fig. 2; Drummond and Eberly[9] have more extensive results for Fresnel numbers from 1 to 16. Excluded from Fig. 2 were phase-wave[10] fluctuations in which the second peak exceeded the first. Figure 3 shows that the transverse profiles retain little of the on-axis ringing found[2] without fluctuations. Ringing can also be removed by inhomogeneous broadening, but the 32-ns T2* of the Cs experiment has little effect; T2* < 1 ns is needed to eliminate plane-wave ringing[6].