Data and plasmoid models of the flares on 22 July 2018. The left panels shows the astrometry of the flare, and the right panel shows the light curves. We used the same setup as in Fig. 8, but with a shorter growth time t_growth = 50r_g/c, Θ_e = 72 and B = 10 G (Table F.1), resulting in a two-peak light curve, with the first peak occurring at t = −22 min (out of the observational window), but mitigated by the negative beaming effect. The secondary peak, which matched the observed flare data shown here, is due to the positive beaming during the cooling phase (as shown by the intrinsic light curve).