Illustration of the jet schematic and the resulting light curve when the magnetic field strength B is changing, while the viewing angle θ_obs and the reconnection layer angle θ′ remain constant (at 0° and 70°, respectively). In our model, in order to maintain a constant jet power P_j, we scale the length of the layer inversely with the increasing B. This results in decreasing the observed time of the reconnection event with increasing B. Higher B also results in a decreased contribution of the higher energy, inverse-Compton (IC) or synchrotron self-Compton (SSC) component, thus also decreasing the fluxes. Jet schematic adapted from Christie et al. (2019).