Binned distributions of the exit energies (red) and the binned contribution of each energy point to the total differential intensity, (blue), for an initial energy of MeV. Thereby panel a shows the distribution of exit times of pseudo-particles for a good magnetic connection between the observational point and the Jovian source and panel b for the case of poor magnetic connection. The dashed lines show the integral distribution of the trajectories’ contribution to the total differential intensity as shown in blue.