Binned distributions of exit times over the whole energy range dominated by Jovian electrons, displayed similarly in Fig. 3. Whereas the right panels show the exit time distributions weighted by their contribution according to Eq. (8), the left side displays the unweighted results of the simulation. The first row (a,b) shows the distributions for the case of good magnetic connection, and the second for the case of poor connection. e,f: differences between the distributions for good and poor magnetic connection, highlighting the influence of magnetic connectivity on the simulation results.