Migration distance, as given by the difference between the final and initial guiding radius for stars with their initial guiding radius inside corotation (top plot), between corotation and OLR (middle), and outside the OLR (bottom plot), divided in an inward (red) and outward motion (blue) (median and 16^th and 84^th percentile.) The black curves are the mean change in the guiding radius induced by the libration of the orbits.