Intensity and anisotropy time profiles of 4 MeV protons propagating in fast and slow solar wind configurations, with and without cross-field diffusion as detailed in the legend. The left (right) panel shows the results for observer A (B) indicated by the cyan (orange) triangle marker as in Fig. 1. Adiabatic deceleration and solar wind convection are neglected, with the exception of accounting for corotation.