Using all available multicomponent radio pulse profiles for pulsars with me
dium to long periods and good polarization data, we have constructed a two-
dimensional image of the mean radio beam shape. This shows a peak near the
centre of the beam but is otherwise relatively uniform with only mild enhan
cements in a few regions. This result supports the patchy beam model for em
ission beams, in which the mean beam shape represents the properties of the
emission mechanism and observed pulse components result from emission sour
ces distributed randomly across the beam.