The differential rotation of the large-scale magnetic features by using Solar Synoptic Charts (1965-1976) is investigated. Variations of the rotation rate of the large-scale formations both in the northern and southern solar hemispheres for various latitudinal intervals are revealed. The large rotation rate of magnetic formations is obtained for patterns having the sign of the global magnetic field. The change of rotation rate of magnetic features studied in all latitudinal intervals coincides with the sign reversal of the global magnetic field.