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We explore the structures of protoclusters and their relationship with high redshift clusters using the Millennium Simulation combined with a semi analytic model. We find that protoclusters are very extended, with 90 per cent of their mass spread across35 h’1 Mpc commoving at z =2 (30 arcmin). The main halo TM, which can manifest as a high redshift cluster or group, is only a minor feature of the protocluster, containing less than 20 per cent of all protocluster galaxies at z = 2.