  The two-year COBE-DMR 53 and 90 GHz sky maps in both ecliptic and galactic
coordinates, are used to determine the normalisation of inflationary, flat,
dark matter dominated universe models. The appropriately normalized cold and
mixed dark matter models, computed for a range of values of Omega_baryon and h,
and several values of the hot to cold dark matter abundance ratio, are then
compared to various measures of structure in the universe.
