The value of the quadrupole anisotropy ∆T/T in the cosmological model with Ω = 1 and the flat spectrum (n = 1) of the growing mode of scalar perturbations is found. It is assumed that the motion of large-scale volume (≡100 h-1Mpc) with a velocity of 700 km/s relative to the MBR reference frame is produced by large-scale inhomogeneities of dark matter distribution. Linear size of the volume cannot be more than 200 h-1Mpc.
Soobshcheniya Spetsial'noj Astrofizicheskoj Observatorii
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