  Spectrum of initial scalar and tensor perturbations created during an
inflationary stage producing a closed or open FRW universe now is discussed. In
the closed case, the CMB temperature anisotropy ${\Delta T/T}$ generated by
scalar perturbations is enhanced for low multipoles. It is argued that in the
open case there is no suppression of low multipoles. A possibility of the
existence of a preferred space direction in the open case is noted.
