  Primordial gravitational waves are created during the de Sitter phase of an
exponentially-expanding (inflationary) universe, due to quantum zero-point
vacuum fluctuations. These waves produce fluctuations in the temperature of the
Cosmic Background Radiation (CBR). We calculate the multipole moments of the
correlation function for these temperature fluctuations in a spatially-closed
Friedman-Robertson-Walker (FRW) cosmological model. The results are compared to
the corresponding multipoles in the spatially-flat case. The differences are
small unless the density parameter today, $\Omega_0$, is greater than 2.
(Submitted to Physical Review D).
