Ellipsoidal Universe Induces Large Scale CMB Polarization

We calculate the large scale polarization of the cosmic microwave background induced by the anisotropy of the spatial geometry of our universe. Assuming an eccentricity at decoupling of about ${0.6410}^{-2}$, we find $\Delta T_{pol}/ T_0 \simeq 0.53 10^{-6}$ quite close to the average level of polarization detected by the Wilkinson Microwave Anisotropy Probe.