Anisotropy data analysis leaves a significant degeneracy between primeval spectral index (n s) and cosmic opacity to CMB photons (τ). Low–l polarization measures, in principle, can remove it. We perform a likelihood analysis to see how cosmic variance possibly affects such a problem. We find that, for a sufficiently low noise level (σ P pix) and if τ is not negligibly low, the degeneracy is gre...