Comparisons of the probability distributions of daily anomalies in long global atmospheric GCM runs made at ECMWF and NCAR at resolutions ranging from T95 (about 130 km) to T2047 (about 6.5 km) are, however, revealing in this regard. The distributions are indeed non-Gaussian, but to an excellent approximation differ only in their widths but not their shapes at the different resolutions. This remarkable result is argued to be consistent with the stochastically generated skewed (SGS) nature of the distributions, and that beyond T511 (about 25 km) the main impact of higher resolution is merely to enhance the effectively stochastic forcing of the large-scale eddies by small-scale fluxes. This suggests that a resolution of about T511, utilizing a suitable combination of deterministic and stochastic parameterizations to accurately represent variances and energy spectra, should be sufficient for S2S predictions. Indeed we have recently confirmed in a large ensemble forecast experiment performed with the NCEP/GFS model (80-member 15-day forecasts at T254 resolution for 100 forecast cases) that adding stochastic parameterizations to the model not only increases the ensemble spread but also unambiguously reduces the error of the ensemble mean forecast. This increases both the deterministic and probabilistic skill of the forecasts at Day 15, and makes it indistinguishable from that of the much higher resolution operational GFS forecasts. The increase of ensemble spread through the additional stochastic forcing is not surprising, but the unambiguous reduction of the ensemble mean error is. It will be shown how it results from a noise-induced modification of the deterministic forecast evolution operator.