While most studies so far have focused on predicting the AIRI, it is more useful and challenging to forecast seasonal rainfall anomaly pattern across India. The 46-year (1960-2005) hindcast made by the five ENSEMBLE coupled models’ multi-model ensemble (MME) yields a temporal correlation coefficient (TCC) skill of 0.43 for predicting AIRI, but only 0.16 for predicting anomaly pattern. Here we developed the Predictable Mode Analysis (PMA) method and a suite of P-E models to predict ISMR anomaly pattern. We show that the first three observed empirical orthogonal function (EOF) patterns of the ISMR have their distinct dynamical origins rooted in the eastern Pacific (EP)-type ENSO, central Pacific (CP)-type ENSO, and Nino4 SST anomalies, respectively. The dynamical models’ skill for predicting ISMR distribution primarily comes from these three potentially predictable modes, which account for about 51% of the total observed variance. Based on understanding the lead-lag relationships between the lower boundary anomalies and the predictable modes, a set of P-E models is established to predict the ISMR anomaly pattern by using the sum of the predictable modes. The cross-validated TCC skill of the P-E models is more than doubled that of ENSEMBLE models’ MME hindcast, suggesting a large room for improvement of the current dynamical prediction. The methodology proposed here can be applied to a wide range of climate prediction and predictability studies. The limitation and future improvement are also discussed.