Future neutrino oscillation measurement focus, at first priority, on the discovery of \sin2 2 \theta 13 describing the coupling between solar and atmospheric oscillations. In this talk, we briefly discuss the prospects to measure \sin2 2 \theta 13 by future reactor and beam experiments, and we illustrate the usefulness of these measurements (and their precision) from the theoretical point of view with an example.
PACS numbers: 14.60.Pq
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