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The relatively large value of $\theta_{13}$ established recently by the DayaBay reactor experiment opens the possibility to determine the neutrino massordering with experiments currently under construction. We investigatesynergies between the NOvA long-baseline accelerator experiment withatmospheric neutrino data from the India-based Neutrino Observatory (INO). Weidentify the requirements on energy and direction reconstruction and detectormass for INO necessary for a significant sensitivity. If neutrino energy anddirection reconstruction at the level of 10% and 10 degree can be achieved byINO a determination of the neutrino mass ordering seems possible around 2020.

Identifying the Neutrino mass Ordering with INO and NOvA