Review Article
Measurement of Atmospheric Neutrino Oscillations with Very Large Volume Neutrino Telescopes
Figure 24
(a) Significance of ORCA and PINGU for rejecting a given hypothesis for the neutrino mass ordering plotted as a function of , after 3 years of data taking. (b) Median significance as a function of time for the benchmark detectors described in the text. The oscillation parameters injected are close to those found in [3] ( for a NMO, for an IMO). From [85, 91].
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