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].
(a)
(b)