Measurement of Atmospheric Neutrino Oscillations with Very Large Volume Neutrino Telescopes

Figure 21

Expected median zenith angle resolution for electron and muon neutrinos in PINGU (solid) and ORCA (dashed). For ORCA individual resolutions for neutrinos and antineutrinos are shown, while a mixture of both is given for PINGU. Resolutions are better for antineutrinos than for neutrinos due to the smaller average inelasticity, leading to a smaller intrinsic scattering angle between the neutrino and the leading lepton. Values taken from [85, 86].