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3D Atmospheric Neutrino Fluxes,
using ICRC01 primary flux Energy and Zenith angle binning Fluxes in bins of neutrino energy (equally spaced bins in logE with 10 bins per decade with the low edge of the first bin at 100 MeV) and zenith angle (20 bins equally spaced in cos(zenith) with bin width 0.1), integrated over azimuth. Note logE means log to base e. Fluxes below 10 GeV are from the 3D calculation. Fluxes above 10 GeV are from the 1D calculation, for a newer version of the high energy fluxes, see here.

Electron neutrinos	Electron antineutrinos	Muon neutrinos	Muon antineutrinos
Kamioka Solar Min Kamioka Solar Max Kamioka High Energy	Kamioka Solar Min Kamioka Solar Max Kamioka High Energy	Kamioka Solar Min Kamioka Solar Max Kamioka High Energy	Kamioka Solar Min Kamioka Solar Max Kamioka High Energy

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The rest of this page gives results from the 3D calculation only (i.e. below 10 GeV)

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Electron neutrinos	Electron antineutrinos	Muon neutrinos	Muon antineutrinos
Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max
Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max

Low energy fluxes, but now with 20 bins per decade in logE.

Electron neutrinos	Electron antineutrinos	Muon neutrinos	Muon antineutrinos
Kamioka Solar Min Kamioka Solar Max	Kamioka Solar Min Kamioka Solar Max	Kamioka Solar Min Kamioka Solar Max	Kamioka Solar Min Kamioka Solar Max
Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max
Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max

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Energy and Azimuth angle binning Fluxes in bins of neutrino energy (equally spaced bins in logE with 10 bins per decade with the low edge of the first bin at 100 MeV, currently fluxes are available up to 10 GeV) and azimuth angles ( there are a total of 18 bins of 20 degrees each, with the low edge of the first bin starting at 0 degrees) for particles within 30 degrees of the horizon (|cos(zenith)| < 0.5).

Electron neutrinos	Electron antineutrinos	Muon neutrinos	Muon antineutrinos
Kamioka Solar Min Kamioka Solar Max	Kamioka Solar Min Kamioka Solar Max	Kamioka Solar Min Kamioka Solar Max	Kamioka Solar Min Kamioka Solar Max
Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max
Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max

Same fluxes, but now with 20 bins per decade in logE.

Electron neutrinos	Electron antineutrinos	Muon neutrinos	Muon antineutrinos
Kamioka Solar Min Kamioka Solar Max	Kamioka Solar Min Kamioka Solar Max	Kamioka Solar Min Kamioka Solar Max	Kamioka Solar Min Kamioka Solar Max
Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max	Soudan (MINOS) Solar Min Soudan (MINOS) Solar Max
Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max	Sudbury (SNO) Solar Min Sudbury (SNO) Solar Max

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g.barr1@physics.ox.ac.uk