Feb. 16, 2015,
The atmospheric neutirno flux table is updated with NRLMSISE-00 atmosphere model.
The details are in Phys. Rev. D92, 023004 (2015) ( eprint).
The flux table is here (HKKM2014) with some new sites.
Other than the atmosphere model, the calculation scheme is the same as previous
one. The fluxes in HKKM2014 for the sites whose fluxes are presented in HKKM2011
are similar to them. For NRLMSISE-00 atmosphere model, see
J. M. Picone, J. Geophys. Res. 107, SIA 15 (2002).

Feb. 28, 2011,
The atmospheric neutirno flux table is updated with JAM interaction model.
The interaction model improved the low energy interactions of cosmic rays and
air nuclei, as shown inPhys. Rev. D83, 123001 (2011) (eprint).
The flux table is here (HKKM2011).
For the JAM interaction model, see
K. Niita et al., Radiat. Meas. 41, 1080 (2006).

The calculation and the fluxes are almost the same as the previous one
for the neutrino energies (>10 GeV).
We also list the referecnces of previous calculation, here.
T. Sanuki et al., Phys. Rev. D75, 043005 (2007) (eprint) and
M. Honda et al., Phys. Rev. D75, 043006 (2007) (eprint).

The previous flux tables are here (hkkms 2006).

Old refrerences:
M. Honda, the talk at C2CR 2005, Prague.
M. Honda et al., the talk at 29th ICRC2005, Pune. The conference paper is here.
M. Honda et al., Phys. Rev. D70, 043008 (2004) [HKKM04] (eprint).
K. Abe et al., A revised version of the conference paper; Abe et al., 28th ICRC2003, Tsukuba.
M. Honda et al., the talk at 28th ICRC2003, Tsukuba. The conference paper is here.
M. Honda, the talk at Noon2003, Kanazawa. The conference paper is here.
M. Honda et al., the talk at 27th ICRC, Hamburg. The conference paper is here.
M. Honda et al., the poster paper at Neutrino 2002, Munich.
For the references earlier than 2000. see Ann. Rev. Nucl. Part. Sci.52:153-199, 2002. (eprint)

Comments or Questions on flux table