  Statistical analysis is performed of the atmospheric neutrino flux models as
compared with the data of Frejus, AMANDA-II, IceCube, ANTARES, and
Super-Kamiokande experiments. The analysis enables the evaluation of the
confidence level of the flux models in comparison with atmospheric neutrino
flux measurements. The flux calculations were performed in the framework of
single computational scheme using a set of hadronic models combined with
parameterizations of the cosmic rays spectrum by Zatsepin & Sokolskaya, and
Hillas & Gaisser. The analysis showed satisfactory agreement of the
conventional $\nu_\mu$ flux models with the measurements. The prompt neutrinos
conrtibution obtained with a set of charm production models (QGSM, SIBYLL 2.3c,
PROSA, GRRST, BEJKRSS, and GM-VFNS) is statistically negligible in the energy
range covered by the neutrino telescopes.
