Abstract
The comparison between the KAMIOKANDE data and theoretical estimations of the low-energy ( E ν <a few GeVs) atmospheric neutrino events is considered. Neutrino spectra calculated in our previous papers are used with the account of corrections due to the cosmic ray muon polarization. The discrepancy between observed and predicted ratios of electron-like and muon-like single-ring event numbers can be explained either by neutrino oscillations ( of ν e ↔ ν μ - type predominantly), or by misidentifying the particle species of single-ring events.
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