We reanalyze the constraints on atmospheric νₑ and ν_μ fluxes due to three-neutrino oscillations and investigate the anomalous neutrino fluxes recently observed at Kamiokande. We find that it is difficult to explain the data by νₑ↔ν_μ oscillations alone. We also show that models of three neutrino flavors with neutrino-mass-squared differences of order 10^-2 eV² can solve both the solar and the atmospheric neutrino problems simultaneously.
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Hidaka et al. (1988) studied this question.
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