We point out that the measurement of the distribution of atmospheric
neutrino events with sufficient resolution in order to observe the
characteristic modulations of neutrino oscillations would provide a unique way
to test the oscillations nature of the atmospheric neutrino anomaly
in the parameter range $5\times 10^{-4} < \Delta m^2 < 2\times 10^{-3}\rm
eV^2$. With an integrated exposure of a few tens of kiloton-year, this method
can cover the lower part of the region of the currently allowed
atmospheric neutrino solution and is therefore complementary to the one
explorable with planned long-baseline neutrino beam experiments. We stress that
experimentally this method relies on the ability to measure high energy muons
(). A large magnetized calorimeter of several kilotons would be
ideally suited for this measurement. The existing LEP detectors augmented with
atmospheric neutrino triggers could also be used to perform such a study.

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