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Cosmic-ray interactions in the Earth’s atmosphere produce copious secondary mesons, providing a natural laboratory for searches for new physics. We investigate the atmospheric production of axions through the rare kaon decay . If sufficiently long-lived, these axions can reach large underground detectors such as Super-Kamiokande and IceCube and decay through the diphoton channel, . Using data from Super-Kamiokande and IceCube, we derive constraints on the axion decay constant for masses up to . We demonstrate that atmospheric kaon decays provide a novel probe of axion parameter space, yielding constraints complementary to existing bounds.

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