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Detector Depth Dependence of the High Energy Atmospheric Neutrino Flux

John M. LoSecco
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Abstract

We note that detector depth can influence the decay path length available for the primary and secondary particles that are the source of atmospheric neutrinos. As a consequence there is a location dependent modulation to the neutrino flux, which could be as large as 5-10% in some directions.

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John M. LoSecco. 2004-06-25. Detector Depth Dependence of the High Energy Atmospheric Neutrino Flux. https://doi.org/10.1103/physrevd.70.097301

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