Measurement of Atmospheric Neutrinos at the Sudbury Neutrino Observatory
The Sudbury Neutrino Observatory consists of a 1 kiloton heavy water Cherenkov detector able to detect and reconstruct high-energy muons created from cosmic ray showers and atmospheric neutrino interactions. By measuring the flux of through-going muons as a function of zenith angle, the SNO experime...
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| Other Authors: | , , |
| Format: | Article |
| Language: | English |
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Elsevier B.V.,
2009-11-25T16:21:11Z.
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| Online Access: | Get fulltext |