Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10700501 | Astroparticle Physics | 2005 | 16 Pages |
Abstract
A module of the NESTOR underwater neutrino telescope was deployed at a depth of 3800 m in order to test the overall detector performance and particularly that of the data acquisition systems. A prolonged period of running under stable operating conditions made it possible to measure the cosmic ray muon flux, I0·cosα(θ), as a function of the zenith angle θ. Measured values of index α and the vertical intensity I0α=4.7±0.5(stat)±0.2(syst)I0=9.0Ã10-9±0.7Ã10-9(stat)±0.4Ã10-9(syst)cm-2s-1sr-1are in good agreement with previous measurements and phenomenological predictions.
Related Topics
Physical Sciences and Engineering
Physics and Astronomy
Astronomy and Astrophysics
Authors
The NESTOR Collaboration The NESTOR Collaboration, G. Aggouras, E.G. Anassontzis, A.E. Ball, G. Bourlis, W. Chinowsky, E. Fahrun, G. Grammatikakis, C. Green, P. Grieder, P. Katrivanos, P. Koske, A. Leisos, E. Markopoulos, P. Minkowsky, D. Nygren,