Περίληψη:
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, I-0 (.) cos(alpha)(theta), as a function of
the zenith angle theta. Measured values of index alpha and the vertical
intensity I-0
(Graphics)
are in good agreement with previous measurements and phenomenological
predictions. (c) 2005 Elsevier B.V. All rights reserved.
Συγγραφείς:
Aggouras, G
Anassontzis, EG
Ball, AE
Bourlis, G and
Chinowsky, W
Fahrun, E
Grammatikakis, G
Green, C and
Grieder, P
Katrivanos, P
Koske, P
Leisos, A
Markopoulos,
E
Minkowsky, P
Nygren, D
Papageorgiou, K
Przybylski, G
and Resvanis, LK
Siotis, I
Sopher, J
Staveris-Polikalas, A
and Tsagli, V
Tsirigotis, A
Zhukov, VA
