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CERN Document Server Намерени са 2,037 записа  1 - 10следващкрай  отиване на запис: Търсенето отне 0.92 секунди. 
1.
(100)
The cosmic ray primary composition between $10^{15}$ and $10^{16}$ ev from Extensive Air Showers electromagnetic and TeV muon data / Aglietta, M ; Alessandro, B ; Ambrosio, M ; Antolini, R ; Antonioli, P ; Arneodo, F ; Baldini, A ; Barbarino, G C ; Barish, B C ; Battistoni, G et al.
The cosmic ray primary composition in the energy range between 10/sup 15/ and 10/sup 16/ eV, i.e., around the "knee" of the primary spectrum, has been studied through the combined measurements of the EAS-TOP air shower array (2005 m a.s.l., 10/sup 5/ m/sup 2/ collecting area) and the MACRO underground detector (963 m a.s.l., 3100 m w.e. of minimum rock overburden, 920 m/sup 2/ effective area) at the National Gran Sasso Laboratories. [...]
2004 - Published in : Astropart. Phys. 20 (2004) 641-52
Подробен запис - Подобни записи
2.
(76)
Study of the primary cosmic ray composition in the knee region with EAS-TOP and MACRO / EAS-TOP Collaboration
INFN-AE-97-46.- Italy : INFN, 1997 - 6 p. Access to fulltext document: TIF PDF;
In : 25th International Conference on Cosmic Rays, v.1-7, Durban, South Africa, 28 Jul - 8 Aug 1997, pp.41-44
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3.
(74)
The cosmic ray proton, helium and CNO fluxes in the 100 TeV energy region from TeV muons and EAS atmospheric Cherenkov light observations of MACRO and EAS-TOP / Aglietta, M ; Alessandro, B ; Ambrosio, M ; Antolini, R ; Antonioli, P ; Arneodo, F ; Baldini, A ; Barbarino, G C ; Barish, B C ; Battistoni, G et al.
The primary cosmic ray (CR) proton, helium and CNO fluxes in the energy range 80-300 TeV are studied at the National Gran Sasso Laboratories by means of EAS-TOP (Campo Imperatore, 2005 m a.s.l.) and MACRO (deep underground, 3100 m w.e., the surface energy threshold for a muon reaching the detector being E/sub mu //sup th/ approximately=1.3 TeV). The measurement is based on: (a) the selection of primaries based on their energy/nucleon (i.e., with energy/nucleon sufficient to produce a muon with energy larger than 1.3 TeV) and the reconstruction of the shower geometry by means of the muons recorded by MACRO in the deep underground laboratories; (b) the detection of the associated atmospheric Cherenkov light (C.l.) signals by means of the C.l. [...]
2004 - Published in : Astropart. Phys. 21 (2004) 223-40
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4.
(61)
The HE muon and neutrino fluxes from measurements of horizontal air showers at EAS-TOP / Aglietta, M ; Alessandro, B
1995
In : 24th International Cosmic-ray Conference, v.0.0, Rome, Italy, 28 Aug - 8 Sep 1995, pp.638-641
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5.
(59)
Study of the primary composition from the Ne data at EAS-TOP / Alessandro, B
1995
In : 24th International Cosmic-ray Conference, v.0.0, Rome, Italy, 28 Aug - 8 Sep 1995, pp.664-667
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6.
(57)
Cosmic ray studies around the "Knee" of the primary spectrum from EAS-TOP / EAS-TOP Collaboration
INFN-AE-96-39. - 1996. - 14 p.
Access to fulltext document - Access to fulltext document - CERN library copies
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7.
(56)
Study of the primary cosmic ray composition in the PeV region with EAS-TOP and Macro / Vallania, P
1995
In : 24th International Cosmic-ray Conference, v.0.0, Rome, Italy, 28 Aug - 8 Sep 1995, pp.710-713
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8.
(56)
Fractal analysis of cosmic ray signals detected in the EAS-TOP experiment / Aglietta, M ; Alessandro, B
1995
In : 24th International Cosmic-ray Conference, v.0.0, Rome, Italy, 28 Aug - 8 Sep 1995, pp.964-967
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9.
(54)
The EAS-TOP studies of the cosmic ray primaries in the knee region / Navarra, G
2005 Published version: PDF;
In : 29th International Cosmic Ray Conference, Pune, India, 3 - 10 Aug 2005, pp.165 (v.6)
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10.
(53)
Measurement of the cosmic ray composition at the knee with the SPASE-2/AMANDA-B10 detectors / Ahrens, J ; Ackermann, M ; Andrés, E ; Bai, X ; Barwick, S W ; Bay, R C ; Becka, T ; Becker, K H ; Bernardini, E ; Bertrand, D et al.
The mass composition of high-energy cosmic rays at energies above 10 /sup 15/ eV can provide crucial information for the understanding of their origin. Air showers were measured simultaneously with the SPASE-2 air shower array and the AMANDA-B10 Cherenkov telescope at the South Pole. [...]
2004 - Published in : Astropart. Phys. 21 (2004) 565-81
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