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Titolo:
RESULTS ON HIGH-ENERGY COSMIC-RAYS BY EAS-TOP AT GRAN-SASSO
Autore:
AGLIETTA M; ALESSANDRO B; ANTONIOLI P; ARNEODO F; BERGAMASCO L; BERTAINA M; FAUTH AC; CASTAGNOLI C; CASTELLINA A; CHIAVASSA A; CASTAGNOLI GC; PIAZZO BD; DISCIASCIO G; FULGIONE W; GALEOTTI P; GHIA PL; IACOVACCI M; MANNOCCHI G; MELAGRANA C; MORELLO C; NAVARRA G; RICCATI L; SAAVEDRA O; TRINCHERO GC; VALLANIA P; VERNETTO S;
Indirizzi:
CNR,IST COSMOGEOFIS,CORSO FIUME 4 I-10133 TURIN ITALY
Titolo Testata:
Nuovo cimento della Societa italiana di fisica. C, Geophysics and space physics
fascicolo: 6, volume: 20, anno: 1997,
pagine: 985 - 1007
SICI:
1124-1896(1997)20:6<985:ROHCBE>2.0.ZU;2-V
Fonte:
ISI
Lingua:
ENG
Soggetto:
DEEP-UNDERGROUND MUONS; EXTENSIVE AIR SHOWERS; CRAB-NEBULA; GAMMA-RAYS; GALACTIC DISK; TEV; ARRAY; CYGNUS-X-3; RADIATION; SEARCH;
Tipo documento:
Article
Natura:
Periodico
Citazioni:
82
Recensione:
Indirizzi per estratti:
Citazione:
M. Aglietta et al., "RESULTS ON HIGH-ENERGY COSMIC-RAYS BY EAS-TOP AT GRAN-SASSO", Nuovo cimento della Societa italiana di fisica. C, Geophysics and space physics, 20(6), 1997, pp. 985-1007

Abstract

Very High-Energy cosmic rays have to be studied through the ground-based detectors of the Extensive Air Showers (EAS) that they produce in the atmosphepe. The main measurements to be performed are of: primary energy spectra, composition, anisotropies, <<neutral primary>> astronomy, and interaction properties. This requires complete detectors of all the EAS components, and for this purpose the EAS-TOP array has been constructed at Campo Imperatore (2000 m a.s.l.) on top of the Gran Sasso underground laboratories. The array has been progressively going into operation since 1988. In this paper we present the status and performances of the different detectors, and the results obtained up to nowon the different items under discussion.

ASDD Area Sistemi Dipartimentali e Documentali, Università di Bologna, Catalogo delle riviste ed altri periodici
Documento generato il 27/11/20 alle ore 07:23:44