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Titolo:
MULTICOMPONENT EXTENSIVE AIR SHOWER OBSERVATIONS AT EAS-TOP
Autore:
AGLIETTA M; ALESSANDRO B; ANTONIOLI P; ARNEODO F; BERGAMASCO L; BERTAINA M; FAUTH AC; CASTAGNOLI C; CASTELLINA A; CHIAVASSA A; CASTAGNOLI GC; PIAZZOLI BD; DISCIASCIO G; FULGIONE W; GALEOTTI P; GHIA PL; IACOVACCI M; DEGODOI AL; MANNOCCHI G; MELAGRANA C; SILVA NM; MORELLO C; NAVARRA G; NOGIMA H; RICCATI L; SAAVEDRA O; TRINCHERO GC; VALLANIA P; VERNETTO S; VIGORITO C;
Indirizzi:
CNR,IST COSMOGEOFIS,CORSO FIUME 4 I-10133 TURIN ITALY IST NAZL FIS NUCL I-10125 TURIN ITALY IST NAZL FIS NUCL I-40126 BOLOGNA ITALY UNIV AQUILA,DIPARTIMENTO FIS I-67010 LAQUILA ITALY IST NAZL FIS NUCL,LAB NAZL GRAN SASSO I-67010 ASSERGI AQ ITALY UNIV TURIN,DIPARTIMENTO FIS GENERALE I-10125 TURIN ITALY UNIV ESTADUAL CAMPINAS,INST FIS BR-13081970 CAMPINAS SP BRAZIL UNIV NAPLES,DIPARTIMENTO SCI FISICHE I-80125 NAPLES ITALY IST NAZL FIS NUCL I-80125 NAPLES ITALY
Titolo Testata:
Nuclear physics. B
, , anno: 1997, supplemento:, 54B
pagine: 263 - 270
SICI:
0550-3213(1997):<263:MEASOA>2.0.ZU;2-4
Fonte:
ISI
Lingua:
ENG
Soggetto:
GRAN-SASSO; DETECTOR; ARRAY; LIGHT;
Tipo documento:
Article
Natura:
Periodico
Settore Disciplinare:
Science Citation Index Expanded
Citazioni:
21
Recensione:
Indirizzi per estratti:
Citazione:
M. Aglietta et al., "MULTICOMPONENT EXTENSIVE AIR SHOWER OBSERVATIONS AT EAS-TOP", Nuclear physics. B, 1997, pp. 263-270

Abstract

The study of cosmic rays at primary energies E-0 > 10(14) eV requiresthe detection of the different components of Extensive Air Showers through ground based stations. EAS-TOP is such an array (located at Campo Imperatore, 2000 m a.s.l., National Gran Sasso Laboratories), including detectors of the electromagnetic, muon (E-mu approximate to GeV atthe surface, and E-mu approximate to TeV in coincidence with the detectors operating in the underground Gran Sasso Laboratories), hadron and atmospheric Cerenkov light components. The combined operation of thedetectors is discussed from the point of view of the capability of measuring the cosmic ray primary spectrum and composition. The main lines for checking the significant features of the high energy hadron interaction model used for the interpretation of the data are outlined.

ASDD Area Sistemi Dipartimentali e Documentali, Università di Bologna, Catalogo delle riviste ed altri periodici
Documento generato il 30/11/20 alle ore 20:09:36