UHE COSMIC-RAY EVENT RECONSTRUCTION BY THE ELECTROMAGNETIC DETECTOR OF EAS-TOP

被引：85
作者：
AGLIETTA, M
ALESSANDRO, B
ANTONIOLI, P
ARNEODO, F
BERGAMASCO, L
FAUTH, AC
CASTAGNOLI, C
CASTELLINA, A
CATTADORI, C
CHIAVASSA, A
CINI, G
PIAZZOLI, BD
DISCIASCIO, G
FULGIONE, W
GALEOTTI, P
GHIA, PL
IACOVACCI, M
MANNOCCHI, G
MORELLO, C
NAVARRA, G
RICCATI, L
SAAVEDRA, O
TRINCHERO, GC
VALLANIA, P
VERNETTO, S
机构：
[1] CNR,IST COSMOGEOF,TURIN,ITALY
[2] IST NAZL FIS NUCL,TURIN,ITALY
[3] IST NAZL FIS NUCL,MILAN,ITALY
[4] INFN,NAPLES,ITALY
[5] UNIV ESTADUAL CAMPINAS,INST FIS,BR-13100 CAMPINAS,SP,BRAZIL
[6] UNIV NAPLES,DIPARTIMENTO SCI FIS,I-80138 NAPLES,ITALY
来源：
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 1993年 / 336卷 / 1-2期
关键词：
D O I：
10.1016/0168-9002(93)91115-4
中图分类号：
TH7 [仪器、仪表];
学科分类号：
0804 ; 080401 ; 081102 ;
摘要：
UHE cosmic rays are studied by means of the detectors of the different components of secondaries produced by their interactions in the atmosphere (EAS). We describe and discuss the reconstruction techniques and accuracies of the e.m. detector of EAS-TOP. They allow, besides independent high resolution measurements of UHE gamma-ray astronomy, good correlation possibilities with the detectors of the different EAS components.
引用
收藏
页码：310 / 321
页数：12
相关论文
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