ANGULAR DISTRIBUTION OF MUON-POOR EXTENSIVE AIR SHOWERS

被引:9
作者
CATZ, P
MAZE, R
GAWIN, J
PRZASNYCKI, M
WDOWCZYK, J
ZAWADZKI, A
机构
[1] Cosmic Ray Physics Laboratory, Verrières le Buisson
[2] Cosmic Ray Physics Laboratory, Lodz
关键词
D O I
10.1103/PhysRevLett.23.988
中图分类号
O4 [物理学];
学科分类号
0702 ;
摘要
Angular distribution of muon-poor extensive air showers was found to be flatter than that of normal showers. The result excludes any possibility that muon-poor showers are initiated by primary photons. It is likely that the showers are generated by some relatively passive particles which are produced through interactions between the primary cosmic rays and the atmospheric nuclei. © 1969 The American Physical Society.
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页码:988 / +
页数:1
相关论文
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VERNOV SN, TO BE PUBLISHED