Properties of 109-1010 GeV extensive air showers at core distances between 100 and 3000 m
Properties of 109-1010 GeV extensive air showers at core distances between 100 and 3000 m
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109-1010 GeV 广泛空气簇射在核心距离 100 至 3000 m 之间的特性
DOI：
10.1088/0305-4616/12/10/017
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发表时间：
1986
期刊：
影响因子：
--
通讯作者：
G. Tanahashi
中科院分区：
文献类型：
--
作者：
T. Teshima;Y. Matsubara;T. Hara;N. Hayashida;M. Honda;F. Ishikawa;T. Kifune;M. Mori;M. Nagano;K. Nishijima;H. Ohoka;Y. Ohno;G. Tanahashi
用新的Akeno 20km2巨型空气簇射(GAS)阵列研究了109-1010GeV广延空气簇射(EAS)的一些性质，如电子和Muon的横向分布、Muon电子密度比、簇射锋面结构和跃迁效应。在较大的核心距离处，电子和Muon的横向分布比迄今报道的公式的外推更陡峭。在脉冲延迟超过R/c(R为核心距离)的范围内，簇射锋面的厚度与林斯利的公式符合得很好。
The authors examine some properties of 109-1010 GeV extensive air showers (EAS), such as the electron and the muon lateral distribution, the ratio of muon electron density, the shower front structure and the transition effects in a scintillator, with the new Akeno 20 km2 giant air showers (GAS) array at core distances between 100 and 3000 m. At large core distances the lateral distributions of both electrons and muons become steeper than extrapolations of the formulae so far reported. The thickness of shower fronts agrees well with Linsley's formula up to 3 km, to the extent that the authors pulses delayed by more than R/c (R is the core distance).