TIME-TRACK COMPLEMENTARITY IN THE STUDY OF EAS LONGITUDINAL DEVELOPMENT

被引:20
作者
DANILOVA, TV [1 ]
DUMORA, D [1 ]
ERLYKIN, AD [1 ]
PROCUREUR, J [1 ]
机构
[1] UNIV BORDEAUX 1,PHYS THEOR LAB,F-33175 GRADIENAM,FRANCE
关键词
D O I
10.1088/0954-3899/20/6/011
中图分类号
O57 [原子核物理学、高能物理学];
学科分类号
070202 ;
摘要
Extensive air shower (EAS) muon production and propagation through the atmosphere were simulated. The incidence angles and arrival time at the observation level were determined for each muon. It is shown that for large distances from EAS cores and for GeV-muons, time and track measurements could be used complementarily to improve the accuracy of the muon production height determination. For TTC detectors of 5 GeV muons attached to EAS arrays at mountains and placed at a distance of about 200-250 m from its centre, the accuracy of the muon production depth estimate is about 35 g CM-2. The influence of the detector location, the muon energy threshold, the observation level and experimental errors is analysed.
引用
收藏
页码:961 / 978
页数:18
相关论文
共 33 条
[1]  
AGUIRRE C, 1979, 16TH INT COSM RAY C, V13, P142
[2]  
AGUIRRE C, 1979, 16TH P ICRC KYOT, V8, P112
[3]  
ATRASHKEVICH VB, 1987, 20TH INT COSM RAY C, V6, P67
[4]  
BLAKE PR, 1981, 17TH P ICRC PAR, V6, P20
[5]  
BLAKE PR, 1979, 16TH INT COSM RAY C, V8, P32
[6]  
BLAKE PR, 1977, 15TH P ICRC PLOVD, V8, P200
[7]  
BLAKE PR, 1970, ACTA PHYS S, V29, P633
[8]  
BLAKE PR, 1983, 18TH P ICRC BANG, V6, P103
[9]  
BLAKE PR, 1985, 19TH P ICRC LA JOLL, V7, P123
[10]  
BURGER J, 1975, 14TH P ICRC MUN, V8, P2784