Arrival-time distribution of muons in extensive air showers at energies of 1017eV to 1018eV

1982 ◽  
Vol 8 (11) ◽  
pp. 1605-1620 ◽  
Author(s):  
P R Blake ◽  
D M Mann ◽  
W F Nash ◽  
B O'Connell ◽  
R B Strutt
Keyword(s):  
Time Distribution ◽  
Arrival Time ◽  
Extensive Air Showers ◽  
Arrival Time Distribution ◽  
Air Showers

The arrival time distribution of muons in extensive air showers

1986 ◽  
Vol 12 (6) ◽  
pp. 547-560 ◽  
Author(s):  
E J de Villiers ◽  
D J van der Walt ◽  
P K F Grieder ◽  
G van Urk
Keyword(s):  
Time Distribution ◽  
Arrival Time ◽  
Extensive Air Showers ◽  
Arrival Time Distribution ◽  
Air Showers

Arrival-time distribution of muons and electrons in large air showers observed at 5200m above sea level

1979 ◽  
Author(s):  
C. Aguirre ◽  
R. Anda ◽  
A. Trepp ◽  
F. Kakimoto ◽  
Y. Mizumoto ◽  
...  
Keyword(s):  
Sea Level ◽  
Time Distribution ◽  
Arrival Time ◽  
Arrival Time Distribution ◽  
Air Showers

SPECTRUM OF COSMIC RAYS WITH ENERGY ABOVE 1017 EV

2005 ◽  
Vol 20 (29) ◽  
pp. 6878-6880 ◽  
Author(s):  
V. P. EGOROVA ◽  
A. V. GLUSHKOV ◽  
A. A. IVANOV ◽  
S. P. KNURENKO ◽  
V. A. KOLOSOV ◽  
...  
Keyword(s):  
Distribution Function ◽  
Energy Spectrum ◽  
Cosmic Rays ◽  
Time Distribution ◽  
Arrival Time ◽  
Lateral Distribution ◽  
Arrival Time Distribution ◽  
Array Data ◽  
Lateral Distribution Function ◽  
High Energies

The energy spectrum of primary cosmic rays with ultra-high energies based on the Yakutsk EAS Array data is presented. For the largest events values of S600 and axis coordinates have been obtained using revised lateral distribution function. The effect of the arrival time distribution at several axis distance on estimated density for Yakutsk and AGASA is considered.

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