Phenomenological characteristics of EAS at sea level: EAS size spectra and fluctuations of EAS

1968 ◽  
Vol 46 (10) ◽  
pp. S197-S200 ◽  
Author(s):  
S. N. Vernov ◽  
G. B. Khristiansen ◽  
A. T. Abrosimov ◽  
V. B. Atrashkevitch ◽  
I. F. Beljaeva ◽  
...  
Keyword(s):  
Experimental Data ◽  
Distribution Function ◽  
Sea Level ◽  
Lateral Distribution ◽  
Size Spectra ◽  
Lateral Distribution Function ◽  
The Individual ◽  
Electron Photon

Experimental EAS spectra of sizes and muon numbers and results on the fluctuations of the electron–photon and muon EAS components at sea level are presented. In constructing size spectra the sizes of showers were determined by use of the individual lateral distribution function. Experimental data were obtained with considerably better statistics than in our previous works.

A new lateral distribution function for electrons in extensive air showers (EAS) detected near sea level

1995 ◽  
Vol 18 (3) ◽  
pp. 325-334 ◽  
Author(s):  
B. Bhattacharyya ◽  
A. Bhadra ◽  
A. Mukherjee ◽  
G. Saha ◽  
S. Sanyal ◽  
...  
Keyword(s):  
Distribution Function ◽  
Sea Level ◽  
Lateral Distribution ◽  
Extensive Air Showers ◽  
Air Showers ◽  
Lateral Distribution Function

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.

Lateral distribution function of charged particles in EAS near the axis

2011 ◽  
Vol 75 (3) ◽  
pp. 357-359 ◽  
Author(s):  
D. D. Dzhappuev ◽  
N. F. Klimenko ◽  
A. U. Kudzhaev ◽  
A. S. Lidvansky ◽  
V. B. Petkov ◽  
...  
Keyword(s):  
Distribution Function ◽  
Charged Particles ◽  
Lateral Distribution ◽  
Lateral Distribution Function

scholarly journals Parameterization of Cherenkov Light Lateral Distribution Function as a Function of the Zenith Angle around the Knee Region

2016 ◽  
Vol 66 ◽  
pp. 71-78
Author(s):  
Marwah M. Abdulsttar ◽  
A.A. Al-Rubaiee ◽  
Abdul Halim K. Ali
Keyword(s):  
Distribution Function ◽  
Zenith Angle ◽  
Lateral Distribution ◽  
Extensive Air Showers ◽  
Cherenkov Light ◽  
Primary Proton ◽  
Air Showers ◽  
Knee Region ◽  
Lateral Distribution Function ◽  
Shower Core

Cherenkov light lateral distribution function (CLLDF) simulation was fullfiled using CORSIKA code for configurations of Tunka EAS array for different zenith angles. The parameterization of the CLLDF was carried out as a function of the destance from tehe shower core in extensive air showers (EAS) and zenith angle on the basis of the CORSIKA simulation for primary proton around the knee region with the energy 3.1015 eV at different zenith angles. The parametrized CLLDF is verified in comparison with the simulation that performed using CORSIKA code for two zenith angles.

scholarly journals Demonstrating of Cosmic Ray Characteristics by Estimating the Cherenkov Light Lateral Distribution Function for Yakutsk Array as a Function of the Zenith Angle

2016 ◽  
Vol 67 ◽  
pp. 21-30
Author(s):  
Marwah M. Abdulsttar ◽  
A.A. Al-Rubaiee ◽  
Abdul Halim K. Ali
Keyword(s):  
Numerical Simulation ◽  
Distribution Function ◽  
Zenith Angle ◽  
Cosmic Ray ◽  
Primary Energy ◽  
Lateral Distribution ◽  
Cherenkov Light ◽  
Air Showers ◽  
Lateral Distribution Function ◽  
Primary Particles

Cherenkov light lateral distribution function (CLLDF) in Extensive Air Showers (EAS) for different primary particles (e-, n , p, F, K and Fe) was simulated using CORSIKA code for conditions and configurations of Yakutsk EAS array with the fixed primary energy 3 PeV around the knee region at different zenith angles. Basing on the results of CLLDF numerical simulation, sets of approximated functions are reconstructed for different primary particles as a function of the zenith angle. A comparison of the parametrized CLLDF with that simulated with Yakutsk EAS array is verified.The parameterized CLLDF also is compared with that measured on the Yakutsk EAS array.

scholarly journals A lateral distribution function for the radio emission of air showers

2016 ◽  
Author(s):  
Anna Nelles ◽  
Stijn Buitink ◽  
Arthur Corstanje ◽  
Emilio Enriquez ◽  
Heino Falcke ◽  
...  
Keyword(s):  
Distribution Function ◽  
Radio Emission ◽  
Lateral Distribution ◽  
Air Showers ◽  
Lateral Distribution Function
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