Monte Carlo study of the arrival time distribution of particles in extensive air showers in the energy range 1–100 TeV
Author:
Publisher
Elsevier BV
Subject
Astronomy and Astrophysics
Reference45 articles.
1. Monte Carlo simulation of photon-induced air showers
2. Time structure of the extensive air shower front
3. Interpretation of the time structure of the EAS disc measured by the GREX/COVER_PLASTEX experiment
4. UHE cosmic ray event reconstruction by the electromagnetic detector of EAS-TOP
5. Distribution of Arrival Times of Air Shower Particles
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1. Measuring temporal characteristics of the Cherenkov radiation signal from extensive air showers of cosmic rays with a wide field-of-view telescope addendum to the Yakutsk array;Physical Review D;2022-02-25
2. The angular resolution of GRAPES-3 EAS array after improved timing and shower front curvature correction based on age and size;Journal of Cosmology and Astroparticle Physics;2020-07-10
3. Simulation of the time structure of Extensive Air Showers with CORSIKA initiated by various primary particles at Alborz-I observatory level;New Astronomy;2018-05
4. Estimating primary energy of cosmic rays by calculating secondary particles density in optimum distance from shower core;International Journal of Modern Physics D;2018-01
5. Time correlation of cosmic-ray-induced neutrons and gamma rays at sea level;Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment;2014-02
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