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A simulation study of the energy released by extensive air showers in the form of MHz radiation is performed using the CoREAS simulation code. We develop an efficient method to extract this radiation energy from air-shower simulations. We…

High Energy Astrophysical Phenomena · Physics 2017-03-20 Christian Glaser , Martin Erdmann , Jörg R. Hörandel , Tim Huege , Johannes Schulz

A simulation study of the energy released by extensive air showers in the form of MHz radiation is performed using the CoREAS simulation code. We develop an efficient method to extract this radiation energy from air-shower simulations. We…

High Energy Astrophysical Phenomena · Physics 2016-09-20 Christian Glaser , Martin Erdmann , Jörg R. Hörandel , Tim Huege , Johannes Schulz

The distribution of depth in which a cosmic ray air shower reaches its maximum number of particles ($X_{max}$) is studied and parametrized. Three functions are studied for proton, carbon, silicon, and iron primary particles with energies…

High Energy Astrophysical Phenomena · Physics 2021-06-01 Luan Arbeletche , Vitor de Souza

Cosmic rays have valuable information about universe surroundings us. Finding energy, mass and arrival direction of primary cosmic ray particle are the most important aspects of extensive air shower studies. In order to determine these…

Instrumentation and Methods for Astrophysics · Physics 2011-03-17 H. Hedayati Kh. , A. Anvari , M. Bahmanabadi , M. Khakian Ghomi , J. Samimi

The impact of the lateral distribution of light in extensive air showers on the detection and reconstruction of shower profiles is investigated for the Auger fluorescence telescopes. Based on three-dimensional simulations, the capability of…

Detailed theoretical study of the mean square radius of extensive air shower electrons has been made in connection with further development of scaling formalism for electron lateral distribution function. A very simple approximation…

Astrophysics · Physics 2007-05-23 R. I. Raikin , A. A. Lagutin , N. Inoue , A. Misaki

The energy spectra of particles arriving at the ground is a significant observable in the analysis of extensive air showers (EAS). Energy distributions at ground were studied for primary particles (12C,56Fe, p, and 28Si) with high primary…

High Energy Astrophysical Phenomena · Physics 2025-04-29 Itab F. Hussein , A. A. Al-Rubaiee

A comparative study of simulated air shower longitudinal profiles is presented. An appropriate thinning level for the calculations is first determined empirically. High statistics results are then provided, over a wide energy range,…

Astrophysics · Physics 2011-05-23 C. L. Pryke

The simulation of Cherenkov light lateral distribution function (CLLDF) in Extensive Air Showers (EAS) was performed by using the Monte Carlo CORSIKA code for configurations of Tunka-133 EAS Cherenkov array. This simulation was carried out…

Instrumentation and Methods for Astrophysics · Physics 2017-11-03 Marwah M. Abdulsttar , A. A. Al-Rubaiee

Using the large hadron calorimeter of the KASCADE experiment, hadronic cores of extensive air showers have been studied. The hadron lateral and energy distributions have been investigated in order to study the reliability of the shower…

Astrophysics · Physics 2009-10-31 T. Antoni , J. R. Hoerandel

The paper proposes a new approach for approximating the lateral distribution functions (LDF) of Cherenkov light emitted by the electromagnetic component of extensive air showers (EAS) in the Earth's atmosphere. The information basis of the…

High Energy Astrophysical Phenomena · Physics 2025-09-09 N. V. Volkov , A. A. Lagutin , A. I. Reviakin , R. T. Bizhanov

We develop a potential algorithm to relate the depth development of ultra high energy extensive air showers and the time delay for individual muons. The time distributions sampled at different positions at ground level by a large air shower…

Astrophysics · Physics 2009-11-10 L. Cazon , R. A. Vazquez , E. Zas

We find that the ratio r_{mu e} of the muon to the electromagnetic component of an extended air shower at the ground level provides an indirect measure of the depth X_{max} of the shower maximum. This result, obtained with the air-shower…

High Energy Astrophysical Phenomena · Physics 2016-10-18 C. A. García Canal , J. I. Illana , M. Masip , S. J. Sciutto

In hadron induced air showers of highest energies (E> 1e18 eV), the lateral distribution functions of electrons and muons are a superposition of many separate electromagnetic sub-showers, initiated by meson decay at different altitudes and…

High Energy Physics - Phenomenology · Physics 2011-05-23 Hans-Joachim Drescher , Glennys R. Farrar

The lateral distribution function (LDF) for coherent electromagnetic radiation from air showers initiated by ultra-high-energy cosmic rays is calculated using a macroscopic description. A new expression is derived to calculate the coherent…

High Energy Astrophysical Phenomena · Physics 2011-01-28 Krijn D. de Vries , Ad M. van den Berg , Olaf Scholten , Klaus Werner

The burst of radio emission by the extensive air shower provides a promising alternative for detecting ultra-high energy cosmic rays.We have developed an independent numerical program to simulate these radio signals. Our code is based on a…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Wei Liu , Xuelei Chen

The aim of this report of the Working Group on Hadronic Interactions and Air Shower Simulation is to give an overview of the status of the field, emphasizing open questions and a comparison of relevant results of the different experiments.…

High Energy Astrophysical Phenomena · Physics 2019-08-16 J. Allen , A. Castellina , R. Engel , K. Kasahara , S. Knurenko , T. Pierog , A. Sabourov , B. T. Stokes , R. Ulrich , S. Ostapchenko , T. Sako

We present a fast one dimensional hybrid method to efficiently simulate extensive air showers up to the highest observed energies. Based on precalculated pion showers and a bootstrap technique, our method predicts the average shower…

Astrophysics · Physics 2011-05-12 Jaime Alvarez-Muñiz , Ralph Engel , T. K. Gaisser , Jeferson A. Ortiz , Todor Stanev

The lateral density data obtained for different secondaries of an extensive air shower (EAS) from an array of detectors are usually described by some suitable lateral density functions (LDFs). Analyzing non-vertical simulated EASs generated…

High Energy Astrophysical Phenomena · Physics 2023-11-14 Animesh Basak , Rajat K. Dey

The Sydney University Giant Air-shower Recorder (SUGAR) measured the muon component of extensive air showers with a unique array of muon detectors. The SUGAR data allow us to reconstruct the empirical dependence of muon density on the…

High Energy Astrophysical Phenomena · Physics 2022-05-18 N. N. Kalmykov , I. S. Karpikov , G. I. Rubtsov , S. V. Troitsky