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We present the experimental data on the knee, as observed in the electromagnatic and high energy muon (E\mu \ge 230 Gev) components.

Astrophysics · Physics 2007-05-23 A. E. Chudakov , V. B. Petkov , V. Ya. Poddubny , A. V. Voevodsky

The lateral distribution of muons with threshold energy e ~ 1*sec(theta) GeV have been studied in showers with energy E>=10^17 eV. The data considered in the analysis have been collected from November 2011 to June 2013. Experimental values…

High Energy Astrophysical Phenomena · Physics 2013-10-07 A. V. Glushkov , A. Sabourov

The main goal of the Andyrchy-BUST experiment is to study the primary cosmic rays spectrum and composition around the knee. The experimental data on the knee, as observed in the electromagnetic and high energy muon components, are…

High Energy Astrophysical Phenomena · Physics 2019-07-12 V. B. Petkov

Frequency distributions of local muon densities in high-energy extensive air-showers (EAS) are presented as signature of the primary cosmic ray energy spectrum in the knee region. Together with the gross shower variables like shower core…

Astrophysics · Physics 2007-05-23 T. Antoni

We have studied how the energy spectrum of muons at production affects some of the most common measurements related to muons in extensive air shower studies, namely, the number of muons at the ground, the slope of the lateral distribution…

High Energy Physics - Phenomenology · Physics 2016-11-28 J. Espadanal , L. Cazon , R. Conceição

Primary cosmic ray particles above energies of about 100 TeV are investigated by large-area ground based detector installations, observing various components of the development of extensive air-showers (EAS). By such an indirect access to…

Astrophysics · Physics 2008-11-26 A. Haungs

We present of measurements of radio emission from EAS at the frequency 32 MHz performed in 2008-2012. Showers were selected by zenith and azimuth directions, sampled by energy. A mean lateral distribution function was fitted to the data…

High Energy Astrophysical Phenomena · Physics 2013-09-27 S. Knurenko , I. Petrov

Ground-based cosmic ray experiments detect cosmic ray mainly by measuring the longitudinal and lateral distribution of secondary particles produced in the extensive air shower (EAS). The EAS of cosmic ray in the knee energy region is…

High Energy Astrophysical Phenomena · Physics 2024-09-30 Feng Zhang , Hu Liu , Fengrong Zhu , Jacob Oloketuyi

Lateral distributions for electrons and muons in extensive air showers measured with the array of the KASCADE experiment are compared to results of simulations based on the high-energy hadronic interaction models QGSJet and SIBYLL. It is…

Astrophysics · Physics 2008-11-26 KASCADE Collaboration , W. D. Apel

It is shown that Extensive Air Shower (EAS) longitudinal development has a critical point where an equilibrium between the main hadronic component and the secondary electromagnetic one exhibits a brake. This results in a change of slope in…

Astrophysics · Physics 2007-07-17 Yuri V. Stenkin

The paper concerns the so-called aligned events observed in cosmic rays. The phenomenon of the alignment of the most energetic subcores of gamma-ray--hadron ($\gamma-h$) families (particles of the highest energies in the central EAS core)…

High Energy Physics - Experiment · Physics 2008-11-26 A. L. Tsyabuk , R. A. Mukhamedshin , Yu. V. Stenkin

Recent results from the KASCADE extensive air shower experiment are presented. After briefly reviewing the status of the experiment we report on tests of hadronic interaction models and emphasize the progress being made in understanding the…

Astrophysics · Physics 2007-05-23 K. -H. Kampert , KASCADE-Collaboration

We put together the experimental results on muon component of extensive air showers (EAS) which were gained with various techniques at the detector complex of the Tien Shan mountain station. According to this comparison, the problem of the…

High Energy Astrophysical Phenomena · Physics 2021-08-24 A. Shepetov , S. Shaulov , O. Likiy , V. Ryabov , T. Sadykov , N. Saduev , V. Zhukov

In this work, the effects of the extensive air showers (EAS) were described by estimating the lateral distribution function (LDF) at very high energies of various cosmic ray particles. LDF was simulated for charged particles such as the…

High Energy Astrophysical Phenomena · Physics 2020-08-06 Hassanen Abdulhussaen Jassim , A. A. Al-Rubaiee , Iman Tarik Al-Alawy

The energy dependence of such characteristics as a ratio of the total number of charged particles to the total flux of EAS Cherenkov radiation, a ratio of E(thr)>=1GeV muon flux density at the distance of 600m from a shower core to charged…

Astrophysics · Physics 2007-11-15 S. P. Knurenko , A. V. Sabourov , I. Ye. Sleptsov

We report the analysis of the Ne-Nmuon coincident events collected by the MACRO/EAS-TOP collaboration at the Gran Sasso Laboratories. The result points to a primary composition becoming heavier around the knee of the primary spectrum (in…

Astrophysics · Physics 2007-05-23 The EAS-TOP , MACRO Collaborations

Purposeful investigation of radiation fluxes strongly delayed in relation to the main particles front of extensive air shower (EAS) was undertaken at the Tien Shan Mountain Cosmic Ray Station. It was found that the passage of the EAS can be…

Analyzing simulated extensive air shower (EAS) events generated with the Monte Carlo code CORSIKA, this paper critically studies the characteristics of lateral distribution of electrons in EAS around the knee energy region of the energy…

High Energy Astrophysical Phenomena · Physics 2016-11-15 Rajat K. Dey , Sandip Dam

New results of 300 hours of operation of the Tunka array are presented. An improved parametrization of the Cherenkov light lateral distribution function (LDF), based on CORSIKA Monte Carlo simulations and the experiment QUEST, has been used…

Measurements of electron, muon, and hadron lateral distributions of extensive air showers as recorded by the KASCADE experiment are presented. The data cover the energy range from about 5x10^14 eV up to almost 10^17 eV and extend from the…

Astrophysics · Physics 2008-11-26 T. Antoni
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