scholarly journals Hybrid Extensive Air Shower Detector Array at the University of Puebla to Study Cosmic Rays

2007 ◽  
pp. 243-251
Author(s):  
O. Martínez ◽  
E. Pérez ◽  
H. Salazar ◽  
L. Villaseñor
Keyword(s):  
Cosmic Rays ◽  
Detector Array ◽  
Extensive Air Shower ◽  
Air Shower ◽  
The University

Electronics for the Extensive Air Shower Detector Array at the University of Puebla

2006 ◽  
Author(s):  
E. Pérez ◽  
R. Conde ◽  
O. Martínez ◽  
T. Murrieta ◽  
H. Salazar ◽  
...  
Keyword(s):  
Detector Array ◽  
Extensive Air Shower ◽  
Air Shower ◽  
The University

scholarly journals Cosmic Ray Energy Spectrum derived from the Data of EAS Cherenkov Light Arrays in the Tunka Valley

2019 ◽  
Vol 210 ◽  
pp. 01003
Author(s):  
V. Prosin ◽  
I. Astapov ◽  
P. Bezyazeekov ◽  
A. Borodin ◽  
M. Brückner ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Energy Range ◽  
Cosmic Ray ◽  
Cherenkov Light ◽  
Differential Energy Spectrum ◽  
Extensive Air Shower ◽  
Air Shower

The extensive air shower Cherenkov light array Tunka-133 collected data during 7 winter seasons from 2009 to 2017. From 2175 hours of data taking, we derived the differential energy spectrum of cosmic rays in the energy range 6 · 1015 2 · 1018 eV. The TAIGA-HiSCORE array is in the process of continuous expansion and modernization. Here we present the results obtained with 28 stations of the first HiSCORE stage from 35 clear moonless nights in the winter of 2017-2018. The combined spectrum of two arrays covers a range of 2 · 1014 – 2 · 1018 eV.

scholarly journals THE EXTENSIVE AIR SHOWER EXPERIMENT KASCADE-GRANDE

2011 ◽  
Vol 01 ◽  
pp. 132-139
Author(s):  
DONGHWA KANG ◽  
W. D. APEL ◽  
J. C. ARTEAGA ◽  
F. BADEA ◽  
K. BEKK ◽  
...  
Keyword(s):  
Energy Spectrum ◽  
Cosmic Rays ◽  
Scintillation Detector ◽  
Array Detector ◽  
Extensive Air Shower ◽  
Air Shower ◽  
Muon Tracking ◽  
Tracking Devices ◽  
Combined Measurements ◽  
Scintillator Array

The extensive air shower experiment KASCADE-Grande (KArlsruhe Shower Core and Array DEtector and Grande array) is located on site of the Forschungszentrum Karlsruhe in Germany. The original KASCADE experiment consisted of a densely packed scintillator array with unshielded and shielded detectors for the measurement of the electromagnetic and muonic shower component independently, as well as muon tracking devices and a hadron calorimeter. The Grande array as an extension of KASCADE consists of 37 scintillation detector stations covering an area of 700×700 m2. The main goal for the combined measurements of KASCADE and Grande is the investigation of the energy spectrum and composition of primary cosmic rays in the energy range of 1016 to 1018 eV. In this paper an overview of the KASCADE-Grande experiment and recent results will be presented.

Estimation of mass composition of high energy cosmic rays via modeling a relation between lateral distribution parameters and shower age

2017 ◽  
Vol 26 (14) ◽  
pp. 1750161
Author(s):  
Saeed Doostmohammadi
Keyword(s):  
Cosmic Rays ◽  
Simulated Data ◽  
High Energy ◽  
Lateral Distribution ◽  
Mass Composition ◽  
Air Showers ◽  
Extensive Air Shower ◽  
High Energy Cosmic Rays ◽  
Air Shower ◽  
Distribution Parameters

Lateral distribution function of extensive air showers of energetic cosmic rays, indicate how secondary particles spread over a surface detectors. There are many different universal formulas between lateral distribution parameters and shower age parameter which can be used to infer about maximum development of extensive air shower (which is a key parameter to estimate the mass composition of primary cosmic rays). At present work, an estimated percent of mass composition of ultra-high energy cosmic rays is investigated by comparison between Ivanov et al. modeling of simulated data, which has been done by CoRSiKa, and Yakutsk experimental data.

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