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Muon density measurements for the light and heavy mass groups of cosmic rays at the KASCADE-Grande observatory

Authors :
H. Bozdog
E. Cantoni
A. Weindl
M. E. Bertaina
J. Milke
S. Ostapchenko
H. J. Mathes
Claus Grupen
K. Bekk
J. C. Arteaga-Velázquez
T. Pierog
F.G. Schröder
P. Łuczak
D. Kang
H.O. Klages
J. Blümer
Ralph Engel
J. Oehlschläger
Markus Roth
H.J. Gils
G.C. Trinchero
V. de Souza
Kai Daumiller
D. Fuhrmann
G. Toma
Jörg R. Hörandel
C. Morello
B. Mitrica
R. Glasstetter
F. Cossavella
T. Huege
F. Di Pierro
K. H. Kampert
P. Doll
W. D. Apel
H. Rebel
S. Schoo
H. Schieler
Alexandru Gherghel-Lascu
A. Chiavassa
H.J. Mayer
K. Link
A. Haungs
J. Zabierowski
I.M. Brancus
J. Wochele
Octavian Sima
D. Heck
H. Ulrich
Source :
Nuclear and Particle Physics Proceedings. :152-157
Publication Year :
2017
Publisher :
Elsevier BV, 2017.

Abstract

KASCADE-Grande was an air-shower experiment aimed to investigate cosmic rays between 1016 and 1018 eV. The instrument was located at the site of the Karlsruhe Institute of Technology, Germany at an altitude of 110 m a.s.l. and covered an area of 0.5 km2. KASCADE-Grande consisted of several detector systems dedicated to measure different components of the cosmic ray induced air showers, e.g. the muon content (Eth > 230 MeV) and the number of charged particles (Eth > 3 MeV) at ground, which are the basis for several energy and composition studies of cosmic rays. In this contribution, using these observables, the KASCADE-Grande data is divided into light and heavy mass groups and their respective muon densities are reconstructed at different zenith angle intervals. The results are compared with the expectations of the post-LHC hadronic-interaction models, EPOS-LHC and QGSJET-II-04, in order to test the validity of the model predictions.

Details

ISSN :
24056014
Database :
OpenAIRE
Journal :
Nuclear and Particle Physics Proceedings
Accession number :
edsair.doi.dedup.....79b46e7a3e954228c532a7f9707fe903
Full Text :
https://doi.org/10.1016/j.nuclphysbps.2017.06.030