Results from recent analysis of KASCADE-Grande data

Author:

Kang Donghwa1,Arteaga-Velázquez Juan Carlos2,Bertaina M.3,Chiavassa Andrea3,Daumiller K.1,de Souza V.4,Engel R.1,Gherghel-Lascu A.5,Grupen C.6,Haungs A.1,Hörandel Jörg7,Huege Tim1,Kampert Karl-Heinz8,Link Katrin1,Mathes Hermann-Josef1,Ostapchenko Sergey9,Pierog Tanguy1,Rivera-Rangel David2,Roth M.1,Schieler H.1,Schröder Frank1,Sima O.10,Weindl A.1,Wochele J.1,Zabierowski J.11

Affiliation:

1. Karlsruhe Institute of Technology

2. Universidad Michoacana de San Nicolás de Hidalgo

3. University of Turin

4. University of Sao Paulo

5. Horia Hulubei National Institute for R and D in Physics and Nuclear Engineering

6. University of Siegen

7. Radboud University Nijmegen

8. University of Wuppertal

9. University of Hamburg

10. University of Bucharest

11. National Centre for Nuclear Research

Abstract

KASCADE and its extension array of KASCADE-Grande were devoted to measure individual air showers of cosmic rays in the primary energy range of 100 TeV to 1 EeV. The experiment has substantially contributed to investigate the energy spectrum and mass composition of cosmic rays in the transition region from galactic to extragalactic origin of cosmic rays as well as to quantify the characteristics of hadronic interaction models in the air shower development through validity tests using the multi-detector information from KASCADE-Grande. Although the data accumulation was completed in 2013, data analysis is still continuing. Recently, we investigated the reliability of the new hadronic interactions models of the SIBYLL version 2.3d only with the energy spectra from the KASCADE-Grande data. The evolution of the muon content of high energy air showers in the atmosphere is studied as well, using EPOS-LHC, SIBYLL 2.3, QGSJET-II-04 and SIBYLL 2.3c. In this talk, recent results from KASCADE-Grande and the update of the KASCADE Cosmic Ray Data Centre (KCDC) will be discussed.

Publisher

Stichting SciPost

Subject

General Medicine

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