Abstract
The KASCADE-Grande experiment measures extensive air showers induced by primary cosmic rays in the energy range 1014 – 1018 eV. The major motivation for KASCADE-Grande is the investigation of the so called ”knee” in the energy spectrum of cosmic rays and its presumed rigidity dependence. A short overview of the experimental setup with focus on the Grande array and its new data acquisition system is given. As an example of analysis the reconstruction of the total muon number is presented.
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References
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Brüggemann, M. et al. (2005). The Kascade-Grande experiment. In: Shapiro, M.M., Stanev, T., Wefel, J.P. (eds) Neutrinos and Explosive Events in the Universe. NATO Science Series, vol 209. Springer, Dordrecht. https://doi.org/10.1007/1-4020-3748-1_31
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DOI: https://doi.org/10.1007/1-4020-3748-1_31
Publisher Name: Springer, Dordrecht
Print ISBN: 978-1-4020-3746-7
Online ISBN: 978-1-4020-3748-1
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