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Abstract
Abstract
KASCADE (KArlsruhe Shower Core and Array DEtector) is determining flux spectra for different primary mass groups to disentangle the knee feature of the primary cosmic-ray energy spectrum. The energy spectra of the light element groups result in a knee-like bending and a steepening above the knee. The topology of the individual knee positions suggests a rigidity dependence. To proof the rigidity dependence the KASCADE array is now extended by a factor 10 in area. The major goal of KASCADE-Grande is the observation of the ’iron-knee’ in the cosmic-ray spectrum at around 100 PeV which is expected following the KASCADE observations.
PACS: 98.70.Sa Cosmic rays
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1 Institut für Kernphysik, Forschungszentrum Karlsruhe, 76021 Karlsruhe, Germany
2 Fachbereich Physik, Universität Wuppertal, 42097 Wuppertal, Germany
3 Institut für Experimentelle Kernphysik, Universität Karlsruhe, 76021 Karlsruhe, Germany
4 Dipartimento di Fisica Generale dell’Università, 10125 Torino, Italy
5 Institut für Experimentelle Kernphysik, Universität Karlsruhe, 76021 Karlsruhe, Germany; Institut für Kernphysik, Forschungszentrum Karlsruhe, 76021 Karlsruhe, Germany
6 National Institute of Physics and Nuclear Engineering, 7690 Bucharest, Romania
7 Fachbereich Physik, Universität Siegen, 57072 Siegen, Germany
8 Cosmic Ray Division, Yerevan Physics Institute, Yerevan 36, Armenia
9 Istituto di Fisica dello Spazio Interplanetario, CNR, 10133 Torino, Italy
10 Soltan Institute for Nuclear Studies, 90950 Lodz, Poland





