The status and capabilities of the KASCADE-Grande extensive air shower experiment are presented. The installation is located at Forschungszentrum Karisruhe and comprises a large collecting area (0.5 km^2) electromagnetic array (Grande) operated jointly with the existing KASCADE detectors. KASCADE-Grande will cover the primary energy range 10^16-10^18 eV overlapping with KASCADE around 10^16 eV, thus providing continuous information on the primary energy and mass of cosmic rays from 3.10^14 eV up to 10^18 eV. The major goal of the measurements is the unambiguous observation of the “iron knee” expected in the cosmic ray spectrum at Ek^Fe =10^17 eV.

Status of the KASCADE-Grande experiment

2003

Abstract

The status and capabilities of the KASCADE-Grande extensive air shower experiment are presented. The installation is located at Forschungszentrum Karisruhe and comprises a large collecting area (0.5 km^2) electromagnetic array (Grande) operated jointly with the existing KASCADE detectors. KASCADE-Grande will cover the primary energy range 10^16-10^18 eV overlapping with KASCADE around 10^16 eV, thus providing continuous information on the primary energy and mass of cosmic rays from 3.10^14 eV up to 10^18 eV. The major goal of the measurements is the unambiguous observation of the “iron knee” expected in the cosmic ray spectrum at Ek^Fe =10^17 eV.
2003
IFSI - Istituto di fisica dello spazio interplanetario
raggi cosmici
astroparticelle
spettro e
composizione
primaria
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/20.500.14243/453105
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