D. Fuhrmann

Ankle-like feature in the energy spectrum of light elements of cosmic rays observed with KASCADE-Grande

Recent results of the KASCADE-Grande experiment provided evidence for a mild knee-like structure in the all-particle spectrum of cosmic rays at

On noise treatment in radio measurements of cosmic ray air showers

E = 10^{16.92 \pm 0.10} \, \mathrm{eV}

Comparing LOPES measurements of air-shower radio emission with REAS 3.11 and CoREAS simulations

, which was found to be due to a steepening in the flux of heavy primary particles. The spectrum of the combined components of light and intermediate masses was found to be compatible with a single power law in the energy range from

A test of the hadronic interaction model EPOS with air shower data

10^{16.3} \, \mathrm{eV}

Thunderstorm observations by air-shower radio antenna arrays

to

Cosmic ray measurements with LOPES: Status and recent results

10^{18} \, \mathrm{eV}

LOPES-3D: An antenna array for full signal detection of air-shower radio emission

. In this paper, we present an update of this analysis by using data with increased statistics, originating both from a larger data set including more recent measurements and by using a larger fiducial area. In addition, optimized selection criteria for enhancing light primaries are applied. We find a spectral feature for light elements, namely a hardening at

KASCADE-Grande Limits on the Isotropic Diffuse Gamma-Ray Flux between 100 TeV and 1 EeV

E = 10^{17.08 \pm 0.08} \, \mathrm{eV}

Probing the evolution of the EAS muon content in the atmosphere with KASCADE-Grande

with a change of the power law index from

Comparison of lopes measurements with coreas and reas 3.11 simulations

-3.25 \pm 0.05