B. Fuchs

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

The wavefront of the radio signal emitted by 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 comparison of the cosmic-ray energy scales of Tunka-133 and KASCADE-Grande via their radio extensions Tunka-Rex and LOPES

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

Cosmic ray measurements with LOPES: Status and recent results

to

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

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

Revised absolute amplitude calibration of the LOPES experiment

. 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

Comparison of lopes measurements with coreas and reas 3.11 simulations

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

LOPES — Recent Results and Open Questions on the Radio Detection of Air Showers

with a change of the power law index from

Reconstructing energy and Xmax of cosmic ray air showers using the radio lateral distribution measured with LOPES

-3.25 \pm 0.05