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Air Shower Measurements with the LOPES Radio Antenna Array
A. Haungs
LOPES is set up at the location of the KASCADE-Grande extensive air shower experiment in Karlsruhe, Germany and aims to measure and investigate radio pulses from Extensive Air Show…
Data acquisition system for the TUNKA-133 array
N. M. Budnev, O. B. Chvalaev, O. A. Gress +19
The new EAS Cherenkov array TUNKA-133, with about 1 km**2 sensitive area, is being installed in the Tunka Valley. The investigated energy range is 10**15-10**18 eV. It will consist…
Tunka-133 EAS Cherenkov Array: Status of 2007
N. M. Budnev, O. V. Chvalaev, O. A. Gress +19
The new EAS Cherenkov array Tunka-133, with about 1 km**2 sensitive area, is being installed in the Tunka Valley since the end of 2005. This array will permit a detailed study of t…
Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei
The Pierre Auger Collaboration
Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival directions of the cosmic rays with the highest energies, which are correlated with the…
Amplified radio emission from cosmic ray air showers in thunderstorms
Stijn Buitink
Cosmic ray air showers produce radio emission, consisting in large part of geosynchrotron emission. Since the radiation mechanism is based on particle acceleration, the atmospheric…
Radio emission of highly inclined cosmic ray air showers measured with LOPES
Jelena Petrovic LOPES collaboration
LOPES-10 (the first phase of LOPES, consisting of 10 antennas) detected a significant number of cosmic ray air showers with a zenith angle larger than 50, and many of the…