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astro-ph200881 cited

Dependence of geosynchrotron radio emission on the energy and depth of maximum of cosmic ray showers

T. Huege, R. Ulrich, R. Engel

Based on CORSIKA and REAS2 simulations, we investigate the dependence of geosynchrotron radio emission from extensive air showers on the energy of the primary cosmic ray and the de…

astro-ph200853 cited

Amplitude calibration of a digital radio antenna array for measuring cosmic ray air showers

S. Nehls, A. Hakenjos, M. J. Arts +9

Radio pulses are emitted during the development of air showers, where air showers are generated by ultra-high energy cosmic rays entering the Earth's atmosphere. These nanosecond s…

astro-ph2007

Radio Detection of Neutrinos from Behind a Mountain

O. Brusova, L. Anchordoqui, T. Huege +1

We explore the sensitivity of a neutrino detector employing strongly directional high gain radio antennae to detect the conversion of neutrinos above eV in a mountain or…

astro-ph2007

REAS2: CORSIKA-based Monte Carlo simulations of geosynchrotron radio emission

T. Huege, R. Ulrich, R. Engel

Simulations of geosynchrotron radio emission from extensive air showers performed with the Monte Carlo code REAS1 used analytical parameterisations to describe the spatial, tempora…

astro-ph2007

Energy and composition sensitivity of geosynchrotron radio emission from EAS

T. Huege, R. Ulrich, R. Engel

We analyse the sensitivity of geosynchrotron radio emission from inclined extensive air showers to the energy and mass of primary cosmic rays. We demonstrate that radio emission me…

astro-ph200667 cited

Monte Carlo simulations of geosynchrotron radio emission from CORSIKA-simulated air showers

T. Huege, R. Ulrich, R. Engel

We present simulations performed with REAS2, a new Monte Carlo code for the calculation of geosynchrotron radio emission from extensive air showers. The code uses thoroughly tested…