activity
20052009
most citedDetection and imaging of atmospheric radio flashes from cosmic ray air showers

336 citations · 586 across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.HE2009★ 4 cited

Measurement of Radio Emission from Extensive Air Showers with LOPES

J. R. Hoerandel

A new method is explored to detect extensive air showers: the measurement of radio waves emitted during the propagation of the electromagnetic shower component in the magnetic fiel…

astro-ph.HE2009★ 1 cited

Investigation of the Properties of Galactic Cosmic Rays with the KASCADE-Grande Experiment

J. R. Hoerandel

The properties of galactic cosmic rays are investigated with the KASCADE-Grande experiment in the energy range between and eV. Recent results are discussed. The…

astro-ph.HE2009★ 1 cited

Test of hadronic interaction models with air shower data

J. R. Hoerandel

The description of high-energy hadronic interactions plays an important role in the (astrophysical) interpretation of air shower data. The parameter space important for the develop…

astro-ph.HE2009★ 78 cited

Lateral Distribution of the Radio Signal in Extensive Air Showers Measured with LOPES

LOPES Collaboration, W. D. Apel, J. C. Arteaga +71

The antenna array 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…

astro-ph2008★ 93 cited

Energy Spectra of Elemental Groups of Cosmic Rays: Update on the KASCADE Unfolding Analysis

KASCADE Collaboration, W. D. Apel

The KASCADE experiment measures extensive air showers induced by cosmic rays in the energy range around the so-called knee. The data of KASCADE have been used in a composition anal…

astro-ph2008★ 11 cited

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…

astro-ph2007★ 54 cited

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…

astro-ph2006★ 4 cited

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…

astro-ph2006★ 1 cited

Radio Emission in Atmospheric Air Showers: First Measurements with LOPES-30

P. G. Isar, S. Nehls, LOPES Collaboration

When Ultra High Energy Cosmic Rays interact with particles in the Earth's atmosphere, they produce a shower of secondary particles propagating toward the ground. LOPES-30 is an abs…

astro-ph2005★ 2 cited

Absolute calibration of the LOPES antenna system

S. Nehls, LOPES Collaboration

Radio emission in extensive air showers arises from an interaction with the geomagnetic field and is subject of theoretical studies. This radio emission has advantages for the dete…

astro-ph2005

Combined LOPES and KASCADE-Grande Data Analysis

A. Haungs, LOPES Collaboration

First analyses of coincident data of the LOPES (LOfar PrototypE Station) radio antennas with the particle air shower experiment KASCADE-Grande show basic correlations in the observ…

astro-ph2005★ 1 cited

Fluctuations in the EAS radio signal derived with improved Monte Carlo simulations based on CORSIKA

Tim Huege

Cosmic ray air showers are known to emit pulsed radio emission which can be understood as coherent geosynchrotron radiation arising from the deflection of electron-positron pairs i…

astro-ph2005★ 336 cited

Detection and imaging of atmospheric radio flashes from cosmic ray air showers

H. Falcke, W. D. Apel, A. F. Badea

The nature of ultrahigh-energy cosmic rays (UHECRs) at energies >10^20 eV remains a mystery. They are likely to be of extragalactic origin, but should be absorbed within ~50 Mpc th…