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The Giant Radio Array for Neutrino Detection (GRAND): Science and design
The Giant Radio Array for Neutrino Detection (GRAND) is a planned large-scale observatory of ultra-high-energy (UHE) cosmic particles, with energies exceeding 108 GeV. Its goal is to solve theExpand
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Ultrahigh Energy Neutrinos at the Pierre Auger Observatory
The observation of ultrahigh energy neutrinos (UHE nu s) has become a priority in experimental astroparticle physics. UHE nu s can be detected with a variety of techniques. In particular, neutrinosExpand
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Techniques for measuring aerosol attenuation using the Central Laser Facility at the Pierre Auger Observatory
The Pierre Auger Observatory in Malargue, Argentina, is designed to study the properties of ultra-high energy cosmic rays with energies above 10(18) eV. It is a hybrid facility that employs aExpand
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The Giant Radio Array for Neutrino Detection (GRAND): Present and Perspectives
The Giant Radio Array for Neutrino Detection (GRAND) aims at detecting ultra-high energy extraterrestrial neutrinos via the extensive air showers induced by the decay of tau leptons created in theExpand
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Detection of Extensive Air Showers with the self-triggered TREND radio array
We demonstrate here the ability of TREND, a self-triggered antenna array, to autonomously detect and identify air showers induced by cosmic rays, from their radio emission, measured in the 50-100 MHzExpand
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Autonomous radio detection of air showers with the TREND50 antenna array
Abstract TREND50 is a radio detection setup of 50 self-triggered antennas working in the 50–100 MHz frequency range and deployed in a radio-quiet valley of the Tianshan mountains (China). TREND50Expand
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Radiodétection des gerbes atmosphériques à l'observatoire Pierre Auger
Les connaissances sur les rayons cosmiques d'ultra haute energie (E>10^{18} eV) ont progresse durant la derniere decennie, en particulier grâce aux resultats remarquables de l'Observatoire PierreExpand
The GRANDproto35 experiment
The very low flux of ultra-high-energy cosmic-rays (UHECRs) requires detectors with a large effective area and high duty cycle to obtain a statistically relevant sample. Radio detection of extensiveExpand
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The AMY experiment: Microwave emission from air shower plasmas
You The Air Microwave Yield (AMY) experiment investigate the molecular bremsstrahlung radiation emitted in the GHz frequency range from an electron beam induced air-shower. The measurements have beenExpand
Radio Morphing - towards a full parametrisation of the radio signal from air showers
Over the last decades, radio detection of air showers has been established as a detection technique for ultra-high-energy cosmic-rays impinging on the Earth's atmosphere with energies far beyond LHCExpand