Radio Morphing: towards a fast computation of the radio signal from air showers

  title={Radio Morphing: towards a fast computation of the radio signal from air showers},
  author={Anne Zilles and Olivier Martineau-Huynh and Kumiko Kotera and Mat{\'i}as Tueros and K. D. de Vries and Washington Rodrigues de Carvalho and Valentin Niess and Nicolas Renault-Tinacci and Valentin Decoene},
  journal={Astroparticle Physics},

Synthesis of radio signals from extensive air showers using previously computed microscopic simulations

The detection of extensive air showers (EAS) through their radio signal is becoming one of the most promising techniques for the study of neutrinos and cosmic rays at the highest energies. For the

Radio-detection of neutrino-induced air showers: The influence of topography

  • V. DecoeneN. Renault-Tinacci A. Zilles
  • Physics
    Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment
  • 2021

Progress in the Simulation and Modelling of Coherent Radio Pulses from Ultra High-Energy Cosmic Particles

In the last decade, many experiments have been planned, designed or constructed to detect Ultra High Energy showers produced by cosmic rays or neutrinos using the radio technique. This technique

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 the

The Giant Radio Array for Neutrino Detection

The Giant Radio Array for Neutrino Detection (GRAND) is a planned array of ~ 2·105 radio antennas deployed over ~ 200 000 km2 in a mountainous site. It aims primarly at detecting high-energy

The Giant Radio Array for Neutrino Detection (GRAND) project

  • K. Kotera
  • Physics
    Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021)
  • 2021
GRAND is designed to detect ultra-high-energy cosmic particles – specially neutrinos, cosmic rays and gamma rays using radio antennas. With ∼ 20 mountainous sites around the world it will cover a

Carbon Footprint Study for the GRAND Project

We present a pioneering estimate of the global yearly greenhouse gas emissions of a large-scale Astrophysics experiment over several decades: the Giant Array for Neutrino Detection (GRAND). The

Design and Initial Performance of the Prototype for the BEACON Instrument for Detection of Ultrahigh Energy Particles

aDept. of Physics, Enrico Fermi Institute, Kavli Institute for Cosmological Physics, University of Chicago, Chicago, IL 60637, bDept. of Physics, Dept. of Astronomy and Astrophysics, Pennsylvania

Modeling and Validating RF-Only Interferometric Triggering with Cosmic Rays for BEACON

Department of Physics, Pennsylvania State University, State College, PA 16802, USA. Physics Department, California Polytechnic State University, San Luis Obispo, CA 93407, USA. Instituto Galego de



Radio detection of Cosmic-Ray Air Showers and High-Energy Neutrinos

Antennas for the detection of radio emission pulses from cosmic-ray induced air showers at the Pierre Auger Observatory

The Pierre Auger Observatory is exploring the potential of the radio detection technique to study extensive air showers induced by ultra-high energy cosmic rays. The Auger Engineering Radio Array

Analytic calculation of radio emission from parametrized extensive air showers: A tool to extract shower parameters

The radio intensity and polarization footprint of a cosmic-ray induced extensive air shower is determined by the time-dependent structure of the current distribution residing in the plasma cloud at

Results of a self-triggered prototype system for radio-detection of extensive air showers at the Pierre Auger Observatory

We describe the experimental setup and the results of RAuger, a small radio-antenna array, consisting of three fully autonomous and self-triggered radio-detection stations, installed close to the

Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy.

The radiation energy provides direct access to the calorimetric energy in the electromagnetic cascade of extensive air showers and allows the direct calibration of any cosmic-ray radio detector against the well-established energy scale of the Pierre Auger Observatory.

Coherent Radiation from Extensive Air Showers in the Ultra-High Frequency Band

Using detailed Monte Carlo simulations we have characterized the features of the radio emission of inclined air showers in the ultrahigh frequency band (300 MHz\char21{}3 GHz). The Fourier spectrum