Radioelectric Field Features of Extensive Air Showers Observed with CODALEMA
arXiv:astro-ph/0608550 · doi:10.1016/j.astropartphys.2006.07.002
Abstract
Based on a new approach to the detection of radio transients associated with extensive air showers induced by ultra high energy cosmic rays, the experimental apparatus CODALEMA is in operation, measuring about 1 event per day corresponding to an energy threshold ~ 5. 10^16 eV. Its performance makes possible for the first time the study of radio-signal features on an event-by-event basis. The sampling of the magnitude of the electric field along a 600 meters axis is analyzed. It shows that the electric field lateral spread is around 250 m (FWHM). The possibility to determine with radio both arrival directions and shower core positions is discussed.
arXiv commentAccepted for publication in Astroparticle Physics
References in corpus (11)
- Extension of the Cosmic-Ray Energy Spectrum Beyond the Predicted Greisen-Zatsepin-Kuz'min Cutoff
- Detection of a Cosmic Ray with Measured Energy Well Beyond the Expected Spectral Cutoff due to Cosmic Microwave Radiation
- Detection and imaging of atmospheric radio flashes from cosmic ray air showers
- Detecting Radio Emission from Cosmic Ray Air Showers and Neutrinos with a Digital Radio Telescope
- Radio-Detection Signature of High Energy Cosmic Rays by the CODALEMA Experiment
- Radio emission from cosmic ray air showers: simulation results and parametrization
- Are vertical cosmic rays the most suitable to radio detection ?
- Recent Results from the RICE Experiment at the South Pole
- A prototype system for detecting the radio-frequency pulse associated with cosmic ray air showers
- The KASCADE-Grande Experiment and the LOPES Project
- Radio Pulses from Cosmic Ray Air Showers
Cited by in corpus (42)
- The Pierre Auger Cosmic Ray Observatory
- Cosmic Rays from the Knee to the Highest Energies
- Radio detection of Cosmic-Ray Air Showers and High-Energy Neutrinos
- Radio detection of cosmic ray air showers in the digital era
- A Macroscopic Description of Coherent Geo-Magnetic Radiation from Cosmic Ray Air Showers
- Energy Estimation of Cosmic Rays with the Engineering Radio Array of the Pierre Auger Observatory
- Measurement of the Radiation Energy in the Radio Signal of Extensive Air Showers as a Universal Estimator of Cosmic-Ray Energy
- Probing the radio emission from air showers with polarization measurements
- Geomagnetic origin of the radio emission from cosmic ray induced air showers observed by CODALEMA
- General description of electromagnetic radiation processes based on instantaneous charge acceleration in `endpoints'
- A Realistic Treatment of Geomagnetic Cherenkov Radiation from Cosmic Ray Air Showers
- Macroscopic Treatment of Radio Emission from Cosmic Ray Air Showers based on Shower Simulations
- Dependence of geosynchrotron radio emission on the energy and depth of maximum of cosmic ray showers
- Lateral Distribution of the Radio Signal in Extensive Air Showers Measured with LOPES
- Simulation of Radiation Energy Release in Air Showers
- The Lateral Distribution Function of Coherent Radio Emission from Extensive Air Showers; Determining the Chemical Composition of Cosmic Rays
- Monte Carlo simulations of geosynchrotron radio emission from CORSIKA-simulated air showers
- The TIANSHAN Radio Experiment for Neutrino Detection
- Accelerator measurements of magnetically-induced radio emission from particle cascades with applications to cosmic-ray air showers
- First Experimental Characterization of Microwave Emission from Cosmic Ray Air Showers
- Observation of Radar Echoes From High-Energy Particle Cascades
- Calibration of the Logarithmic-Periodic Dipole Antenna (LPDA) Radio Stations at the Pierre Auger Observatory using an Octocopter
- The cosmic-ray air-shower signal in Askaryan radio detectors
- The air shower maximum probed by Cherenkov effects from radio emission
- Frequency spectra of cosmic ray air shower radio emission measured with LOPES
- Monte Carlo simulations of air showers in atmospheric electric fields
- Macroscopic Model of Geomagnetic-Radiation from Air Showers
- Classification and Recovery of Radio Signals from Cosmic Ray Induced Air Showers with Deep Learning
- Macroscopic Geo-Magnetic Radiation Model; Polarization effects and finite volume calculations
- On the nature of radio-wave radiation from particle cascades
- Radiowave Detection of Ultra-High Energy Neutrinos and Cosmic Rays
- Feasibility of radar detection of extensive air showers
- Prospects for determining air shower characteristics through geosynchrotron emission arrival times
- Air Shower Measurements with the LOPES Radio Antenna Array
- The Radar Echo Telescope for Cosmic Rays: Pathfinder Experiment for a Next-Generation Neutrino Observatory
- Development of a radio-detection method array for the observation of ultra-high energy neutrino induced showers
- Design of a low noise, wide band, active dipole antenna for a cosmic ray radiodetection experiment
- Measurement of Radio Emission from Extensive Air Showers with LOPES
- First results from the FPGA/NIOS Adaptive FIR Filter Using Linear Prediction Implemented in the AERA Radio Stations to Reduce Narrow Band RFI for Radio Detection of Cosmic Rays
- Radio detection of cosmic ray air showers with LOPES
- Numerical Simulation of Radio Signal from Extended Air Showers
- Radio pulses from cosmic ray air showers - Boosted Coulomb and Cherenkov fields