LOPES-3D, an antenna array for full signal detection of air-shower radio emission

Abstract

To better understand the radio signal emitted by extensive air-showers and to further develop the radio detection technique of high-energy cosmic rays, the LOPES experiment was reconfigured to LOPES-3D. LOPES-3D is able to measure all three vectorial components of the electric field of radio emission from cosmic ray air showers. The additional measurement of the vertical component ought to increase the reconstruction accuracy of primary cosmic ray parameters like direction and energy, provides an improved sensitivity to inclined showers, and will help to validate simulation of the emission mechanisms in the atmosphere. LOPES-3D will evaluate the feasibility of vectorial measurements for large scale applications. In order to measure all three electric field components directly, a tailor-made antenna type (tripoles) was deployed. The change of the antenna type necessitated new pre-amplifiers and an overall recalibration. The reconfiguration and the recalibration procedure are presented and the operationality of LOPES-3D is demonstrated.

References in corpus (8)

• Measurement of the energy spectrum of cosmic rays above 10^18 eV using the Pierre Auger Observatory
• Detection and imaging of atmospheric radio flashes from cosmic ray air showers
• Geomagnetic origin of the radio emission from cosmic ray induced air showers observed by CODALEMA
• New method for the time calibration of an interferometric radio antenna array
• Amplitude calibration of a digital radio antenna array for measuring cosmic ray air showers
• Frequency spectra of cosmic ray air shower radio emission measured with LOPES
• Radio detection of cosmic rays in the Pierre Auger Observatory
• Radio Detection of Particles from the Cosmos

Cited by in corpus (9)

• LOFAR: The LOw-Frequency ARray
• Radio detection of Cosmic-Ray Air Showers and High-Energy Neutrinos
• Radio detection of cosmic ray air showers in the digital era
• Measurement of cosmic-ray air showers with the Tunka Radio Extension (Tunka-Rex)
• Reconstruction of the energy and depth of maximum of cosmic-ray air-showers from LOPES radio measurements
• Observation of inclined EeV air showers with the radio detector of the Pierre Auger Observatory
• Design and Initial Performance of the Prototype for the BEACON Instrument for Detection of Ultrahigh Energy Particles
• Final results of the LOPES radio interferometer for cosmic-ray air showers
• A new basic air shower observable sensitive to the cosmic-ray elemental mass