Skip to main navigation Skip to search Skip to main content

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

  • The Pierre Auger Collaboration
  • Université de Nantes
  • Université Joseph Fourier Grenoble
  • Instituto Superior Tecnico
  • Università di Torino and Sezione INFN
  • University of Wisconsin-Madison
  • Fermilab
  • University of São Paulo
  • CNEA-UNCuyo-CONICET
  • New York University
  • Ohio State University
  • UNSAM
  • Universidad Tecnológica Nacional
  • Universidad Nacional Autonoma de Mexico
  • Universidad de Santiago de Compostela
  • Universidade Estadual de Campinas
  • Università di Napoli 'Federico II' and Sezione INFN
  • Radboud University Nijmegen
  • University of Wisconsin-Milwaukee
  • Rudjer Boškovi'c Institute
  • Universidad Complutense de Madrid
  • Laboratoire de Physique Nucléaire et de Hautes Energies
  • IN2P3/ULP
  • Observatorio Pierre Auger and Comisión Nacional de Energía Atómica
  • University Politehnica of Bucharest
  • University of Adelaide
  • University of Maryland, College Park
  • Institut für Prozessdatenverarbeitung und Elektronik
  • Institut für Experimentelle Kernphysik (IEKP)
  • Bergische Universität Wuppertal
  • Max-Planck-Institut für Radioastronomie
  • Universidad de Alcalá

Research output: Contribution to journalArticlepeer-review

36 Scopus citations

Abstract

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 center of the Surface Detector (SD) of the Pierre Auger Observatory in Argentina. The setup has been designed for the detection of the electric field strength of air showers initiated by ultra-high energy cosmic rays, without using an auxiliary trigger from another detection system. Installed in December 2006, RAuger was terminated in May 2010 after 65 registered coincidences with the SD. The sky map in local angular coordinates (i.e., zenith and azimuth angles) of these events reveals a strong azimuthal asymmetry which is in agreement with a mechanism dominated by a geomagnetic emission process. The correlation between the electric field and the energy of the primary cosmic ray is presented for the first time, in an energy range covering two orders of magnitude between 0.1 EeV and 10 EeV. It is demonstrated that this setup is relatively more sensitive to inclined showers, with respect to the SD. In addition to these results, which underline the potential of the radio-detection technique, important information about the general behavior of self-triggering radio-detection systems has been obtained. In particular, we will discuss radio self-triggering under varying local electric-field conditions.

Original languageBritish English
Article numberP11023
JournalJournal of Instrumentation
Volume7
Issue number11
DOIs
StatePublished - 1 Nov 2012

Keywords

  • Antennas
  • Large detector systems for particle and astroparticle physics

Fingerprint

Dive into the research topics of 'Results of a self-triggered prototype system for radio-detection of extensive air showers at the Pierre Auger Observatory'. Together they form a unique fingerprint.

Cite this