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Influence of atmospheric electric fields on the radio emission from extensive air showers

  • T. N.G. Trinh
  • , O. Scholten
  • , S. Buitink
  • , A. M. Van Den Berg
  • , A. Corstanje
  • , U. Ebert
  • , J. E. Enriquez
  • , H. Falcke
  • , J. R. Hörandel
  • , C. Köhn
  • , A. Nelles
  • , J. P. Rachen
  • , L. Rossetto
  • , C. Rutjes
  • , P. Schellart
  • , S. Thoudam
  • , S. Ter Veen
  • , K. D. De Vries
  • KVI-Center for Advanced Radiation Technology
  • Interuniversity Institute for High Energies (ULB-VUB)
  • Vrije Universiteit Brussel
  • Radboud University Nijmegen
  • Science Park 123
  • Eindhoven University of Technology
  • NIKHEF
  • Netherlands Institute of Radio Astronomy (ASTRON)
  • Max-Planck-Institut für Radioastronomie
  • Technical University of Denmark
  • University of California-Irvine

Research output: Contribution to journalArticlepeer-review

21 Scopus citations

Abstract

The atmospheric electric fields in thunderclouds have been shown to significantly modify the intensity and polarization patterns of the radio footprint of cosmic-ray-induced extensive air showers. Simulations indicated a very nonlinear dependence of the signal strength in the frequency window of 30-80 MHz on the magnitude of the atmospheric electric field. In this work we present an explanation of this dependence based on Monte Carlo simulations, supported by arguments based on electron dynamics in air showers and expressed in terms of a simplified model. We show that by extending the frequency window to lower frequencies, additional sensitivity to the atmospheric electric field is obtained.

Original languageBritish English
Article number023003
JournalPhysical Review D
Volume93
Issue number2
DOIs
StatePublished - 19 Jan 2016

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