Radio emission from air showers measured with LOFAR

  • FOR THE LOFAR COLLABORATION

Research output: Chapter in Book/Report/Conference proceedingConference contributionpeer-review

1 Scopus citations

Abstract

The LOFAR cosmic ray experiment uniquely offers both the high antenna density and low radio frequency interference environment necessary to study the different processes within the air shower development that produce radio frequency emission. A detailed understanding of these processes allows radio emission measurements to be used to derive shower parameters such as Xmax. Here we will discuss the analysis and calibration methods used to reconstruct the full three-dimensional electric field vector at each of the ∼ 2300 antennas spread over an ∼ 4 km2 area in the LOFAR core. We will present the first high-precision measurements of the shape of the wavefront of the radio emission, as well as polarization measurements of the radio emission at different locations on the ground. These are an indicator of the interplay of different emission mechanisms such as Geomagnetic radiation, charge excess and the Askaryan effect, or Cherenkov effects.

Original languageBritish English
Title of host publicationProceedings of the 33rd International Cosmic Rays Conference, ICRC 2013
ISBN (Electronic)9788589064293
StatePublished - 2013
Event33rd International Cosmic Rays Conference, ICRC 2013 - Rio de Janeiro, Brazil
Duration: 2 Jul 20139 Jul 2013

Publication series

NameProceedings of the 33rd International Cosmic Rays Conference, ICRC 2013
Volume2013-October

Conference

Conference33rd International Cosmic Rays Conference, ICRC 2013
Country/TerritoryBrazil
CityRio de Janeiro
Period2/07/139/07/13

Keywords

  • Air showers
  • Cosmic rays
  • Experiments
  • LOFAR
  • Polarization
  • Radio detection

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