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Sökning: WFRF:(Hörandel J. R.) > (2019)

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1.
  • Winchen, T., et al. (författare)
  • Cosmic ray physics with the LOFAR radio telescope
  • 2019
  • Ingår i: 26th Extended European Cosmic Ray Symposium, 6–10 July 2018, Altai State University, Barnaul-Belokurikha, Russian Federation. - : Institute of Physics (IOP). ; , s. 1-6
  • Konferensbidrag (refereegranskat)abstract
    • The LOFAR radio telescope is able to measure the radio emission from cosmic ray induced air showers with hundreds of individual antennas. This allows for precision testing of the emission mechanisms for the radio signal as well as determination of the depth of shower maximum X max , the shower observable most sensitive to the mass of the primary cosmic ray, to better than 20 g cm -2 . With a densely instrumented circular area of roughly 320 m 2 , LOFAR is targeting for cosmic ray astrophysics in the energy range 10 16 -10 18 eV. In this contribution we give an overview of the status, recent results, and future plans of cosmic ray detection with the LOFAR radio telescope. © Published under licence by IOP Publishing Ltd.
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2.
  • Winchen, T., et al. (författare)
  • Status of the lunar detection mode for cosmic particles of LOFAR
  • 2019
  • Ingår i: Journal of Physics. - : Institute of Physics (IOP). ; , s. 1-7
  • Konferensbidrag (refereegranskat)abstract
    • Cosmic particles hitting Earth's moon produce radio emission via the Askaryan effect. If the resulting radio ns-pulse can be detected by radio telescopes, this technique potentially increases the available collective area for ZeV scale particles by several orders of magnitude compared to current experiments. The LOw Frequency ARray (LOFAR) is the largest radio telescope operating in the optimum frequency regime for this technique. In this contribution, we report on the status of the implementation of the lunar detection mode at LOFAR. © Published under licence by IOP Publishing Ltd.
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