First Experimental Characterization of Microwave Emission from Cosmic Ray Air Showers.

نویسندگان

  • R Smída
  • F Werner
  • R Engel
  • J C Arteaga-Velázquez
  • K Bekk
  • M Bertaina
  • J Blümer
  • H Bozdog
  • I M Brancus
  • A Chiavassa
  • F Cossavella
  • F Di Pierro
  • P Doll
  • B Fuchs
  • D Fuhrmann
  • C Grupen
  • A Haungs
  • D Heck
  • J R Hörandel
  • D Huber
  • T Huege
  • K-H Kampert
  • D Kang
  • H Klages
  • M Kleifges
  • O Krömer
  • K Link
  • P Luczak
  • M Ludwig
  • H J Mathes
  • S Mathys
  • H J Mayer
  • M Melissas
  • C Morello
  • P Neunteufel
  • J Oehlschläger
  • N Palmieri
  • J Pekala
  • T Pierog
  • J Rautenberg
  • H Rebel
  • M Riegel
  • M Roth
  • F Salamida
  • H Schieler
  • S Schoo
  • F G Schröder
  • O Sima
  • J Stasielak
  • G Toma
  • G C Trinchero
  • M Unger
  • M Weber
  • A Weindl
  • H Wilczyński
  • M Will
  • J Wochele
  • J Zabierowski
چکیده

We report the first direct measurement of the overall characteristics of microwave radio emission from extensive air showers. Using a trigger provided by the KASCADE-Grande air shower array, the signals of the microwave antennas of the Cosmic-Ray Observation via Microwave Emission experiment have been read out and searched for signatures of radio emission by high-energy air showers in the GHz frequency range. Microwave signals have been detected for more than 30 showers with energies above 3×10^{16}  eV. The observations presented in this Letter are consistent with a mainly forward-directed and polarized emission process in the GHz frequency range. The measurements show that microwave radiation offers a new means of studying air showers at E≥10^{17}  eV.

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عنوان ژورنال:
  • Physical review letters

دوره 113 22  شماره 

صفحات  -

تاریخ انتشار 2014