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Instruments and Methods for the Radio Detection of High Energy Cosmic Rays [electronic resource] / by Frank G. Schrȵder.

Por: Tipo de material: TextoTextoSeries Springer Theses, Recognizing Outstanding Ph.D. Research | Springer Theses, Recognizing Outstanding Ph.D. ResearchEditor: Berlin, Heidelberg : Springer Berlin Heidelberg : Imprint: Springer, 2012Descripción: XVIII, 190 p. online resourceTipo de contenido:
  • text
Tipo de medio:
  • computer
Tipo de soporte:
  • online resource
ISBN:
  • 9783642336607
Trabajos contenidos:
  • SpringerLink (Online service)
Tema(s): Formatos físicos adicionales: Sin títuloClasificación CDD:
  • 523.01 23
Clasificación LoC:
  • QB460-466
Recursos en línea:
Contenidos:
Springer eBooksResumen: Cosmic rays consist of elementary particles with enormous energy which originate from outside our solar system and constantly hit the Earths atmosphere. Where do these cosmic rays originate? How does nature accelerate the cosmic-ray particles to energies with orders of magnitude beyond the limits of manmade particle accelerators? What can we learn by measuring the interactions of the cosmic rays with the atmosphere? Digital radio-antenna arrays offer a promising, complementary measurement method for high-energy cosmic rays. This thesis reports on substantial advances in the development of the radio technique, which will be used to address these questions in future experiments.
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Cosmic Rays -- Radio Experiments for Air Shower Detection -- Time Calibration of LOPES -- A Reference Beacon for the Auger Engineering Radio Array -- Treatment of Noise -- Lateral Distribution -- Pulse Arrival Time Distributions.

Cosmic rays consist of elementary particles with enormous energy which originate from outside our solar system and constantly hit the Earths atmosphere. Where do these cosmic rays originate? How does nature accelerate the cosmic-ray particles to energies with orders of magnitude beyond the limits of manmade particle accelerators? What can we learn by measuring the interactions of the cosmic rays with the atmosphere? Digital radio-antenna arrays offer a promising, complementary measurement method for high-energy cosmic rays. This thesis reports on substantial advances in the development of the radio technique, which will be used to address these questions in future experiments.

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