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

Por: Schrȵder, Frank G [author.]Tipo de material: TextoTextoSeries 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 portador: online resourceISBN: 9783642336607Trabajos contenidos: SpringerLink (Online service)Tema(s): Physics | Physics | Astrophysics and Astroparticles | Particle and Nuclear PhysicsFormatos físicos adicionales: Sin títuloClasificación CDD: 523.01 Clasificación LoC:QB460-466Recursos en línea: de clik aquí para ver el libro electrónico
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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