Instruments and Methods for the Radio Detection of High Energy Cosmic Rays

Cosmic rays consist of elementary particles with enormous energy which originate from outside our solar system and constantly hit the Earth s atmosphere. Where do these cosmic rays originate? How does nature accelerate the cosmic-ray particles to energies with orders of magnitude beyond the limits o...

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Detalhes bibliográficos
Autor principal: Schröder, Frank G.
Formato: Livre numérique
Idioma:Anglais
Publicado em: Berlin, Heidelberg : Springer Berlin Heidelberg [20..].
Cham : Springer Nature
Edição:1st ed. 2012.
Colecção:Springer Theses, Recognizing Outstanding Ph.D. Research
Acesso em linha:Accès sur la plateforme de l'éditeur
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Accès Université d'Orléans
Accès INSA CVL
Nota: Archives Springer e-books (Licence nationale)
Archives Springer e-books (Licence nationale)
Autres localisations: Voir dans le Sudoc
Edition sous un autre format:• Instruments and methods for the radio detection of high energy cosmic rays, Frank G. Schröder, Berlin, Springer, 2012, 1 vol. (XVIII-188 p.), Springer theses, 978-3-642-33659-1
• Instruments and Methods for the Radio Detection of High Energy Cosmic Rays, Texte imprimé, 9783642336614
• Instruments and Methods for the Radio Detection of High Energy Cosmic Rays, Texte imprimé, 9783642448676
• Instruments and methods for the radio detection of high energy cosmic rays, Frank G. Schröder, Berlin, Springer, 2012, 1 vol. (XVIII-188 p.), Springer theses, 978-3-642-33659-1
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520 |a Cosmic rays consist of elementary particles with enormous energy which originate from outside our solar system and constantly hit the Earth s 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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