Large-Scale Cosmic-Ray Anisotropy with KASCADE
T. Antoni,W. D. Apel,A.F. Badea,K. Bekk,A. Bercuci,H. Blümer,H. Bozdog,I.M. Brancus,C. Büttner,Kai Daumiller,P. Doll,R. Engel,J. Engler,F. Fessler,H.J. Gils,R. Glasstetter,Andreas Haungs,D. Heck,Jörg R. Hörandel,Karl-Heinz Kampert,H.O. Klages,Gernot Maier,H. J. Mathes,H.J. Mayer,J. Milke,Marcio Aparecido Muller,R. Obenland,J. Oehlschläger,S. Ostapchenko,S. Ostapchenko,M. Petcu,H. Rebel,A. Risse,M. Risse,Markus Roth,G. Schatz,H. Schieler,J. Scholz,T. Thouw,H. Ulrich,J. van Buren,A. Vardanyan,A. Weindl,J. Wochele,J. Zabierowski +44 more
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TLDR
In this article, the results of an analysis of the large-scale anisotropy of cosmic rays in the PeV range were presented, and the Rayleigh formalism was applied to the right ascension distribution of extensive air showers measured by the KASCADE (Karlsruhe Shower Core and Array Detector) experiment.Abstract:
We present the results of an analysis of the large-scale anisotropy of cosmic rays in the PeV range. The Rayleigh formalism is applied to the right ascension distribution of extensive air showers measured by the KASCADE (Karlsruhe Shower Core and Array Detector) experiment. The data set contains about 108 extensive air showers in the energy range 0.7-6 PeV. No hints of anisotropy are visible in the right ascension distributions in this energy range. This accounts for all showers, as well as for subsets containing showers induced by predominantly light or heavy primary particles, respectively. Upper flux limits for Rayleigh amplitudes are determined to be between 10-3 at a primary energy of 0.7 PeV and 10-2 at 6 PeV.read more
Citations
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The end of the galactic cosmic-ray energy spectrum - a phenomenological view
TL;DR: In this paper, the poly gonato model is used to explain two structures in the all-particle energy spectrum of cosmic rays, the knee at 4.4 PeV and the second knee around 400 PeV.
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The end of the galactic cosmic-ray energy spectrum - a phenomenological view
TL;DR: In this article, the polygonato model is used to explain the second knee of the periodic table and the propagation path length of the cosmic ray at energies from 10 14 to 10 19 eV.
Book ChapterDOI
Primary Cosmic Radiation and Astrophysical Aspects
TL;DR: In this article, the authors briefly summarize the current situation of our knowledge of the primary cosmic radiation in the vicinity of the Earth, and discuss the high energy radiation that is responsible for air shower phenomena, whose composition and spectral features are still subject to debate.
Journal ArticleDOI
KASCADE-Grande: An overview and first results
M. E. Bertaina,W. D. Apel,J.C. Arteaga,F. Badea,K. Bekk,J. Blümer,H. Bozdog,I.M. Brancus,M. Brüggemann,Peter Buchholz,A. Chiavassa,F. Cossavella,Kai Daumiller,V. de Souza,F. Di Pierro,P. Doll,R. Engel,J. Engler,M. Finger,D. Fuhrmann,Piera Luisa Ghia,H.J. Gils,R. Glasstetter,Claus Grupen,A. Haungs,D. Heck,J.R. Hörandel,Tim Huege,Paula Gina Isar,K. H. Kampert,D. Kickelbick,H.O. Klages,Y. Kolotaev,P. Luczak,H. J. Mathes,H.J. Mayer,C. Meurer,J. Milke,B. Mitrica,A. Morales,C. Morello,G. Navarra,S. Nehls,J. Oehlschläger,S. Ostapchenko,S. Over,M. Petcu,T. Pierog,S. Plewnia,H. Rebel,Markus Roth,H. Schieler,Octavian Sima,M. Stümpert,G. Toma,G.C. Trinchero,H. Ulrich,J. van Buren,Wolfgang Walkowiak,A. Weindl,J. Wochele,J. Zabierowski +61 more
TL;DR: The KASCADE-Grande experiment as mentioned in this paper is a multi-component extensive air-shower experiment to study cosmic rays and their interactions at primary energies 10 14 −10 18 eV.
Journal ArticleDOI
A large area limited streamer tube detector for the air shower experiment KASCADE-Grande
TL;DR: In this article, the authors describe the technical layout and operation of the LST system, the methods and procedures for studying the characteristics and performance of this detector component, and the reconstruction of basic air shower (EAS) observables.
References
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CORSIKA: A Monte Carlo code to simulate extensive air showers
TL;DR: In this paper, the evolution of the information seeking and use models for professionals, essentially, the information access practices, is discussed. But two main categories can be distinguished : the informationseeking and use model versus the information retrieval model, and we will evaluate them in order to see if a convergence is possible with the same vocabulary and procedures.
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Journal ArticleDOI
The cosmic-ray experiment KASCADE
T. Antoni,W. D. Apel,F. Badea,K. Bekk,A. Bercuci,H. Blümer,H. Bozdog,I.M. Brancus,C. Büttner,Ashot Chilingarian,Kai Daumiller,P. Doll,J. Engler,F. Feßler,H.J. Gils,R. Glasstetter,R. Haeusler,Andreas Haungs,Dieter Heck,Jörg R. Hörandel,A. Iwan,Karl-Heinz Kampert,H.O. Klages,Gernot Maier,Hermann-Josef Mathes,H.J. Mayer,J. Milke,Marcio Aparecido Muller,R. Obenland,J. Oehlschläger,S. Ostapchenko,M. Petcu,H. Rebel,M. Risse,Markus Roth,G. Schatz,Harald Schieler,J. Scholz,T. Thouw,H. Ulrich,A. Vardanyan,J.H. Weber,A. Weindl,J. Wentz,J. Wochele,J. Zabierowski,S. Zagromski +46 more
TL;DR: The KASCADE experiment as mentioned in this paper was designed to measure air showers of primary cosmic-ray energies in the PeV region and to investigate the knee phenomenon in the all-particle energy spectrum.
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