First results of the air shower experiment KASCADE
| Autor: | A. Haungs, T. Antoni, W.D. Apel, F. Badea, K. Bekk, K. Bernlöhr, H. Blümer, E. Bollmann, H. Bozdog, I.M. Brancus, C. Büttner, A. Chilingarian, K. Daumiller, P. Doll, J. Engler, F. Feßler, H.J. Gils, R. Glasstetter, R. Haeusler, W. Hafemann, D. Heck, J.R. Hörandel, T. Holst, K.-H. Kampert, H. Keim, J. Kempa, H.O. Klages, J. Knapp, D. Martello, H.J. Mathes, P. Matussek, H.J. Mayer, J. Milke, D. Mühlenberg, J. Oehlschläger, M. Petcu, H. Rebel, M. Risse, M. Roth, G. Schatz, F.K. Schmidt, T. Thouw, H. Ulrich, A. Vardanyan, B. Vulpescu, J.H. Weber, J. Wentz, T. Wiegert, J. Wochelea, J. Zabierowski, S. Zagromski |
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| Přispěvatelé: | A., Haung, T., Antoni, W. D., Apel, F., Badea, K., Bekk, K., Bernlohr, H., Blumer, E., Bollmann, H., Bozdog, I. M., Brancu, C., Buttner, A., Chilingarian, K., Daumiller, P., Doll, J., Engler, F., Fessler, H. J., Gil, R., Glasstetter, R., Haeusler, W., Hafemann, D., Heck, J. R., Horandel, T., Holst, K. H., Kampert, H., Keim, J., Kempa, H. O., Klage, J., Knapp, Martello, Daniele, H. J., Mathe, P., Matussek, H. J., Mayer, J., Milke, D., Muhlenberg, J., Oehlschlager, M., Petcu, H., Rebel, M., Risse, M., Roth, G., Schatz, F. K., Schmidt, T., Thouw, H., Ulrich, A., Vardanyan, B., Vulpescu, J. H., Weber, J., Wentz, T., Wiegert, J., Wochele, J., Zabierowski, S., Zagromski |
| Jazyk: | angličtina |
| Rok vydání: | 2000 |
| Předmět: |
Physics
Nuclear and High Energy Physics Elemental composition Range (particle radiation) Physics::Instrumentation and Detectors Astrophysics::High Energy Astrophysical Phenomena Astrophysics (astro-ph) Detector Astrophysics::Instrumentation and Methods for Astrophysics FOS: Physical sciences Cosmic ray Astrophysics Atomic and Molecular Physics and Optics Nuclear physics Shower Air shower KASCADE Energy spectrum |
| Zdroj: | Scopus-Elsevier ResearcherID |
| Popis: | The main goals of the KASCADE (KArlsruhe Shower Core and Array DEtector) experiment are the determination of the energy spectrum and elemental composition of the charged cosmic rays in the energy range around the knee at ca. 5 PeV. Due to the large number of measured observables per single shower a variety of different approaches are applied to the data, preferably on an event-by-event basis. First results are presented and the influence of the high-energy interaction models underlying the analyses is discussed. 3 pages, 3 figures included, to appear in the TAUP 99 Proceedings, Nucl. Phys. B (Proc. Suppl.), ed. by M. Froissart, J. Dumarchez and D. Vignaud |
| Databáze: | OpenAIRE |
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