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All-particle cosmic ray energy spectrum in the 3-200 PeV energy range
Speakers
- Dr. R.M. MARTIROSOV
Primary authors
- Dr. R.M. MARTIROSOV (Yerevan Physics Institute)
Co-authors
- Dr. A.P. GARYAKA (Yerevan Physics Institute)
- Prof. S.V. TER-ANTONYAN (Yerevan Physics Institute)
- Prof. A.D. ERLYKIN (Moscow Lebedev Physical Institute)
- N.M. NIKOLSKAYA (Moscow Lebedev Physical Institute)
- Dr. Y.A GALLANT (University of Montpellier II)
- Prof. L.W. JONES (University of Michigan)
- Prof. J. PROCUREUR (University of Bordeaux)
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Abstract content
We present the all-particle primary cosmic ray energy spectrum obtained by a parametric event-by-event determination of the primary energy. The results are obtained on the basis of an expanded experimental data from the GAMMA experiment. The method was developed using the CORSIKA EAS simulation code with the SYBILL interaction model and taking into account the response of the GAMMA detectors and reconstruction uncertainties of the EAS parameters.
If this papers is presented for a collaboration, please specify the collaboration
GAMMA collaboration
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 4 (HE part 1), pages 119-122
