3-11 July 2007
Merida, Mexico
Mexico/General timezone
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Contribution Oral

Merida, Mexico - Yucatan II+III+IV (Fiesta Americana)
HE.1.1.A

The chemical composition of primary cosmic rays in the energy range ~10^15 eV from muon energy spectrum with the Okayama muon telescope

Speakers

  • Mr. Hiroki MATSUMOTO

Primary authors

Co-authors

Abstract content

The chemical composition of primary cosmic rays in the energy range ~10^15 eV are going to be examined from muon energy spectra using the AIRES simulation program. The muon energy spectra observed by the compact extensive air shower array and the solid iron magnet spectrometer are compared with simulation result.

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 39-42