3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
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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
- Mr. Hiroki MATSUMOTO (Okayama University of Science)
Co-authors
- Prof. Atsushi IYONO (Okayama University of Science)
- Ms. Maki MASUDA (Okayama University of Science)
- Prof. Isao YAMAMOTO (Okayama University of Science)
- Prof. Tomonori WADA (Okayama University)
- Dr. Kazuhide OKEI (Okayama University)
- Prof. Yasuhiko YAMASHITA (Okayama University)
- Dr. Syuhei TSUJI (Kawasaki Medical School)
- Prof. Takao NAKATSUKA (Okayama Shoka University)
- Dr. Nobuaki OCHI (Yonago National College of Technology)
Files
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