Published July 2001 | Version v1
Journal article

Present experiment of BASJE group at Mt. Chacaltaya

  • 1. Ehime University, Dept. of Physics, Matsuyama, Ehime (Japan)
  • 2. Tokyo Institute of Technology, Dept. of Physics, Meguro, Tokyo (Japan)
  • 3. The Institute of Physics and Chemistry Research, Wako, Saitama (Japan)
  • 4. National Space Development Agency of Japan, Tsukuba, Ibaraki (Japan)
  • 5. Instituto de Investigaciones en Informatica, Universidad Mayor de San Andres, La Paz (Bolivia)
  • 6. Oayama University, Dept. of Physics, Okayama (Japan)
  • 7. Nagoya University of Foreign Studies, Nissin, Aichi (Japan)
  • 8. Fukui University of Technology, Faculty of General Education, Fukui (Japan)
  • 9. Solar-Terrestrial Environment Laboratory, Nagoya University, Nagoya, Aichi (Japan)
  • 10. National Astronomical Observatory, Mitaka, Tokyo (Japan)

Description

A compact air shower array to observe primary cosmic rays above a few TeV has been installed at Mt. Chacaltaya in Bolivia since 1996. This array is available to observe the air showers above 6 TeV and the longitudinal development curves above 50 TeV. The purpose of the observations is to study the chemical composition and the energy spectrum of cosmic rays in the energy region including the knee of the energy spectrum. First, the consistency between direct measurements (balloon-borne experiments) and air shower observations in the energy region from 50 TeV to 80 TeV is examined and confirmed. Next, the chemical composition and the energy spectrum are derived from the air shower observations. In the study, the longitudinal developments of shower particles are calculated by Monte Carlo simulations, assuming different chemical compositions above 80 TeV. The characteristics of the present air shower array and the comparison of the preliminary observed results with that of the simulations are presented

Additional details

Publishing Information

Journal Title
Nuovo Cimento. C
Journal Volume
24CS2
Journal Issue
4-5
Journal Page Range
p. 507-512
ISSN
0390-5551
CODEN
NIFCAS