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2002 Fiscal Year Final Research Report Summary

Study of Extremely High Energy Cosmic Rays beyond Greisen Cut off (10^<20>eV)

Research Project

Project/Area Number 12304012
Research Category

Grant-in-Aid for Scientific Research (A)

Allocation TypeSingle-year Grants
Section一般
Research Field 素粒子・核・宇宙線
Research InstitutionInstitute for Cosmic Ray Research, The University of Tokyo

Principal Investigator

HAYASHIDA Naoaki  Institute for Cosmic Ray Research, The University of Tokyo, Research Associate, 宇宙線研究所, 助手 (50114616)

Co-Investigator(Kenkyū-buntansha) YOSHIDA Shigeru  Faculty of Science, Chiba University, Associate Professor, 理学部, 助教授 (00272518)
TAKITA Masato  Institute for Cosmic Ray Research, The University of Tokyo, Associate Professor, 宇宙線研究所, 助教授 (20202161)
FUKUSHIMA Masaki  Institute for Cosmic Ray Research, The University of Tokyo, Professor, 宇宙線研究所, 教授 (30241227)
CHIKAWA Michiyuki  Science and Technology, Kinki University, Associate Professor, 理工学部, 助教授 (50179941)
Project Period (FY) 2000 – 2002
KeywordsCosmic ray / Cherenkov light / Fluorescence light / LIDAR system
Research Abstract

The Akeno Giant Air Shower Array (AGASA) has been operated for 12 years, then Extremely High Energy (EHE) cosmic ray events(11events) above Greisen cut off energy of 10^<20> eV were observed. Cosmic ray protons is believed to lose their energy by the pion production through the interaction with 2.7K microwave background radiation. EHE cosmic rays observed by AGASA clearly exceed this critical energy and is really interesting in its nature. In this project, to confirm the energy determination of AGASA, we have built air fluorescence imaging detector (CRIS ―― Cosmic Ray Imaging System) at the center of the Akeno Observatory.
In 2000 and 2001, we have build CRIS detector which cover 2 steradian around zenith and LIDAR system to monitor atmospheric transparency. The Lidar system has been successfully in operation since the winter of 2001, and the atmospheric monitoring at near UV region for cosmic ray measurement purpose was established. This result was already published in the journal, Nuclear Instrument and Method. In 2002, very intensive observation of 300 hrs in cherenkov mode was carried out, then we have observed more than 10,000 of high energy cosmic rays and studied the cosmic ray energy spectrum around the knee region (10^<14〜>10^<16>eV).

  • Research Products

    (8 results)

All Other

All Publications (8 results)

  • [Publications] K.Shinozaki et al.: "Upper Limit on Gamma-Ray Flux above 10^<19> eV Estimated by the Akeno Giant Air Shower Array Experiment"Astrophys J.. 571. L117-L120 (2002)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] T.Yamamoto et al.: "Development of Atmospheric Monitoring System at Akeno Observatory for the Telescope Array Project"Nucl. Instrum. Meth.. A488. 191-208 (2002)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] Y.Uchihori et al.: "Cluster analysis of extremely high energy cosmic rays in the northern sky"Astro Particle Physics. 13. 151-160 (2000)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] M.Takeda et al.: "Energy determination in the Akeno Giant Air Shower Array experiment"Astro Particle Physics astrop-ph/0209422. (掲載決定). (2003)

    • Description
      「研究成果報告書概要(和文)」より
  • [Publications] K.Shinozaki et al.: "Upper Limit on Gamma-Ray Flux above 10^<19> eV Estimated by the Adeno Giant Air Shower Array Experiment"Astrophysical J.. 571. L117-L120 (2002)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] T.Yamamoto et al.: "Development of Atmospheric Monitoring System at Akeno Observatory for the Telescope Array Project"Nucl.Instrum. & Meth.. A448. 191-208 (2002)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] Y.Uchihori et al.: "Cluster analysis of extremely high energy cosmic rays in the northern sky"Astro Particle Physics. 13. 151-160 (2000)

    • Description
      「研究成果報告書概要(欧文)」より
  • [Publications] M.Takeda et al.: "Energy determination in the Akeno Giant Air Shower Array experiment"To be published in Astro Particle Physics, asto-ph/0209422.

    • Description
      「研究成果報告書概要(欧文)」より

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Published: 2004-04-14  

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