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Explanation
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INDEX
What's Cosmic Ray?
About Each Projects
About Each Projects

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Super-Kamiokande:
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Detection of neutrinos and search for proton decays in a large water tank

Cangaroo:
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Very high energy cosmic gamma ray observation at a desert in Australia

AGASA:
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Measurements of highest energy cosmic rays with a wide area AS detector

Tibet:
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Search for point sources of VHE cosmic gamma at Tibet heights

Telescope Array:
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Aiming at highest energy cosmic ray physics by detecting weak light from atmosphere

Gravitational Wave Group:
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R & D for detection of unknown phenomena 'gravitational waves'

SDSS:
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Making 3-D map of very distant galaxies with specific wide view telescopes as an international collaboration with Princeton University etc

Theory Group:
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Theoretical studies for verifying Grand Unified Theory and early Universe

Norikura:
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Various studies (e.g. of solar neutrons) utilizing high altitude of the location

Research Center for Cosmic Neutrinos:
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To explore new physics by merging worldwide information on cosmic neutrinos
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Copyright (C) 2000-2001 Institute for Cosmic Ray Research, University of Tokyo