Main Research Projects Menu
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SuperKam
Cangaroo Group
AGASA Group
Tibet Division
Telescope Array Group
Gravitational Wave Group
SDSS Group
Theory Group
Norikura Observatory
RCCN
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What's Cosmic Ray?
About Each Projects
About Each Projects
Super-Kamiokande:
Detection of neutrinos and search for proton decays in a large water tank
Cangaroo:
Very high energy cosmic gamma ray observation at a desert in Australia
AGASA:
Measurements of highest energy cosmic rays with a wide area AS detector
Tibet:
Search for point sources of VHE cosmic gamma at Tibet heights
Telescope Array:
Aiming at highest energy cosmic ray physics by detecting weak light from atmosphere
Gravitational Wave Group:
R & D for detection of unknown phenomena 'gravitational waves'
SDSS:
Making 3-D map of very distant galaxies with specific wide view telescopes as an international collaboration with Princeton University etc
Theory Group:
Theoretical studies for verifying Grand Unified Theory and early Universe
Norikura:
Various studies (e.g. of solar neutrons) utilizing high altitude of the location
Research Center for Cosmic Neutrinos:
To explore new physics by merging worldwide information on cosmic neutrinos
Copyright (C) 2000-2001 Institute for Cosmic Ray Research, University of Tokyo