Ultra High Energy Cosmic Rays
Observatories for ultra-high-energy cosmic rays:
- MARIACHI - Mixed Apparatus for Radar Investigation of Cosmic-rays of High Ionization located on Long Island, USA.
- GRAPES-3 (Gamma Ray Astronomy PeV EnergieS 3rd establishment) is a project for cosmic ray study with air shower detector array and large area muon detectors at Ooty in southern India.
- LOPES (telescope) - LOFAR PrototypE Station is located in Karlsruhe, Germany is part of the LOFAR project.
- AGASA - Akeno Giant Air Shower Array in Japan
- High Resolution Fly's Eye Cosmic Ray Detector (HiRes)
- Yakutsk Extensive Air Shower Array
- Pierre Auger Observatory
- Extreme Universe Space Observatory
- Telescope Array Project
- Antarctic Impulse Transient Antenna (ANITA) detects ultra-high-energy cosmic neutrinos believed to be caused by ultra-high-energy cosmic rays
- The COSMICi project at FAMU is developing technology for a distributed network of low-cost detectors for UHECR showers in collaboration with MARIACHI.
Read more about this topic: Cosmic-ray Observatory
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