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  2. Cherenkov detector - Wikipedia

    en.wikipedia.org/wiki/Cherenkov_detector

    Cherenkov threshold detectors have been used for fast timing and time of flight measurements in particle detectors. More elaborate designs use the amount of light produced. Recording light from both primary and secondary particles, for a Cherenkov calorimeter the total light yield is proportional to the incident particle energy.

  3. Neutrino detector - Wikipedia

    en.wikipedia.org/wiki/Neutrino_detector

    In a Cherenkov detector, a large volume of clear material such as water or ice is surrounded by light-sensitive photomultiplier tubes. A charged lepton produced with sufficient energy and moving through such a detector does travel somewhat faster than the speed of light in the detector medium (although somewhat slower than the speed of light in ...

  4. NEVOD - Wikipedia

    en.wikipedia.org/wiki/NEVOD

    NEVOD (Russian: НЕВОД, НЕйтринный ВОдный Детектор, Neutrino Water Detector; nevod means "dragnet" in Russian) is a neutrino detector and cosmic ray experiment that attempts to detect Cherenkov radiation arising from interactions between water and charged particles (mostly muons). It represents the first attempt to ...

  5. Accelerator Neutrino Neutron Interaction Experiment - Wikipedia

    en.wikipedia.org/wiki/Accelerator_Neutrino...

    The Accelerator Neutrino Neutron Interaction Experiment (ANNIE) is a water Cherenkov detector experiment designed to examine the nature of neutrino interactions. This experiment studies phenomena like proton decay, and neutrino oscillations, by analyzing neutrino interactions in gadolinium-loaded water and measuring their neutron yield.

  6. Cosmic-ray observatory - Wikipedia

    en.wikipedia.org/wiki/Cosmic-ray_observatory

    KASCADE-(Grande) – KArlsruhe Shower Core and Array DEtector (and its extension called 'Grande') Large High Altitude Air Shower Observatory; LOPES – the LOFAR PrototypE Station is the radio extension of KASCADE. TAIGA – Tunka Advanced Instrument for cosmic ray physics and Gamma Astronomy; HAWC High Altitude Water Cherenkov

  7. High Resolution Fly's Eye Cosmic Ray Detector - Wikipedia

    en.wikipedia.org/wiki/High_Resolution_Fly's_Eye...

    A follow-on experiment to the High Resolution Fly's Eye and Akeno Giant Air Shower Array (AGASA) experiments is the Telescope Array Project which began data collection in central Utah in 2007. A similar approach, but with the water-Cherenkov detectors, has been employed for the Pierre Auger Observatory which began collecting data in 2004.

  8. High Altitude Water Cherenkov Experiment - Wikipedia

    en.wikipedia.org/wiki/High_Altitude_Water...

    HAWC August 14, 2014 HAWC with the Pico de Orizaba in the background, August 2014. The High Altitude Water Cherenkov Experiment or High Altitude Water Cherenkov Observatory (also known as HAWC) is a gamma-ray and cosmic ray observatory located on the flanks of the Sierra Negra volcano in the Mexican state of Puebla at an altitude of 4100 meters, at

  9. Detection of internally reflected Cherenkov light - Wikipedia

    en.wikipedia.org/wiki/Detection_of_internally...

    In particle detectors a detection of internally reflected Cherenkov light (DIRC) detector measures the velocity of charged particles and is used for particle identification. It is a design of a ring imaging Cherenkov detector where Cherenkov light that is contained by total internal reflection inside the solid radiator has its angular ...