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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

    Cherenkov radiation is produced whenever charged particles such as electrons or muons are moving through a given detector medium somewhat faster than the speed of light in that medium. In a Cherenkov detector, a large volume of clear material such as water or ice is surrounded by light-sensitive photomultiplier tubes.

  4. List of neutrino experiments - Wikipedia

    en.wikipedia.org/wiki/List_of_neutrino_experiments

    Cherenkov water detector NEVOD ATM, CR ν μ: ν μ + n → μ − + p ν μ + p → μ + + n: CC Water (H 2 O) Cherenkov: ≈2 GeV Moscow, Russia 1993– NEXT Neutrino Experiment with a Xenon Time Projection Chamber BB 136 Xe → 136 Ba + 2 e −: BB Gaseous Xenon Time projection chamber: ≈10 keV Canfranc, Spain 2016– NOνA: NuMI Off-Axis ...

  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. NEVOD - Wikipedia

    en.wikipedia.org/wiki/NEVOD

    NEVOD started operations in 1994 and was described in a journal in 1995, [3] and has since been used both for primary research and for educational purposes. [4] Since the start of NEVOD experiment's operation, many detectors have been added to the original Cherenkov detector, becoming the NEVOD experimental complex.

  7. Pierre Auger Observatory - Wikipedia

    en.wikipedia.org/wiki/Pierre_Auger_Observatory

    Surface detector (SD) station, or 'tank', of the Pierre Auger Observatory. In 1967 University of Leeds had developed a water-Cherenkov detector (or surface station; a small water basin, 1.2 m deep; also called tank) and created a 12 km 2 detection area Haverah Park using 200 such tanks. They were arranged in groups of four in a triangular (Y ...