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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.
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 information preserved until it reaches the light sensors at the detector perimeter. The Cherenkov light is following a zigzag path between parallel surfaces. The light detectors would ...
This is a list of open-source hardware projects, including computer systems and components, cameras, radio, telephony, science education, machines and tools, robotics, renewable energy, home automation, medical and biotech, automotive, prototyping, test equipment, and musical instruments.
The ring-imaging detection technique was first proposed by Jacques Séguinot and Tom Ypsilantis, working at CERN in 1977. [1] Their research and development, of high precision single-photon detectors and related optics, lay the foundations for the design [2] [3] development [4] and construction of the first large-scale Particle Physics RICH detectors, at CERN's OMEGA facility [5] [6] [7] and ...
Gigaton Volume Detector S, ATM, LS, AGN, PUL ν e, ν μ, ν τ: CC, NC Water (H 2 O) Cherenkov: ≈10 GeV Lake Baikal, Russia 1993– BOREXINO: BORon EXperiment LS ν e: ν x + e − → ν x + e −: ES LOS shielded by water Scintillation: 250–665 keV Gran Sasso, Italy May 2007– BUST: Baksan Underground Scintillation Telescope Scintillation
A water detector is an electronic device that is designed to detect the presence of water for purposes such as to provide an alert in time to allow the prevention of water leakage. A common design is a small cable or device that lies flat on a floor and relies on the electrical conductivity of water to decrease the resistance across two contacts.
We also recommend installing additional carbon monoxide detectors about five to 20 feet from any sources of CO gas, like the furnace, water heater, or fireplace.
Although it was never completed, DUMAND was in a sense a precursor of the Antarctic Muon And Neutrino Detector Array (AMANDA), and the water Cherenkov neutrino telescopes in the Mediterranean (ANTARES, NEMO and the NESTOR Project). The DUMAND hardware was also donated to NESTOR, to reduce costs and cut on development and construction time. [2]