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  2. Air shower (room) - Wikipedia

    en.wikipedia.org/wiki/Air_shower_(room)

    Air showers are typically placed between a gowning area and cleanroom; after workers don appropriate garb and personal protective equipment, they enter the shower so that the pressurized air nozzles remove any residual particles from coveralls. Once the program cycle is complete, users exit through a second door into the cleanroom.

  3. Air shower - Wikipedia

    en.wikipedia.org/wiki/Air_shower

    Air shower can refer to the following terms: Air shower (physics) , the shower of particles produced when a high energy cosmic ray hits an atom high in the atmosphere Air shower (room) , a specialized antechamber of a cleanroom

  4. Telescope Array Project - Wikipedia

    en.wikipedia.org/wiki/Telescope_Array_Project

    The experiment is designed to observe air showers induced by ultra-high-energy cosmic ray using a combination of ground array and air-fluorescence techniques. It is located in the high desert in Millard County, Utah, United States, at about 1,400 meters (4,600 ft) above sea level.

  5. Akeno Observatory - Wikipedia

    en.wikipedia.org/wiki/Akeno_Observatory

    Akeno Observatory features AGASA, the Akeno Giant Air Shower Array, which studies the origins of very high energy cosmic rays. [2] Construction of the observatory began in 1975, and in 1977 it became the second attached institution with ICRR.

  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. Pierre Auger Observatory - Wikipedia

    en.wikipedia.org/wiki/Pierre_Auger_Observatory

    When an air shower hits multiple Cherenkov Detectors on the ground, the direction of the ray can be calculated using basic geometrics. The longitudinal axis point can be determined from the densities in each affected ground station. Depending on the time difference of impact places, the angle of the axis can be determined. Only when the axis ...

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  9. Chicago Air Shower Array - Wikipedia

    en.wikipedia.org/wiki/Chicago_Air_Shower_Array

    The Chicago Air Shower Array (CASA) was a significant ultra high high-energy astrophysics experiment operating in the 1990s. It consisted of a very large array of scintillation detectors located at Dugway Proving Grounds in Utah , USA, approximately 80 kilometers southwest of Salt Lake City .