CHerenkov Detectors In Mine PitS
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CHerenkov Detectors In Mine PitS
Cherenkov (sometimes spelled Čerenkov or Cerenkov) is a common Russian surname, which may refer to: *Andrei Cherenkov (born 1976), Russian professional football manager and former player *Andrew Cherenkov, a fictional character in the video game ''Xenosaga Episode I'' *Fyodor Cherenkov (1959-2014), Soviet and Russian footballer *Pavel Alekseyevich Cherenkov (1904–1990), Soviet physicist and a recipient of the Nobel Prize in physics in 1958 See also

*Cherenkov Array at Themis, an atmospheric Cherenkov imaging telescope *Cherenkov detector, a particle detector **Ring-imaging Cherenkov detector *Cherenkov luminescence imaging *Cherenkov radiation, particular occurrence of electromagnetic radiation *Cherenkov Telescope Array, a multinational worldwide project *High Altitude Water Cherenkov Experiment *Imaging Atmospheric Cherenkov Technique *Radio Ice Cherenkov Experiment *Track Imaging Cherenkov Experiment * {{surname Russian-language surnames ...
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Andrei Cherenkov
Andrei Nikolayevich Cherenkov (; born 8 October 1976) is a Russian professional Association football, football manager and a former player. He is the manager of FC Zorkiy Krasnogorsk. Club career He made his debut for FC Rostselmash Rostov-on-Don on 12 September 1998 in a Russian Cup (football), Russian Cup game against FC Lada-Grad Dimitrovgrad. He made his second appearance for Rostselmash on 17 July 1999 in an 1999 UEFA Intertoto Cup, Intertoto Cup game against NK Varaždin (1931–2015), Varaždin. He played in the Russian Football National League for FC SKA-Energiya Khabarovsk in 2003. References

1976 births Living people Russian men's footballers Men's association football forwards FC Zhemchuzhina-Sochi players FC Rostov players FC SKA-Khabarovsk players FC Torpedo Minsk players FC Nika Krasny Sulin players FC Novokuznetsk players FC Dynamo Vologda players FC Smena Komsomolsk-na-Amure players Belarusian Premier League players Russian expatriate men's footballers Ex ...
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Andrew Cherenkov
''Xenosaga Episode I: Der Wille zur Macht'' is a role-playing video game developed by Monolith Soft and published by Namco for the PlayStation 2; the game was released in 2002 in Japan and 2003 in North America. It was never released in Europe. It is the first entry in the ''Xenosaga'' trilogy and forms part of the wider '' Xeno'' metaseries. Gameplay features exploration of environments through a linear narrative, while battles use turn-based combat with the player characters fighting both on foot and piloting large mecha dubbed A.G.W.S.; combat in turn features a system of button combinations for attack types, and multiple leveling systems. Set far in the future when humanity has left Earth, the plot follows Shion Uzuki, an employee of Vector Industries; and KOS-MOS, a battle android designed to fight the hostile alien Gnosis. Forced to escape a Gnosis attack and head for the planet of Second Miltia, Shion and KOS-MOS are pulled into a fight between the Galaxy Federation and the ...
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Fyodor Cherenkov
Fyodor Fyodorovich Cherenkov (; 25 July 1959 – 4 October 2014) was a Soviet and Russian football midfielder who played for Spartak Moscow (1977–90 and 1991–94) and Red Star Football Club (1990–91). Playing career Cherenkov played for Spartak Moscow for almost his entire professional club career (1977–1994; he also played for the youth team between 1971–1977), aside from a brief spell with Red Star Saint-Ouen from 1990–91. For the time spent in Spartak he received the Club Loyalty Award in 1989. He was awarded "The Attack Organizer" award in 1988 and 1989, as the most useful attack player. At international level, Cherenkov made 34 appearances for the Soviet Union national team, scoring 12 goals. He won a bronze medal at the 1980 Summer Olympics. Although widely regarded by Spartak's fans as the team's best player ever, he was always dropped by the national team on the eve of several major tournaments, including two World Cups and a European Championship. St ...
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Pavel Alekseyevich Cherenkov
Pavel Alekseyevich Cherenkov ( ; July 28, 1904 – January 6, 1990) was a Soviet physicist who shared the 1958 Nobel Prize in Physics with Ilya Frank and Igor Tamm "for the discovery and interpretation of the Cherenkov effect". Biography Cherenkov was born in 1904 to Alexey Cherenkov and Mariya Cherenkova in the small village of Novaya Chigla. This town is in present-day Voronezh Oblast, Russia. In 1928, he graduated from the Department of Physics and Mathematics of Voronezh State University. In 1930, he took a post as a senior researcher in the Lebedev Physical Institute. That same year he married Maria Putintseva, daughter of A.M. Putintsev, a Professor of Russian Literature. They had a son, Alexey, and a daughter, Yelena. Cherenkov was promoted to section leader, and in 1940 was awarded the degree of Doctor of Physico-Mathematical Sciences. In 1953, he was confirmed as Professor of Experimental Physics. Starting in 1959, he headed the institute's photo-meson processes ...
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Cherenkov Array At Themis
The Cherenkov Array at Themis (CAT) was an imaging atmospheric Cherenkov telescope (IACT) for detection of very-high-energy gamma rays (~200 GeV to a few tens of TeV). The project started operation in Autumn 1996 on the site of the former solar plant Thémis, France. References External linksCherenkov Array at Themis (CAT)on the internetTélescope de l'expérience CAT (Cerenkov array at Themis) sur le site de la centrale solaire THEMIS— photo of CAT CATat INSPIRE-HEP INSPIRE-HEP is an open access digital library for the field of high energy physics (HEP). It is the successor of the Stanford Physics Information Retrieval System (SPIRES) database, the main literature database for high energy physics since the 1 ... database * High energy particle telescopes {{observatory-stub ...
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Cherenkov Detector
A Cherenkov detector (pronunciation: /tʃɛrɛnˈkɔv/; Russian: Черенко́в) is a type particle detector designed to detect and identify particles by the Cherenkov Radiation produced when a charged particle travels through the medium of the detector. Fundamental A particle passing through a material at a velocity greater than that at which light can travel through the material emits light. This is similar to the production of a sonic boom when an airplane is traveling through the air faster than sound waves can move through the air. The direction this light is emitted is on a cone with angle θc about the direction in which the particle is moving, with cos(θc) =  (c = the vacuum speed of light, n = the refractive index of the medium, and v is the speed of the particle). The angle of the cone θc thus is a direct measure of the particle's speed. The Frank–Tamm formula gives the number of photons produced. Aspects Most Cherenkov detectors aim at recording the ...
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Ring-imaging Cherenkov Detector
The ring-imaging Cherenkov, or RICH, detector is a device for identifying the type of an electrically charged subatomic particle of known momentum, that traverses a transparent refractive medium, by measurement of the presence and characteristics of the Cherenkov radiation emitted during that traversal. RICH detectors were first developed in the 1980s and are used in high energy elementary particle-, nuclear- and astro-physics experiments. The RICH detector Origins The ring-imaging detection technique was first proposed by Jacques Séguinot and Tom Ypsilantis, working at CERN in 1977. Their research and development, of high precision single-photon detectors and related optics, lay the foundations for the design development and construction of the first large-scale Particle Physics RICH detectors, at CERN's OMEGA facility and LEP (Large Electron–Positron Collider) DELPHI experiment. Principles A ring-imaging Cherenkov (RICH) detector allows the identification of electr ...
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Cherenkov Luminescence Imaging
Cherenkov luminescence imaging (CLI) is an emerging imaging modality, similar to bioluminescence imaging, that captures visible photons emitted by Cherenkov radiation Cherenkov radiation () is electromagnetic radiation emitted when a charged particle (such as an electron) passes through a dielectric medium (such as distilled water) at a speed greater than the phase velocity (speed of propagation of a wavefro .... It basically is the optical imaging of radiotracers that emit charged particles traveling faster than the phase velocity of light in that particular medium. It can be used to quickly evaluate radio tracers in preclinical research but also to obtain clinical images in patients. While radioactivity itself can not be modified, the emitted light provides an opportunity to generate radioactivity-based activatable or "smart" imaging agents that sense for example enzymatic activity. References * External links * Imaging {{measurement-stub ...
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Cherenkov Radiation
Cherenkov radiation () is electromagnetic radiation emitted when a charged particle (such as an electron) passes through a dielectric medium (such as distilled water) at a speed greater than the phase velocity (speed of propagation of a wavefront in a medium) of light in that medium. A classic example of Cherenkov radiation is the characteristic blue glow of an underwater nuclear reactor. Its cause is similar to the cause of a sonic boom, the sharp sound heard when faster-than-sound movement occurs. The phenomenon is named after Soviet physicist Pavel Cherenkov. History The radiation is named after the Soviet scientist Pavel Cherenkov, the 1958 Nobel Prize winner, who was the first to detect it experimentally under the supervision of Sergey Vavilov at the Lebedev Institute in 1934. Therefore, it is also known as Vavilov–Cherenkov radiation. Cherenkov saw a faint bluish light around a radioactive preparation in water during experiments. His doctorate thesis was on lumin ...
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Cherenkov Telescope Array
The Cherenkov Telescope Array Observatory (CTAO) is a multinational project to build a new generation of ground-based gamma-ray instruments in the energy range extending from some tens of GeV to about 300 TeV. It is proposed as an open observatory and will consist of two arrays of imaging atmospheric Cherenkov telescopes, a first array at the Northern Hemisphere, on the Spanish island of La Palma, with emphasis on the study of extragalactic objects at the lowest possible energies, and a second array at the Southern Hemisphere, in the Atacama Desert in Chile, which is to cover the full energy range and concentrate on galactic sources. The physics program of the CTAO goes beyond high-energy astrophysics into cosmology and fundamental physics. Building on the technology of current-generation ground-based gamma-ray detectors ( MAGIC, HESS, and VERITAS), the CTAO will be ten times more sensitive and have unprecedented accuracy in its detection of high-energy gamma rays. Curr ...
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High Altitude Water Cherenkov Experiment
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 . HAWC is the successor to the Milagro gamma-ray observatory in New Mexico, which was also a gamma-ray observatory based around the principle of detecting gamma-rays indirectly using the water Cherenkov method. HAWC is a joint collaboration between a large number of American and Mexican universities and scientific institutions, including the University of Maryland, the National Autonomous University of Mexico, the National Institute of Astrophysics, Optics and Electronics, Los Alamos National Laboratory, NASA/Goddard Space Flight Center, the University of California, Santa Cruz, Michigan Technological University, Michigan State University, Benemérita Universidad Autónoma de Puebla, the Universidad de Guadalaja ...
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Imaging Atmospheric Cherenkov Technique
IACT (imaging atmospheric r airCherenkov telescope r technique is a device or method to detect very-high-energy gamma ray photons in the photon energy range of 50 GeV to 50  TeV. As of 2017, there are four operating IACT systems: High Energy Stereoscopic System (H.E.S.S.), Major Atmospheric Gamma Imaging Cherenkov Telescopes (MAGIC), First G-APD Cherenkov Telescope (FACT), and Very Energetic Radiation Imaging Telescope Array System (VERITAS). The Major Atmospheric Cerenkov Experiment Telescope (MACE) is under construction in Hanle, Ladakh, India and is set to be the highest and second-largest IACT. The Cherenkov Telescope Array (CTA) is a multinational project to build next-generation IACTs and is scheduled to begin data collection in 2022. Background Due to the rapidly falling flux of gamma-ray photons from cosmic sources in this energy regime, space-based detectors become ineffective due to their small collection areas which are often limited to some tens or hun ...
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