Cherenkov Water Detectors in Particle Physics and Cosmic Rays
Abstract Among various types of Cherenkov detectors (solid, liquid and gaseous) created for different studies, the most impressive development was gained by water detectors: from the first detector with a volume of several liters in which the Cherenkov radiation was discovered, to the IceCube detect...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Petrukhin, A. A. [verfasserIn] Yashin, I. I. [verfasserIn] |
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| Format: |
E-Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2017 |
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| Schlagwörter: |
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| Übergeordnetes Werk: |
Enthalten in: Physics of atomic nuclei - New York, NY : AIP, 1996, 80(2017), 10 vom: Dez., Seite 1557-1566 |
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| Übergeordnetes Werk: |
volume:80 ; year:2017 ; number:10 ; month:12 ; pages:1557-1566 |
| Links: |
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| DOI / URN: |
10.1134/S1063778817110138 |
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| Katalog-ID: |
SPR019627408 |
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| 520 | |a Abstract Among various types of Cherenkov detectors (solid, liquid and gaseous) created for different studies, the most impressive development was gained by water detectors: from the first detector with a volume of several liters in which the Cherenkov radiation was discovered, to the IceCube detector with a volume of one cubic kilometer. The review of the development of Cherenkov water detectors for various purposes and having different locations − ground-based, underground and underwater–is presented in the paper. The prospects of their further development are also discussed. | ||
| 650 | 4 | |a Cherenkov radiation |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a Cherenkov water detectors |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a cosmic rays |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a neutrino telescopes |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a gamma-ray astronomy |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a muons |7 (dpeaa)DE-He213 | |
| 650 | 4 | |a extensive air showers |7 (dpeaa)DE-He213 | |
| 700 | 1 | |a Yashin, I. I. |e verfasserin |4 aut | |
| 773 | 0 | 8 | |i Enthalten in |t Physics of atomic nuclei |d New York, NY : AIP, 1996 |g 80(2017), 10 vom: Dez., Seite 1557-1566 |w (DE-627)312347936 |w (DE-600)2006377-5 |x 1562-692X |7 nnns |
| 773 | 1 | 8 | |g volume:80 |g year:2017 |g number:10 |g month:12 |g pages:1557-1566 |
| 856 | 4 | 0 | |u https://dx.doi.org/10.1134/S1063778817110138 |z lizenzpflichtig |3 Volltext |
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| allfields |
10.1134/S1063778817110138 doi (DE-627)SPR019627408 (SPR)S1063778817110138-e DE-627 ger DE-627 rakwb eng 530 ASE 33.40 bkl 33.50 bkl 39.22 bkl Petrukhin, A. A. verfasserin aut Cherenkov Water Detectors in Particle Physics and Cosmic Rays 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Among various types of Cherenkov detectors (solid, liquid and gaseous) created for different studies, the most impressive development was gained by water detectors: from the first detector with a volume of several liters in which the Cherenkov radiation was discovered, to the IceCube detector with a volume of one cubic kilometer. The review of the development of Cherenkov water detectors for various purposes and having different locations − ground-based, underground and underwater–is presented in the paper. The prospects of their further development are also discussed. Cherenkov radiation (dpeaa)DE-He213 Cherenkov water detectors (dpeaa)DE-He213 cosmic rays (dpeaa)DE-He213 neutrino telescopes (dpeaa)DE-He213 gamma-ray astronomy (dpeaa)DE-He213 muons (dpeaa)DE-He213 extensive air showers (dpeaa)DE-He213 Yashin, I. I. verfasserin aut Enthalten in Physics of atomic nuclei New York, NY : AIP, 1996 80(2017), 10 vom: Dez., Seite 1557-1566 (DE-627)312347936 (DE-600)2006377-5 1562-692X nnns volume:80 year:2017 number:10 month:12 pages:1557-1566 https://dx.doi.org/10.1134/S1063778817110138 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 ASE 33.50 ASE 39.22 ASE AR 80 2017 10 12 1557-1566 |
| spelling |
10.1134/S1063778817110138 doi (DE-627)SPR019627408 (SPR)S1063778817110138-e DE-627 ger DE-627 rakwb eng 530 ASE 33.40 bkl 33.50 bkl 39.22 bkl Petrukhin, A. A. verfasserin aut Cherenkov Water Detectors in Particle Physics and Cosmic Rays 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Among various types of Cherenkov detectors (solid, liquid and gaseous) created for different studies, the most impressive development was gained by water detectors: from the first detector with a volume of several liters in which the Cherenkov radiation was discovered, to the IceCube detector with a volume of one cubic kilometer. The review of the development of Cherenkov water detectors for various purposes and having different locations − ground-based, underground and underwater–is presented in the paper. The prospects of their further development are also discussed. Cherenkov radiation (dpeaa)DE-He213 Cherenkov water detectors (dpeaa)DE-He213 cosmic rays (dpeaa)DE-He213 neutrino telescopes (dpeaa)DE-He213 gamma-ray astronomy (dpeaa)DE-He213 muons (dpeaa)DE-He213 extensive air showers (dpeaa)DE-He213 Yashin, I. I. verfasserin aut Enthalten in Physics of atomic nuclei New York, NY : AIP, 1996 80(2017), 10 vom: Dez., Seite 1557-1566 (DE-627)312347936 (DE-600)2006377-5 1562-692X nnns volume:80 year:2017 number:10 month:12 pages:1557-1566 https://dx.doi.org/10.1134/S1063778817110138 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 ASE 33.50 ASE 39.22 ASE AR 80 2017 10 12 1557-1566 |
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10.1134/S1063778817110138 doi (DE-627)SPR019627408 (SPR)S1063778817110138-e DE-627 ger DE-627 rakwb eng 530 ASE 33.40 bkl 33.50 bkl 39.22 bkl Petrukhin, A. A. verfasserin aut Cherenkov Water Detectors in Particle Physics and Cosmic Rays 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Among various types of Cherenkov detectors (solid, liquid and gaseous) created for different studies, the most impressive development was gained by water detectors: from the first detector with a volume of several liters in which the Cherenkov radiation was discovered, to the IceCube detector with a volume of one cubic kilometer. The review of the development of Cherenkov water detectors for various purposes and having different locations − ground-based, underground and underwater–is presented in the paper. The prospects of their further development are also discussed. Cherenkov radiation (dpeaa)DE-He213 Cherenkov water detectors (dpeaa)DE-He213 cosmic rays (dpeaa)DE-He213 neutrino telescopes (dpeaa)DE-He213 gamma-ray astronomy (dpeaa)DE-He213 muons (dpeaa)DE-He213 extensive air showers (dpeaa)DE-He213 Yashin, I. I. verfasserin aut Enthalten in Physics of atomic nuclei New York, NY : AIP, 1996 80(2017), 10 vom: Dez., Seite 1557-1566 (DE-627)312347936 (DE-600)2006377-5 1562-692X nnns volume:80 year:2017 number:10 month:12 pages:1557-1566 https://dx.doi.org/10.1134/S1063778817110138 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 ASE 33.50 ASE 39.22 ASE AR 80 2017 10 12 1557-1566 |
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10.1134/S1063778817110138 doi (DE-627)SPR019627408 (SPR)S1063778817110138-e DE-627 ger DE-627 rakwb eng 530 ASE 33.40 bkl 33.50 bkl 39.22 bkl Petrukhin, A. A. verfasserin aut Cherenkov Water Detectors in Particle Physics and Cosmic Rays 2017 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier Abstract Among various types of Cherenkov detectors (solid, liquid and gaseous) created for different studies, the most impressive development was gained by water detectors: from the first detector with a volume of several liters in which the Cherenkov radiation was discovered, to the IceCube detector with a volume of one cubic kilometer. The review of the development of Cherenkov water detectors for various purposes and having different locations − ground-based, underground and underwater–is presented in the paper. The prospects of their further development are also discussed. Cherenkov radiation (dpeaa)DE-He213 Cherenkov water detectors (dpeaa)DE-He213 cosmic rays (dpeaa)DE-He213 neutrino telescopes (dpeaa)DE-He213 gamma-ray astronomy (dpeaa)DE-He213 muons (dpeaa)DE-He213 extensive air showers (dpeaa)DE-He213 Yashin, I. I. verfasserin aut Enthalten in Physics of atomic nuclei New York, NY : AIP, 1996 80(2017), 10 vom: Dez., Seite 1557-1566 (DE-627)312347936 (DE-600)2006377-5 1562-692X nnns volume:80 year:2017 number:10 month:12 pages:1557-1566 https://dx.doi.org/10.1134/S1063778817110138 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_SPRINGER SSG-OPC-AST SSG-OPC-ASE GBV_ILN_11 GBV_ILN_20 GBV_ILN_22 GBV_ILN_23 GBV_ILN_24 GBV_ILN_31 GBV_ILN_32 GBV_ILN_39 GBV_ILN_40 GBV_ILN_60 GBV_ILN_62 GBV_ILN_63 GBV_ILN_65 GBV_ILN_69 GBV_ILN_70 GBV_ILN_73 GBV_ILN_74 GBV_ILN_90 GBV_ILN_95 GBV_ILN_100 GBV_ILN_101 GBV_ILN_105 GBV_ILN_110 GBV_ILN_120 GBV_ILN_138 GBV_ILN_150 GBV_ILN_151 GBV_ILN_152 GBV_ILN_161 GBV_ILN_170 GBV_ILN_171 GBV_ILN_187 GBV_ILN_206 GBV_ILN_213 GBV_ILN_224 GBV_ILN_230 GBV_ILN_250 GBV_ILN_281 GBV_ILN_285 GBV_ILN_293 GBV_ILN_370 GBV_ILN_602 GBV_ILN_636 GBV_ILN_702 GBV_ILN_2001 GBV_ILN_2003 GBV_ILN_2004 GBV_ILN_2005 GBV_ILN_2006 GBV_ILN_2007 GBV_ILN_2008 GBV_ILN_2009 GBV_ILN_2010 GBV_ILN_2011 GBV_ILN_2014 GBV_ILN_2015 GBV_ILN_2020 GBV_ILN_2021 GBV_ILN_2025 GBV_ILN_2026 GBV_ILN_2027 GBV_ILN_2031 GBV_ILN_2034 GBV_ILN_2037 GBV_ILN_2038 GBV_ILN_2039 GBV_ILN_2044 GBV_ILN_2048 GBV_ILN_2049 GBV_ILN_2050 GBV_ILN_2055 GBV_ILN_2056 GBV_ILN_2057 GBV_ILN_2059 GBV_ILN_2061 GBV_ILN_2064 GBV_ILN_2065 GBV_ILN_2068 GBV_ILN_2070 GBV_ILN_2086 GBV_ILN_2088 GBV_ILN_2093 GBV_ILN_2106 GBV_ILN_2107 GBV_ILN_2108 GBV_ILN_2110 GBV_ILN_2111 GBV_ILN_2112 GBV_ILN_2113 GBV_ILN_2116 GBV_ILN_2118 GBV_ILN_2119 GBV_ILN_2122 GBV_ILN_2129 GBV_ILN_2143 GBV_ILN_2144 GBV_ILN_2147 GBV_ILN_2148 GBV_ILN_2152 GBV_ILN_2153 GBV_ILN_2188 GBV_ILN_2190 GBV_ILN_2232 GBV_ILN_2336 GBV_ILN_2446 GBV_ILN_2470 GBV_ILN_2472 GBV_ILN_2507 GBV_ILN_2522 GBV_ILN_2548 GBV_ILN_4035 GBV_ILN_4037 GBV_ILN_4046 GBV_ILN_4112 GBV_ILN_4125 GBV_ILN_4242 GBV_ILN_4246 GBV_ILN_4249 GBV_ILN_4251 GBV_ILN_4305 GBV_ILN_4306 GBV_ILN_4307 GBV_ILN_4313 GBV_ILN_4322 GBV_ILN_4323 GBV_ILN_4324 GBV_ILN_4325 GBV_ILN_4326 GBV_ILN_4333 GBV_ILN_4334 GBV_ILN_4335 GBV_ILN_4336 GBV_ILN_4338 GBV_ILN_4393 GBV_ILN_4700 33.40 ASE 33.50 ASE 39.22 ASE AR 80 2017 10 12 1557-1566 |
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| author |
Petrukhin, A. A. |
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Petrukhin, A. A. ddc 530 bkl 33.40 bkl 33.50 bkl 39.22 misc Cherenkov radiation misc Cherenkov water detectors misc cosmic rays misc neutrino telescopes misc gamma-ray astronomy misc muons misc extensive air showers Cherenkov Water Detectors in Particle Physics and Cosmic Rays |
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530 ASE 33.40 bkl 33.50 bkl 39.22 bkl Cherenkov Water Detectors in Particle Physics and Cosmic Rays Cherenkov radiation (dpeaa)DE-He213 Cherenkov water detectors (dpeaa)DE-He213 cosmic rays (dpeaa)DE-He213 neutrino telescopes (dpeaa)DE-He213 gamma-ray astronomy (dpeaa)DE-He213 muons (dpeaa)DE-He213 extensive air showers (dpeaa)DE-He213 |
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ddc 530 bkl 33.40 bkl 33.50 bkl 39.22 misc Cherenkov radiation misc Cherenkov water detectors misc cosmic rays misc neutrino telescopes misc gamma-ray astronomy misc muons misc extensive air showers |
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ddc 530 bkl 33.40 bkl 33.50 bkl 39.22 misc Cherenkov radiation misc Cherenkov water detectors misc cosmic rays misc neutrino telescopes misc gamma-ray astronomy misc muons misc extensive air showers |
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ddc 530 bkl 33.40 bkl 33.50 bkl 39.22 misc Cherenkov radiation misc Cherenkov water detectors misc cosmic rays misc neutrino telescopes misc gamma-ray astronomy misc muons misc extensive air showers |
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Cherenkov Water Detectors in Particle Physics and Cosmic Rays |
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Cherenkov Water Detectors in Particle Physics and Cosmic Rays |
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Petrukhin, A. A. |
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Physics of atomic nuclei |
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Petrukhin, A. A. Yashin, I. I. |
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verfasserin |
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cherenkov water detectors in particle physics and cosmic rays |
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Cherenkov Water Detectors in Particle Physics and Cosmic Rays |
| abstract |
Abstract Among various types of Cherenkov detectors (solid, liquid and gaseous) created for different studies, the most impressive development was gained by water detectors: from the first detector with a volume of several liters in which the Cherenkov radiation was discovered, to the IceCube detector with a volume of one cubic kilometer. The review of the development of Cherenkov water detectors for various purposes and having different locations − ground-based, underground and underwater–is presented in the paper. The prospects of their further development are also discussed. |
| abstractGer |
Abstract Among various types of Cherenkov detectors (solid, liquid and gaseous) created for different studies, the most impressive development was gained by water detectors: from the first detector with a volume of several liters in which the Cherenkov radiation was discovered, to the IceCube detector with a volume of one cubic kilometer. The review of the development of Cherenkov water detectors for various purposes and having different locations − ground-based, underground and underwater–is presented in the paper. The prospects of their further development are also discussed. |
| abstract_unstemmed |
Abstract Among various types of Cherenkov detectors (solid, liquid and gaseous) created for different studies, the most impressive development was gained by water detectors: from the first detector with a volume of several liters in which the Cherenkov radiation was discovered, to the IceCube detector with a volume of one cubic kilometer. The review of the development of Cherenkov water detectors for various purposes and having different locations − ground-based, underground and underwater–is presented in the paper. The prospects of their further development are also discussed. |
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Cherenkov Water Detectors in Particle Physics and Cosmic Rays |
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https://dx.doi.org/10.1134/S1063778817110138 |
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Yashin, I. I. |
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Yashin, I. I. |
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| doi_str |
10.1134/S1063778817110138 |
| up_date |
2024-07-04T02:22:12.381Z |
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|
| score |
7.401211 |