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  • The Pierre Auger Observatory is designed for study of the universe's high energy particles, which evolve in the high layers of the atmosphere, where an elementary particle strikes with energy above 1019 eV (1.6 J!). However, there is no scientific consensus about cosmic ray origin. The Auger Observatory is projected to gather the data needed to solve that puzzle. One of the detection technique is to observe these showers by fluorescent detectors, which are able to record the cascade development where the secondary particle causes atmospheric nitrogen to fluoresce.
  • The Pierre Auger Observatory is designed for study of the universe's high energy particles, which evolve in the high layers of the atmosphere, where an elementary particle strikes with energy above 1019 eV (1.6 J!). However, there is no scientific consensus about cosmic ray origin. The Auger Observatory is projected to gather the data needed to solve that puzzle. One of the detection technique is to observe these showers by fluorescent detectors, which are able to record the cascade development where the secondary particle causes atmospheric nitrogen to fluoresce. (en)
  • Observatoř Pierre Auger je konstruována pro studium vysokoenergetických částic z vesmíru. Jeden ze dvou způsobů detekce je zaznamenávání vznikajících spršek částic pomocí fluorescenčních teleskopů, tyto detektory se skládají z optických teleskopů. Jako zobrazovací prvek je zde použito segmentované zrcadlo. V článku jsou prezentovány některé zkušenosti s měřením tloušťky krycí křemenné vrstvy. (cs)
Title
  • Some experience with testing of reflecting layers on mirrors for the project Pierre Auger
  • Zkušenosti s měřením reflexních vrstev u zrcadel používaných pro projekt Pierre Auger (cs)
  • Some experience with testing of reflecting layers on mirrors for the project Pierre Auger (en)
skos:prefLabel
  • Some experience with testing of reflecting layers on mirrors for the project Pierre Auger
  • Zkušenosti s měřením reflexních vrstev u zrcadel používaných pro projekt Pierre Auger (cs)
  • Some experience with testing of reflecting layers on mirrors for the project Pierre Auger (en)
skos:notation
  • RIV/68378271:_____/04:00021119!RIV06-AV0-68378271
http://linked.open.../vavai/riv/strany
  • 224;230
http://linked.open...avai/riv/aktivita
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  • P(LA 134), P(LN00A006), Z(AV0Z1010920)
http://linked.open...vai/riv/dodaniDat
http://linked.open...aciTvurceVysledku
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http://linked.open...dnocenehoVysledku
  • 586997
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  • RIV/68378271:_____/04:00021119
http://linked.open...riv/jazykVysledku
http://linked.open.../riv/klicovaSlova
  • reflecting layers; mirrors; Pierre Auger (en)
http://linked.open.../riv/klicoveSlovo
http://linked.open...ontrolniKodProRIV
  • [2A9E1FD5802E]
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  • Rožnov pod Radhoštěm
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  • Rožnov pod Radhoštěm
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  • SILICON 2004: The Ninth Scientific and Business Conference
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http://linked.open...UplatneniVysledku
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  • Boháčová, Martina
  • Hrabovský, Miroslav
  • Křepelka, Jaromír
  • Mandát, Dušan
  • Nožka, Libor
  • Palatka, Miroslav
  • Pech, Miroslav
  • Schovánek, Petr
  • Řídký, Jan
  • Rössler, T.
http://linked.open...vavai/riv/typAkce
http://linked.open.../riv/zahajeniAkce
http://linked.open...n/vavai/riv/zamer
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  • TECON Scientific
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