Number of the records: 1  

The Pierre Auger Observatory and its Upgrade

  1. 1.
    SYSNO ASEP0539340
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JOstatní články
    TitleThe Pierre Auger Observatory and its Upgrade
    Author(s) Aab, A. (NL)
    Abreu, P. (PT)
    Aglietta, M. (IT)
    Bakalová, Alena (FZU-D) ORCID
    Blažek, Jiří (FZU-D) ORCID, RID
    Boháčová, Martina (FZU-D) RID, ORCID
    Chudoba, Jiří (FZU-D) RID, ORCID
    Ebr, Jan (FZU-D) RID, ORCID
    Juryšek, Jakub (FZU-D) ORCID
    Mandát, Dušan (FZU-D) RID, ORCID
    Palatka, Miroslav (FZU-D) RID, ORCID, SAI
    Pech, Miroslav (FZU-D) RID, ORCID
    Prouza, Michael (FZU-D) RID, ORCID
    Řídký, Jan (FZU-D) RID, ORCID
    dos Santos, Eva M. Martins (FZU-D) ORCID
    Schovánek, Petr (FZU-D) RID, ORCID
    Tobiška, Petr (FZU-D) ORCID
    Trávníček, Petr (FZU-D) RID, ORCID
    Vícha, Jakub (FZU-D) RID, ORCID
    Yushkov, Alexey (FZU-D) ORCID
    Number of authors375
    Source TitleScience Reviews - from the end of the world. - : Centro de Estudios sobre Ciencia
    Roč. 1, č. 4 (2020), s. 8-33
    Number of pages26 s.
    Languageeng - English
    CountryAR - Argentina
    Keywordscosmic rays ; Pierre Auger Observatory
    Subject RIVBF - Elementary Particles and High Energy Physics
    OECD categoryParticles and field physics
    R&D ProjectsLTT18004 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    LM2018102 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    LM2015038 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    EF18_046/0016010 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    EF16_013/0001402 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    Method of publishingOpen access
    Institutional supportFZU-D - RVO:68378271
    AnnotationThe Pierre Auger Observatory was built to study cosmic rays of the highest energies. It is installed in the Departments of Malargue and San Rafael in the Province of Mendoza, Argentina. The Observatory is based on a hybrid design, comprised by two detector systems: a surface array of 1660 water Cherenkov detectors is complemented with 27 fluorescence telescopes which overlook the atmosphere above the surface array. Covering a total area in excess of 3000 km2, it is the largest and most precise observatory of its kind. It has been in full operation for over a decade now. In this article we review the objectives and design properties of the Pierre Auger Observatory, present its performance and the main scientific results obtained so far, and we describe the Upgrade that is well underway to enhance its capabilities for the next decade of measurements.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2021
    Electronic addresshttp://scirevfew.net/index.php/sciencereviews/issue/view/4/5
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