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A study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory

  1. 1.
    SYSNO ASEP0355247
    Document TypeJ - Journal Article
    R&D Document TypeJournal Article
    Subsidiary JČlánek ve WOS
    TitleA study of the effect of molecular and aerosol conditions in the atmosphere on air fluorescence measurements at the Pierre Auger Observatory
    Author(s) Abraham, J. (AR)
    Abreu, P. (AR)
    Aglietta, M. (AR)
    Boháčová, Martina (FZU-D) RID, ORCID
    Chudoba, Jiří (FZU-D) RID, ORCID
    Kárová, Tatiana (FZU-D)
    Mandát, Dušan (FZU-D) RID, ORCID
    Nečesal, Petr (FZU-D)
    Nožka, Libor (FZU-D) RID, ORCID
    Nyklíček, Michal (FZU-D)
    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
    Schovancová, Jaroslava (FZU-D)
    Schovánek, Petr (FZU-D) RID, ORCID
    Šmída, Radomír (FZU-D) RID
    Trávníček, Petr (FZU-D) RID, ORCID
    Number of authors18
    Source TitleAstroparticle Physics. - : Elsevier - ISSN 0927-6505
    Roč. 33, č. 2 (2010), s. 108-129
    Number of pages22 s.
    Languageeng - English
    CountryNL - Netherlands
    Keywordsathmospheric effects ; cosmic rays ; Pierre Auger Observatory
    Subject RIVBF - Elementary Particles and High Energy Physics
    R&D ProjectsLC527 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    1M06002 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    KJB100100904 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
    KJB300100801 GA AV ČR - Academy of Sciences of the Czech Republic (AV ČR)
    LA08016 GA MŠMT - Ministry of Education, Youth and Sports (MEYS)
    CEZAV0Z10100502 - FZU-D (2005-2011)
    AV0Z10100522 - FZU-D (2005-2011)
    UT WOS000275514800007
    DOI10.1016/j.astropartphys.2009.12.005
    AnnotationThe air fluorescence detector of the Pierre Auger Observatory is designed to perform calorimetric measurements of extensive air showers created by cosmic rays of above 1018 eV. The Observatory contains a group of monitoring instruments to record atmospheric conditions across the detector site, an area exceeding 3000 km2. The atmospheric data are used extensively in the reconstruction of air showers, and are particularly important for the correct determination of shower energies and the depths of shower maxima. This paper contains a summary of the molecular and aerosol conditions measured at the Pierre Auger Observatory since the start of regular operations in 2004, and includes a discussion of the impact of these measurements on air shower reconstructions. Between 1018 and 1020 eV, the systematic uncertainties due to all atmospheric effects increase from 4% to 8% in measurements of shower energy, and 4 g/cm-2 to 8 g/cm-2 in measurements of the shower maximum.
    WorkplaceInstitute of Physics
    ContactKristina Potocká, potocka@fzu.cz, Tel.: 220 318 579
    Year of Publishing2011
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