Number of the records: 1  

Detection of ultra-high energy cosmic ray showers with a single-pixel fluorescence telescope

  1. 1.
    0463937 - FZÚ 2021 RIV NL eng J - Journal Article
    Fujii, T. - Malacari, M. - Bertaina, M. - Casolino, E. - Dawson, B. - Horváth, P. - Hrabovský, M. - Jiang, J. - Mandát, Dušan - Matalon, A. - Matthews, J.N. - Motloch, P. - Palatka, Miroslav - Pech, Miroslav - Privitera, P. - Schovánek, Petr - Takizawa, Y. - Thomas, S.B. - Trávníček, Petr - Yamazaki, K.
    Detection of ultra-high energy cosmic ray showers with a single-pixel fluorescence telescope.
    Astroparticle Physics. Roč. 74, Feb (2016), s. 64-72. ISSN 0927-6505. E-ISSN 1873-2852
    R&D Projects: GA MŠMT(CZ) LG13007; GA MŠMT LM2015038
    Institutional support: RVO:68378271
    Keywords : ultra-high energy cosmic rays * fluorescence detector * extensive air shower
    OECD category: Particles and field physics
    Impact factor: 3.257, year: 2016
    Method of publishing: Limited access
    https://doi.org/10.1016/j.astropartphys.2015.10.006

    We present a concept for large-area, low-cost detection of ultra-high energy cosmic rays (UHECRs) with a Fluorescence detector Array of Single-pixel Telescopes (FAST), addressing the requirements for the next generation of UHECR experiments. In the FAST design, a large field of view is covered by a few pixels at the focal plane of a mirror or Fresnel lens. We report first results of a FAST prototype installed at the Telescope Array site, consisting of a single 200 mm photomultiplier tube at the focal plane of a 1 m(2) Fresnel lens system taken from the prototype of the JEM-EUSO experiment. The FAST prototype took data for 19 nights, demonstrating remarkable operational stability. We detected laser shots at distances of several kilometers as well as 16 highly significant UHECR shower candidates.
    Permanent Link: http://hdl.handle.net/11104/0263016

     
     
Number of the records: 1  

  This site uses cookies to make them easier to browse. Learn more about how we use cookies.