• DocumentCode
    1518488
  • Title

    A technique to produce mirrors for the Auger Observatory

  • Author

    Borreani, G. ; Cartiglia, N. ; Cester, R. ; de Capoa, A. ; de Oliveira, M.A.L. ; Marchetto, F. ; Maurizio, D. ; Pastrone, N.

  • Author_Institution
    Torino Univ., Italy
  • Volume
    48
  • Issue
    3
  • fYear
    2001
  • fDate
    6/1/2001 12:00:00 AM
  • Firstpage
    395
  • Lastpage
    399
  • Abstract
    The Fluorescence Detector of the Pierre Auger Cosmic Ray Observatory will provide a measurement of the parameters of extensive air showers with energy >1019 eV. The mirror of the Fluorescence Detector prototype has dimension ~3.6×3.6 m2 , and is composed of 49 trapezoidal segments of approximately 50×50 cm2. Each segment is curved using a steel mold in which the glass sags in a controlled environment. The glass is then aluminized under vacuum and coated with oxide (Al2O3 ). The oxide thickness is chosen to maximize the reflectivity in the wavelength range of fluorescence light (300 nm<λ<400 nm). The 49 mirror segments, plus eight spare ones, are now ready for installation. The authors discuss the production technique of the segments for the Torino prototype mirror
  • Keywords
    astronomical telescopes; cosmic ray apparatus; cosmic ray showers; mirrors; 1E19 eV; 300 to 400 nm; Al2O3; Al2O3 coating thickness; Fluorescence Detector; Pierre Auger Cosmic Ray Observatory; Torino prototype mirror; curved glass; extensive air showers; fluorescence light; installation; mirror production technique; mirror segments; reflectivity; steel mold; trapezoidal segments; Detectors; Energy measurement; Fluorescence; Glass; Mirrors; Observatories; Production; Prototypes; Reflectivity; Steel;
  • fLanguage
    English
  • Journal_Title
    Nuclear Science, IEEE Transactions on
  • Publisher
    ieee
  • ISSN
    0018-9499
  • Type

    jour

  • DOI
    10.1109/23.940087
  • Filename
    940087