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
Link To Document :
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