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Abstrakty
We describe an unusual optical layout of the fluorescence detector telescope which is a part of the Pierre Auger Observatory. The fluorescence detector is a very fast telescope with the relative aperture fno ~ 0.77 and the large field of view 30×30 degrees. The primary objective for the Auger fluorescence telescope is to measure accurately the longitudinal development profiles of air showers of the cosmic rays above 10 EeV energy.
Słowa kluczowe
Czasopismo
Rocznik
Tom
Strony
445--456
Opis fizyczny
Bibliogr. 6 poz.
Twórcy
autor
- Joint Laboratory of Optics of Palacky University and Institute of Physics of the Academy of Sciences of the Czech Republic, 17 Listopadu 50,77207 Olomouc, Czech Republic
autor
- Joint Laboratory of Optics of Palacky University and Institute of Physics of the Academy of Sciences of the Czech Republic, 17 Listopadu 50,77207 Olomouc, Czech Republic
autor
- Joint Laboratory of Optics of Palacky University and Institute of Physics of the Academy of Sciences of the Czech Republic, 17 Listopadu 50,77207 Olomouc, Czech Republic
autor
- Joint Laboratory of Optics of Palacky University and Institute of Physics of the Academy of Sciences of the Czech Republic, 17 Listopadu 50,77207 Olomouc, Czech Republic
autor
- Institute of Physics of the Academy of Sciences of the Czech Republic, 17 Listopadu 50, 77207 Olomouc, Czech Republic
autor
- Institute of Physics of the Academy of Sciences of the Czech Republic, 17 Listopadu 50, 77207 Olomouc, Czech Republic
autor
- Institute of Physics of the Academy of Sciences of the Czech Republic, 17 Listopadu 50, 77207 Olomouc, Czech Republic
autor
- Institute of Physics of the Academy of Sciences of the Czech Republic, 17 Listopadu 50, 77207 Olomouc, Czech Republic
autor
- Institute of Physics of the Academy of Sciences of the Czech Republic, 17 Listopadu 50, 77207 Olomouc, Czech Republic
Bibliografia
- [1] The Pierre Auger Observatory - Design Report, 1997
- [2] Hrabovsky M., Pałatka M., Schovanek P., Grygar J., Ridky J., Soukup L., The optical analysis of the proposed Schmidt camera design. Auger technical note, GAP-99-25: www.auger.org/admin-cgi-bin-woda-gap_notes.pl.
- [3] Linfoot E.H., Recent Advances in Optics, Clarendon Press, Oxford 1955, pp. 202-208.
- [4] Pałatka M., Hrabovsky M., Schovanek P., Ridky J., Grygar J., Soukup L., Bifocal Optical System of the Schmidt Camera (Design of the Corrector Ring), Auger technical note, GAP-2000-002: www.auger.org/admin-cgi-bin-woda-gap_notes.pl.
- [5] Pałatka M., Hrabovsky M., Schovanek P., Ridky J., Grygar J., Soukup L., Analysis of Possible Substitution of the Aspheric Surface of the Corrector Annulus by the Shape with Simpler Production Technology, Auger technical note, GAP-2000-003: www.auger.org/admin-cgi-bin-woda-gap_notes.pl
- [6] SIGMA 2100, Optical Design Software, KIDGER OPTICS.
Typ dokumentu
Bibliografia
Identyfikator YADDA
bwmeta1.element.baztech-article-BPW1-0014-0031