Paper
3 March 2003 Focal surface for EUSO telescope
Hirohiko M. Shimizu, M. Ameri, F. Cadoux, Osvaldo Catalano, C. Chapron, S. Cuneo, Toshikazu Ebisuzaki, Flavio Fontanelli, Valerio Gracco, Philippe Gorodetzky, Yoshiya Kawasaki, P. Musico, Patric Nedelec, T. Patzak, M. Pallavicini, Alessandro Petrolini, E. Plagnol, F. Pratolongo, Mario Sannino, Naoto Sakaki, Yoshiyuki Takahashi, M. Takeda, Yoshiyuki Takizawa, Masahiro Teshima
Author Affiliations +
Abstract
The Extreme Universe Space Observatory (EUSO) is a wide angle refractive telescope in near-ultraviolet wavelength region to detect extremely high energy cosmic rays by observing time-resolved air-fluorescence images of the extensive air showers from the International Space Station. The focal surface detector of the EUSO is designed to be a mosaic of multianode photomultipliers to realize the single photoelectron counting capability. We describe the current status of the conceptual design and the feasibility study of the focal surface of the EUSO telescope.
© (2003) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Hirohiko M. Shimizu, M. Ameri, F. Cadoux, Osvaldo Catalano, C. Chapron, S. Cuneo, Toshikazu Ebisuzaki, Flavio Fontanelli, Valerio Gracco, Philippe Gorodetzky, Yoshiya Kawasaki, P. Musico, Patric Nedelec, T. Patzak, M. Pallavicini, Alessandro Petrolini, E. Plagnol, F. Pratolongo, Mario Sannino, Naoto Sakaki, Yoshiyuki Takahashi, M. Takeda, Yoshiyuki Takizawa, and Masahiro Teshima "Focal surface for EUSO telescope", Proc. SPIE 4858, Particle Astrophysics Instrumentation, (3 March 2003); https://doi.org/10.1117/12.458155
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KEYWORDS
Space telescopes

Telescopes

Photomultipliers

Photons

Atmospheric Cherenkov telescopes

Magnetism

Luminescence

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