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Contribution Poster
The Focal Surface of the JEM-EUSO Telescope
Speakers
- Dr. Yoshiya KAWASAKI
Primary authors
- Dr. Yoshiya KAWASAKI (RIKEN)
Co-authors
- Prof. Hirokazu IKEDA (ISAS/JAXA)
- Dr. Tosikazu EBISUZAKI (RIKEN)
- Dr. Yosiyuki TAKIZAWA (RIKEN)
- Dr. Mario BERTAINA (Universita' di Torino)
- Dr. Mitsuteru SATO (RIKEN)
- Prof. Fumiyoshi KAJINO (Konan University)
- Mr. Toshiyuki SAWABE (Konan University)
- Dr. Philippe GORODETZKY (APC Paris)
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Abstract content
The Extreme Universe Space Observatory on JEM/EF (JEM-EUSO) is a space mission to study extremely high-energy cosmic rays. The JEM-EUSO instrument is a wide-angle refractive telescope in near-ultraviolet wavelength region to observe time-resolved atmospheric fluorescence images of the extensive air showers from the International Space Station. The focal surface is a spherical curved surface, and its area amounts to about 4.5 m2. The focal surface detector is covered with about 6,000 multi-anode photomultipliers (MAPMTs). The focal surface detector consists of Photo-Detector-Modules, each of which consists of 9 Elementary Cells (ECs). The EC contains 4 units of the MAPMTs. Therefore, about 1,500 ECs or about 160 PDMS are arranged on the whole of the focal surface of JEM- EUSO. The EC is a basic unit of the front-end electronics. The PDM is a basic unit of the data acquisition system.
If this papers is presented for a collaboration, please specify the collaboration
JEM-EUSO
Reference
Proceedings of the 30th International Cosmic Ray Conference; Rogelio Caballero, Juan Carlos D'Olivo, Gustavo Medina-Tanco, Lukas Nellen, Federico A. Sánchez, José F. Valdés-Galicia (eds.); Universidad Nacional Autónoma de México, Mexico City, Mexico, 2008; Vol. 5 (HE part 2), pages 1037-1040