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  • The EUSO-Balloon pathfinder
    Allard, D.; Andreev, V.; Asano, K.; Barrillon, P.; Batsch, T.; Belenguer, T.; Bellotti, R.; Berlind, A. A.; Blaksley, C.; Błȩcki, J.; Bonamente, M.; Briz, S.; Bruno, A.; Cafagna, F.; Cassardo, C.; Catalano, C.; Catalano, G.; Csorna, S.; del Peral, L.; Dell’Oro, A.; Dupieux, M.; Falk, S.; Fernández-Gómez, I.; Flamini, M.; Fukushima, M.; Galeotti, P.; Gelmini, G.; Gorodetzky, P.; Guzmán, A.; Harlov, B.; Hernández Carretero, J.; Higashide, K.; Inoue, S.; Insolia, A.; Kajino, F.; Kajino, T.; Kawasaki, Y.; Khrenov, B. A.; Kim, J. -S.; Kreykenbohm, I.; Kusenko, A.; Licandro, J.; Lim, H.; López, F.; Mannheim, K.; Maravilla, D.; Matev, R.; Medina-Tanco, G.; Miyamoto, H.; Monnier-Ragaigne, D.; Nagataki, S.; Nakamura, T.; Neronov, A.; Nonaka, T.; Ogio, S.; Ohmori, H.; Olinto, A. V.; Osteria, G.; Pennypacker, C.; Picozza, P.; Pierog, T.; Pollini, A.; Prat, P.; Prieto, H.; Putis, M.; Reardon, P.; Ricci, M.; Rothkaehl, H.; Roudil, G.; Sabau, M. D.; Salazar, H.; Santiago Crúz, L.; Sanz Palomino, M.; Sato, M.; Schanz, T.; Segreto, A.; Sharakin, S.; Shibata, T.; Shimizu, H. M.; Shinozaki, K.; Shirahama, T.; Sledd, J.; Supanitsky, D.; Tajima, F.; Tajima, T.; Takizawa, Y.; Tibolla, O.; Tkachev, L.; Tomida, T.; Tone, N.; Tsuno, K.; Uchihori, Y.; Unger, M.; Valdés-Galicia, J. F.; Valore, L.; Vigorito, C.; Watts, J.; Wibig, T.; Włodarczyk, Z.; Zuccaro Marchi, A.

    Experimental astronomy, 11/2015, Letnik: 40, Številka: 1
    Journal Article

    EUSO-Balloon is a pathfinder for JEM-EUSO, the Extreme Universe Space Observatory which is to be hosted on-board the International Space Station. As JEM-EUSO is designed to observe Ultra-High Energy Cosmic Rays (UHECR)-induced Extensive Air Showers (EAS) by detecting their ultraviolet light tracks “from above”, EUSO-Balloon is a nadir-pointing UV telescope too. With its Fresnel Optics and Photo-Detector Module, the instrument monitors a 50 km 2 ground surface area in a wavelength band of 290–430 nm, collecting series of images at a rate of 400,000 frames/sec. The objectives of the balloon demonstrator are threefold: a) perform a full end-to-end test of a JEM-EUSO prototype consisting of all the main subsystems of the space experiment, b) measure the effective terrestrial UV background, with a spatial and temporal resolution relevant for JEM-EUSO. c) detect tracks of ultraviolet light from near space for the first time. The latter is a milestone in the development of UHECR science, paving the way for any future space-based UHECR observatory. On August 25, 2014, EUSO-Balloon was launched from Timmins Stratospheric Balloon Base (Ontario, Canada) by the balloon division of the French Space Agency CNES. From a float altitude of 38 km, the instrument operated during the entire astronomical night, observing UV-light from a variety of ground-covers and from hundreds of simulated EASs, produced by flashers and a laser during a two-hour helicopter under-flight.