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pro vyhledávání: '"I Tsushima"'
Akademický článek
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Akademický článek
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Autor:
H. Aoki, K. Hashimoto, K. Honda, N. Inoue, N. Kawasumi, N. Martinic, C. Navia O, N. Ochi, N. Ohmori, A. Ohsawa, C. Oliveira, K. Shinozaki, M. Tamada, R. Ticona, I. Tsushima
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 151:223-226
An experiment using an air shower array, a hadron calorimeter and an emulsion chamber is under way at Mt. Chacaltaya (5200 m, Bolivia). One of the highest energy events, having a halo (∼ 1 cm) in the centre of the family together with many γ -ray
Autor:
H Aoki, K Hashimoto, K Honda, N Inoue, N Kawasumi, N Martinic, C Navia O, N Ochi, N Ohmori, A Ohsawa, L C Oliveira, K Shinozaki, M Tamada, R Ticona, I Tsushima
Publikováno v:
Journal of Physics G: Nuclear and Particle Physics. 30:137-155
A hybrid experiment to operate simultaneously an air shower array, a hadron calorimeter and an emulsion chamber is under way at Mt Chacaltaya (5200 m, Bolivia). An event with a halo, a blackened area of ~1 cm on x-ray film of the emulsion chamber, wa
Autor:
M. Tamada, I. Tsushima, K. Shinozaki, N. Kawasumi, N. Ohmori, R. Ticona, N. Inoue, C. E. Navia, N. Martinic, K. Honda, H. Aoki, L. C. Oliveira, Akinori Ohsawa, Keitaro Hashimoto
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 122:189-192
An experiment of an air shower array, a hadron calorimeter and an emulsion chamber is under way at Mt. Chacaltaya (5,200 m). Analysis of a halo event, detected by hybrid detectors, is presented. The data available for the event are on the halo ( E ha
Autor:
N. Kawasumi, Nobuyuki Sakurai, M. Sasaki, T. Yamamoto, H. Ohoka, Fumio Kakimoto, Michiyuki Chikawa, S. Mizobuchi, I. Tsushima, N. Inoue, M. Sasano, M. Nagano, K. Shinozaki, S. Kawakami, Naoaki Hayashida, K. Honda, R. Torii, S. Kawaguchi, H. Yoshii, Masaki Fukushima, K. Kamata, S. Osone, Yoshiya Kawasaki, Y. Morizane, Y. Uchihori, Ayman Mahrous, K. Kadota, K. Mase, R. A. Vázquez, S. Yoshida, Masahiro Takeda, Naoto Sakaki, Masahiro Teshima
Publikováno v:
The Astrophysical Journal. 571:L117-L120
The origin of the highest energy cosmic rays (≥1020 eV) is not well understood. Interesting models called "top-down" scenarios have been proposed to explain the origin. The γ-ray flux in ultra-high-energy cosmic rays is a key parameter for giving
Autor:
C. Aguirre, Akinori Ohsawa, R. Ticona, K. Honda, K. Shinozaki, N. Inoue, H. Aoki, Y. Maeda, Keitaro Hashimoto, I. Tsushima, N. Kawasumi, N. Ohmori, N. Martinic, M. Tamada
Publikováno v:
Nuclear Physics B - Proceedings Supplements. 97:158-161
An experiment of an air shower array, a hadron calorimeter (8 m 2 ) and an emulsion chamber (8 m 2 , 15 cm Pb) is under way at Mt. Chacaltaya (5200 m above sea level, Bolivia), in order to study the hadron interactions and the primary cosmic rays in
Observations of T[CLC]e[/CLC]V Gamma-Ray Flares from Markarian 501with the Telescope Array Prototype
Autor:
N. Hotta, M. Sasaki, K. Honda, M. Nagano, Naoaki Hayashida, Yoshihiko Mizumoto, Tetsuya T. Yamamoto, Jun Nishimura, Y. Yamamoto, H. Kitamura, Masaki Nishizawa, E. Kusano, H. Yoshii, H. Lafoux, M. Ohnishi, M. Chikawa, Y. Kawasaki, M. Sakata, T. Matsuyama, Y. Hayashi, Masahiro Teshima, S. Kabe, N. Chamoto, T. Sugiyama, S. F. Taylor, K. Sakumoto, S. Kawakami, T. Ouchi, N. Sakaki, S. Yoshida, Y. Uchihori, T. Yuda, H. Hirasawa, H. Shimodaira, T. Takahashi, N. Ito, To. Saito, R. Torii, H. Kuramochi, T. Kashiwagi, E. C. Loh, F. Kajino, N. Kawasumi, N. Inoue, M. Tsukiji, K. Mizutani, Pierre Sokolsky, H. Ohoka, I. Tsushima, A. Shiomi, D. Nishikawa, F. Ishikawa, K. Hibino, M. Sasano
Publikováno v:
The Astrophysical Journal. 504:L71-L74
We will report the observations of TeV gamma ray flares from Markarian 501 using Telescope Array Prototype. The observation were carried out continuously from the end of March to the end of July in 1997. The energy spectrum, and the time variation of
Publikováno v:
Physical Review D. 56:3833-3843
Autor:
H. Ohoka, I. Tsushima, Y. Uchihori, N. Kawasumi, K. Kadota, K. Honda, K. Murakami, Fumio Kakimoto, K. Kamata, Yutaka Matsubara, H. Yoshii, S. Yoshida, N. Inoue, Masahiro Teshima, M. Nagano, M. Takeda, Naoaki Hayashida, S. Kawaguchi, Morihiro Honda
Publikováno v:
Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment. 385:268-276
The data acquisition system of the Akeno Giant Air Shower Array (AGASA) is described. The AGASA array covers an area of about 100 km2 and has been operated since 1990 to study the origin of extremely high energy cosmic rays. In the early stage of our