Browsing by Autor "I. Tsushima"
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Item type: Item , Análisis de la radiación gamma de UAE en el hemisferio sur(1995) R. Ticona; I. Poma; K. Honda; I. Tsushima; N Kawazumi; K. Hashimoto; T. MatanoItem type: Item , Combination of emulsion chamber and air shower array at Mt. Chacaltaya(American Institute of Physics, 1993) N. Kawasumi; I. Tsushima; Ken Honda; K. Hashimoto; Tsuneo Matano; K. Mori; Naoya Inoue; Rolando Ticona; Akinori Ohsawa; M. TamadaData of 34 familes with the accompanying air showers, observed by the combination of emulsion chamber and air shower array at Mt. Chacaltaya, are presented. Comparison with the simulation calculation concludes that a change is necessary in the characteristics of hadron interactions in E0≥1015 eV.Item type: Item , Simultaneous observation of families and accompanied air showers at Mt. Chacaltaya(American Physical Society, 1996) N. Kawasumi; I. Tsushima; K. Honda; K. Hashimoto; T. Matano; N. Inoue; K. Mori; A. Ohsawa; M. Tamada; N. OhmoriSimultaneous observations of families and accompanied air showers with emulsion chambers and the air shower array of electronic equipment at Mt. Chacaltaya (5200 m, 540 g/${\mathrm{cm}}^{2}$) reveal that families bear the data of nuclear interactions generated deep in the atmosphere. 47 outstanding families with \ensuremath{\Sigma}${\mathit{E}}_{\ensuremath{\gamma}}$\ensuremath{\ge}10 TeV are correlated with the accompanied air showers of the size ${10}^{5}$--${10}^{8}$. A scatter plot of the average family energy versus the size of the relative air shower requires further energy fractionizing process(es) in the propagation of high energy cosmic rays in the atmosphere, such as a larger dissipative mechanism in nuclear interaction, heavier chemical composition of the primary cosmic rays, etc. We reach the conclusion that nuclear interaction changes its features in the energy region ${\mathit{E}}_{0}$\ensuremath{\gtrsim}${10}^{16}$ eV, because the heavier composition, proposed so far, is not sufficient for the required dissipative process. A comparison with the data from the HADRON experiment at a similar altitude with a similar technique shows that no larger deviations are present between both experiments. \textcopyright{} 1996 The American Physical Society.Item type: Item , Simultaneous observation of families and accompanied air showers at Mt. Chacaltaya I(Elsevier BV, 1997) K. Honda; N. Kawasumi; I. Tsushima; K. Hashimoto; T. Nishida; T. Matano; N. Inoue; A. Ohsawa; M. Tamada; N. OhmoriItem type: Item , Simultaneous observation of families and associated air showers at Mt. Chacaltaya(Springer Nature, 1996) N. Kawasumi; I. Tsushima; K. Honda; K. Hashimoto; T. Matano; N. Inoue; K. Mori; K. Yokoi; A. Ohsawa; M. TamadaItem type: Item , Study of primary cosmic ray composition from gamma ray families in air shower cores(Elsevier BV, 1997) K. Honda; N. Kawasumi; I. Tsushima; K. Hashimoto; T. Nishida; T. Matano; N. Inoue; A. Ohsawa; M. Tamada; N. OhmoriItem type: Item , VHE gamma-rays with energies above 1014 eV observed at Mt.Chacaltaya(Elsevier BV, 1990) N. Inoue; T. Matano; K. Mori; K. Hashimoto; K. Honda; N. Kawasumi; I. Tsushima; Z. Aliaga; N. Martinić; A. ReguerínItem type: Item , What can we study through families and accompanied air showers?(Elsevier BV, 1999) T. Matano; T. Nishida; N. Kawasumi; I. Tsushima; K. Hashimoto; K. Honda; N. Inoue; K. Mori; A. Ohsawa; K. Yokoi