EPJ Web of Conferences (Jan 2017)

Cosmic ray nuclei detection in the balloon borne nuclear emulsion gamma ray telescope flight in Australia (GRAINE 2015)

  • Iyono Atsushi,
  • Yamamoto Saya,
  • Aoki Shigeki,
  • Hara Toshio,
  • Kuretsubo Kenji,
  • Marushima Toshitsugu,
  • Matsumoto Haruka,
  • Mizutani Fukashi,
  • Ozaki Keita,
  • Shibayama Emi,
  • Suzuki Atsumu,
  • Takahashi Satoru,
  • Tateishi Yurie,
  • Yabu Misato,
  • Yamada Kyohei,
  • Kodama Koichi,
  • Hamada Kaname,
  • Kawahara Hiroaki,
  • Komatani Ryosuke,
  • Komatsu Masahiro,
  • Miyanishi Motoaki,
  • Morishita Misaki,
  • Morishima Kunihiro,
  • Nakamura Mitsuhiro,
  • Naganawa Naotaka,
  • Nanano Toshiyuki,
  • Nishio Akira,
  • Niwa Kimio,
  • Otsuka Naoto,
  • Rokujo Hiroki,
  • Sato Osamu,
  • Yoshimoto Masahiro

DOI
https://doi.org/10.1051/epjconf/201614506003
Journal volume & issue
Vol. 145
p. 06003

Abstract

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Nuclear emulsion plates for studying elementary particle physics as well as cosmic ray physics are very powerful tracking tools with sub-micron spatial resolutions of charged particle trajectories. Even if gamma rays have to be detected, electron-positron pair tracks can provide precise information to reconstruct their direction and energy with high accuracy. Recent developments of emulsion analysis technology can digitally handle almost all tracks recorded in emulsion plates by using the Hyper Track Selector of the OPERA group at NAGOYA University. On the other hand, the potential of time resolutions have been equipped by emulsion multilayer shifter technology in the GRAINE (Gamma Ray Astro-Imager with Nuclear Emulsion) experiments, the aims of which are to detect cosmic gamma rays such as the Vela pulsar stellar object by precise emulsion tracking analysis and to study cosmic ray particle interactions and chemical compositions. In this paper, we focus on the subject of cosmic ray nuclei detection in the GRAINE balloon flight experiments launched at Alice Springs, Australia in May 2015.