التفاصيل البيبلوغرافية
| العنوان: |
Cosmic ray nuclei detection in the balloon borne nuclear emulsion gamma ray telescope flight in Australia (GRAINE 2015). |
| المؤلفون: |
Atsushi Iyono, Saya Yamamoto, Shigeki Aoki, Toshio Hara, Kenji Kuretsubo, Toshitsugu Marushima, Haruka Matsumoto, Fukashi Mizutani, Keita Ozaki, Emi Shibayama, Atsumu Suzuki, Satoru Takahashi, Yurie Tateishi, Misato Yabu, Kyohei Yamada, Koichi Kodama, Kaname Hamada, Hiroaki Kawahara, Ryosuke Komatani, Masahiro Komatsu |
| المصدر: |
EPJ Web of Conferences; 2017, Vol. 145, p1-5, 5p |
| مصطلحات موضوعية: |
COSMIC rays, NUCLEAR emulsions, GAMMA rays, PHYSICS equipment, PARTICLE interactions |
| مستخلص: |
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. [ABSTRACT FROM AUTHOR] |
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| قاعدة البيانات: |
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