First results obtained by RUNJOB compaign

E. Kamioka, A. V. Apanasenko, V. A. Berezovskaya, M. Fujii, T. Fukuda, M. Hareyama, G. Hashimoto, M. Ichimura, T. Kobayashi, V. Kopenkin, S. Kuramata, V. I. Lapshin, A. K. Managadze, H. Matsutani, N. P. Misnikova, T. Misu, R. A. Mukhamedshin, A. Nakamura, M. Namiki, H. NanjoS. I. Nikolsky, K. Ogura, S. Ohta, D. S. Oshuev, P. A. Publichencko, I. V. Rakobolskaya, T. M. Roganova, G. P. Sazhina, H. Semba, T. Shibata, T. Shiota, H. Sugimoto, L. G. Sveshnikova, V. M. Taran, Z. Watanabe, N. Yajima, T. Yamagami, I. V. Yashin, E. A. Zamchalova, G. T. Zatsepin, I. S. Zayarnaya

研究成果: Article査読

9 被引用数 (Scopus)

抄録

We report experimental results obtained by using a wide-gap type emulsion chamber flown in the first Japanese-Russo joint balloon project, called RUNJOB (RUssia-Nippon JOint Balloon-program). Two balloons were launched from Kamchatka in July 1995, and both were recovered successfully near the Volga River. The exposure time was 130 hours for the first flight and 168 hours for the second. The mean ceiling altitude, in both flights, was 32 km corresponding to 10 g/cm 2 . Total area of the emulsion chamber was 0.8 m 2 , and the thickness 0.385 and 2.28 collision m.f.p.'s for vertically incident proton- and iron-primaries, respectively. We detected 381 showers using Fuji-#200-type X-ray film; of these 174 showers were due to atmospheric secondary γ -rays, and the rest 207 came from nuclear components. The energy range covers 20Ο200 TeV for proton-primary, 3Ο30 TeV/nucleon for helium-primary, and 0.7Ο5 TeV/nucleon for iron-primary. We give the energy spectra for various elements (proton, helium, ..., iron) as well as the all-particle spectrum and the average mass of the cosmic-ray primaries.

本文言語English
ページ(範囲)1839-1845
ページ数7
ジャーナルAdvances in Space Research
26
11
DOI
出版ステータスPublished - 2000 12
外部発表はい

ASJC Scopus subject areas

  • 航空宇宙工学
  • 天文学と天体物理学
  • 地球物理学
  • 大気科学
  • 宇宙惑星科学
  • 地球惑星科学(全般)

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