Estimation of chemical abundance of primary cosmic-ray nuclei over Alice Springs using balloon-borne passive detectors-Reference-Cited by-同舟云学术

Estimation of chemical abundance of primary cosmic-ray nuclei over Alice Springs using balloon-borne passive detectors

Published:1991-11 Issue:6 Volume:14 Page:595-603
ISSN:0390-5551
Container-title:Il Nuovo Cimento C
language:en
Short-container-title:Il Nuovo Cimento C

Author:

Bhattacharyya D. P.,Basu B.,Pal P.,Chakrabarty S.,Fujii M.

Publisher

Springer Science and Business Media LLC

Subject

General Medicine

Link

http://link.springer.com/content/pdf/10.1007/BF02507387.pdf

Reference15 articles.

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2. S. Tasaka, Y. Sato, N. Tateyama, H. Sugimoto, F. Fumuro andK. Hoshino:Nucl. Instrum. Methods A,236, 400 (1985).

3. T. Hayashi andT. Doke:Nucl. Instrum. Methods,174, 349 (1980).

4. T. Doke, T. Hayashi, K. Ito, T. Yanagimachi, S. Kobayashi, K. Nagano andM. Miyajima:Proceedings of the XVI International Cosmic Ray Conference, Kyoto, Vol.1 (1979), p. 364.

5. D. P. Bhattacharyya, P. Pal, B. Basu, S. C. Mukherjee, A. K. Ganguly andM. Fujii:Nuovo Cimento C,14, 35 (1991).

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