Chemical composition of the primary cosmic rays near the top of the atmosphere-Reference-Cited by-同舟云学术

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Chemical composition of the primary cosmic rays near the top of the atmosphere

Published:1991-01 Issue:1 Volume:14 Page:35-40
ISSN:0390-5551
Container-title:Il Nuovo Cimento C
language:en
Short-container-title:Il Nuovo Cimento C

Author:

Bhattacharyya D. P.,Pal P.,Basu B.,Mukherjee S. C.,Ganguly A. K.,Fujii M.

Publisher

Springer Science and Business Media LLC

Subject

General Medicine

Link

http://link.springer.com/content/pdf/10.1007/BF02509255.pdf

Reference25 articles.

1. V. S. Chohan, V. S. Bhatia, S. B. Pahbi andS. Biswas:Proceedings of the XIII International Cosmic Ray Conference, Denver, 1973, Vol.1 (University of Denver, Colorado), p. 244.

2. O. C. Allkofer andW. Heinrich:Health Phys.,27, 543 (1974).

3. G. Singh andV. S. Bhatia:Astrophys. Space Sci.,60, 59 (1979).

4. P. K. Das andT. D. Goswami:Proceedings of the XVIII International Cosmic Ray Conference, Bangalore, 1983, Vol.2 (Tata Institute of Fundamental Research, Bombay), p. 6.

5. S. C. Arora, R. Hasan andM. S. Swami:Proceedings of the XVIII International Cosmic Ray Conference, Bangalore, 1983, Vol.2 (Tata Institute of Fundamental Research, Bombay), p. 10.

Cited by 2 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Study of fragmentation in56Fe+27Al interactions at 1.88A GeV using CR-39 (DOP) solid-state nuclear-track detector;Il Nuovo Cimento C;1992-01

2. Estimation of chemical abundance of primary cosmic-ray nuclei over Alice Springs using balloon-borne passive detectors;Il Nuovo Cimento C;1991-11

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