Mean Path Length of High Energy Galactic Cosmic Rays in the Galactic Disk-Reference-Cited by-同舟云学术

Mean Path Length of High Energy Galactic Cosmic Rays in the Galactic Disk

Published:1973-01 Issue:109 Volume:241 Page:98-100
ISSN:0300-8746
Container-title:Nature Physical Science
language:en
Short-container-title:Nature Physical Science

Author:

AUDOUZE J.,CESARSKY CATHERINE J.

Publisher

Springer Science and Business Media LLC

Subject

General Medicine

Link

http://www.nature.com/articles/physci241098a0.pdf

Reference15 articles.

1. Juliusson, E., Meyer, P., and Müller, D., Phys. Rev. Lett., 29, 445 (1972).

2. Ginzburg, V. L., and Syrovatskii, S. I., The Origin of Cosmic Rays (Pergamon Press, Oxford, 1964).

3. Meneguzzi, M., Audouze, J., and Reeves, H., Astron. Astrophys., 15, 337 (1971).

4. Buffington, A., Smith, L. H., and Smooth, G., in Proc. Twelfth Intern. Conf. Cosmic Rays, Hobart, 1971 (edit. by Fenton, A. G., and Fenton, K. B.), 1, 147 (University of Tasmania, 1972).

5. Cartwright, B. G., Garcia-Munoz, M., and Simpson, J. A., in Proc. Twelfth Intern. Conf. Cosmic Rays, Hobart, 1971 (edit. by Fenton, A. G., and Fenton, K. B.), 1, 215 (University of Tasmania, 1972).

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