The steady state of the primary and secondary components of cosmic rays

Author:

Cowsik R.,Pal Yash,Tandon S. N.,Verma R. P.

Abstract

The steady state of primary and secondary components of cosmic rays has been calculated for a specific class of models. The results reproduce the observed experimental spectra down to ~50 MeV/n.

Publisher

Canadian Science Publishing

Subject

General Physics and Astronomy

Reference2 articles.

Cited by 9 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. Positrons and Antiprotons in Galactic Cosmic Rays;Annual Review of Nuclear and Particle Science;2016-10-19

2. An Overview of Cosmic Ray Research: Composition, Acceleration and Propagation;Genesis and Propagation of Cosmic Rays;1988

3. Cosmic-ray propagation in the Galaxy and in the heliosphere - The path-length distribution at low energy;The Astrophysical Journal Supplement Series;1987-05

4. Alpha-spallation cross sections at 920 MeV (230 MeV/N) inAl27,O16,C12, andBe9, and application to cosmic-ray transport;Physical Review C;1974-05-01

5. Cosmic Rays in the Galaxy;Annual Review of Astronomy and Astrophysics;1969-09

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