A METHOD FOR DETERMINING THE AGE OF COSMIC RAYS IN THE GALAXY

Huang Yong-nian

doi:10.11728/cjss1982.03.224

Volume 2 Issue 3

Aug. 1982

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Article Navigation > Chinese Journal of Space Science > 1982 > 2(3): 224-230

Huang Yong-nian. A METHOD FOR DETERMINING THE AGE OF COSMIC RAYS IN THE GALAXY[J]. Chinese Journal of Space Science, 1982, 2(3): 224-230. doi: 10.11728/cjss1982.03.224

Citation:

Huang Yong-nian. A METHOD FOR DETERMINING THE AGE OF COSMIC RAYS IN THE GALAXY[J]. Chinese Journal of Space Science, 1982, 2(3): 224-230. doi: 10.11728/cjss1982.03.224

Huang Yong-nian. A METHOD FOR DETERMINING THE AGE OF COSMIC RAYS IN THE GALAXY[J]. Chinese Journal of Space Science, 1982, 2(3): 224-230. doi: 10.11728/cjss1982.03.224

Citation:

Huang Yong-nian. A METHOD FOR DETERMINING THE AGE OF COSMIC RAYS IN THE GALAXY[J]. Chinese Journal of Space Science, 1982, 2(3): 224-230. doi: 10.11728/cjss1982.03.224

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A METHOD FOR DETERMINING THE AGE OF COSMIC RAYS IN THE GALAXY

doi: 10.11728/cjss1982.03.224 cstr: 32142.14.cjss1982.03.224

Huang Yong-nian

Institute of Space Physics, Academic, Sinica

Received Date: 1981-12-02
Rev Recd Date: 1900-01-01
Publish Date: 1982-08-24

Abstract

Abstract

This paper presents a way to determine the age of cosmic rays in the galaxy by using the data on the ratio of the abundance of manganese to iron from,the Danish-French isotope instrument on board HEAO-3.The leaky-box model and the exponential path-length distribution have been adopted in this paper.