THE PROPAGATION OF COSMIC RAYS IN INTERSTELLAR MATTER:PATHLENGTH,RESIDENCE TIME AND AGE

Huang Yong-nian; Cheng Tung-yuan; Zhang Gong-liang

doi:10.11728/cjss1983.02.157

Volume 3 Issue 2

Apr. 1983

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Article Navigation > Chinese Journal of Space Science > 1983 > 3(2): 157-161

Huang Yong-nian, Cheng Tung-yuan, Zhang Gong-liang. THE PROPAGATION OF COSMIC RAYS IN INTERSTELLAR MATTER:PATHLENGTH,RESIDENCE TIME AND AGE[J]. Chinese Journal of Space Science, 1983, 3(2): 157-161. doi: 10.11728/cjss1983.02.157

Citation:

Huang Yong-nian, Cheng Tung-yuan, Zhang Gong-liang. THE PROPAGATION OF COSMIC RAYS IN INTERSTELLAR MATTER:PATHLENGTH,RESIDENCE TIME AND AGE[J]. Chinese Journal of Space Science, 1983, 3(2): 157-161. doi: 10.11728/cjss1983.02.157

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THE PROPAGATION OF COSMIC RAYS IN INTERSTELLAR MATTER:PATHLENGTH,RESIDENCE TIME AND AGE

doi: 10.11728/cjss1983.02.157 cstr: 32142.14.cjss1983.02.157

Institute of Space Physics, Academia Sinica

Received Date: 1982-09-23
Rev Recd Date: 1900-01-01
Publish Date: 1983-04-24

Abstract

Abstract

The escape path length,the residence time and lifetime of cosmic rays in the Galaxy are determined by analyzing the HEAO-3 C-2 data on the relative abundance of manganese to iron in terms of the solutions of cosmic ray propagation equations derived in paper [1].