The propagation of cosmic rays in interstellar matter Pathlength, residence time and age

Details The propagation of cosmic rays in interstellar matter Pathlength, residence time and age The propagation of cosmic rays in interstellar matter Pathlength, residence time and age

Sep 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983chjss...3q.157h&link_type=abstract

(Chinese Journal of Space Science, vol. 3, no. 2, 1983, p. 157-161) Chinese Astronomy and Astrophysics (ISSN 0275-1062), vol. 7,

Astronomy and Astrophysics

Astrophysics

Galactic Cosmic Rays, Interstellar Matter, Wave Propagation, Energy Spectra, Heao 3, Manganese Isotopes, Proton Energy, Radioactive Decay, Space Density

Scientific paper

The solution of the propagation equation of galactic cosmic rays obtained by Huang (1983) is employed to analyze HEAO-3 C-2 data. The escape path length distribution parameters, residence time, and the lifetime of high-energy particles are calculated. The age of the cosmic rays is calculated from the decay of Mn-54. The dependence of the residence time on the interstellar density is determined for three selected energies.

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