A method for determining the age of cosmic rays in the Galaxy

Details A method for determining the age of cosmic rays in the Galaxy A method for determining the age of cosmic rays in the Galaxy

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983chjss...2..224h&link_type=abstract

(Chinese Journal of Space Science, vol. 2, Sept. 1982, p. 224-230) Chinese Physics (ISSN 0273-429X), vol. 3, Jan.-Mar. 1983, p.

Physics

Cosmic Rays, Galactic Radiation, Abundance, Chronology, Heao 3, Interstellar Matter, Iron Isotopes, Manganese Isotopes

Scientific paper

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.

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