Implications of the experimental results on high energy cosmic rays with regard to their origin

Details Implications of the experimental results on high energy cosmic rays with regard to their origin Implications of the experimental results on high energy cosmic rays with regard to their origin

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....2..288f&link_type=abstract

In its 19th Intern. Cosmic Ray Conf., Vol. 2 p 288-291 (SEE N85-34006 22-93)

Other

Anisotropy, Cosmic Ray Showers, Energy Spectra, Galactic Evolution, Heavy Nuclei, Diffusion, Interstellar Matter, Magnetic Fields

Scientific paper

It was shown in an earlier report that current cosmic ray evidence supports a change in the cosmic ray composition in the region between 10 to the 6th power and 10 to the 8th power GeV total energy in the direction of a smaller average value of A. Compared to normal celestial abundances, the heavy nuclei are much less abundant, and, in fact, the composition measurements above 10 to the 8th power GeV are consistent with there being only protons. Here, these results combined with those of the energy spectrum and anisotropy of the comsic rays and other astrophysical information will be examined to try to determine their implications for the origin of the cosmic rays. In this paper, consideration is given to the implications of one or more than one type of source in the galaxy to see which are consistent with the interpretation of current measurements. The nature of the source types that would be required are discussed.

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