Energy dependence of the Si/Fe ratio in the galactic cosmic rays

Details Energy dependence of the Si/Fe ratio in the galactic cosmic rays Energy dependence of the Si/Fe ratio in the galactic cosmic rays

Apr 1975

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975apj...197..489g&link_type=abstract

Astrophysical Journal, vol. 197, Apr. 15, 1975, pt. 1, p. 489-493.

Astronomy and Astrophysics

Astrophysics

7

Cosmic Rays, Energy Spectra, Galactic Radiation, Heavy Nuclei, Iron, Silicon, Astronomical Models, Balloon-Borne Instruments, Explorer Satellites, Kinetic Energy, Mass Ratios, Radiation Spectra, Satellite-Borne Instruments, Scintillation Counters

Scientific paper

New measurements are reported of the Si/Fe ratio and the differential energy spectra of galactic cosmic-ray Si and Fe, taking into account the energy range from 35 MeV to 4 GeV per nucleon. The measured data were obtained with the aid of satellite and balloon-borne instrumentation. It is found that for the region below 1 GeV per nucleon the local interstellar spectra computed are consistent with previous galactic cosmic-ray propagation models obtained by Shapiro and Silberberg (1970) and Mason (1972).

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