Variations in the propagation of UH-nuclei

Details Variations in the propagation of UH-nuclei Variations in the propagation of UH-nuclei

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....3....1w&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 3 p 1-4 (SEE N85-34862 23-93)

Astronomy and Astrophysics

Astronomy

Astronomical Models, Heavy Nuclei, Interstellar Matter, Ionization Potentials, Nuclides, Primary Cosmic Rays, Galactic Radiation, Potential Energy, Propagation Velocity, Variations

Scientific paper

Calculations of the propagation of UH-nuclei were improved by extending the number of individual nuclides considered, and by using more recent evaluations of the rigidity dependence of the escape length, the possible source composition, and altered cross sections. The effects of using different expressions for the dependence of abundances on first ionization potentials (FIP) are outlined. The sensitivity of the calculated elemental abundances to the various changes made in the propagation assumptions are discussed.

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