22Ne excess in cosmic rays from the inner galaxy

Details 22Ne excess in cosmic rays from the inner galaxy 22Ne excess in cosmic rays from the inner galaxy

Sep 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000aipc..528..417s&link_type=abstract

ACCELERATION AND TRANSPORT OF ENERGETIC PARTICLES OBSERVED IN THE HELIOSPHERE: ACE 2000 Symposium. AIP Conference Proceedings, V

Other

4

Cosmic Rays

Scientific paper

The abundances of heavy cosmic ray nuclei at the solar system are calculated in a 3 dimension galactic model with cylindrical symmetry and with diffusive confinement. In this model the overabundance of 22Ne is energy dependent. A comparison with HEAO data is suggestive of a radial dependent source of 22Ne in the galaxy steeper than the source of the other heavy cosmic rays. .

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